From a6f0273fa2b8d74829a096c471316bd8a41fcd86 Mon Sep 17 00:00:00 2001 From: stefano scardigli Date: Wed, 10 Apr 2024 12:27:37 +0200 Subject: [PATCH 1/2] again... --- .../data/inaf_cpcp_superdarn_datacube.rst | 238 +++++++++--- .../data/inaf_cpcp_superdarn_image.rst | 48 --- .../data/inaf_data_solopas_timeseries.rst | 161 +++++--- .../products/data/inaf_exosphere_model.rst | 34 -- .../data/inaf_flux1h_svirco_timeseries.rst | 84 ++-- .../data/inaf_flux1m_svirco_timeseries.rst | 43 --- .../data/inaf_flux5m_svirco_timeseries.rst | 95 +++-- .../data/inaf_flux_nmtg_timeseries.rst | 37 -- .../products/data/inaf_gsmaps_datacube.rst | 93 +++-- .../products/data/inaf_m2flare_tableset.rst | 159 ++++++-- .../products/data/inaf_na_mercexo_image.rst | 171 +++++++-- .../data/inaf_p_svirco_timeseries.rst | 42 -- .../products/data/inaf_s1sep_tableset.rst | 236 +++++++++--- .../products/data/inaf_s2sep_tableset.rst | 236 +++++++++--- .../data/inaf_swflux_merc_tableset.rst | 45 --- 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--- a/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst +++ b/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst @@ -1,52 +1,196 @@ -======================================== -INAF SuperDARN Cross Polar Cap Potential -======================================== +============================= +SuperDARN Polar Cap Potential +============================= .. contents:: The tiny table of contents -SuperDARN maximum potential difference measured across the polar caps. - -:download:`Further readings (pdf) <../../private/inaf_cpcp_superdarn_datacube-SuperDARN_data_handling.pdf>`. - - - -**Providers**: - -- **SupeDARN radars British Antarctic Survey repository** - sources: - - - https://www.bas.ac.uk/project/superdarn/ - - - - - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-05-04T16:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +The Super Dual Auroral Radar Network (SuperDARN) is an international network of +High Frequency coherent scatter radars. A map of the fields of view of the radars +currently in operation can be seen in Figure 1: INAF-IAPS manages the radar pair of +Dome C East (DCE) and Dome C North (DCN) located at the Concordia station, in +Antarctica, whose fields of view are shaded in green in the figure. +The SuperDARN concept is described in detail in [2]. A SuperDARN radar is a bistatic +apparatus (i.e. the same antennae and the same electronics are used to both transmit +and receive signals to/from the ionosphere), which works in the 8-20 MHz frequency +range: coded sequences of radio pulses are steered through a field of view several tens +degrees wide along a number of “beams” (directions), so that the whole field of view +is covered in one or two minutes, depending on the operating mode. Along each beam, +the pulse sequence defines from 75 to 100 range gates, from 180 km up to 3000 km +from the radar site, where the radio signals encounter plasma density irregularities in +the ionosphere, which cause such signals to be scattered back along the same direction. +As ionospheric irregularities are dragged in the large scale convection at high latitudes, the measure of the Doppler phase shift between the emitted and backscattered waves +allows to infer the velocity of the ambient plasma with respect to the sounded direction +and gate. + +**References** + +https://www.sciencedirect.com/science/article/abs/pii/S136468260600263X + +[1] SuperDARN Data Analysis Working Group, Thomas, E. G., Reimer, A. S., Bland, +E. C., Burrell, A. G., Grocott, A., Ponomarenko, P. V., Schmidt, M. T., Shepherd, S. G., +Sterne, K. T., and Walach, M.-T, SuperDARN Radar Software Toolkit (RST) 5.0 (v5.0). +Zenodo (2022). https://doi.org/10.5281/zenodo.7467337 + +[2] Greenwald, R.A., Baker, K.B., Dudeney, J.R. et al., DARN/SuperDARN, A global +view of the dynamics of high-latitude convection, Space Sci Rev, 71, 761–796 (1995). +https://doi.org/10.1007/BF00751350 + +[3] Ruohoniemi, J.M., and K.B. Baker, Large-scale imaging of high-latitude +convection with Super Dual Auroral Radar Network HF radar observations, J. Geophys. Res., Space Physics, 103, 20797-20811 (1998).https://doi.org/10.1029/98JA01288 + +[4] Thomas, E. G., and S. G. Shepherd, Statistical Patterns of Ionospheric Convection +Derived From Mid-latitude, High-Latitude, and Polar SuperDARN HF Radar +Observations, J. Geophys. Res., Space Physics, 123(4), 3196-3216 (2018). +https://doi.org/10.1002/2018JA025280 + +[5] Baker, K. B., and S. Wing, A new coordinate system for conjugate studies at high latitudes, J. Geophys. Res., 94(A7), 9139 (1989).https://doi.org/10.1029/JA094iA07p09139 +[6] Shepherd, S. G., Altitude-Adjusted Corrected Geomagnetic Coordinates: Definition +and Functional Approximations, J. Geophys. Res., Space Physics, 119(9), 7501-7521 +(2014). https://doi.org/10.1002/2014JA020264 + +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - ASCII - - -| **Sample**: SuperDARN_CPCP - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- 2320.2 meta data mapping: meta data mapping (MANCA NELLA TENDINA) -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** inaf_cpcp_superdarn_datacube + +**publisher:** INAF + +**alphanumeric_code:** 31 + +**id_tmp:** 71 + +**short_name:** SuperDARN CPCP + +**identifier:** aspis://inaf/cpcp_superdarn_datacube + +**dynamic:** static + +**size:** 200MB + +**format:** csv + +**type:** timeseries + +**records_number:** 1515672 + +**time_start:** 2015-06-21 + +**time_stop:** 2017-09-11 + +**spatial:** IONO + +**messenger:** electrons, + +**spectral_min:** 0 + +**spectral_max:** 1 + +**spectral_units:** dimensionless + +**observable:** IMF,GEOINDEX + +**latest update:** 2024-04-04 01:53:25 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - Time representation ISO8601: YYYY-MO-DYTHR:MN:SC + * - 2 + - hem + - + - string + - Flag identifying the hemisphere where data are taken for a given record. “N”=North; “S”=South + * - 3 + - ndata + - counts + - int + - Number of velocity vectors actually measured by the radars in the given time interval + * - 4 + - minlat + - deg + - int + - Low latitude limit for the convection: it is the 0 described in Section 2. + * - 5 + - latpole + - deg + - float + - Geographic latitude of the AACGM pole (North or South). It can be useful for coordinate transformations. + * - 6 + - lonpole + - deg + - float + - Geographic longitude of the AACGM pole (North or South). It can be useful for coordinate transformations. + * - 7 + - radpole + - Earth radii (Re=6371.2 km) + - float + - Distance from the centre of the Earth of the AACGM pole. + * - 8 + - imfbx + - nT + - float + - GSM* x component of the interplanetary magnetic field. Data are taken from DSCOVR spacecraft, ballistically propagated to the centre of the Earth, median filtered and averaged in the 2 minutes time intervals of the radar scans. IMF is used to select the model patterns to be added to the measured vectors in order to reconstruct convection in the whole polar cap. + * - 9 + - imfby + - nT + - float + - GSM* y component of the interplanetary magnetic field. + * - 10 + - imfbz + - nT + - float + - GSM* z component of the interplanetary magnetic field. + * - 11 + - imfbt + - nT + - float + - IMF strength. Btot = sqrt(Bx^2 + By^2 + Bz^2) + * - 12 + - kpr + - + - string + - Range of geomagnetic Kp index during the given time interval. This parameter is used to select the model patterns to be added to the measured vectors in order to reconstruct convection in the whole polar cap. This field represents an information useful to be reported in the convection maps. + * - 13 + - cpcp + - V + - float + - Cross Polar Cap Potential: Maximum potential difference through the polar cap. + * - 14 + - maxpot + - V + - float + - Maximum positive value of the electric potential. + * - 15 + - minpot + - V + - float + - Minimum negative value of the electric potential. + * - 16 + - l + - counts + - int + - l-order of the harmonic expansion of the potential. + * - 17 + - m + - counts + - int + - m-order of the harmonic expansion of the potential. -l ≤ m ≤ l + * - 18 + - coef + - V + - float + - Alm coefficient of the harmonic expansion of the potential. If m<0, then the coefficient is the Blm in Eq. 2. diff --git a/docs/source/products/data/inaf_cpcp_superdarn_image.rst b/docs/source/products/data/inaf_cpcp_superdarn_image.rst deleted file mode 100644 index 0e0ebb7..0000000 --- a/docs/source/products/data/inaf_cpcp_superdarn_image.rst +++ /dev/null @@ -1,48 +0,0 @@ -===================================== -INAF SuperDARN Convection Maps (data) -===================================== - -.. contents:: The tiny table of contents - -Ionospheric convection maps at high latitudes in both hemispheres derived from the raw SuperDARN data retrieved from the BAS repository. - -**Providers**: - -- **SupeDARN radars British Antarctic Survey repository** - sources: - - - https://www.bas.ac.uk/project/superdarn/ - - - - - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-05-04T16:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - PNG - - -| **Sample**: SuperDARN_Maps_data - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- 2320.2 meta data mapping: meta data mapping (MANCA NELLA TENDINA) -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/inaf_data_solopas_timeseries.rst b/docs/source/products/data/inaf_data_solopas_timeseries.rst index c303fa2..cb30f8d 100644 --- a/docs/source/products/data/inaf_data_solopas_timeseries.rst +++ b/docs/source/products/data/inaf_data_solopas_timeseries.rst @@ -1,61 +1,122 @@ -========================================= -INAF Solar Orbiter-PAS data -========================================= +================================ +INAF-IAPS Solar Orbiter-PAS data +================================ .. contents:: The tiny table of contents -The product contains density N, speed vector V, pressure tensor P, temperature components (Tx, Ty, Tz), and the velocity of the satellite V_solo, computed using the data collected by the Proton-Alpha Sensor (PAS) onboard Solar Orbiter. -PAS measures the 3D distribution functions of the dominant ions of the solar wind, from 200 eV to 20 KeV, without mass and charge selection. In practice, this concerns mostly the proton and alfa populations (unseparated). At full resolution, PAS collects the 3D ion distribution function in about 1 second, even though the moments have a cadence of 4 seconds, while in “snapshot” mode the phase space sampling is reduced, allowing a greater cadence for the moments. +The product contains density N, speed vector V, pressure tensor P, temperature components (Tx, Ty, Tz), and the velocity of the satellite V_solo, computed using the data collected by the Proton-Alpha Sensor (PAS) onboard Solar Orbiter. +PAS measures the 3D distribution functions of the dominant ions of the solar wind, from 200 eV to 20 KeV, without mass and charge selection. In practice, this concerns mostly the proton and alfa populations (unseparated). At full resolution, PAS collects the 3D ion distribution function in about 1 second, even though the moments have a cadence of 4 seconds, while in “snapshot” mode the phase space sampling is reduced, allowing a greater cadence for the moments. + Data is hosted on http://soar.esac.esa.int/soar/ **References** -R. D’Amicis et al, Astronomy &Astrophysics 656, A21 (2021) - -B. Lavraud et al, Astronomy &Astrophysics 656, A37 (2021) - -D. Perrone et al, Astronomy &Astrophysics 668, A189 (2022) - +R. D’Amicis et al, Astronomy &Astrophysics 656, A21 (2021) + +B. Lavraud et al, Astronomy &Astrophysics 656, A37 (2021) + +D. Perrone et al, Astronomy &Astrophysics 668, A189 (2022) + R. De Marco et al, Astronomy &Astrophysics, 669, A108 (2023) -**Providers**: - -- **Solar Orbiter** - source: - - - SWA-PAS - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-20T19:10:47+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - cdf - - -| **Sample**: https://drive.google.com/file/d/1X_6RZeN72zjR11g2DYNoMTr6DP6vDg_t/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.3: Mirroring: bulk static -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- 2330.1: wiki -- 2320.2: metadata mapping -- SAMP: Sul Solar Orbiter ARchive questi dati possono essere condivisi via SAMP - +**internal_name:** inaf_data_solopas_timeseries + +**publisher:** INAF-IAPS, Plasma & Space Weather Group + +**alphanumeric_code:** 14 + +**id_tmp:** 72 + +**short_name:** SolO-PAS_data + +**identifier:** aspis://inaf/data_solopas_timeseries + +**dynamic:** a file each day (file size between 3 and 4 Mb). As a general rule, one month of data is uploaded each month, generally relating to 3 months before the upload date + +**size:** 2GB + +**format:** dsv + +**type:** timeseries + +**records_number:** 38653 + +**time_start:** 2020-07-06 + +**time_stop:** 2022-01-31 + +**spatial:** IP + +**messenger:** Protons + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** SW,SEP + +**latest update:** 2024-04-04 01:54:59 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - Datetime [UTC ] + * - 2 + - N + - cm^-3 + - float + - Protono Density [cm^-3] + * - 3 + - VR + - Km/s + - float + - Proton Velocity along the R direction [Km/s] + * - 4 + - VT + - Km/s + - float + - Proton Velocity along the T direction [Km/s] + * - 5 + - VN + - Km/s + - float + - Proton Velocity along the N direction [Km/s] + * - 6 + - T + - eV + - float + - Proton Temperature [eV] + * - 7 + - VR_SolO + - Km/s + - float + - Spacecraft Velocity along the R direction [Km/s] + * - 8 + - VT_SolO + - Km/s + - float + - Spacecraft Velocity along the T direction [Km/s] + * - 9 + - VN_SolO + - Km/s + - float + - Spacecraft Velocity along the N direction [Km/s] diff --git a/docs/source/products/data/inaf_exosphere_model.rst b/docs/source/products/data/inaf_exosphere_model.rst deleted file mode 100644 index 377192f..0000000 --- a/docs/source/products/data/inaf_exosphere_model.rst +++ /dev/null @@ -1,34 +0,0 @@ -============================================================ -INAF Montecarlo, single particle exospheric model of Mercury -============================================================ - -.. contents:: The tiny table of contents - -The model is based on the code by Mura et al., described in doi:10.1016/j.icarus.2008.11.014, doi:10.1016/j.pss.2006.11.028 and integrated in doi: 10.1016/j.pss.2011.08.012 - -**Providers**: - -INAF - -| **Product Type**: software - -| **Status**: Active - -| **Creation date**: 2022-05-10T16:05:00+02:00 - -| **Last Update**: 2022-05-10T04:10:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: ND - -| **Data formats**: ND - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -- ext2220.5: On demand computation - diff --git a/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst b/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst index c88d3de..ece0c56 100644 --- a/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst +++ b/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst @@ -1,46 +1,78 @@ -========================================= -INAF SVIRCO neutron monitor (1h) -========================================= +============================================= +SVIRCO Observatory - the Rome neutron monitor +============================================= .. contents:: The tiny table of contents -Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. +Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 1h. Average intensity of January-February 1997 = 100% -Resolution: 1h. +**References** -Average intensity of January-February 1997 = 100% -**Providers**: -- **SVIRCO neutron monitor** +Data description +~~~~~~~~~~~~~~~~ +**internal_name:** inaf_flux1h_svirco_timeseries -| **Product Type**: data +**publisher:** INAF -| **Status**: Active +**alphanumeric_code:** 42C -| **Creation date**: 2022-04-28T13:31:08+02:00 +**id_tmp:** 73 -| **Last Update**: 2023-10-01T12:00:00+02:00 +**short_name:** flux1h_SVIRCO -Data Description -~~~~~~~~~~~~~~~~ +**identifier:** inaf_flux1h_svirco_timeseries + +**dynamic:** Data collection grows in time. + +**size:** 13MB + +**format:** CSV + +**type:** timeseries + +**records_number:** 479976 + +**time_start:** 1966-04-01 + +**time_stop:** 2020-12-31 + +**spatial:** GROUND + +**messenger:** Nucleons + +**spectral_min:** 6.3 -| **Data type**: timeseries +**spectral_max:** 9999 -| **Data formats**: - ASCII +**spectral_units:** GeV +**observable:** GLE,GCR -| **Sample**: https://drive.google.com/file/d/17ahUkpirH-DUWnqBr731ExAgjMBGNeJ4/view?usp=sharing +**latest update:** 2024-03-28 05:08:05 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.3: Mirroring: bulk static -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - Time + * - 2 + - I + - % + - float + - % - Normalized Intensity of the cosmic ray secondary nucleonic component measured by the Rome neutron monitor. The counting rates have been normalized to the reference value of January-February 1997 (= 100%). diff --git a/docs/source/products/data/inaf_flux1m_svirco_timeseries.rst b/docs/source/products/data/inaf_flux1m_svirco_timeseries.rst deleted file mode 100644 index 56a72c4..0000000 --- a/docs/source/products/data/inaf_flux1m_svirco_timeseries.rst +++ /dev/null @@ -1,43 +0,0 @@ -========================================= -INAF SVIRCO neutron monitor (1m) -========================================= - -.. contents:: The tiny table of contents - -Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 1min -Average intensity of January-February 1997 = 100% - -**Providers**: - -- **SVIRCO neutron monitor** - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-28T13:31:08+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - ASCII - - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -- int2130.3: Mirroring: bulk static -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst b/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst index 274a7e9..3248096 100644 --- a/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst +++ b/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst @@ -1,43 +1,88 @@ -========================================= -INAF SVIRCO neutron monitor (5m) -========================================= +============================================== +SVIRCO Obser vatory - the Rome neutron monitor +============================================== .. contents:: The tiny table of contents -Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 5min -Average intensity of January-February 1997 = 100% +Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 5min Average intensity of January-February 1997 = 100% -**Providers**: +**References** -- **SVIRCO neutron monitor** -| **Product Type**: data +Data description +~~~~~~~~~~~~~~~~ -| **Status**: Active +**internal_name:** inaf_flux5m_svirco_timeseries -| **Creation date**: 2022-04-28T13:31:08+02:00 +**publisher:** INAF -| **Last Update**: 2023-10-01T12:00:00+02:00 +**alphanumeric_code:** 42B -Data Description -~~~~~~~~~~~~~~~~ +**id_tmp:** 74 + +**short_name:** flux5m_SVIRCO + +**identifier:** inaf_flux5m_svirco_timeseries + +**dynamic:** Data collection grows in time. + +**size:** 80MB + +**format:** CSV + +**type:** timeseries + +**records_number:** 2007072 + +**time_start:** 1997-05-21 + +**time_stop:** 2017-01-01 + +**spatial:** GROUND + +**messenger:** Neutrons + +**spectral_min:** 6.3 -| **Data type**: image +**spectral_max:** 9999 -| **Data formats**: - ASCII +**spectral_units:** GeV +**observable:** GLE,GCR -| **Sample**: https://drive.google.com/file/d/1U4o3cRHggf7_9f8V_qCVvgRt0RufDxIw/view?usp=sharing +**latest update:** 2024-03-28 05:08:05 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - time + * - 2 + - inc + - counts + - int + - Counting rates (not pressure corrected) of the cosmic ray secondary nucleonic component measured by the Rome neutron monitor + * - 3 + - pressure + - hPa + - float + - Pressure measured at the SVIRCO Observatory + * - 4 + - corr + - counts + - int + - Efficiency and pressure corrected counting rates of the cosmic ray secondary nucleonic component measured by the Rome neutron monitor diff --git a/docs/source/products/data/inaf_flux_nmtg_timeseries.rst b/docs/source/products/data/inaf_flux_nmtg_timeseries.rst deleted file mode 100644 index 218f8b4..0000000 --- a/docs/source/products/data/inaf_flux_nmtg_timeseries.rst +++ /dev/null @@ -1,37 +0,0 @@ -========================================= -INAF Testa Grigia neutron monitor data -========================================= - -.. contents:: The tiny table of contents - -Counting rate of the neutron monitor operating at the Testa Grigia Station (3480 m, Cervinia, Italy). The aim is to study the cosmic ray intensity variations in correlation with solar activity and space weather phenomena. - -**Providers**: - -- **Testa Grigia Station** - source: - - - Neutron Monitor - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-29T15:00:52+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text - - -| **Sample**: https://drive.google.com/file/d/1Y317ed51_CDLsOEVGXh05uC4WibUFXS5/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -ND diff --git a/docs/source/products/data/inaf_gsmaps_datacube.rst b/docs/source/products/data/inaf_gsmaps_datacube.rst index da5f939..60bd736 100644 --- a/docs/source/products/data/inaf_gsmaps_datacube.rst +++ b/docs/source/products/data/inaf_gsmaps_datacube.rst @@ -1,53 +1,88 @@ ===================================================== -INAF Grad-Shafranov Reconstruction of Magnetic Clouds +IAPS Grad-Shafranov Reconstruction of Magnetic Clouds ===================================================== .. contents:: The tiny table of contents Quasi 3-d magnetic field maps of magnetic field configuration within magnetic clouds for geoeffective target SWE events. Such maps will be estimated through the Grad-Shafranov reconstruction from single-spacecraft plasma and magnetic field data. -**Providers**: +**References** -- **Wind** - sources: - - MFI - - SWE -- **Solar Orbiter** - sources: - - SWA - - MAG -- **Small Scale Magnetic Flux Rope Database** - source: +Data description +~~~~~~~~~~~~~~~~ - - http://fluxrope.info/ +**internal_name:** inaf_gsmaps_datacube +**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali -| **Product Type**: data +**alphanumeric_code:** 25 -| **Status**: Active +**id_tmp:** 96 -| **Creation date**: 2022-04-26T12:00:39+02:00 +**short_name:** gsmaps-cubes -| **Last Update**: 2023-10-01T12:00:00+02:00 +**identifier:** aspis://inaf/gsmaps_datacube -Data Description -~~~~~~~~~~~~~~~~ +**dynamic:** static + +**size:** 300kB + +**format:** nc + +**type:** spectrum + +**records_number:** 3 + +**time_start:** 1997-01-01 + +**time_stop:** 2022-01-01 + +**spatial:** IP + +**messenger:** Magnetic field,Magnetic vector potential,Flux rope coordinates + +**spectral_min:** -| **Data type**: spectral-cubes +**spectral_max:** -| **Data formats**: - mat +**spectral_units:** +**observable:** phys.magField,phys.potential,phys.size -| **Sample**: https://drive.google.com/file/d/1Sij8YjsMeCS_vVwOxHzTDreAHYNy6p0r/view?usp=sharing +**latest update:** 2024-03-28 05:08:05 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - datetime - Time associated with the Grad-Shafranov reconstruction + * - 2 + - data_name + - char + - string + - the name of the file with the data + * - 3 + - prew_name + - char + - string + - the name of the full preview file + * - 4 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/inaf_m2flare_tableset.rst b/docs/source/products/data/inaf_m2flare_tableset.rst index e6ffa75..5511286 100644 --- a/docs/source/products/data/inaf_m2flare_tableset.rst +++ b/docs/source/products/data/inaf_m2flare_tableset.rst @@ -1,49 +1,128 @@ -========================================= -INAF > M2 SXR Flare Catalogue -========================================= +============================== +IAPS ≥M2 SXR Flare Catalogue +============================== .. contents:: The tiny table of contents -The catalogue will contain the > M2 Soft X- Ray (SXR) flares from 1995 to 2017. The columns in the table are defined as follows: (1) event number; (2) date of the SXR flare; (3) peak time of SXR flare; (4) peak SXR classification (saturated events flagged with an S in which case (3) refers to the onset of saturation); (5) flare location; (6) time-integrated SXR intensity (nominally between the 1/3 power points on rise and fall); (7) time-integrated 1 MHz Wind/WAVES intensity from 10 minutes before the onset of integration for the SXR burst to 10 minutes after the SXR burst peak; (8) Waves frequency used. +The catalogue will contain the > M2 Soft X- Ray (SXR) flares from 1995 to 2017. The columns in the table are defined as follows: (1) event number (2) date of the SXR flare (3) peak time of SXR flare (4) peak SXR classification (saturated events flagged with an S in which case (3) refers to the onset of saturation), (5) flare location, (6) time-integrated SXR intensity (nominally between the 1/3 power points on rise and fall), (7) time-integrated 1 MHz Wind/WAVES intensity from 10 minutes before the onset of integration for the SXR burst to 10 minutes after the SXR burst peak, (8) Waves frequency used. -**Providers**: +**References** -- **GOES** - sources: - - 1-8 Å soft X-ray flux - - http://www.ngdc.noaa.gov/stp/satellite/goes/dataaccess.html -- **Wind** - sources: - - Waves 1 MHz radio flux - - ftp://solar-radio.gsfc.nasa.gov/ - - -| **Product Type**: lookup-table - -| **Status**: Active - -| **Creation date**: 2022-04-26T12:00:39+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - xlsx - - -| **Sample**: https://docs.google.com/spreadsheets/d/1VU7WudVr_W81M7c8KldIwKS8-dqGXWrU/edit?usp=sharing&ouid=115498353997648557775&rtpof=true&sd=true - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** inaf_m2flare_tableset + +**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali + +**alphanumeric_code:** 7 + +**id_tmp:** 75 + +**short_name:** IAPS-M2SXR + +**identifier:** aspis://inaf/m2flare_tableset + +**dynamic:** static + +**size:** 100kB + +**format:** xlsx + +**type:** tableset + +**records_number:** 1040 + +**time_start:** 1995-01-01 + +**time_stop:** 2017-05-03 + +**spatial:** SUN + +**messenger:** Photons + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** phys.flux + +**latest update:** 2024-03-28 05:08:05 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - Onset date and time of each flare event + * - 2 + - Date + - yyyy/mm/dd + - datetime + - Onset date of each flare event + * - 3 + - SXR Peak Time + - hh:mm:ss XM + - datetime + - Time corresponding to the peak SXR flux + * - 4 + - SXR Class + - + - string + - Classification of SXR bursts according to their peak intensities + * - 5 + - SXR Class Label + - + - string + - Letter indicating the Peak SXR flux range, according to the standard SXR classification + * - 6 + - SXR Class Intensity + - + - float + - Number indicating the factor for the flare within the class + * - 7 + - Location Halpha-line + - + - string + - Averaged heliographic position of flare central region from observations on the H-alpha spectral line + * - 8 + - HGS lat + - deg + - float + - Averaged heliographic latitude of flare central region from observations on the H-alpha spectral line + * - 9 + - HGS lon + - deg + - float + - Averaged heliographic longitude of flare central region from observations on the H-alpha spectral line + * - 10 + - SXR Fluence + - J/m^2 + - float + - Time integrated SXR intensity between the 1/3 power points on rise and fall (J m^2) + * - 11 + - Wind/Waves Fluence + - sfu*min + - float + - Time integrated 1 MHz intensity from Wind/Waves from 10 minutes before the onset of integration for the SXR burst to 10 minutes after the SXR burst peak (sfu x min) + * - 12 + - Frequency + - kHz + - int + - Used Wind/Waves frequency close to 1 MHz (Hz) diff --git a/docs/source/products/data/inaf_na_mercexo_image.rst b/docs/source/products/data/inaf_na_mercexo_image.rst index 82363fa..3c2ad68 100644 --- a/docs/source/products/data/inaf_na_mercexo_image.rst +++ b/docs/source/products/data/inaf_na_mercexo_image.rst @@ -1,38 +1,153 @@ =============================================== -INAF Bidimensional maps of Mercury Na exosphere +INAF-bidimensional maps of Mercury Na exosphere =============================================== .. contents:: The tiny table of contents -Dataset of observations of Mercury's exosphere in the sodium D lines. Data are taken from the ground-based solar telescope THEMIS (years 2009-2013). They have been produced in both D1 and D2 lines (when both available) and converted into bi-dimensional maps of Rayleigh emission. Estimation of the “seeing” parameter is included in the jpeg files. Here the original fits files are given too for the whole database (2007-2014), and it may be expanded to the most recent data from 2021 and 2022 (TBC). Data can be provided both uncalibrated and/or calibrated (TBD). +Dataset of observations of Mercury's exosphere in the sodium D lines. Data are taken from the ground-based solar telescope THEMIS (years 2009-2013). They have been produced in both D1 and D2 lines (when both available) and converted into bi-dimensional maps of Rayleigh emission. Estimation of the “seeing” parameter is included in the jpeg files. Here the original fits files are given too for the whole data base (2007-2014), and it may be expanded to the most recent data from 2021 and 2022 (TBC). Data can be provided both uncalibrated and/or calibrated (TBD). -**Providers**: +**References** -- **THEMIS solar telescope** +Leblanc, F., Doressoundiram, A., Schneider, N., Mangano, V., López Ariste, A., Lemen, C., Gelly, B., Barbieri, C. and Cremonese, G., 2008. High latitude peaks in Mercury's sodium exosphere: Spectral signature using THEMIS solar telescope. Geophysical Research Letters, 35(18). + +Leblanc, F., Doressoundiram, A., Schneider, N., Massetti, S., Wedlund, M., López Ariste, A., Barbieri, C., Mangano, V. and Cremonese, G., 2009. Short‐term variations of Mercury's Na exosphere observed with very high spectral resolution. Geophysical research letters, 36(7). + +Mangano, V., Massetti, S., Milillo, A., Mura, A., Orsini, S. and Leblanc, F., 2013. Dynamical evolution of sodium anisotropies in the exosphere of Mercury. Planetary and Space Science, 82, pp.1-10. + +Mangano, V., Massetti, S., Milillo, A., Plainaki, C., Orsini, S., Rispoli, R. and Leblanc, F., 2015. THEMIS Na exosphere observations of Mercury and their correlation with in-situ magnetic field measurements by MESSENGER. Planetary and Space Science, 115, pp.102-109. + +Massetti, S., Mangano, V., Milillo, A., Mura, A., Orsini, S. and Plainaki, C., 2017. Short‐term observations of double‐peaked Na emission from Mercury's exosphere. Geophysical Research Letters, 44(7), pp.2970-2977. + +Orsini, S., Mangano, V., Milillo, A., Plainaki, C., Mura, A., Raines, J.M., De Angelis, E., Rispoli, R., Lazzarotto, F. and Aronica, A., 2018. Mercury sodium exospheric emission as a proxy for solar perturbations transit. Scientific reports, 8(1), p.928. - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-29T17:15:42+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: spectral-cubes - -| **Data formats**: - fts - - -| **Sample**: https://drive.google.com/file/d/1AFgzCjHNFMLXNNFVL9He7mBPKBE7k2E0/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI - +**internal_name:** inaf_na_mercexo_image + +**publisher:** Valeria Mangano, INAF-IAPS + +**alphanumeric_code:** 57 + +**id_tmp:** 76 + +**short_name:** Merc_exos_Na_fts + +**identifier:** aspis://inaf/na_mercexo_image + +**dynamic:** period 2009-2013 is static, but if we decide to include also most recent data, it will grow in time. + +**size:** 1GB + +**format:** fits + +**type:** image + +**records_number:** 7 + +**time_start:** 2009-04-17 + +**time_stop:** 2013-05-25 + +**spatial:** Mercury + +**messenger:** photons + +**spectral_min:** 5890 + +**spectral_max:** 5896 + +**spectral_units:** Angstrom + +**observable:** IMF,SW,CME + +**latest update:** 2024-04-04 01:59:34 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - date and time of start of spectral scan + * - 2 + - heliocentric_longitude + - deg + - float + - Mercury heliocentric longitude [deg] + * - 3 + - heliocentric_latitude + - deg + - float + - Mercury heliocentric latitude [deg] + * - 4 + - heliocentric_distance + - AU + - float + - Mercury heliocentric distance [AU] + * - 5 + - true_anomaly_angle + - deg + - float + - Mercury True Anomaly Angle [deg] + * - 6 + - phase_angle + - deg + - float + - Mercury Phase Angle [deg] + * - 7 + - disk_visibility + - % + - float + - Percentage of Mercury disk lit by the Sun + * - 8 + - seeing + - arcsec + - float + - estimated seeing during the spectral scan [arcsec] + * - 9 + - seeing err + - arcsec + - float + - error associated with the seeing estimation [arcsec] + * - 10 + - ave emission + - kR + - float + - Average value of the D2 Na emission [kR] + * - 11 + - emission err + - kR + - float + - error associated with the Average value of the Na emission [kR] + * - 12 + - type + - char + - string + - code for emission peaks morphology according to doi.org/10.1016/j.pss.2015.04.001 + * - 13 + - data_name + - char + - string + - the name of the file with the data + * - 14 + - prew_name + - char + - string + - the name of the full preview file + * - 15 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/inaf_p_svirco_timeseries.rst b/docs/source/products/data/inaf_p_svirco_timeseries.rst deleted file mode 100644 index 2f2e0fc..0000000 --- a/docs/source/products/data/inaf_p_svirco_timeseries.rst +++ /dev/null @@ -1,42 +0,0 @@ -========================================= -INAF SVIRCO NM Pressure -========================================= - -.. contents:: The tiny table of contents - -Average of pressure from Rome neutron monitor. Resolution: 1day - -**Providers**: - -- **SVIRCO neutron monitor** - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-28T13:31:08+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: timeseries - -| **Data formats**: - ASCII - - -| **Sample**: https://drive.google.com/file/d/17ahUkpirH-DUWnqBr731ExAgjMBGNeJ4/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/inaf_s1sep_tableset.rst b/docs/source/products/data/inaf_s1sep_tableset.rst index 268b27c..1e164d2 100644 --- a/docs/source/products/data/inaf_s1sep_tableset.rst +++ b/docs/source/products/data/inaf_s1sep_tableset.rst @@ -1,53 +1,203 @@ -========================================= -INAF S1 SEP Catalogue -========================================= +============================ +IAPS S1 SEP events Catalogue +============================ .. contents:: The tiny table of contents The catalogue contains SEP events observed at the Earth of class S1, i.e. with flux in the range [10, 100) pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux >= 100 pfu at > 10 MeV are listed in the companion table S2 SEP Catalogue. -**Providers**: +**References** -- **GOES** - sources: - - 1-8 Å soft X-ray flux, proton flux - - http://www.ngdc.noaa.gov/stp/satellite/goes/dataaccess.html -- **SOHO/LASCO CME Catalog** - source: - - https://cdaw.gsfc.nasa.gov/CME_list/ -- **Wind** - sources: - - - Waves 1 MHz radio flux - - ftp://solar-radio.gsfc.nasa.gov/ - - -| **Product Type**: lookup-table - -| **Status**: Active - -| **Creation date**: 2022-04-26T12:00:39+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - xlsx - - -| **Sample**: https://docs.google.com/spreadsheets/d/1leYT7LT1H0JNKZtFZMQQsm3XhNkYifJM/edit?usp=sharing&ouid=115498353997648557775&rtpof=true&sd=true - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** inaf_s1sep_tableset + +**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali + +**alphanumeric_code:** 16A + +**id_tmp:** 77 + +**short_name:** IAPS-S1 SEP events + +**identifier:** aspis://inaf/s1sep_tableset + +**dynamic:** static + +**size:** 100kB + +**format:** csv + +**type:** tableset + +**records_number:** 68 + +**time_start:** 1995-01-01 + +**time_stop:** 2014-09-10 + +**spatial:** Earth + +**messenger:** Protons,Photons + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** flare,CME,SEP + +**latest update:** 2024-03-28 05:08:05 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - utc + - datetime + - UTC - Time of the peak of the SEP associated soft X -ray (SXR) flare. When the time coincides with that of the CME no information about the actual time was available. + * - 2 + - SXR_class + - char + - char + - Char - Class of the SEP associated flare according to their peak intensities + * - 3 + - Flare_Latitude + - deg + - float + - Degrees - Averaged heliographic latitude of the SEP associated flare central region from observations of the H-alpha spectral line + * - 4 + - Flare_Longitude + - deg + - float + - Degrees - Averaged heliographic longitude of the SEP associated flare central region from observations of the H-alpha spectral line. The value 180 indicates longitudes >90, when it cannot be better determined. The value -180 indicates longitudes >90, when + * - 5 + - CME_NOAA_date + - utc + - datetime + - UTC - Date and time of the associated CME from the NOAA list (https://umbra.nascom.nasa.gov/SEP/) + * - 6 + - CME_SOHO_date + - utc + - datetime + - UTC - In case the CME NOAA Date was not present or not considered reliable in the previous column, the date and time of the associated CME from the SOHO list (https://cdaw.gsfc.nasa.gov/CME_list/UNIVERSAL_ver1/1998_05/univ1998_05.html) is given in this c + * - 7 + - CME_central_PA + - deg + - float + - Degrees - CME position angle measured from Solar North in degrees (counter-clockwise). The value 360 indicates a halo CME. + * - 8 + - Halo_CME_type + - char + - char + - Char - Halo CMEs are indicated in the 'CME_Central_PA' column with 360. In this column the letters ('S', 'BA', 'OA') in the brackets show type of halo CMEs. Halo CMEs can be symmetric (S) or asymmetric with respect to the occulting disk. Brightness asymme + * - 9 + - CME_angular_width + - deg + - float + - Degrees - Angular width of the CME. For values =361 more information are available in the sOHO LASCO CME catalogue (https://cdaw.gsfc.nasa.gov/CME_list/). + * - 10 + - CME_Speed_Art1 + - km/s + - float + - km/s - CME speed from catalogue of article 1 (Art1) Papaioannou et a. 2016 (doi: 10.1051/swsc/2016035) + * - 11 + - Radio_burst_type_II + - char + - int + - Int - Occurrence of type II radio burst: the value 1 indicates that the burst occurred the value 2 indicates that the burst occurred with a probability >50% the value 3 indicates that the burst occurred with a probability <50 the value 0 indicates that th + * - 12 + - Radio_burst_type_IV + - char + - int + - Int - Occurrence of type IV radio burst: the value 1 indicates that the burst occurred the value 2 indicates that the burst occurred with a probability >50% the value 3 indicates that the burst occurred with a probability <50 the value 0 indicates that th + * - 13 + - CME_Speed_Art2 + - km/s + - float + - km/s - CME speed from catalogue of article2 (ART2) Gopalswamy et al. 2015 (doi: 10.48550/arXiv.1509.04216) + * - 14 + - SOHO_CME_linear_speed + - km/s + - float + - km/s - Speed from SOHO catalogue obtained through linear fit of height-time measurements + * - 15 + - SOHO_CME_speed_2nd + - km/s + - float + - km/s - Speed from SOHO catalogue obtained through quadratic fit of height-time measurements. The speed is evaluated at the time of final height measurement + * - 16 + - SOHO_CME_speed_20_Rs + - km/s + - float + - km/s - Speed from SOHO catalogue obtained through quadratic fit of height-time measurements. The speed is evaluated when the CME is at a height of 20 solar radii + * - 17 + - CME_acceleration + - km/s^2 + - float + - km/s^2 - Acceleration of the CME + * - 18 + - SXR_Fluence + - J/m^2 + - float + - J m^2 - Time integrated SXR intensity between the 1/3 power points on rise and fall (see Laurenza et al., 2009, doi: 10.1029/2007SW000379) + * - 19 + - Radio_Fluence + - sfu*min + - float + - sfu*min - Time integrated 1 MHz intensity from Wind/Waves from 10 minutes before the onset of integration for the SXR burst to 10 minutes after the SXR burst peak (see Laurenza et al., 2009, doi: 10.1029/2007SW000379) + * - 20 + - Frequency + - kHz + - float + - kHz - Used Wind/Waves frequency close to 1 MHz in computing the Radio_Fluence in the previous column + * - 21 + - SEP_onset + - utc + - datetime + - UTC - SEP onset time + * - 22 + - SEP_threshold + - utc + - datetime + - UTC - Time at which the >10 MeV proton flux exceeds the 10 pfu threshold + * - 23 + - SEP_Peak_time + - utc + - datetime + - UTC - Peak proton flux time at >10 MeV energies + * - 24 + - SEP_end + - utc + - datetime + - UTC - Time at the end of the SEP event at >10 MeV energies + * - 25 + - Peak_proton_flux + - pfu + - float + - pfu=1/(cm^2 s sr) - Peak proton flux at >10 MeV energies + * - 26 + - Proton_fluence + - #/(cm^2*sr) + - float + - #/(cm^2 sr) - Time integrated proton flux in the onset-end time interval + * - 27 + - GLE + - char + - char + - Char - YES or NO flag indicating the presence or the absence of a Ground Level Enhancement event, respectively. diff --git a/docs/source/products/data/inaf_s2sep_tableset.rst b/docs/source/products/data/inaf_s2sep_tableset.rst index 3346c00..717b419 100644 --- a/docs/source/products/data/inaf_s2sep_tableset.rst +++ b/docs/source/products/data/inaf_s2sep_tableset.rst @@ -1,53 +1,203 @@ -========================================= -INAF S2 SEP Catalogue -========================================= +============================ +IAPS S2 SEP events Catalogue +============================ .. contents:: The tiny table of contents The catalogue contains SEP events observed at the Earth of class S2, i.e. with flux >100 pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux in the interval [10, 100) pfu at > 10 MeV are listed in the companion table S1 SEP Catalogue. -**Providers**: +**References** -- **GOES** - sources: - - 1-8 Å soft X-ray flux, proton flux - - http://www.ngdc.noaa.gov/stp/satellite/goes/dataaccess.html -- **SOHO/LASCO CME Catalog** - source: - - https://cdaw.gsfc.nasa.gov/CME_list/ -- **Wind** - sources: - - - Waves 1 MHz radio flux - - ftp://solar-radio.gsfc.nasa.gov/ - - -| **Product Type**: lookup-table - -| **Status**: Active - -| **Creation date**: 2022-04-26T12:00:39+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - xlsx - - -| **Sample**: https://docs.google.com/spreadsheets/d/1gCs2nKrZwW9egaU4xGTZXuerfGXkhd0b/edit?usp=sharing&ouid=115498353997648557775&rtpof=true&sd=true - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** inaf_s2sep_tableset + +**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali + +**alphanumeric_code:** 16B + +**id_tmp:** 78 + +**short_name:** IAPS-S2 SEP events + +**identifier:** aspis://inaf/s1sep_tableset + +**dynamic:** static + +**size:** 100kB + +**format:** csv + +**type:** tableset + +**records_number:** 60 + +**time_start:** 1995-01-01 + +**time_stop:** 2014-09-10 + +**spatial:** Earth + +**messenger:** Protons,Photons + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** flare,CME,SEP + +**latest update:** 2024-03-28 05:08:06 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - utc + - datetime + - UTC - Time of the peak of the SEP associated soft X -ray (SXR) flare. When the time coincides with that of the CME no information about the actual time was available. + * - 2 + - SXR_class + - char + - char + - Char - Class of the SEP associated flare according to their peak intensities + * - 3 + - Flare_Latitude + - deg + - float + - Degrees - Averaged heliographic latitude of the SEP associated flare central region from observations of the H-alpha spectral line + * - 4 + - Flare_Longitude + - deg + - float + - Degrees - Averaged heliographic longitude of the SEP associated flare central region from observations of the H-alpha spectral line. The value 91 indicates longitudes >90 the value 121 indicates longitudes >120 the value -91 indicates longitudes<-90. + * - 5 + - CME_NOAA_date + - utc + - datetime + - UTC - Date and time of the associated CME from the NOAA list (https://umbra.nascom.nasa.gov/SEP/) + * - 6 + - CME_SOHO_date + - utc + - datetime + - UTC - In case the CME NOAA Date was not present or not considered reliable in the previous column, the date and time of the associated CME from the SOHO list (https://cdaw.gsfc.nasa.gov/CME_list/UNIVERSAL_ver1/1998_05/univ1998_05.html) is given in this c + * - 7 + - CME_central_PA + - deg + - float + - Degrees - CME position angle measured from Solar North in degrees (counter-clockwise). The value 360 indicates a halo CME. + * - 8 + - Halo_CME_type + - char + - char + - Char - Halo CMEs are indicated in the 'CME_Central_PA' column with 360. In this column the letters ('S', 'BA', 'OA') in the brackets show type of halo CMEs. Halo CMEs can be symmetric (S) or asymmetric with respect to the occulting disk. Brightness asymme + * - 9 + - CME_angular_width + - deg + - float + - Degrees - Angular width of the CME. For values =-361 more information are available in the sOHO LASCO CME catalogue (https://cdaw.gsfc.nasa.gov/CME_list/). + * - 10 + - CME_Speed_Art1 + - km/s + - float + - km/s - CME speed from catalogue of article 1 (Art1) Papaioannou et a. 2016 (doi: 10.1051/swsc/2016035) + * - 11 + - Radio_burst_type_II + - char + - int + - Int - Occurrence of type II radio burst: the value 1 indicates that the burst occurred the value 2 indicates that the burst occurred with a probability >50% the value 3 indicates that the burst occurred with a probability <50 the value 0 indicates that th + * - 12 + - Radio_burst_type_IV + - char + - int + - Int - Occurrence of type IV radio burst: the value 1 indicates that the burst occurred the value 2 indicates that the burst occurred with a probability >50% the value 3 indicates that the burst occurred with a probability <50 the value 0 indicates that th + * - 13 + - CME_Speed_Art2 + - km/s + - float + - km/s - CME speed from catalogue of article2 (ART2) Gopalswamy et al. 2015 (doi: 10.48550/arXiv.1509.04216) + * - 14 + - SOHO_CME_linear_speed + - km/s + - float + - km/s - Speed from SOHO catalogue obtained through linear fit of height-time measurements + * - 15 + - SOHO_CME_speed_2nd + - km/s + - float + - km/s - Speed from SOHO catalogue obtained through quadratic fit of height-time measurements. The speed is evaluated at the time of final height measurement + * - 16 + - SOHO_CME_speed_20_Rs + - km/s + - float + - km/s - Speed from SOHO catalogue obtained through quadratic fit of height-time measurements. The speed is evaluated when the CME is at a height of 20 solar radii + * - 17 + - CME_acceleration + - km/s^2 + - float + - km/s^2 - Acceleration of the CME + * - 18 + - SXR_Fluence + - J/m^2 + - float + - J m^2 - Time integrated SXR intensity between the 1/3 power points on rise and fall (see Laurenza et al., 2009, doi: 10.1029/2007SW000379) + * - 19 + - Radio_Fluence + - sfu*min + - float + - sfu*min - Time integrated 1 MHz intensity from Wind/Waves from 10 minutes before the onset of integration for the SXR burst to 10 minutes after the SXR burst peak (see Laurenza et al., 2009, doi: 10.1029/2007SW000379) + * - 20 + - Frequency + - kHz + - float + - kHz - Used Wind/Waves frequency close to 1 MHz in computing the Radio_Fluence in the previous column + * - 21 + - SEP_onset + - utc + - datetime + - UTC - SEP onset time + * - 22 + - SEP_threshold + - utc + - datetime + - UTC - Time at which the >10 MeV proton flux exceeds the 10 pfu threshold + * - 23 + - SEP_Peak_time + - utc + - datetime + - UTC - Peak proton flux time at >10 MeV energies + * - 24 + - SEP_end + - utc + - datetime + - UTC - Time at the end of the SEP event at >10 MeV energies + * - 25 + - Peak_proton_flux + - pfu + - float + - pfu=1/(cm^2 s sr) - Peak proton flux at >10 MeV energies + * - 26 + - Proton_fluence + - #/(cm^2*sr) + - float + - #/(cm^2 sr) - Time integrated proton flux in the onset-end time interval + * - 27 + - GLE + - char + - char + - Char - YES or NO flag indicating the presence or the absence of a Ground Level Enhancement event, respectively. diff --git a/docs/source/products/data/inaf_swflux_merc_tableset.rst b/docs/source/products/data/inaf_swflux_merc_tableset.rst deleted file mode 100644 index d2d0b9d..0000000 --- a/docs/source/products/data/inaf_swflux_merc_tableset.rst +++ /dev/null @@ -1,45 +0,0 @@ -======================================================== -INAF Simulated Maps of SW Flux at the Surface of Mercury -======================================================== - -.. contents:: The tiny table of contents - -Simulated flux maps of SW precipitating onto the surface of Mercury for a subset of IMF condition, with surface resolution of 1° (LAT/LON) and IMF binning of 5 nT (from -20 to 20 nT) - -**Providers**: - -Missing providers - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-05-04T16:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - PNG - - -| **Sample**: Simulated_SW_Flux - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- 2320.2 meta data mapping: meta data mapping (MANCA NELLA TENDINA) -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- ext 2330.1 MANCA DALLA LISTA A TENDINA: MANCA DALLA LISTA A TENDINA??? - diff --git a/docs/source/products/data/inaf_tps_datacube.rst b/docs/source/products/data/inaf_tps_datacube.rst index 3080e9a..8e6184b 100644 --- a/docs/source/products/data/inaf_tps_datacube.rst +++ b/docs/source/products/data/inaf_tps_datacube.rst @@ -1,48 +1,88 @@ ================================================ -INAF Test Particle Simulation on Magnetic Clouds +IAPS Test Particle Simulation on Magnetic Clouds ================================================ .. contents:: The tiny table of contents Galactic cosmic ray intensity variations associated to the passage of magnetic clouds. The particle intensity variation is estimated through a dedicated full-orbit test-particle simulation. -**Providers**: +**References** -- **Solar Modulation Parameter Table Oulu NM** - source: - - https://cosmicrays.oulu.fi/phi/phi.html -- **Grad-Shafranov reconstruction maps** - source: - - in ASPIS +Data description +~~~~~~~~~~~~~~~~ +**internal_name:** inaf_tps_datacube -| **Product Type**: data +**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali -| **Status**: Active +**alphanumeric_code:** 51 -| **Creation date**: 2022-04-26T12:00:39+02:00 +**id_tmp:** 97 -| **Last Update**: 2023-10-01T12:00:00+02:00 +**short_name:** IAPS-TPS -Data Description -~~~~~~~~~~~~~~~~ +**identifier:** aspis://inaf/tps_datacube + +**dynamic:** static + +**size:** 300kB + +**format:** nc + +**type:** spectrum + +**records_number:** 3 + +**time_start:** 1997-01-01 + +**time_stop:** 2022-01-01 + +**spatial:** Interplanetary Space (not L1 and Planets),Sun-Earth L1 + +**messenger:** Particle intensity variation + +**spectral_min:** -| **Data type**: spectral-cubes +**spectral_max:** -| **Data formats**: - mat +**spectral_units:** +**observable:** phys.flux,phys.particle.proton -| **Sample**: https://drive.google.com/file/d/1DueJgqzWtUO3-ptb1AmgaotZuIaPYEzY/view?usp=sharing +**latest update:** 2024-03-28 05:08:06 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - datetime - Time associated with the simulation + * - 2 + - data_name + - char + - string + - the name of the file with the data + * - 3 + - prew_name + - char + - string + - the name of the full preview file + * - 4 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/inaf_vbcorr_psp_tableset.rst b/docs/source/products/data/inaf_vbcorr_psp_tableset.rst deleted file mode 100644 index c64a4f9..0000000 --- a/docs/source/products/data/inaf_vbcorr_psp_tableset.rst +++ /dev/null @@ -1,47 +0,0 @@ -=================================================================================== -INAF PSP velocity-magnetic field correlation coefficient data of solar wind streams -=================================================================================== - -.. contents:: The tiny table of contents - -The velocity - magnetic field (v-b) correlation coefficient unables to identify Alfvénic solar wind intervals (along with almost constant magnetic field magnitude and proton number density). It is derived as the ratio between the covariance of velocity and magnetic field (in Alfvén units) components and the product of their standard deviations, in a time window ranging between tens of minutes to hours. In principle, this formula should be applied to every component of the velocity (V_i) and magnetic fields (B_i) (with i = R, T, N in RTN coordinate system or i = X, Y, Z in GSE coordinate system). The total correlation coefficient is then derived as the average from the three components. However, for the sake of simplicity, we consider only the N component since more Alfvénic than the other two. - -**Providers**: - -- **Parker Solar Probe** - sources: - - - Solar Wind Electrons Alphas and Protons investigation (SWEAP) - - FIELDS - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-05-06T10:39:35+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: timeseries - -| **Data formats**: - ascii - - -| **Sample**: https://drive.google.com/file/d/1C7lxF193kgoyLwgAU_3UzE29kWigLTQ9/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- int2320.2: metadata mapping -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/inaf_vbcorr_solo_tableset.rst b/docs/source/products/data/inaf_vbcorr_solo_tableset.rst deleted file mode 100644 index e4ca620..0000000 --- a/docs/source/products/data/inaf_vbcorr_solo_tableset.rst +++ /dev/null @@ -1,47 +0,0 @@ -==================================================================================== -INAF SolO velocity-magnetic field correlation coefficient data of solar wind streams -==================================================================================== - -.. contents:: The tiny table of contents - -The velocity - magnetic field (v-b) correlation coefficient unables to identify Alfvénic solar wind intervals (along with almost constant magnetic field magnitude and proton number density). It is derived as the ratio between the covariance of velocity and magnetic field (in Alfvén units) components and the product of their standard deviations, in a time window ranging between tens of minutes to hours. In principle, this formula should be applied to every component of the velocity (V_i) and magnetic fields (B_i) (with i = R, T, N in RTN coordinate system or i = X, Y, Z in GSE coordinate system). The total correlation coefficient is then derived as the average from the three components. However, for the sake of simplicity, we consider only the N component since more Alfvénic than the other two. - -**Providers**: - -- **Solar Orbiter** - sources: - - - Solar Wind Analyzer - Proton and Alpha Sensor (SWA-PAS) - - Magnetometer (MAG) - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-29T18:38:35+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: timeseries - -| **Data formats**: - ascii - - -| **Sample**: https://drive.google.com/file/d/1C7lxF193kgoyLwgAU_3UzE29kWigLTQ9/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- int2320.2: metadata mapping -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/inaf_vbcorr_wind_tableset.rst b/docs/source/products/data/inaf_vbcorr_wind_tableset.rst index 267f837..ad9a0c6 100644 --- a/docs/source/products/data/inaf_vbcorr_wind_tableset.rst +++ b/docs/source/products/data/inaf_vbcorr_wind_tableset.rst @@ -1,47 +1,94 @@ -==================================================================================== -INAF Wind velocity-magnetic field correlation coefficient data of solar wind streams -==================================================================================== +====================================================================================== +IAPS - Wind velocity-magnetic field correlation coefficient data of solar wind streams +====================================================================================== .. contents:: The tiny table of contents The velocity - magnetic field (v-b) correlation coefficient unables to identify Alfvénic solar wind intervals (along with almost constant magnetic field magnitude and proton number density). It is derived as the ratio between the covariance of velocity and magnetic field (in Alfvén units) components and the product of their standard deviations, in a time window ranging between tens of minutes to hours. In principle, this formula should be applied to every component of the velocity (V_i) and magnetic fields (B_i) (with i = R, T, N in RTN coordinate system or i = X, Y, Z in GSE coordinate system). The total correlation coefficient is then derived as the average from the three components. However, for the sake of simplicity, we consider only the N component since more Alfvénic than the other two. -**Providers**: +**References** -- **WIND** - sources: +D’Amicis et al, GRL, 34, L05108, 2007; Frontiers in Physics, 8, 541, 2020 + +Telloni et al, ApJ, 916, 64, 2021 + +D’Amicis et al, A&A, 656, A21, 2021 + +Tu et al., JGR, 94, 11739, 1989 - - 3-D Plasma and Energetic Particle Investigation (3DP) - - Magnetic Field Instrument (MFI) +Data description +~~~~~~~~~~~~~~~~ +**internal_name:** inaf_vbcorr_wind_tableset -| **Product Type**: data +**publisher:** INAF-IAPS, Fisica dei Plasmi Spaziali e Space Weather -| **Status**: Active +**alphanumeric_code:** 24C -| **Creation date**: 2022-05-06T10:39:35+02:00 +**id_tmp:** 98 -| **Last Update**: 2023-10-01T12:00:00+02:00 +**short_name:** wind_v-b_corr -Data Description -~~~~~~~~~~~~~~~~ +**identifier:** aspis://inaf/vbcorr_wind_tableset + +**dynamic:** static + +**size:** 35MB + +**format:** csv + +**type:** tableset + +**records_number:** 538 + +**time_start:** 1998-10-01 + +**time_stop:** 2022-05-06 + +**spatial:** L1 + +**messenger:** protons + +**spectral_min:** 0 -| **Data type**: timeseries +**spectral_max:** 0 -| **Data formats**: - ascii +**spectral_units:** - +**observable:** SW -| **Sample**: https://drive.google.com/file/d/1C7lxF193kgoyLwgAU_3UzE29kWigLTQ9/view?usp=sharing +**latest update:** 2024-04-04 02:05:02 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- int2320.2: metadata mapping -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - 2017-03-25T00:00:06 [UTC] - the UTC time associated to the masure + * - 2 + - vb_coeff_corr + - number + - float + - -0.98 [dimensionless] the Pearson's correlation coefficient between the normal components of velocity and magnetic field + * - 3 + - sample + - number + - int + - 75 [samples] the number of observations available in the 30-min window + * - 4 + - scale + - min + - int + - 30 [minutes] the length of the window, i.e. 30 min diff --git a/docs/source/products/data/inaf_walen_cluster_tableset.rst b/docs/source/products/data/inaf_walen_cluster_tableset.rst deleted file mode 100644 index bab6560..0000000 --- a/docs/source/products/data/inaf_walen_cluster_tableset.rst +++ /dev/null @@ -1,49 +0,0 @@ -========================================= -INAF Reconnection test results (CLUSTER) -========================================= - -.. contents:: The tiny table of contents - -The Walén test quality index is derived from the density, velocity and magnetic field measurements provided by the CLUSTER mission during magnetopause crossings - -**Providers**: - -- **CIS and FGM data provided by the CLUSTER mission** - sources: - - - https://cdaweb.gsfc.nasa.gov/ - - CIS Principal Investigator: I. Dandouras (IRAP) - - FGM Principal Invastigator: E. Lucek, (IC) - - -| **Product Type**: lookup-table - -| **Status**: Active - -| **Creation date**: 2022-04-29T18:30:57+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - ASCII - - -| **Sample**: Walén_test_CLUSTER - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- 2320.2 meta data mapping: meta data mapping (MANCA NELLA TENDINA) -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- ext 2330.1 MANCA DALLA LISTA A TENDINA: MANCA DALLA LISTA A TENDINA??? - diff --git a/docs/source/products/data/inaf_walen_mms_tableset.rst b/docs/source/products/data/inaf_walen_mms_tableset.rst deleted file mode 100644 index 1bf9ec8..0000000 --- a/docs/source/products/data/inaf_walen_mms_tableset.rst +++ /dev/null @@ -1,47 +0,0 @@ -========================================= -INAF Reconnection test results (MMS) -========================================= - -.. contents:: The tiny table of contents - -The Walén test quality index is derived from the density, velocity and magnetic field measurements provided by the Magnetospheric Multiscale Mission (MMS) mission during magnetopause crossings - -**Providers**: - -- **FPI/DIS and FGM data provided by the MMS mission** - sources: - - - https://cdaweb.gsfc.nasa.gov/ - - Fast Plasma Investigation (FPI) Lead Co-I, Phase E: Dr. Daniel Gershman, NASA GSFC, (from 2020) - - Flux Gate Magnetometer Lead Co-I: Prof. C. T. Russell, UCLA - - -| **Product Type**: lookup-table - -| **Status**: Active - -| **Creation date**: 2022-04-29T18:30:57+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - ASCII - - -| **Sample**: Walén_test_MMS - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/inaf_walen_themis_tableset.rst b/docs/source/products/data/inaf_walen_themis_tableset.rst deleted file mode 100644 index 7adac18..0000000 --- a/docs/source/products/data/inaf_walen_themis_tableset.rst +++ /dev/null @@ -1,49 +0,0 @@ -========================================= -INAF Reconnection test results (THEMIS) -========================================= - -.. contents:: The tiny table of contents - -The Walén test quality index is derived from the density, velocity and magnetic field measurements provided by the Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission during magnetopause crossings - -**Providers**: - -- **ESA and FGM data provided by the THEMIS mission** - sources: - - - https://cdaweb.gsfc.nasa.gov/ - - ESA Principal Investigator: C. W. Carlson (UCB) - - FGM Principal Invastigator: K. H. Glassmeier, TU-BS - - -| **Product Type**: lookup-table - -| **Status**: Active - -| **Creation date**: 2022-04-29T18:30:57+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - ASCII - - -| **Sample**: Walén_test_THEMIS - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- 2320.2 meta data mapping: meta data mapping (MANCA NELLA TENDINA) -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- ext 2330.1 MANCA DALLA LISTA A TENDINA: MANCA DALLA LISTA A TENDINA??? - diff --git a/docs/source/products/data/infn_saandose_samadha_timeseries.rst b/docs/source/products/data/infn_saandose_samadha_timeseries.rst index 806906d..b46635f 100644 --- a/docs/source/products/data/infn_saandose_samadha_timeseries.rst +++ b/docs/source/products/data/infn_saandose_samadha_timeseries.rst @@ -1,38 +1,83 @@ -================================================== -INFN SAMADHA neutron dose rate at Mount Chacaltaya -================================================== +============================================= +SAMADHA neutron dose rate at Mount Chacaltaya +============================================= .. contents:: The tiny table of contents SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) is an INFN project aimed to monitor the neutron dose rate due to cosmic rays at the Chacaltaya Station (Bolivia, 5200 m) inside the South Atlantic Anomaly region, to study possible correlation between space weather events and dose rate at the ground, considering the proximity of the Van Allen Belts to the Earth's surface in the SAA region. -**Providers**: +**References** -- **SAMADHA project** - source: +http://samadha.to.infn.it - - neutron dosimeter (rem counter) +Data description +~~~~~~~~~~~~~~~~ +**internal_name:** infn_saandose_samadha_timeseries -| **Product Type**: data +**publisher:** SAMADHA -| **Status**: Inactive +**alphanumeric_code:** 75A -| **Creation date**: 2022-04-29T16:11:31+02:00 +**id_tmp:** 99 -| **Last Update**: 2023-10-01T12:00:00+02:00 +**short_name:** SAA_Ndose -Data Description -~~~~~~~~~~~~~~~~ +**identifier:** aspis://infn/saandose_samadha_timeseries + +**dynamic:** one dataset per day (50 kB/day) + +**size:** 50kB + +**format:** text + +**type:** tableset + +**records_number:** 2358 + +**time_start:** 2022-10-01 + +**time_stop:** 2023-12-31 + +**spatial:** Earth's Ground + +**messenger:** neutrons + +**spectral_min:** 0 -| **Data type**: tableset +**spectral_max:** 0 -| **Data formats**: - text +**spectral_units:** 0 +**observable:** -| **Sample**: ND +**latest update:** 2024-04-04 02:14:12 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -ND +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime of the measurement + * - 2 + - dose_rate + - nSv/h + - float + - neutron ambient dose rate equivalent H*(10) average over 4 hours (nSv/h) + * - 3 + - dose_rate_error + - nSv/h + - float + - neutron dose rate measure error (nSv/h) diff --git a/docs/source/products/data/infn_tgndose_samadha_timeseries.rst b/docs/source/products/data/infn_tgndose_samadha_timeseries.rst index e5c5bd3..674c0e3 100644 --- a/docs/source/products/data/infn_tgndose_samadha_timeseries.rst +++ b/docs/source/products/data/infn_tgndose_samadha_timeseries.rst @@ -1,37 +1,83 @@ -============================================== -INFN SAMADHA neutron dose rate at Testa Grigia -============================================== +========================================= +SAMADHA neutron dose rate at Testa Grigia +========================================= .. contents:: The tiny table of contents Monitoring of the neutron dose rate due to cosmic rays at the Testa Grigia Station (3480 m, Cervinia, Italy), to study possible correlation between space weather events and dose rate at the ground. This measurement is part of the INFN project SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) aimed to monitor the neutron dose inside the South Atlantic Anomaly (SAA) region in Bolivia. The data taken at Testa Grigia are a term of comparison for those collected in the SAA region. -**Providers**: +**References** -- **SAMADHA** - source: +http://samadha.to.infn.it - - neutron detector (rem counter) +Data description +~~~~~~~~~~~~~~~~ +**internal_name:** infn_tgndose_samadha_timeseries -| **Product Type**: data +**publisher:** samadha -| **Status**: Active +**alphanumeric_code:** 75B -| **Creation date**: 2022-04-29T16:11:31+02:00 +**id_tmp:** 79 -| **Last Update**: 2023-10-01T12:00:00+02:00 +**short_name:** TG_Ndose -Data Description -~~~~~~~~~~~~~~~~ +**identifier:** aspis://infn/tgndose_samadha_timeseries + +**dynamic:** one dataset per day (50 kB/day) + +**size:** 50kB + +**format:** text + +**type:** timeseries + +**records_number:** 2835 + +**time_start:** 2021-09-01 + +**time_stop:** 2023-12-31 + +**spatial:** Earth's Ground + +**messenger:** neutrons + +**spectral_min:** 0 + +**spectral_max:** 0 -| **Data type**: tableset +**spectral_units:** 0 -| **Data formats**: - text +**observable:** +**latest update:** 2024-04-04 02:15:39 -| **Sample**: ND +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -Capabilities -~~~~~~~~~~~~ +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 -ND + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime of the measurement + * - 2 + - dose_rate + - nSv/h + - float + - neutron ambient dose rate equivalent H*(10) average over 4 hours (nSv/h) + * - 3 + - dose_rate_error + - nSv/h + - float + - neutron dose rate measure error (nSv/h) diff --git a/docs/source/products/data/ingv_alert_aqu_timeseries.rst b/docs/source/products/data/ingv_alert_aqu_timeseries.rst index 34d644b..47abb7a 100644 --- a/docs/source/products/data/ingv_alert_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_alert_aqu_timeseries.rst @@ -1,51 +1,131 @@ -========================================= -INGV L'Aquila GIC level alert -========================================= +====================================================== +INGV geomagnetic data, GIC indices and alert: L'Aquila +====================================================== .. contents:: The tiny table of contents -From both components of GIC index for L'Aquila observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) +From both components of GIC index for L'Aquila observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) + +This tableset contains a set of data corresponding to products with ids 8, 47 and 48. In detail it contains the definitive values of the X,Y and Z components (in NEC coordinates) and of total intensity F of the geomagnetic field recorded at ground magnetic observatories managed by INGV. Besides, it contains the values of the GicX and GicY indices calculated from the Y and X components, respectively. To finish it contains values of the risk (i.e. alertX and alertY) , corresponding to the estimated values of the GicX and GicY indices. +Data sampling is of 1-minute. -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- int2130.4: Scheduled computation -- ext2230.4: Computation: ASPIS.py - +**internal_name:** ingv_alert_aqu_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 48A + +**id_tmp:** 80 + +**short_name:** INGV_AQU_alert + +**identifier:** aspis:///ingv/INGV_AQU_alert + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-04-04 02:27:54 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_alert_cts_timeseries.rst b/docs/source/products/data/ingv_alert_cts_timeseries.rst index 12f6c1c..9c7018c 100644 --- a/docs/source/products/data/ingv_alert_cts_timeseries.rst +++ b/docs/source/products/data/ingv_alert_cts_timeseries.rst @@ -1,51 +1,128 @@ -==================================== -INGV Castello Tesino GIC level alert -==================================== +============================================================= +INGV geomagnetic data, GIC indices and alert: Castello Tesino +============================================================= .. contents:: The tiny table of contents From both components of GIC index for Castello Tesino observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- int2130.4: Scheduled computation -- ext2230.4: Computation: ASPIS.py - +**internal_name:** ingv_alert_cts_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 48B + +**id_tmp:** 81 + +**short_name:** INGV_CTS_alert + +**identifier:** aspis:///ingv/INGV_CTS_alert + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:07 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_alert_dur_timeseries.rst b/docs/source/products/data/ingv_alert_dur_timeseries.rst index 1428320..76388d4 100644 --- a/docs/source/products/data/ingv_alert_dur_timeseries.rst +++ b/docs/source/products/data/ingv_alert_dur_timeseries.rst @@ -1,51 +1,128 @@ -============================ -INGV Duronia GIC level alert -============================ +===================================================== +INGV geomagnetic data, GIC indices and alert: Duronia +===================================================== .. contents:: The tiny table of contents From both components of GIC index for Duronia observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- int2130.4: Scheduled computation -- ext2230.4: Computation: ASPIS.py - +**internal_name:** ingv_alert_dur_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 48C + +**id_tmp:** 82 + +**short_name:** INGV_DUR_alert + +**identifier:** aspis:///ingv/INGV_DUR_alert + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:07 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_alert_lmp_timeseries.rst b/docs/source/products/data/ingv_alert_lmp_timeseries.rst index b1848ad..a13abd8 100644 --- a/docs/source/products/data/ingv_alert_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_alert_lmp_timeseries.rst @@ -1,51 +1,128 @@ -========================================= -INGV Lampedusa GIC level alert -========================================= +======================================================= +INGV geomagnetic data, GIC indices and alert: Lampedusa +======================================================= .. contents:: The tiny table of contents From both components of GIC index for Lampedusa observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- int2130.4: Scheduled computation -- ext2230.4: Computation: ASPIS.py - +**internal_name:** ingv_alert_lmp_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 48D + +**id_tmp:** 83 + +**short_name:** INGV_LMP_alert + +**identifier:** aspis:///ingv/INGV_LMP_alert + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:08 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst b/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst index 2f767c0..80a2ba5 100644 --- a/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst @@ -1,48 +1,113 @@ -=========================================== -INGV Autoscaled data Bahia Blanca Ionosonde -=========================================== +====================================== +Autoscaled data Bahia Blanca Ionosonde +====================================== .. contents:: The tiny table of contents Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Bahia Blanca -**Providers**: +**References** -- **AIS-INGV ionosonde** +http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-20T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1UcgQyPUV0iRVqQH1HeZU_JCtGnLPFEXC/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- http://ws-eswua.rm.ingv.it/ais.\php/records/bbj3r_auto: Web service endpoint - +**internal_name:** ingv_autoiono_bbla_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 12A + +**id_tmp:** 1 + +**short_name:** AutoIonoBBla + +**identifier:** aspis://ingv/autoiono_bbla_timeseries + +**dynamic:** The Data bulk size refers to one year of data. The Bahia Blanca AIS-INGV ionosonde started sounding in September 2016, this is why in the Number of datasets field you will find the number 7 (years 2016-2022). This collection grows in real time, because th + +**size:** 15MB + +**format:** csv + +**type:** timeseries + +**records_number:** 1558 + +**time_start:** 2016-09-26 + +**time_stop:** 2022-04-14 + +**spatial:** IONO + +**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** + +**latest update:** 2024-04-04 05:53:16 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of the sounding + * - 2 + - geo_lat + - deg + - float + - latitude + * - 3 + - geo_lon + - deg + - float + - longitude + * - 4 + - fof2 + - MHz + - float + - (MHz) maximum frequency reflected by the F2 layer + * - 5 + - muf3000f2 + - MHz + - float + - (MHz) maximum usable frequency for a distance of 3000 km centered over the ionosonde site + * - 6 + - m3000f2 + - dimensionless + - float + - (adimensional) propagation factor + * - 7 + - fof1 + - MHz + - float + - (MHz) maximum frequency reflected by the F1 layer + * - 8 + - ftes + - MHz + - float + - (MHz) maximum frequency reflected by the sporadic E layer + * - 9 + - h_es + - km + - integer + - (km) virtual height of the sporadic E layer diff --git a/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst b/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst index 7b5cdf3..59b1916 100644 --- a/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst @@ -1,48 +1,113 @@ -========================================= -INGV Autoscaled data Gibilmanna Ionosonde -========================================= +==================================== +Autoscaled data Gibilmanna Ionosonde +==================================== .. contents:: The tiny table of contents Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna -**Providers**: +**References** -- **AIS-INGV ionosonde** +http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-19T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1C4xMpwbbQMeRjtlVbCHnMRFN1p20xWOA/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- http://ws-eswua.rm.ingv.it/ais.\php/records/gm037_auto: Web service endpoint - +**internal_name:** ingv_autoiono_gibi_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 12B + +**id_tmp:** 2 + +**short_name:** AutoIonoGibi + +**identifier:** aspis://ingv/autoiono_gibi_timeseries + +**dynamic:** The Data bulk size refers to one year of data. The Gibilmanna AIS-INGV ionosonde started sounding in November 2002, this is why in the Number of datasets field you will find the number 21 (years 2002-2022). This collection grows in real time, because the + +**size:** 15MB + +**format:** csv + +**type:** timeseries + +**records_number:** 5793 + +**time_start:** 2002-11-26 + +**time_stop:** 2022-04-14 + +**spatial:** IONO + +**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** + +**latest update:** 2024-04-04 05:55:21 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of the sounding + * - 2 + - geo_lat + - deg + - float + - latitude + * - 3 + - geo_lon + - deg + - float + - longitude + * - 4 + - fof2 + - MHz + - float + - (MHz) maximum frequency reflected by the F2 layer + * - 5 + - muf3000f2 + - MHz + - float + - (MHz) maximum usable frequency for a distance of 3000 km centered over the ionosonde site + * - 6 + - m3000f2 + - dimensionless + - float + - (adimensional) propagation factor + * - 7 + - fof1 + - MHz + - float + - (MHz) maximum frequency reflected by the F1 layer + * - 8 + - ftes + - MHz + - float + - (MHz) maximum frequency reflected by the sporadic E layer + * - 9 + - h_es + - km + - integer + - (km) virtual height of the sporadic E layer diff --git a/docs/source/products/data/ingv_autoiono_rome_timeseries.rst b/docs/source/products/data/ingv_autoiono_rome_timeseries.rst index 687e4d1..e31ce5a 100644 --- a/docs/source/products/data/ingv_autoiono_rome_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_rome_timeseries.rst @@ -1,48 +1,113 @@ -========================================= -INGV Autoscaled data Rome Ionosonde -========================================= +============================== +Autoscaled data Rome Ionosonde +============================== .. contents:: The tiny table of contents Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Rome -**Providers**: +**References** -- **AIS-INGV ionosonde** +http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1xbQN9F_L_R3x_gXI3YBkwlv_ZVaNDPTV/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- http://ws-eswua.rm.ingv.it/ais.\php/records/rm041_auto: Web service endpoint - +**internal_name:** ingv_autoiono_rome_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 12C + +**id_tmp:** 3 + +**short_name:** AutoIonoRome + +**identifier:** aspis://ingv/autoiono_rome_timeseries + +**dynamic:** The Data bulk size refers to one year of data. The Rome AIS-INGV ionosonde started sounding in November 2004, this is why in the Number of datasets field you will find the number 19 (years 2004-2022). This collection grows in real time, because the ionoso + +**size:** 15MB + +**format:** csv + +**type:** timeseries + +**records_number:** 7303 + +**time_start:** 2004-11-25 + +**time_stop:** 2022-04-14 + +**spatial:** IONO + +**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** + +**latest update:** 2024-04-04 05:56:30 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of the sounding + * - 2 + - geo_lat + - deg + - float + - latitude + * - 3 + - geo_lon + - deg + - float + - longitude + * - 4 + - fof2 + - MHz + - float + - (MHz) maximum frequency reflected by the F2 layer + * - 5 + - muf3000f2 + - MHz + - float + - (MHz) maximum usable frequency for a distance of 3000 km centered over the ionosonde site + * - 6 + - m3000f2 + - dimensionless + - float + - (adimensional) propagation factor + * - 7 + - fof1 + - MHz + - float + - (MHz) maximum frequency reflected by the F1 layer + * - 8 + - ftes + - MHz + - float + - (MHz) maximum frequency reflected by the sporadic E layer + * - 9 + - h_es + - km + - integer + - (km) virtual height of the sporadic E layer diff --git a/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst b/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst index c09ff80..bf95bc7 100644 --- a/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst @@ -1,48 +1,113 @@ -====================================== -INGV Autoscaled data Tucuman Ionosonde -====================================== +================================= +Autoscaled data Tucuman Ionosonde +================================= .. contents:: The tiny table of contents Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Tucuman -**Providers**: +**References** -- **AIS-INGV ionosonde** +http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-20T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1IWVF_Oo4Np7n8tuPXXxjc_991gdu1Ga2/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- http://ws-eswua.rm.ingv.it/ais.\php/records/tuj2O_auto: Web service endpoint - +**internal_name:** ingv_autoiono_tucu_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 12D + +**id_tmp:** 4 + +**short_name:** AutoIonoTucu + +**identifier:** aspis://ingv/autoiono_tucu_timeseries + +**dynamic:** The Data bulk size refers to one year of data. The Tucuman AIS-INGV ionosonde started sounding in August 2007, this is why in the Number of datasets field you will find the number 16 (years 2007-2022). This collection grows in real time, because the ionos + +**size:** 15MB + +**format:** csv + +**type:** timeseries + +**records_number:** 6283 + +**time_start:** 2007-08-04 + +**time_stop:** 2022-04-14 + +**spatial:** IONO + +**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** + +**latest update:** 2024-04-04 05:57:34 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of the sounding + * - 2 + - geo_lat + - deg + - float + - latitude + * - 3 + - geo_lon + - deg + - float + - longitude + * - 4 + - fof2 + - MHz + - float + - (MHz) maximum frequency reflected by the F2 layer + * - 5 + - muf3000f2 + - MHz + - float + - (MHz) maximum usable frequency for a distance of 3000 km centered over the ionosonde site + * - 6 + - m3000f2 + - dimensionless + - float + - (adimensional) propagation factor + * - 7 + - fof1 + - MHz + - float + - (MHz) maximum frequency reflected by the F1 layer + * - 8 + - ftes + - MHz + - float + - (MHz) maximum frequency reflected by the sporadic E layer + * - 9 + - h_es + - km + - integer + - (km) virtual height of the sporadic E layer diff --git a/docs/source/products/data/ingv_b_swarm_image.rst b/docs/source/products/data/ingv_b_swarm_image.rst index dd738ce..c01e835 100644 --- a/docs/source/products/data/ingv_b_swarm_image.rst +++ b/docs/source/products/data/ingv_b_swarm_image.rst @@ -1,39 +1,103 @@ -========================================= -INGV Swarm vector magnetic field maps -========================================= +================================ +Swarm vector magnetic field maps +================================ .. contents:: The tiny table of contents Vector magnetic field maps in quasi-dipole latitude vs magnetic local time coordinates derived from the Swarm constellation data acquired at 1 second cadence from 1 January 2014 to 31 December 2020. The output consists in nine .jpg or .png files mapping the three components of the vector magnetic field in polar and equatorial projections (3 images for the three components) for each of the 3 satellites of the Swarm constellation. Each map has a size of about 300 kB. -**Providers**: +**References** -- **ESA's Swarm constellation** - source: - - Vector Field Magnetometer +Data description +~~~~~~~~~~~~~~~~ -| **Product Type**: data +**internal_name:** ingv_b_swarm_image -| **Status**: Active +**publisher:** INGV group -| **Creation date**: 2022-04-13T16:16:20+02:00 +**alphanumeric_code:** 35B -| **Last Update**: 2023-10-01T12:00:00+02:00 +**id_tmp:** 62 -Data Description -~~~~~~~~~~~~~~~~ +**short_name:** Swarm_B_maps + +**identifier:** aspis://ingv/b_swarm_image + +**dynamic:** static + +**size:** 300kB + +**format:** FITS + +**type:** image + +**records_number:** 24 + +**time_start:** 2014-01-01 + +**time_stop:** 2020-12-31 + +**spatial:** Earth's Ionosphere + +**messenger:** + +**spectral_min:** 0 -| **Data type**: image +**spectral_max:** 0 -| **Data formats**: - .jpg/.png +**spectral_units:** +**observable:** phys.magField -| **Sample**: https://drive.google.com/file/d/1hyNQW6Gk_AaqXG3KGbKtRZ7c1KCAjTZu/view?usp=sharing +**latest update:** 2024-03-28 05:08:09 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time + * - 2 + - time_start + - UTC + - datetime + - acquisition start + * - 3 + - time_end + - UTC + - datetime + - acquisition end + * - 4 + - swarm + - char + - char + - Swarm spacecraft (A, B, C) + * - 5 + - data_name + - char + - char + - image file Fits + * - 6 + - prew_name + - char + - char + - preview file + * - 7 + - thumb_name + - char + - char + - thumbnail file diff --git a/docs/source/products/data/ingv_b_swarm_timeseries.rst b/docs/source/products/data/ingv_b_swarm_timeseries.rst index d21f090..a50603e 100644 --- a/docs/source/products/data/ingv_b_swarm_timeseries.rst +++ b/docs/source/products/data/ingv_b_swarm_timeseries.rst @@ -1,41 +1,143 @@ -=========================================================== -INGV 1 Hz Swarm on track values of vector geomagnetic field -=========================================================== +======================================================================================= +1 Hz Swarm on track values of observed, external and projected vector geomagnetic field +======================================================================================= .. contents:: The tiny table of contents In situ time series of vector geomagnetic field derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of one has a size of about 14.5 GB. The sample file attached is extracted from one month of data acquired by Swarm A -**Providers**: +**References** -- **ESA's Swarm constellation** - source: - - Vector Field Magnetometer - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - text file - - -| **Sample**: https://drive.google.com/file/d/1OYqsJFyLOpuHCv7C90iN1YiX7K5wDerE/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_b_swarm_timeseries + +**publisher:** INGV group + +**alphanumeric_code:** 35A + +**id_tmp:** 52 + +**short_name:** Swarm_B_tseries + +**identifier:** aspis://ingv/b_swarm_timeseries + +**dynamic:** static + +**size:** 20GB + +**format:** text file + +**type:** tableset + +**records_number:** 2634060 + +**time_start:** 2014-01-01 + +**time_stop:** 2022-12-31 + +**spatial:** Earth's Ionosphere + +**messenger:** + +**spectral_min:** 0 + +**spectral_max:** 0 + +**spectral_units:** + +**observable:** phys.magField + +**latest update:** 2024-03-28 05:08:09 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime in ISO format + * - 2 + - geo_lat + - deg + - float + - geographic latitude (deg) + * - 3 + - geo_lon + - deg + - float + - geographic longitude (deg) + * - 4 + - qd_lat + - deg + - float + - quasi-dipole latitude (deg) + * - 5 + - qd_lon + - deg + - float + - quasi-dipole longitude (deg) + * - 6 + - mlt + - hours + - float + - magnetic local time (hours) + * - 7 + - bx + - nT + - float + - observed magnetic field toward North (nT) + * - 8 + - by + - nT + - float + - observed magnetic field toward East (nT) + * - 9 + - bz + - nT + - float + - observed magnetic field toward Earth's center (nT) + * - 10 + - bex + - nT + - float + - external magnetic field toward North (nT) + * - 11 + - bey + - nT + - float + - external magnetic field toward East (nT) + * - 12 + - bez + - nT + - float + - external magnetic field toward Earth's center (nT) + * - 13 + - bpar + - nT + - float + - external magnetic field component parallel to the main field (nT) + * - 14 + - bper + - nT + - float + - signed external magnetic field component (direction of East component) perpendicular to the main field (nT) + * - 15 + - swarm + - - + - char + - satellite of the swarm constellation (A, B or C) diff --git a/docs/source/products/data/ingv_be_swarm_image.rst b/docs/source/products/data/ingv_be_swarm_image.rst deleted file mode 100644 index 4c9b27d..0000000 --- a/docs/source/products/data/ingv_be_swarm_image.rst +++ /dev/null @@ -1,39 +0,0 @@ -============================================== -INGV Swarm external vector magnetic field maps -============================================== - -.. contents:: The tiny table of contents - -Maps of vector magnetic field of external origin (i.e., obtained from the difference between the observed total field and a model of the main field) in quasi-dipole latitude vs magnetic local time coordinates derived from the Swarm constellation data acquired at 1 second cadence from 1 January 2014 to 31 December 2020. The output consists in nine .jpg or .png files mapping the three components of the vector magnetic field in polar and equatorial projections (3 images for the three components) for each of the 3 satellites of the Swarm constellation. Each map has a size of about 300 kB. - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Vector Field Magnetometer - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - .jpg/.png - - -| **Sample**: https://drive.google.com/file/d/13CvC3-FP3UyZ2Bg9XseP4Zzxp-6u8W5O/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_be_swarm_timeseries.rst b/docs/source/products/data/ingv_be_swarm_timeseries.rst deleted file mode 100644 index edd78f6..0000000 --- a/docs/source/products/data/ingv_be_swarm_timeseries.rst +++ /dev/null @@ -1,41 +0,0 @@ -==================================================================== -INGV 1 Hz Swarm on track values of external vector geomagnetic field -==================================================================== - -.. contents:: The tiny table of contents - -In situ time series of vector geomagnetic field of external origin (i.e., difference between the observed total field and the modelled main field) derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of one has a size of about 13 GB. The sample file attached is extracted from one month of data acquired by Swarm A - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Vector Field Magnetometer - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text file - - -| **Sample**: https://drive.google.com/file/d/1mA4cJG6aheoLylI-g4ywwSCFU1vvttfT/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_bep_swarm_image.rst b/docs/source/products/data/ingv_bep_swarm_image.rst deleted file mode 100644 index 80ef7cb..0000000 --- a/docs/source/products/data/ingv_bep_swarm_image.rst +++ /dev/null @@ -1,39 +0,0 @@ -=============================================== -INGV Swarm projected vector magnetic field maps -=============================================== - -.. contents:: The tiny table of contents - -Maps of vector magnetic field of external origin (i.e., obtained from the difference between the observed total field and a model of the main field) projected along the directions parallel and perpendicular to the main field in quasi-dipole latitude vs magnetic local time coordinates derived from the Swarm constellation data acquired at 1 second cadence from 1 January 2014 to 31 December 2020. The output consists in six .jpg or .png files mapping the two projected components of the external vector magnetic field in polar and equatorial projections (3 images for the two components) for each of the 3 satellites of the Swarm constellation. Each map has a size of about 400 kB. - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Vector Field Magnetometer - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - .jpg/.png - - -| **Sample**: https://drive.google.com/file/d/1uulMEArObSwF4VOeCORGiwqj3E-1J4tO/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_bep_swarm_timeseries.rst b/docs/source/products/data/ingv_bep_swarm_timeseries.rst deleted file mode 100644 index 5471af7..0000000 --- a/docs/source/products/data/ingv_bep_swarm_timeseries.rst +++ /dev/null @@ -1,41 +0,0 @@ -===================================================================== -INGV 1 Hz Swarm on track values of projected vector geomagnetic field -===================================================================== - -.. contents:: The tiny table of contents - -In situ time series of vector geomagnetic field of external origin (i.e., difference between the observed total field and the modelled main field) projected along the directions parallel and perpendicular to the main field derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of one has a size of about 13 GB. The sample file attached is extracted from one month of data acquired by Swarm A - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Vector Field Magnetometer - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text file - - -| **Sample**: https://drive.google.com/file/d/1Xk3pLMGF7Ktg6s9UdZbBHkp1xjg3p62e/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_bvect_cses_tableset.rst b/docs/source/products/data/ingv_bvect_cses_tableset.rst index 661fedd..7bdb335 100644 --- a/docs/source/products/data/ingv_bvect_cses_tableset.rst +++ b/docs/source/products/data/ingv_bvect_cses_tableset.rst @@ -1,69 +1,98 @@ -===================================================== -INGV CSES-01 on track values of vector magnetic field -===================================================== +================================================ +CSES-01 on track values of vector magnetic field +================================================ .. contents:: The tiny table of contents -Yearly data from HPM instrument onboard CSES-01 from 11 July 2018 to 31 May 2021 (based on availability of continuous data). +In situ time series of vector magnetic field derived from the CSES-01 satellite from 1 January 2019 to 30 September 2021. The output is a single .txt formatted file for both diurnal and nocturnal orbits, each of which has a size of about 3 GB. The sample file attached is extracted from one minute acquired by CSES-01 -Each file contains 6 columns: +**References** -#. UTC (ISO format); -#. Geographic Latitude (deg); -#. Geographic Longitude (deg); - -#. magnetic field vector time series (Bx) with a 1 Hz sampling in NEC coordinates and units nT. - -#. magnetic field vector time series (By) with a 1 Hz sampling in NEC coordinates and units nT. - -#. magnetic field vector time series (Bz) with a 1 Hz sampling in NEC coordinates and units nT. +Data description +~~~~~~~~~~~~~~~~ -Sub-Sub-folders: +**internal_name:** ingv_bvect_cses_tableset -* “csv”: Yearly .csv data. +**publisher:** INGV group -* “FIGURE”: Statistical maps of vector magnetic field (three components) in .fits format. Maps are available at two spatial resolutions: 1x1 deg^2 (high resolution) and 5x5 deg^2 (low resolution). For practical purposes use low-resolution maps. High-resolution maps are tagged, e.g., “Btot_x_DAY\_…”. Low-resolution maps are tagged, e.g., “Bx_Mean_DAY\_…”. In both cases the mean value within each bin is representative of the bin itself. +**alphanumeric_code:** 46B -* “nc”: Yearly netCDF data. +**id_tmp:** 84 -* “npy”: Statistical maps of vector magnetic field (three components) in .npy format. Maps are available at two spatial resolutions: 1x1 deg^2 (high resolution) and 5x5 deg^2 (low resolution). For practical purposes use low-resolution maps. High-resolution maps are tagged, e.g., “Btot_x_DAY\_…”. Low-resolution maps are tagged, e.g., “binned_5x5_Bx…_DAY…”. Maps are available with two different values representative of each bin: the mean and the median, respectively. +**short_name:** CSES_Bvect_ts -**References:** +**identifier:** aspis://ingv/bvect_cses_tableset -* `Shen, X., Zhang, X., Yuan, S. et al. The state-of-the-art of the China Seismo-Electromagnetic Satellite mission. Sci. China Technol. Sci. 61, 634–642 (2018). https://doi.org/10.1007/s11431-018-9242-0 `_ +**dynamic:** static -**Providers**: +**size:** 3GB -- **CSES-01 mission** - source: +**format:** csv - - High Precision Magnetometer +**type:** timeseries +**records_number:** 10356758 -| **Product Type**: data +**time_start:** 2019-01-01 -| **Status**: Active +**time_stop:** 2021-09-30 -| **Creation date**: 2022-04-13T16:16:20+02:00 +**spatial:** Earth's Ionosphere -| **Last Update**: 2023-10-01T12:00:00+02:00 +**messenger:** -Data Description -~~~~~~~~~~~~~~~~ +**spectral_min:** 0 -| **Data type**: tableset +**spectral_max:** 0 -| **Data formats**: - text file +**spectral_units:** +**observable:** phys.density,phys.electron -| **Sample**: https://drive.google.com/file/d/1Pw-9K9iSgmShWu5faeYLAA_xnNYJJji1/view?usp=sharing +**latest update:** 2024-03-28 05:08:09 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime + * - 2 + - geo_lat + - deg + - float + - Geographic latitude (deg) + * - 3 + - geo_lon + - deg + - float + - Geographic longitude (deg) + * - 4 + - bx + - nT + - float + - Magnetic field towards the North direction (nT) + * - 5 + - by + - nT + - float + - Magnetic field towards the East direction (nT) + * - 6 + - bz + - nT + - float + - Magnetic field towards the Earth's centre direction (nT) diff --git a/docs/source/products/data/ingv_evect_cses_tableset.rst b/docs/source/products/data/ingv_evect_cses_tableset.rst index 2d02669..11760ed 100644 --- a/docs/source/products/data/ingv_evect_cses_tableset.rst +++ b/docs/source/products/data/ingv_evect_cses_tableset.rst @@ -1,66 +1,98 @@ -===================================================== -INGV CSES-01 on track values of vector electric field -===================================================== +================================================ +CSES-01 on track values of vector electric field +================================================ .. contents:: The tiny table of contents -Yearly and orbital data from EFD instrument onboard CSES-01 from 1 January 2019 to 30 September 2021 (based on availability of continuous data). +In situ time series of vector electric field derived from the CSES-01 satellite from 1 January 2019 to 30 September 2021. The output is a single .txt formatted file for both diurnal and nocturnal orbits, each of which has a size of about 3 GB. The sample file attached is extracted from about ten minutes acquired by CSES-01 -Each file contains 6 columns: +**References** -#. UTC (ISO format); -#. Geographic Latitude (deg); -#. Geographic Longitude (deg); - -#. electric field vector time series (Ex) with a 0.5 Hz sampling in NEC coordinates and units mV/m. - -#. electric field vector time series (Ey) with a 0.5 Hz sampling in NEC coordinates and units mV/m. +Data description +~~~~~~~~~~~~~~~~ -#. electric field vector time series (Ez) with a 0.5 Hz sampling in NEC coordinates and units mV/m. +**internal_name:** ingv_evect_cses_tableset -Sub-Sub-folders: +**publisher:** INGV group -* “csv”: Yearly and orbital .csv data. +**alphanumeric_code:** 46A -* “FIGURE”: Statistical maps of vector electric field (three components) in .fits format. Maps are available at two spatial resolutions: 1x1 deg^2 (high resolution) and 5x5 deg^2 (low resolution). For practical purposes use low-resolution maps. High-resolution maps are tagged, e.g., “Ex_DAY\_…”. Low-resolution maps are tagged, e.g., “Ex_Mean_DAY\_…”. In both cases the mean value within each bin is representative of the bin itself. +**id_tmp:** 85 -* “npy”: Statistical maps of vector electric field (three components) in .npy format. Maps are available at two spatial resolutions: 1x1 deg^2 (high resolution) and 5x5 deg^2 (low resolution). For practical purposes use low-resolution maps. High-resolution maps are tagged, e.g., “Ex_DAY\_…”. Low-resolution maps are tagged, e.g., “binned_5x5_Ex…_DAY…”. Maps are available with two different values representative of each bin: the mean and the median, respectively. +**short_name:** CSES_Evec_ts +**identifier:** aspis://ingv/evect_cses_tableset -**References:** +**dynamic:** static -**Providers**: +**size:** 3GB -- **CSES-01 mission** - source: +**format:** csv - - Electric Field Detector +**type:** tableset +**records_number:** 9769594 -| **Product Type**: data +**time_start:** 2019-01-01 -| **Status**: Active +**time_stop:** 2021-09-30 -| **Creation date**: 2022-04-13T16:16:20+02:00 +**spatial:** Earth's Ionosphere -| **Last Update**: 2023-10-01T12:00:00+02:00 +**messenger:** -Data Description -~~~~~~~~~~~~~~~~ +**spectral_min:** 0 -| **Data type**: tableset +**spectral_max:** 0 -| **Data formats**: - text file +**spectral_units:** +**observable:** phys.density,phys.electron -| **Sample**: https://drive.google.com/file/d/1xPLSlHW3WSOFR7NRzvoQQD2YXKeEagEl/view?usp=sharing +**latest update:** 2024-03-28 05:08:09 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime + * - 2 + - geo_lat + - deg + - float + - Latitude (deg) + * - 3 + - geo_lon + - deg + - float + - Longitude (deg) + * - 4 + - Ex + - mV/m + - float + - Electric field towards the North direction (mv/m) + * - 5 + - Ey + - mV/m + - float + - Electric field towards the East direction (mv/m) + * - 6 + - Ez + - mV/m + - float + - Electric field towards the Earth's centre direction (mv/m) diff --git a/docs/source/products/data/ingv_field_cses_image.rst b/docs/source/products/data/ingv_field_cses_image.rst deleted file mode 100644 index a37df46..0000000 --- a/docs/source/products/data/ingv_field_cses_image.rst +++ /dev/null @@ -1,40 +0,0 @@ -==================================================== -INGV CSES-01 vector magnetic and electric field maps -==================================================== - -.. contents:: The tiny table of contents - -Vector magnetic and electric field maps in quasi-dipole latitude vs magnetic longitude derived from the CSES-01 satellite data acquired from 1 January 2019 to 30 September 2021. The output consists in six .jpg or .png files mapping vector magnetic and electric fields in equatorial projection in the dayside and the nightside (2 images each of the six components of electric and magnetic fields). Each map has a size of about 200 kB. No sample file attached. - -**Providers**: - -- **CSES-01** - sources: - - - High Precision Magnetometer - - Electric Field Detector - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - .jpg/.png - - -| **Sample**: - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_gic_aqu_timeseries.rst b/docs/source/products/data/ingv_gic_aqu_timeseries.rst index fa4261a..96a9dfa 100644 --- a/docs/source/products/data/ingv_gic_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_gic_aqu_timeseries.rst @@ -1,49 +1,128 @@ -========================================= -INGV L'Aquila GIC index -========================================= +====================================================== +INGV geomagnetic data, GIC indices and alert: L'Aquila +====================================================== .. contents:: The tiny table of contents -GIC index for L'Aquila observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. Since for L'Aquila observatory only preliminary data are available, before obtaining GICxy index it will be necessary to estimate X and Y from H and D preliminary data. +GIC index for L'Aquila observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. Since for L'Aquila observatory only preliminary data are available, before obtaining GICxy index it will be necessary to estimate X and Y from H and D preliminary data. -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: https://drive.google.com/file/d/1vErznq6BolwTigDUp-F6E2NDaDa6Lx9Z/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_gic_aqu_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 47A + +**id_tmp:** 7 + +**short_name:** INGV_AQU_gic + +**identifier:** aspis:///ingv/INGV_AQU_gic + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:09 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_gic_cts_timeseries.rst b/docs/source/products/data/ingv_gic_cts_timeseries.rst index ab61cfd..8c4523e 100644 --- a/docs/source/products/data/ingv_gic_cts_timeseries.rst +++ b/docs/source/products/data/ingv_gic_cts_timeseries.rst @@ -1,49 +1,128 @@ -========================================= -INGV Castello Tesino GIC index -========================================= +============================================================= +INGV geomagnetic data, GIC indices and alert: Castello Tesino +============================================================= .. contents:: The tiny table of contents -GIC index for Castello Tesino observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. If definitive values for Castello Tesino are available GICxy indices will calculates directly from X and Y 1-minute data, otherwise an estimate of X and Y will be first obtained from H and D preliminary data. +GIC index for Castello Tesino observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. If definitive values for Castello Tesino are available GICxy indices will calculates directly from X and Y 1-minute data, otherwise an estimate of X and Y will be first obtained from H and D preliminary data. -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: https://drive.google.com/file/d/1vErznq6BolwTigDUp-F6E2NDaDa6Lx9Z/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_gic_cts_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 47B + +**id_tmp:** 8 + +**short_name:** INGV_CTS_gic + +**identifier:** aspis:///ingv/INGV_CTS_gic + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:09 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_gic_dur_timeseries.rst b/docs/source/products/data/ingv_gic_dur_timeseries.rst index 03e718a..997436d 100644 --- a/docs/source/products/data/ingv_gic_dur_timeseries.rst +++ b/docs/source/products/data/ingv_gic_dur_timeseries.rst @@ -1,49 +1,128 @@ -========================================= -INGV Duronia GIC index -========================================= +===================================================== +INGV geomagnetic data, GIC indices and alert: Duronia +===================================================== .. contents:: The tiny table of contents -GIC index for Duronia observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. If definitive values for Duronia are available GICxy indices will calculates directly from X and Y 1-minute data, otherwise an estimate of X and Y will be first obtained from H and D preliminary data. +GIC index for Duronia observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. If definitive values for Duronia are available GICxy indices will calculates directly from X and Y 1-minute data, otherwise an estimate of X and Y will be first obtained from H and D preliminary data. -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: https://drive.google.com/file/d/1vErznq6BolwTigDUp-F6E2NDaDa6Lx9Z/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_gic_dur_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 47C + +**id_tmp:** 9 + +**short_name:** INGV_DUR_gic + +**identifier:** aspis:///ingv/INGV_DUR_gic + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:10 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_gic_int_timeseries.rst b/docs/source/products/data/ingv_gic_int_timeseries.rst index c6a23fb..c12f5a3 100644 --- a/docs/source/products/data/ingv_gic_int_timeseries.rst +++ b/docs/source/products/data/ingv_gic_int_timeseries.rst @@ -1,49 +1,133 @@ -============================================ -INGV GIC index for INTERMAGNET observatories -============================================ +============================================================================ +Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories +============================================================================ .. contents:: The tiny table of contents -As specified for product INTmag, data from INTERMAGNET observatories will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. For the selected observatories GIC index (specifically GICx and GICy) will be calculated. +As specified for product INTmag, data from INTERMAGNET observatories will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. For the selected observatories GIC index (specifically GICx and GICy) will be calculated. -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_gic_int_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 47E + +**id_tmp:** 10 + +**short_name:** INGV_INT_gic + +**identifier:** aspis:///ingv/INGV_INT_gic + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 120MB + +**format:** csv + +**type:** timeseries + +**records_number:** 1274399 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:10 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - IAGA_code + - dimensionless + - string + - IAGA identifier of the observatory + * - 3 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 4 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 5 + - Altitude + - m + - float + - m + * - 6 + - X + - nT + - float + - nT (X component in NEC frame) + * - 7 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 8 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 9 + - F + - nT + - float + - nT total intensity + * - 10 + - GICx + - dimensionless + - float + - no description + * - 11 + - GICy + - dimensionless + - float + - no description + * - 12 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 13 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_gic_lmp_timeseries.rst b/docs/source/products/data/ingv_gic_lmp_timeseries.rst index 7ac4016..3e501e2 100644 --- a/docs/source/products/data/ingv_gic_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_gic_lmp_timeseries.rst @@ -1,49 +1,128 @@ -========================================= -INGV Lampedusa GIC index -========================================= +======================================================= +INGV geomagnetic data, GIC indices and alert: Lampedusa +======================================================= .. contents:: The tiny table of contents -GIC index for Lampedusa observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. Since for Lampedusa observatory only preliminary data are available, before obtaining GICxy index it will be necessary to estimate X and Y from H and D preliminary data. +GIC index for Lampedusa observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. Since for Lampedusa observatory only preliminary data are available, before obtaining GICxy index it will be necessary to estimate X and Y from H and D preliminary data. -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: https://drive.google.com/file/d/1vErznq6BolwTigDUp-F6E2NDaDa6Lx9Z/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_gic_lmp_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 47D + +**id_tmp:** 11 + +**short_name:** INGV_LMP_gic + +**identifier:** aspis:///ingv/INGV_LMP_gic + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:10 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_gic_wdc_timeseries.rst b/docs/source/products/data/ingv_gic_wdc_timeseries.rst index e3c974e..d86724c 100644 --- a/docs/source/products/data/ingv_gic_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_gic_wdc_timeseries.rst @@ -1,49 +1,133 @@ -======================================================================= -INGV GIC index for World Data Center of Geomagnetism (WDC)observatories -======================================================================= +======================================================================================================== +Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories +======================================================================================================== .. contents:: The tiny table of contents -As specified for product WDCmag, data from World Data Center of Geomagnetism observatories will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. For the selected observatories GIC index (specifically GICx and GICy) will be calculated. +As specified for product WDCmag, data from World Data Center of Geomagnetism observatories will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. For the selected observatories GIC index (specifically GICx and GICy) will be calculated. -**Providers**: +**References** -- **INGV** - source: - - Algorithm - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-30T18:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_gic_wdc_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 47F + +**id_tmp:** 12 + +**short_name:** INGV_WDC_gic + +**identifier:** aspis:///ingv/INGV_WDC_gic + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 120MB + +**format:** csv + +**type:** timeseries + +**records_number:** 1274399 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:10 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - IAGA_code + - dimensionless + - string + - IAGA identifier of the observatory + * - 3 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 4 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 5 + - Altitude + - m + - float + - m + * - 6 + - X + - nT + - float + - nT (X component in NEC frame) + * - 7 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 8 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 9 + - F + - nT + - float + - nT total intensity + * - 10 + - GICx + - dimensionless + - float + - no description + * - 11 + - GICy + - dimensionless + - float + - no description + * - 12 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 13 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_lol_swarm_image.rst b/docs/source/products/data/ingv_lol_swarm_image.rst deleted file mode 100644 index 9dcf914..0000000 --- a/docs/source/products/data/ingv_lol_swarm_image.rst +++ /dev/null @@ -1,58 +0,0 @@ -======================================================================== -INGV GPS Loss of Lock (LoL) events global maps from ESA Swarm satellites -======================================================================== - -.. contents:: The tiny table of contents - -Global maps of GPS LoL (Loss of Lock) events, as derived by total electron content observations from the Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2020. - -Swarm is an ESA constellation constituted by three low-Earth-orbit satellites launched at the end of 2013, and still operating, in a circular near-polar orbit. Two of them (Swarm A and C) have the same orbit configuration: an inclination of 87.35°, an initial altitude of about 460 km, and an initial east–west separation of about 1°–1.5° in longitude. The third (Swarm B) has a different orbital configuration: an inclination of 87.75° and an initial altitude of about 520 km. Precise Orbit Determination (POD) antennas are GPS -receivers through which TEC values are estimated. Level 2 (L2) TEC data contain time series of vertical and slant (both absolute and relative) TEC for each GPS satellite in view (at most eight due to the instrumentation design). Swarm’s data are freely downloadable at ftp://swarm-diss.eo.esa.int. - -**References:** - -* `De Michelis et al. (2022), Space Weather, 20, e2022SW003129. `_ - -* `Lovati et al. (2023a), Scientific Reports, 9287. `_ - -* `Lovati et al. (2023b), Journal of Geophysical Research: Space Physics, 128, e2023JA031411. `_ - -* `Pezzopane et al. (2021), Remote Sensing, 13, 2209. `_ - -**Providers**: - -- **Swarm A satellite** - source: - - - ESA Swarm A Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ -- **Swarm B satellite** - source: - - - ESA Swarm B Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ -- **Swarm C satellite** - source: - - - ESA Swarm C Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - text files - - -| **Sample**: https://drive.google.com/file/d/11vcJiTgmVprf6R0vGb33RVg2WAv_l4OS/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_lol_swarm_timeseries.rst b/docs/source/products/data/ingv_lol_swarm_timeseries.rst deleted file mode 100644 index 8cb547f..0000000 --- a/docs/source/products/data/ingv_lol_swarm_timeseries.rst +++ /dev/null @@ -1,60 +0,0 @@ -======================================================================== -INGV GPS Loss of Lock (LoL) events time series from ESA Swarm satellites -======================================================================== - -.. contents:: The tiny table of contents - -GPS LoL (Loss of Lock) events, as derived by total electron content observations from the Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2020. - -Swarm is an ESA constellation constituted by three low-Earth-orbit satellites launched at the end of 2013, and still operating, in a circular near-polar orbit. Two of them (Swarm A and C) have the same orbit configuration: an inclination of 87.35°, an initial altitude of about 460 km, and an initial east–west separation of about 1°–1.5° in longitude. The third (Swarm B) has a different orbital configuration: an inclination of 87.75° and an initial altitude of about 520 km. Precise Orbit Determination (POD) antennas are GPS -receivers through which TEC values are estimated. Level 2 (L2) TEC data contain time series of vertical and slant (both absolute and relative) TEC for each GPS satellite in view (at most eight due to the instrumentation design). Swarm’s data are freely downloadable at ftp://swarm-diss.eo.esa.int. - -**References:** - -De Michelis et al. (2022), Space Weather, 20, e2022SW003129. https://doi.org/10.1029/2022SW003129 - -Lovati et al. (2023a), Scientific Reports, 9287. https://doi.org/10.1038/s41598-023-34727-2 - -Lovati et al. (2023b), Journal of Geophysical Research: Space Physics, 128, e2023JA031411. https://doi.org/10.1029/2023JA031411 - -Pezzopane et al. (2021), Remote Sensing, 13, 2209. https://doi.org/10.3390/rs13112209 - -**Providers**: - -- **Swarm A satellite** - source: - - - ESA Swarm A Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ -- **Swarm B satellite** - source: - - - ESA Swarm B Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ -- **Swarm C satellite** - source: - - - ESA Swarm C Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text files - - -| **Sample**: https://drive.google.com/file/d/13AWtsY9wFNcdxXAXp4jD0FXkAhxE5ulb/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst b/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst index 8bfffe6..c5d0e4a 100644 --- a/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst @@ -1,38 +1,103 @@ -============================================ -INGV Long Term MUF maps centered on Cagliari -============================================ +======================================= +Long Term MUF maps centered on Cagliari +======================================= .. contents:: The tiny table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Cagliari over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**Providers**: +**References** -- **INGV model** -| **Product Type**: lookup-table +Data description +~~~~~~~~~~~~~~~~ -| **Status**: Inactive +**internal_name:** ingv_ltmuf_cagliari_tableset -| **Creation date**: 2022-04-27T06:26:08+00:00 +**publisher:** INGV -| **Last Update**: 2023-10-01T12:00:00+02:00 +**alphanumeric_code:** 28A -Data Description -~~~~~~~~~~~~~~~~ +**id_tmp:** 63 + +**short_name:** LTMUFCagliari + +**identifier:** aspis://ingv/ltmuf_cagliari_tableset + +**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + +**size:** 1MB + +**format:** dat,png + +**type:** tableset + +**records_number:** 48 + +**time_start:** 2017-09-07 + +**time_stop:** 2017-09-08 + +**spatial:** IONO + +**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere + +**spectral_min:** 0 -| **Data type**: image +**spectral_max:** 0 -| **Data formats**: - png +**spectral_units:** +**observable:** -| **Sample**: https://drive.google.com/file/d/1OlmXoC8dVV9COHgbs_Nuv7egePhEMVaF/view?usp=sharing +**latest update:** 2024-03-28 05:08:10 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of sounding + * - 2 + - Lat + - deg + - float + - latitude + * - 3 + - Long + - deg + - float + - longitude + * - 4 + - site + - char + - char + - site name + * - 5 + - data_name + - char + - char + - dataset filename + * - 6 + - prew_name + - char + - char + - image filename + * - 7 + - thumb_name + - char + - char + - diff --git a/docs/source/products/data/ingv_ltmuf_catania_tableset.rst b/docs/source/products/data/ingv_ltmuf_catania_tableset.rst index adea00f..e65976e 100644 --- a/docs/source/products/data/ingv_ltmuf_catania_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_catania_tableset.rst @@ -1,38 +1,103 @@ -=========================================== -INGV Long Term MUF maps centered on Catania -=========================================== +====================================== +Long Term MUF maps centered on Catania +====================================== .. contents:: The tiny table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**Providers**: +**References** -- **INGV model** -| **Product Type**: lookup-table +Data description +~~~~~~~~~~~~~~~~ -| **Status**: Inactive +**internal_name:** ingv_ltmuf_catania_tableset -| **Creation date**: 2022-04-27T06:26:08+00:00 +**publisher:** INGV -| **Last Update**: 2023-10-01T12:00:00+02:00 +**alphanumeric_code:** 28B -Data Description -~~~~~~~~~~~~~~~~ +**id_tmp:** 70 + +**short_name:** LTMUFCatania + +**identifier:** aspis://ingv/ltmuf_catania_tableset + +**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + +**size:** 1MB + +**format:** dat,png + +**type:** tableset + +**records_number:** 48 + +**time_start:** 2017-09-07 + +**time_stop:** 2017-09-08 + +**spatial:** IONO + +**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere + +**spectral_min:** 0 -| **Data type**: image +**spectral_max:** 0 -| **Data formats**: - png +**spectral_units:** +**observable:** -| **Sample**: https://drive.google.com/file/d/15P1zVVveGqEHLFJzTcSwwpELDv9J-nqR/view?usp=sharing +**latest update:** 2024-03-28 05:08:10 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of the sounding + * - 2 + - Lat + - deg + - float + - (MHz) maximum frequency reflected by the F2 layer + * - 3 + - Long + - deg + - float + - (MHz) maximum frequency reflected by the F1 layer + * - 4 + - site + - char + - char + - (MHz) maximum frequency reflected by the sporadic E layer + * - 5 + - data_name + - char + - char + - (MHz) maximum usable frequency for a distance of 3000 km centered over the ionosonde site + * - 6 + - prew_name + - char + - char + - (adimensional) propagation factor + * - 7 + - thumb_name + - char + - char + - (km) virtual height of the sporadic E layer diff --git a/docs/source/products/data/ingv_ltmuf_milan_tableset.rst b/docs/source/products/data/ingv_ltmuf_milan_tableset.rst index 9166bc9..325f463 100644 --- a/docs/source/products/data/ingv_ltmuf_milan_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_milan_tableset.rst @@ -1,38 +1,103 @@ -========================================= -INGV Long Term MUF maps centered on Milan -========================================= +===================================== +Long Term MUF maps centered on Milano +===================================== .. contents:: The tiny table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**Providers**: +**References** -- **INGV model** -| **Product Type**: lookup-table +Data description +~~~~~~~~~~~~~~~~ -| **Status**: Inactive +**internal_name:** ingv_ltmuf_milan_tableset -| **Creation date**: 2022-04-27T06:26:08+00:00 +**publisher:** INGV -| **Last Update**: 2023-10-01T12:00:00+02:00 +**alphanumeric_code:** 28C -Data Description -~~~~~~~~~~~~~~~~ +**id_tmp:** 68 + +**short_name:** LTMUFMilano + +**identifier:** aspis://ingv/ltmuf_milano_tableset + +**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + +**size:** 1MB + +**format:** dat,png + +**type:** tableset + +**records_number:** 48 + +**time_start:** 2017-09-07 + +**time_stop:** 2017-09-08 + +**spatial:** IONO + +**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere + +**spectral_min:** 0 -| **Data type**: image +**spectral_max:** 0 -| **Data formats**: - png +**spectral_units:** +**observable:** -| **Sample**: https://drive.google.com/file/d/1fFM0mShvAoHlf_HlOVh7rjvQ5Ai5dyV3/view?usp=sharing +**latest update:** 2024-03-28 05:08:11 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of the sounding + * - 2 + - Lat + - deg + - float + - (MHz) maximum frequency reflected by the F2 layer + * - 3 + - Long + - deg + - float + - (MHz) maximum frequency reflected by the F1 layer + * - 4 + - site + - char + - char + - (MHz) maximum frequency reflected by the sporadic E layer + * - 5 + - data_name + - char + - char + - (MHz) maximum usable frequency for a distance of 3000 km centered over the ionosonde site + * - 6 + - prew_name + - char + - char + - (adimensional) propagation factor + * - 7 + - thumb_name + - char + - char + - (km) virtual height of the sporadic E layer diff --git a/docs/source/products/data/ingv_ltmuf_rome_tableset.rst b/docs/source/products/data/ingv_ltmuf_rome_tableset.rst index 21b20d2..061f2e1 100644 --- a/docs/source/products/data/ingv_ltmuf_rome_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_rome_tableset.rst @@ -1,38 +1,103 @@ -========================================= -INGV Long Term MUF maps centered on Rome -========================================= +=================================== +Long Term MUF maps centered on Roma +=================================== .. contents:: The tiny table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**Providers**: +**References** -- **INGV model** -| **Product Type**: lookup-table +Data description +~~~~~~~~~~~~~~~~ -| **Status**: Inactive +**internal_name:** ingv_ltmuf_rome_tableset -| **Creation date**: 2022-04-26T06:26:08+00:00 +**publisher:** INGV -| **Last Update**: 2023-10-01T12:00:00+02:00 +**alphanumeric_code:** 28D -Data Description -~~~~~~~~~~~~~~~~ +**id_tmp:** 69 + +**short_name:** LTMUFRoma + +**identifier:** aspis://ingv/ltmuf_roma_tableset + +**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + +**size:** 1MB + +**format:** dat,png + +**type:** tableset + +**records_number:** 48 + +**time_start:** 2017-09-07 + +**time_stop:** 2017-09-08 + +**spatial:** IONO + +**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere + +**spectral_min:** 0 -| **Data type**: image +**spectral_max:** 0 -| **Data formats**: - png +**spectral_units:** +**observable:** -| **Sample**: https://drive.google.com/file/d/1reQwlgS-qA36yenYJyp9Ch8NJ_nKfjq4/view?usp=sharing +**latest update:** 2024-03-28 05:08:11 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of the sounding + * - 2 + - Lat + - deg + - float + - (MHz) maximum frequency reflected by the F2 layer + * - 3 + - Long + - deg + - float + - (MHz) maximum frequency reflected by the F1 layer + * - 4 + - site + - char + - char + - (MHz) maximum frequency reflected by the sporadic E layer + * - 5 + - data_name + - char + - char + - (MHz) maximum usable frequency for a distance of 3000 km centered over the ionosonde site + * - 6 + - prew_name + - char + - char + - (adimensional) propagation factor + * - 7 + - thumb_name + - char + - char + - (km) virtual height of the sporadic E layer diff --git a/docs/source/products/data/ingv_mag_aqu_timeseries.rst b/docs/source/products/data/ingv_mag_aqu_timeseries.rst index 8669ef5..7032fc4 100644 --- a/docs/source/products/data/ingv_mag_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_mag_aqu_timeseries.rst @@ -1,49 +1,128 @@ -========================================= -INGV Preliminary L'Aquila magnetic data -========================================= +====================================================== +INGV geomagnetic data, GIC indices and alert: L'Aquila +====================================================== .. contents:: The tiny table of contents -1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at L'Aquila magnetic observatory (IAGA code: AQU; Latitude: 42.383000°; Longitude: 13.316000°; Altitude: 682.000 m). In detail, preliminary "pseudo" H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. +1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at L'Aquila magnetic observatory (IAGA code: AQU Latitude: 42.383000° Longitude: 13.316000° Altitude: 682.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**Providers**: +**References** -- **INGV** - source: - - Magnetometer - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:15:32+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1UE2W00Je7pZyYU8CudoQQQd-un1jSnq-/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised -- int2130.4: Scheduled computation -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_mag_aqu_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 8A + +**id_tmp:** 17 + +**short_name:** INGV_AQU_mag + +**identifier:** aspis:///ingv/INGV_AQU_mag + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:11 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_mag_cts_timeseries.rst b/docs/source/products/data/ingv_mag_cts_timeseries.rst index d4b0d82..db53559 100644 --- a/docs/source/products/data/ingv_mag_cts_timeseries.rst +++ b/docs/source/products/data/ingv_mag_cts_timeseries.rst @@ -1,49 +1,128 @@ -============================================== -INGV Preliminary Castello Tesino magnetic data -============================================== +============================================================= +INGV geomagnetic data, GIC indices and alert: Castello Tesino +============================================================= .. contents:: The tiny table of contents -1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino (TN) magnetic observatory (IAGA code: CTS; Latitude: 46.047000°; Longitude: 11.649000°; Altitude: 1175.000 m). In detail, preliminary \"pseudo\" H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. For this observatory also definitive data are available. +1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino (TN) magnetic observatory (IAGA code: CTS Latitude: 46.047000° Longitude: 11.649000° Altitude : 1175.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. For this observatory also definitive data are available. -**Providers**: +**References** -- **INGV** - source: - - Magnetometer - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:15:32+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/15yM6Xmkguu_jWEBbUAWx96DS-oFT12Ze/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.3: Mirroring: bulk static -- int2130.4: Scheduled computation -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_mag_cts_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 8B + +**id_tmp:** 18 + +**short_name:** INGV_CTS_mag + +**identifier:** aspis:///ingv/INGV_CTS_mag + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:11 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_mag_dmc_timeseries.rst b/docs/source/products/data/ingv_mag_dmc_timeseries.rst index c4acd8a..a810c5b 100644 --- a/docs/source/products/data/ingv_mag_dmc_timeseries.rst +++ b/docs/source/products/data/ingv_mag_dmc_timeseries.rst @@ -1,49 +1,128 @@ -========================================= -INGV Preliminary Dome C magnetic data -========================================= +==================================================== +INGV geomagnetic data, GIC indices and alert: Dome C +==================================================== .. contents:: The tiny table of contents -1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Dome C magnetic observatory(AGA code: DMC; Latitude: -75.250000°; Longitude: 124.167000°; Altitude: 3250.000 m). In detail, preliminary "pseudo" H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. +1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Dome C magnetic observatory(AGA code: DMC Latitude: -75.250000° Longitude: 124.167000° Altitude: 3250.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**Providers**: +**References** -- **INGV** - source: - - Magnetometer - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:45:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1PaR0RkOng2lMedAoXQ8iDA_gyPsw9Yq6/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised -- int2130.4: Scheduled computation -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_mag_dmc_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 8D + +**id_tmp:** 19 + +**short_name:** INGV_DMC_mag + +**identifier:** aspis:///ingv/INGV_DMC_mag + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:12 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_mag_dur_timeseries.rst b/docs/source/products/data/ingv_mag_dur_timeseries.rst index 6241743..f598575 100644 --- a/docs/source/products/data/ingv_mag_dur_timeseries.rst +++ b/docs/source/products/data/ingv_mag_dur_timeseries.rst @@ -1,49 +1,128 @@ -========================================= -INGV Preliminary Duronia magnetic data -========================================= +===================================================== +INGV geomagnetic data, GIC indices and alert: Duronia +===================================================== .. contents:: The tiny table of contents -1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Duronia magnetic observatory (IAGA code: DUR; Latitude: 41.650000°; Longitude: 14.466000°; Altitude: 895.000 m). In detail, preliminary "pseudo" H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. For this observatory also definitive data are available. +1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Duronia magnetic observatory (IAGA code: DUR Latitude: 41.650000° Longitude: 14.466000° Altitude: 895.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. For this observatory also definitive data are available. -**Providers**: +**References** -- **INGV** - source: - - Magnetometer - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:30:32+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1K-0hlt1a4jF-UvR1JW9tp4tOPOfqQtKf/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised -- int2130.4: Scheduled computation -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_mag_dur_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 8E + +**id_tmp:** 20 + +**short_name:** INGV_DUR_mag + +**identifier:** aspis:///ingv/INGV_DUR_mag + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:12 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_mag_int_timeseries.rst b/docs/source/products/data/ingv_mag_int_timeseries.rst index e144d21..84e5be3 100644 --- a/docs/source/products/data/ingv_mag_int_timeseries.rst +++ b/docs/source/products/data/ingv_mag_int_timeseries.rst @@ -1,46 +1,133 @@ -================================================= -INGV Magnetic data from INTERMAGNET observatories -================================================= +============================================================================ +Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories +============================================================================ .. contents:: The tiny table of contents -The INTERMAGNET programme exists to establish a global network of cooperating digital magnetic observatories, adopting modern standard specifications for measuring and recording equipment, in order to facilitate data exchanges and the production of geomagnetic products in close to real time. From the INTERMAGNET website it is possible to download 1-minute averages (in daily files) of vector components in either (H, D, Z) or (X, Y, Z) reference frame from world wide magnetic observatories. For this reason, it is not possible to exhaustively fill this form. For instance, the time window of data availability changes from observatory to observatory as well as the tern provided (either (H, D, Z) or (X, Y, Z)) . Data from INTERMAGNET will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. Data can be downloaded as .gz files from an ftp (ftp://ftp.seismo.nrcan.gc.ca/intermagnet/). Each file contains 1 day of 1-minute magnetic data for a single INTERMAGNET observatory +The INTERMAGNET programme exists to establish a global network of cooperating digital magnetic observatories, adopting modern standard specifications for measuring and recording equipment, in order to facilitate data exchanges and the production of geomagnetic products in close to real time. From the INTERMAGNET website it is possible to download 1-minute averages (in daily files) of vector components in either (H, D, Z) or (X, Y, Z) reference frame from world wide magnetic observatories. For this reason, it is not possible to exhaustively fill this form. For instance, the time window of data availability changes from observatory to observatory as well as the tern provided (either (H, D, Z) or (X, Y, Z)) . Data from INTERMAGNET will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. Data can be downloaded as .gz files from an ftp (ftp://ftp.seismo.nrcan.gc.ca/intermagnet/). Each file contains 1 day of 1-minute magnetic data for a single INTERMAGNET observatory -**Providers**: +**References** -- **INTERMAGNET** - source: - - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:45:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - gz - - -| **Sample**: https://drive.google.com/file/d/1uF7geNrIEDfwITv1TVKVW6mlfZdllnog/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.3: Mirroring: bulk static -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_mag_int_timeseries + +**publisher:** INTERMAGNET + +**alphanumeric_code:** 9A + +**id_tmp:** 21 + +**short_name:** INGV_INT_mag + +**identifier:** aspis:///ingv/INGV_INT_mag + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 120MB + +**format:** csv + +**type:** timeseries + +**records_number:** 1274399 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:12 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - IAGA_code + - dimensionless + - string + - IAGA identifier of the observatory + * - 3 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 4 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 5 + - Altitude + - m + - float + - m + * - 6 + - X + - nT + - float + - nT (X component in NEC frame) + * - 7 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 8 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 9 + - F + - nT + - float + - nT total intensity + * - 10 + - GICx + - dimensionless + - float + - no description + * - 11 + - GICy + - dimensionless + - float + - no description + * - 12 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 13 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_mag_lmp_timeseries.rst b/docs/source/products/data/ingv_mag_lmp_timeseries.rst index 0c12fb0..cdf193b 100644 --- a/docs/source/products/data/ingv_mag_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_mag_lmp_timeseries.rst @@ -1,49 +1,128 @@ -========================================= -INGV Preliminary Lampedusa magnetic data -========================================= +======================================================= +INGV geomagnetic data, GIC indices and alert: Lampedusa +======================================================= .. contents:: The tiny table of contents -1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Lampedusa magnetic observatory (IAGA code: LMP; Latitude: 35.517000°; Longitude: 12.545000°; Altitude: 93.000 m). In detail, preliminary "pseudo" H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. +1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Lampedusa magnetic observatory (IAGA code: LMP Latitude: 35.517000° Longitude: 12.545000° Altitude: 93.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**Providers**: +**References** -- **INGV** - source: - - Magnetometer - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:45:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1wbpQau6gT6AFwrZfIS7RygMeN8eDoxhc/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised -- int2130.4: Scheduled computation -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_mag_lmp_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 8G + +**id_tmp:** 22 + +**short_name:** INGV_LMP_mag + +**identifier:** aspis:///ingv/INGV_LMP_mag + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:12 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_mag_tnb_timeseries.rst b/docs/source/products/data/ingv_mag_tnb_timeseries.rst index d0213d8..97a05bb 100644 --- a/docs/source/products/data/ingv_mag_tnb_timeseries.rst +++ b/docs/source/products/data/ingv_mag_tnb_timeseries.rst @@ -1,49 +1,128 @@ -============================================= -INGV Preliminary Terra Nova Bay magnetic data -============================================= +============================================================ +INGV geomagnetic data, GIC indices and alert: Terra Nova Bay +============================================================ .. contents:: The tiny table of contents -1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Terra Nova Bay magnetic observatory (IAGA code: TNB; Latitude: -74.693000°; Longitude: 164.099000°; Altitude: 59.000 m). In detail, preliminary "pseudo" H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. +1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Terra Nova Bay magnetic observatory (IAGA code: TNB Latitude: -74.693000° Longitude: 164.099000° Altitude: 59.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**Providers**: +**References** -- **INGV** - source: - - Magnetometer - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:45:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1W21VxLPQ7io_P6Zsew_Mc0Lf-YMP6asz/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised -- int2130.4: Scheduled computation -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_mag_tnb_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 8H + +**id_tmp:** 23 + +**short_name:** INGV_TNB_mag + +**identifier:** aspis:///ingv/INGV_TNB_mag + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:12 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_mag_wdc_timeseries.rst b/docs/source/products/data/ingv_mag_wdc_timeseries.rst index aad7747..fa9c8ab 100644 --- a/docs/source/products/data/ingv_mag_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_mag_wdc_timeseries.rst @@ -1,49 +1,133 @@ -============================================================================= -INGV Magnetic data from World Data Center of Geomagnetism (WDC) observatories -============================================================================= +======================================================================================================== +Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories +======================================================================================================== .. contents:: The tiny table of contents The mission of the World Data Center for Geomagnetism is to provide geomagnetic field data supplied from a worldwide network of magnetic observatories, as well as geomagnetic indices (AE index, ASY/SYM index, and Dst index) derived in this data center to researchers specializing mostly in solar terrestrial physics, and geomagnetism in order to facilitate the global exchange of the geomagnetic field data including the geomagnetic indices. From the WDC websites it is possible to download 1-minute averages (in daily files) of vector components in either (H, D, Z) or (X, Y, Z) reference frame from world wide magnetic observatories. For this reason, it is not possible to exhaustively fill this form. For instance, the time window of data availability changes from observatory to observatory as well as the tern provided (either (H, D, Z) or (X, Y, Z)) . Data from WDC will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. The set of WDC observatories well overlap to the set of INTERMAGNET observatories. WDC data can be retrieved through queries to a web service (http://www.wdc.bgs.ac.uk/dataportal/webservice_doc.html). At the present moment, however, the service and the website are not working properly and it is not possible to download a sample file. -**Providers**: +**References** -- **World Data Center for Geomagnetism** - source: - - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:45:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json -- txt - - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.3: Mirroring: bulk static -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_mag_wdc_timeseries + +**publisher:** World Data Center for Geomagnetism + +**alphanumeric_code:** 9B + +**id_tmp:** 24 + +**short_name:** INGV_WDC_mag + +**identifier:** aspis:///ingv/INGV_WDC_mag + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 120MB + +**format:** csv + +**type:** timeseries + +**records_number:** 1274399 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:12 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - IAGA_code + - dimensionless + - string + - IAGA identifier of the observatory + * - 3 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 4 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 5 + - Altitude + - m + - float + - m + * - 6 + - X + - nT + - float + - nT (X component in NEC frame) + * - 7 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 8 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 9 + - F + - nT + - float + - nT total intensity + * - 10 + - GICx + - dimensionless + - float + - no description + * - 11 + - GICy + - dimensionless + - float + - no description + * - 12 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 13 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_magdef_cts_timeseries.rst b/docs/source/products/data/ingv_magdef_cts_timeseries.rst index dacaf8d..187adac 100644 --- a/docs/source/products/data/ingv_magdef_cts_timeseries.rst +++ b/docs/source/products/data/ingv_magdef_cts_timeseries.rst @@ -1,50 +1,129 @@ -============================================= -INGV Definitive Castello Tesino magnetic data -============================================= +============================================================= +INGV geomagnetic data, GIC indices and alert: Castello Tesino +============================================================= .. contents:: The tiny table of contents -1-minute averages of the components (X, Y, Z in the NEC, i.e. North-East-Center frame) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino magnetic observatory (IAGA code: CTS; Latitude: 46.047000°; Longitude: 11.649000°; Altitude: 1175.000 m). These are the definitive values that will be used to calculate GICx and GICy indices. These data are definitive, new definitive data are added yearly. -They can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. +1-minute averages of the components (X, Y, Z in the NEC, i.e. North-East-Center frame) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino magnetic observatory (IAGA code: CTS Latitude: 46.047000° Longitude: 11.649000° Altitude: 1175.000 m). These are the definitive values that will be used to calculate GICx and GICy indices. These data are definitive, new definitive data are added yearly. +They can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**Providers**: +**References** -- **INGV** - source: - - Magnetometer - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:15:32+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1p-bhkzvlG95gfNPU1IqGmyErAtOCXsDF/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.3: Mirroring: bulk static -- int2130.4: Scheduled computation -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_magdef_cts_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 8C + +**id_tmp:** 25 + +**short_name:** INGV_CTS_magdef + +**identifier:** aspis:///ingv/INGV_CTS_magdef + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:11 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_magdef_dur_timeseries.rst b/docs/source/products/data/ingv_magdef_dur_timeseries.rst index fe91a09..40d43f6 100644 --- a/docs/source/products/data/ingv_magdef_dur_timeseries.rst +++ b/docs/source/products/data/ingv_magdef_dur_timeseries.rst @@ -1,50 +1,129 @@ -========================================= -INGV Definitive Duronia magnetic data -========================================= +===================================================== +INGV geomagnetic data, GIC indices and alert: Duronia +===================================================== .. contents:: The tiny table of contents -1-minute averages of the components (X, Y, Z in the NEC, i.e. North-East-Center frame) and of total intensity (F) of the Earth's geomagnetic field measured at Duronia magnetic observatory (IAGA code: DUR; Latitude: 41.650000°; Longitude: 14.466000°; Altitude: 895.000 m). These are the definitive values that will be used to calculate GICx and GICy indices. These data are definitive, new definitive data are added yearly. -They can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. +1-minute averages of the components (X, Y, Z in the NEC, i.e. North-East-Center frame) and of total intensity (F) of the Earth's geomagnetic field measured at Duronia magnetic observatory (IAGA code: DUR Latitude: 41.650000° Longitude: 14.466000° Altitude: 895.000 m). These are the definitive values that will be used to calculate GICx and GICy indices. These data are definitive, new definitive data are added yearly. +They can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**Providers**: +**References** -- **INGV** - source: - - Magnetometer - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-21T18:15:32+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: timeseries - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1OdV8phrfCOHEM_mUMSpNK1_opyOr9w-7/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.3: Mirroring: bulk static -- int2130.4: Scheduled computation -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** ingv_magdef_dur_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 8F + +**id_tmp:** 26 + +**short_name:** INGV_DUR_magdef + +**identifier:** aspis:///ingv/INGV_DUR_magdef + +**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 84960 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** GROUND + +**messenger:** + +**spectral_min:** 1 + +**spectral_max:** 1 + +**spectral_units:** 1/minute + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:11 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - no description + * - 2 + - Geo_Lat + - deg + - float + - Geographic Latitude ° + * - 3 + - Geo_Lon + - deg + - float + - Geographic Longitude ° + * - 4 + - Altitude + - m + - float + - m + * - 5 + - X + - nT + - float + - nT (X component in NEC frame) + * - 6 + - Y + - nT + - float + - nT (Y component in NEC frame) + * - 7 + - Z + - nT + - float + - nT (Z component in NEC frame) + * - 8 + - F + - nT + - float + - nT total intensity + * - 9 + - GICx + - dimensionless + - float + - no description + * - 10 + - GICy + - dimensionless + - float + - no description + * - 11 + - AlertX + - dimensionless + - integer + - Alert based on GicX index + * - 12 + - AlertY + - dimensionless + - integer + - Alert based on GicY index diff --git a/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst b/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst index ad3cd73..053d383 100644 --- a/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst @@ -1,42 +1,103 @@ -============================================ -INGV Nowcasting MUF map centered on Cagliari -============================================ +======================================= +Nowcasting MUF map centered on Cagliari +======================================= .. contents:: The tiny table of contents +Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Cagliari over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ +**References** -Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Cagliari over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**Providers**: +Data description +~~~~~~~~~~~~~~~~ -- **INGV model** +**internal_name:** ingv_ncmuf_cagliari_tableset +**publisher:** INGV -| **Product Type**: lookup-table +**alphanumeric_code:** 28E -| **Status**: Inactive +**id_tmp:** 27 -| **Creation date**: 2022-04-26T06:26:08+00:00 +**short_name:** NCMUFCagliari -| **Last Update**: 2023-10-01T12:00:00+02:00 +**identifier:** aspis://ingv/ncmuf_cagliari_tableset -Data Description -~~~~~~~~~~~~~~~~ +**dynamic:** The map is a nowcasting map, generated every 15 minutes. + +**size:** 1MB + +**format:** png,dat + +**type:** tableset + +**records_number:** 192 + +**time_start:** 2017-09-07 + +**time_stop:** 2017-09-08 + +**spatial:** IONO + +**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere + +**spectral_min:** -| **Data type**: image +**spectral_max:** -| **Data formats**: - png +**spectral_units:** +**observable:** -| **Sample**: https://drive.google.com/file/d/1OlmXoC8dVV9COHgbs_Nuv7egePhEMVaF/view?usp=sharing +**latest update:** 2024-03-28 05:08:13 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of sounding + * - 2 + - Lat + - deg + - float + - latitude + * - 3 + - Long + - deg + - float + - longitude + * - 4 + - site + - char + - char + - site name + * - 5 + - data_name + - char + - char + - dataset filename + * - 6 + - prew_name + - char + - char + - image filename + * - 7 + - thumb_name + - char + - char + - thumbnail filename diff --git a/docs/source/products/data/ingv_ncmuf_catania_tableset.rst b/docs/source/products/data/ingv_ncmuf_catania_tableset.rst index 7f29d73..e257ba3 100644 --- a/docs/source/products/data/ingv_ncmuf_catania_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_catania_tableset.rst @@ -1,38 +1,103 @@ -=========================================== -INGV Nowcasting MUF map centered on Catania -=========================================== +====================================== +Nowcasting MUF map centered on Catania +====================================== .. contents:: The tiny table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**Providers**: +**References** -- **INGV model** -| **Product Type**: lookup-table +Data description +~~~~~~~~~~~~~~~~ -| **Status**: Inactive +**internal_name:** ingv_ncmuf_catania_tableset -| **Creation date**: 2022-04-26T06:26:08+00:00 +**publisher:** INGV -| **Last Update**: 2023-10-01T12:00:00+02:00 +**alphanumeric_code:** 28F -Data Description -~~~~~~~~~~~~~~~~ +**id_tmp:** 28 + +**short_name:** NCMUFCatania + +**identifier:** aspis://ingv/ncmuf_catania_tableset + +**dynamic:** The map is a nowcasting map, generated every 15 minutes. + +**size:** 1MB + +**format:** png,dat + +**type:** tableset + +**records_number:** 192 + +**time_start:** 2017-09-07 + +**time_stop:** 2017-09-08 + +**spatial:** IONO + +**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere + +**spectral_min:** -| **Data type**: image +**spectral_max:** -| **Data formats**: - png +**spectral_units:** +**observable:** -| **Sample**: https://drive.google.com/file/d/15P1zVVveGqEHLFJzTcSwwpELDv9J-nqR/view?usp=sharing +**latest update:** 2024-03-28 05:08:13 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of sounding + * - 2 + - Lat + - deg + - float + - latitude + * - 3 + - Long + - deg + - float + - longitude + * - 4 + - site + - char + - char + - site name + * - 5 + - data_name + - char + - char + - dataset filename + * - 6 + - prew_name + - char + - char + - image filename + * - 7 + - thumb_name + - char + - char + - thumbnail filename diff --git a/docs/source/products/data/ingv_ncmuf_milan_tableset.rst b/docs/source/products/data/ingv_ncmuf_milan_tableset.rst index cfceabf..6a29c09 100644 --- a/docs/source/products/data/ingv_ncmuf_milan_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_milan_tableset.rst @@ -1,38 +1,103 @@ -========================================= -INGV Nowcasting MUF map centered on Milan -========================================= +===================================== +Nowcasting MUF map centered on Milano +===================================== .. contents:: The tiny table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**Providers**: +**References** -- **INGV model** -| **Product Type**: lookup-table +Data description +~~~~~~~~~~~~~~~~ -| **Status**: Inactive +**internal_name:** ingv_ncmuf_milan_tableset -| **Creation date**: 2022-04-26T06:26:08+00:00 +**publisher:** INGV -| **Last Update**: 2023-10-01T12:00:00+02:00 +**alphanumeric_code:** 28G -Data Description -~~~~~~~~~~~~~~~~ +**id_tmp:** 29 + +**short_name:** NCMUFMilano + +**identifier:** aspis://ingv/ncmuf_milano_tableset + +**dynamic:** The map is a nowcasting map, generated every 15 minutes. + +**size:** 1MB + +**format:** png,dat + +**type:** tableset + +**records_number:** 192 + +**time_start:** 2017-09-07 + +**time_stop:** 2017-09-08 + +**spatial:** IONO + +**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere + +**spectral_min:** -| **Data type**: image +**spectral_max:** -| **Data formats**: - png +**spectral_units:** +**observable:** -| **Sample**: https://drive.google.com/file/d/1fFM0mShvAoHlf_HlOVh7rjvQ5Ai5dyV3/view?usp=sharing +**latest update:** 2024-03-28 05:08:13 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of sounding + * - 2 + - Lat + - deg + - float + - latitude + * - 3 + - Long + - deg + - float + - longitude + * - 4 + - site + - char + - char + - site name + * - 5 + - data_name + - char + - char + - dataset filename + * - 6 + - prew_name + - char + - char + - image filename + * - 7 + - thumb_name + - char + - char + - thumbnail filename diff --git a/docs/source/products/data/ingv_ncmuf_rome_tableset.rst b/docs/source/products/data/ingv_ncmuf_rome_tableset.rst index 32c22ea..acf8ec2 100644 --- a/docs/source/products/data/ingv_ncmuf_rome_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_rome_tableset.rst @@ -1,38 +1,103 @@ -========================================= -INGV Nowcasting MUF map centered on Rome -========================================= +=================================== +Nowcasting MUF map centered on Roma +=================================== .. contents:: The tiny table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**Providers**: +**References** -- **INGV model** -| **Product Type**: lookup-table +Data description +~~~~~~~~~~~~~~~~ -| **Status**: Inactive +**internal_name:** ingv_ncmuf_rome_tableset -| **Creation date**: 2022-04-26T06:26:08+00:00 +**publisher:** INGV -| **Last Update**: 2023-10-01T12:00:00+02:00 +**alphanumeric_code:** 28H -Data Description -~~~~~~~~~~~~~~~~ +**id_tmp:** 30 + +**short_name:** NCMUFCatania + +**identifier:** aspis://ingv/ncmuf_roma_tableset + +**dynamic:** The map is a nowcasting map, generated every 15 minutes. + +**size:** 1MB + +**format:** png,dat + +**type:** tableset + +**records_number:** 192 + +**time_start:** 2017-09-07 + +**time_stop:** 2017-09-08 + +**spatial:** IONO + +**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere + +**spectral_min:** -| **Data type**: image +**spectral_max:** -| **Data formats**: - png +**spectral_units:** +**observable:** -| **Sample**: https://drive.google.com/file/d/1reQwlgS-qA36yenYJyp9Ch8NJ_nKfjq4/view?usp=sharing +**latest update:** 2024-03-28 05:08:14 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of sounding + * - 2 + - Lat + - deg + - float + - latitude + * - 3 + - Long + - deg + - float + - longitude + * - 4 + - site + - char + - char + - site name + * - 5 + - data_name + - char + - char + - dataset filename + * - 6 + - prew_name + - char + - char + - image filename + * - 7 + - thumb_name + - char + - char + - thumbnail filename diff --git a/docs/source/products/data/ingv_ne_swarm_image.rst b/docs/source/products/data/ingv_ne_swarm_image.rst deleted file mode 100644 index faed328..0000000 --- a/docs/source/products/data/ingv_ne_swarm_image.rst +++ /dev/null @@ -1,39 +0,0 @@ -========================================= -INGV Swarm electron density maps -========================================= - -.. contents:: The tiny table of contents - -Electron density maps in quasi-dipole latitude vs magnetic local time coordinates derived from the Swarm constellation data acquired at 1 second cadence from 1 January 2014 to 31 December 2020. The output consists in three .jpg or .png files mapping electron density in polar and equatorial projections (3 images) for each of the 3 satellites of the Swarm constellation. Each map has a size of about 320 kB. The sample file attached is a map from the Swarm A satellite in the Northern hemisphere polar projection. - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Electric Field Instrument - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - .jpg/.png - - -| **Sample**: https://drive.google.com/file/d/1pXXfgoqoD5YRUo_iLFRfQ1Sdt3di2b6C/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_ne_swarm_timeseries.rst b/docs/source/products/data/ingv_ne_swarm_timeseries.rst deleted file mode 100644 index 6ad4884..0000000 --- a/docs/source/products/data/ingv_ne_swarm_timeseries.rst +++ /dev/null @@ -1,41 +0,0 @@ -=================================================== -INGV 1 Hz Swarm on track values of electron density -=================================================== - -.. contents:: The tiny table of contents - -In situ time series of electron density derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of one has a size of about 9 GB. The sample file attached is extracted from one year of data acquired by Swarm A - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Electric Field Instrument - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text file - - -| **Sample**: https://drive.google.com/file/d/1SiAElXYZ9HfAWb8IaRZslTCH-otz-5B0/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_plasma_cses_image.rst b/docs/source/products/data/ingv_plasma_cses_image.rst deleted file mode 100644 index 2502217..0000000 --- a/docs/source/products/data/ingv_plasma_cses_image.rst +++ /dev/null @@ -1,51 +0,0 @@ -================================================== -INGV CSES-01 electron density and temperature maps -================================================== - -.. contents:: The tiny table of contents - -Electron density and temperature maps in quasi-dipole latitude vs magnetic longitude derived from the CSES-01 satellite data acquired from 1 January 2019 to 30 September 2021. The output consists in four .jpg or .png files mapping electron density and temperature in equatorial projection in the dayside and the nightside (2 images for density, 2 for temperature). Each map has a size of about 200 kB. No sample file attached. - -* “FIGURE”: Statistical maps of electron density and temperature in .fits format. Maps are available at two spatial resolutions: 1x1 deg^2 (high resolution) and 5x5 deg^2 (low resolution). For practical purposes use low-resolution maps. High-resolution maps are tagged, e.g., “Ne_DAY\_…”. Low-resolution maps are tagged, e.g., “Ne_Mean_DAY\_…”. In both cases the mean value within each bin is representative of the bin itself. - -* “npy”: Statistical maps of electron density and temperature in .npy format. Maps are available at two spatial resolutions: 1x1 deg^2 (high resolution) and 5x5 deg^2 (low resolution). For practical purposes use low-resolution maps. High-resolution maps are tagged, e.g., “Ne_DAY\_…”. Low-resolution maps are tagged, e.g., “binned_5x5_Ne…_DAY…”. Maps are available with two different values representative of each bin: the mean and the median, respectively. - -References: - -* `Shen, X., Zhang, X., Yuan, S. et al. The state-of-the-art of the China Seismo-Electromagnetic Satellite mission. Sci. China Technol. Sci. 61, 634–642 (2018). https://doi.org/10.1007/s11431-018-9242-0 `_ - -* `M. Pezzopane et al., "On the Best Settings to Calculate Ionospheric Irregularity Indices From the In Situ Plasma Parameters of CSES-01," in IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, vol. 15, pp. 4058-4071, 2022, doi: 10.1109/JSTARS.2022.3170339. `_ - -* `Pignalberi, A.; Pezzopane, M.; Coco, I.; Piersanti, M.; Giannattasio, F.; De Michelis, P.; Tozzi, R.; Consolini, G. Inter-Calibration and Statistical Validation of Topside Ionosphere Electron Density Observations Made by CSES-01 Mission. Remote Sens. 2022, 14, 4679. https://doi.org/10.3390/rs14184679 `_ - -**Providers**: - -- **CSES-01** - source: - - - Langmuir Probes - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - .jpg/.png - - -| **Sample**: - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_plasma_cses_timeseries.rst b/docs/source/products/data/ingv_plasma_cses_timeseries.rst deleted file mode 100644 index 806e67d..0000000 --- a/docs/source/products/data/ingv_plasma_cses_timeseries.rst +++ /dev/null @@ -1,76 +0,0 @@ -================================================================ -INGV CSES-01 on track values of electron density and temperature -================================================================ - -.. contents:: The tiny table of contents - -Yearly and orbital data from LAP instrument onboard CSES-01 from 1 January 2019 to 30 September 2021 (based on availability of continuous data). - -Each file contains 5 columns: - -#. UTC (ISO format); - -#. Geographic Latitude (deg); - -#. Geographic Longitude (deg); - -#. electron density (m^-3); - -#. electron temperature (K) with variable sampling (1.5 Hz and 3 Hz). - -Sub-Sub-folders: - -* “csv”: Yearly and orbital .csv data. - -* “FIGURE”: Statistical maps of electron density and temperature in .fits format. Maps are available at two spatial resolutions: 1x1 deg^2 (high resolution) and 5x5 deg^2 (low resolution). For practical purposes use low-resolution maps. High-resolution maps are tagged, e.g., “Ne_DAY\_…”. Low-resolution maps are tagged, e.g., “Ne_Mean_DAY\_…”. In both cases the mean value within each bin is representative of the bin itself. - -* “nc”: Orbital netCDF data. - -* “npy”: Statistical maps of electron density and temperature in .npy format. Maps are available at two spatial resolutions: 1x1 deg^2 (high resolution) and 5x5 deg^2 (low resolution). For practical purposes use low-resolution maps. High-resolution maps are tagged, e.g., “Ne_DAY\_…”. Low-resolution maps are tagged, e.g., “binned_5x5_Ne…_DAY…”. Maps are available with two different values representative of each bin: the mean and the median, respectively. - - -References: - -* `Shen, X., Zhang, X., Yuan, S. et al. The state-of-the-art of the China Seismo-Electromagnetic Satellite mission. Sci. China Technol. Sci. 61, 634–642 (2018). https://doi.org/10.1007/s11431-018-9242-0 `_ - -* `M. Pezzopane et al., "On the Best Settings to Calculate Ionospheric Irregularity Indices From the In Situ Plasma Parameters of CSES-01," in IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, vol. 15, pp. 4058-4071, 2022, doi: 10.1109/JSTARS.2022.3170339. `_ - -* `Pignalberi, A.; Pezzopane, M.; Coco, I.; Piersanti, M.; Giannattasio, F.; De Michelis, P.; Tozzi, R.; Consolini, G. Inter-Calibration and Statistical Validation of Topside Ionosphere Electron Density Observations Made by CSES-01 Mission. Remote Sens. 2022, 14, 4679. https://doi.org/10.3390/rs14184679 `_ - - - - - -**Providers**: - -- **CSES-01 mission** - source: - - - Langmuir Probe - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text file - - -| **Sample**: https://drive.google.com/file/d/1qH3A4Ve4cBpSvwV7HUOB5009c_71c-lF/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_rodi1hz_swarm_timeseries.rst b/docs/source/products/data/ingv_rodi1hz_swarm_timeseries.rst deleted file mode 100644 index f3e0c9b..0000000 --- a/docs/source/products/data/ingv_rodi1hz_swarm_timeseries.rst +++ /dev/null @@ -1,67 +0,0 @@ -======================================================================== -INGV RODI ionospheric index time series at 1Hz from ESA Swarm satellites -======================================================================== - -.. contents:: The tiny table of contents - -Time series of RODI (Rate Of change of electron Density Index) ionospheric index, as derived by in-situ electron density observations from the ESA Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2020. Along with RODI values, time and position of the satellite, flags, and some quantities related to RODI calculation are also provided. - -Data for ionospheric indices calculation are collected by the ESA Swarm satellites mission. Swarm is a constellation constituted by three low-Earth-orbit satellites launched at the end of 2013, and still operating, in a circular near-polar orbit. Two of them (Swarm A and C) have the same orbit configuration (inclination of 87.4°, initial altitude of about 460 km, east-west separation of about 1°–1.5° in longitude). The third (Swarm B) has a different orbital configuration (inclination of 88°, initial altitude of about 520 km) compared to the couple Swarm A and C. In-situ electron density (Ne) and electron temperature (Te) observations are collected by Langmuir Probes (LP). Precise Orbit Determination (POD) antennas are GPS receivers from which the TEC is determined, both vertical and slant, for each GPS satellite in view. Swarm’s data are freely downloadable at ftp://swarm-diss.eo.esa.int. - -**References:** - -De Michelis et al. (2020), Journal of Geophysical Research: Space Physics, 125, e2020JA027934. https://doi.org/10.1029/2020JA027934 - -De Michelis, et al. (2021a), Remote Sensing, 13, 759. https://doi.org/10.3390/rs13040759 - -De Michelis, et al. (2021b), Scientific Reports, 11, 6183, https://doi.org/10.1038/s41598-021-84985-1 - -De Michelis et al. (2022), Remote Sensing, 14, 918. https://doi.org/10.3390/rs14040918 - -Pignalberi (2021), Computers and Geosciences, 48, 104675, https://doi.org/10.1016/j.cageo.2020.104675 - -Pignalberi et al. (2021), Universe, 7, 290. https://doi.org/10.3390/universe7080290 - - - - - -**Providers**: - -- **Swarm A satellite** - source: - - - ESA Swarm A Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ -- **Swarm B satellite** - source: - - - ESA Swarm B Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ -- **Swarm C satellite** - source: - - - ESA Swarm C Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text files - - -| **Sample**: https://drive.google.com/file/d/1sSHMySdvBr5zZmr_sXx9qF9c5xA7elAv/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_rodi_swarm_image.rst b/docs/source/products/data/ingv_rodi_swarm_image.rst deleted file mode 100644 index 7876c40..0000000 --- a/docs/source/products/data/ingv_rodi_swarm_image.rst +++ /dev/null @@ -1,61 +0,0 @@ -================================================================= -INGV RODI ionospheric index global maps from ESA Swarm satellites -================================================================= - -.. contents:: The tiny table of contents - -Global maps of RODI (Rate Of change of electron Density Index) ionospheric index, as derived by in-situ electron density observation from the Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2020. - -Data for ionospheric indices calculation are collected by the ESA Swarm satellites mission. Swarm is a constellation constituted by three low-Earth-orbit satellites launched at the end of 2013, and still operating, in a circular near-polar orbit. Two of them (Swarm A and C) have the same orbit configuration (inclination of 87.4°, initial altitude of about 460 km, east-west separation of about 1°–1.5° in longitude). The third (Swarm B) has a different orbital configuration (inclination of 88°, initial altitude of about 520 km) compared to the couple Swarm A and C. In-situ electron density (Ne) and electron temperature (Te) observations are collected by Langmuir Probes (LP). Precise Orbit Determination (POD) antennas are GPS receivers from which the TEC is determined, both vertical and slant, for each GPS satellite in view. Swarm’s data are freely downloadable at ftp://swarm-diss.eo.esa.int. - -**References:** - -De Michelis et al. (2020), Journal of Geophysical Research: Space Physics, 125, e2020JA027934. https://doi.org/10.1029/2020JA027934 - -De Michelis, et al. (2021a), Remote Sensing, 13, 759. https://doi.org/10.3390/rs13040759 - -De Michelis, et al. (2021b), Scientific Reports, 11, 6183, https://doi.org/10.1038/s41598-021-84985-1 - -De Michelis et al. (2022), Remote Sensing, 14, 918. https://doi.org/10.3390/rs14040918 - -Pignalberi (2021), Computers and Geosciences, 48, 104675, https://doi.org/10.1016/j.cageo.2020.104675 - -Pignalberi et al. (2021), Universe, 7, 290. https://doi.org/10.3390/universe7080290 - -**Providers**: - -- **Swarm A satellite** - source: - - - ESA Swarm A Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ -- **Swarm B satellite** - source: - - - ESA Swarm B Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ -- **Swarm C satellite** - source: - - - ESA Swarm C Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - png - - -| **Sample**: https://drive.google.com/file/d/1vDuwPL6J03bQawISvTZWKhmXD0MjgX60/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_rotei1hz_swarm_timeseries.rst b/docs/source/products/data/ingv_rotei1hz_swarm_timeseries.rst deleted file mode 100644 index 6043b1d..0000000 --- a/docs/source/products/data/ingv_rotei1hz_swarm_timeseries.rst +++ /dev/null @@ -1,64 +0,0 @@ -========================================================================= -INGV ROTEI ionospheric index time series at 1Hz from ESA Swarm satellites -========================================================================= - -.. contents:: The tiny table of contents - -Time series of ROTEI (Rate Of change of electron TEmperature Index) ionospheric index, as derived by in-situ electron temperature observations from the ESA Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2020. Along with ROTEI values, time and position of the satellite, flags, and some quantities related to ROTEI calculation are also provided. - -Data for ionospheric indices calculation are collected by the ESA Swarm satellites mission. Swarm is a constellation constituted by three low-Earth-orbit satellites launched at the end of 2013, and still operating, in a circular near-polar orbit. Two of them (Swarm A and C) have the same orbit configuration (inclination of 87.4°, initial altitude of about 460 km, east-west separation of about 1°–1.5° in longitude). The third (Swarm B) has a different orbital configuration (inclination of 88°, initial altitude of about 520 km) compared to the couple Swarm A and C. In-situ electron density (Ne) and electron temperature (Te) observations are collected by Langmuir Probes (LP). Precise Orbit Determination (POD) antennas are GPS receivers from which the TEC is determined, both vertical and slant, for each GPS satellite in view. Swarm’s data are freely downloadable at ftp://swarm-diss.eo.esa.int. - -**References:** - -De Michelis et al. (2020), Journal of Geophysical Research: Space Physics, 125, e2020JA027934. https://doi.org/10.1029/2020JA027934 - -De Michelis, et al. (2021a), Remote Sensing, 13, 759. https://doi.org/10.3390/rs13040759 - -De Michelis, et al. (2021b), Scientific Reports, 11, 6183, https://doi.org/10.1038/s41598-021-84985-1 - -De Michelis et al. (2022), Remote Sensing, 14, 918. https://doi.org/10.3390/rs14040918 - -Pignalberi (2021), Computers and Geosciences, 48, 104675, https://doi.org/10.1016/j.cageo.2020.104675 - -Pignalberi et al. (2021), Universe, 7, 290. https://doi.org/10.3390/universe7080290 - - -**Providers**: - -- **Swarm A satellite** - source: - - - ESA Swarm A Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ -- **Swarm B satellite** - source: - - - ESA Swarm B Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ -- **Swarm C satellite** - source: - - - ESA Swarm C Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text files - - -| **Sample**: https://drive.google.com/file/d/1R6ssT78KgLLBwxsEMGRWqNcLdGlLF3aY/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_rotei_swarm_image.rst b/docs/source/products/data/ingv_rotei_swarm_image.rst deleted file mode 100644 index ea64b38..0000000 --- a/docs/source/products/data/ingv_rotei_swarm_image.rst +++ /dev/null @@ -1,62 +0,0 @@ -================================================================== -INGV ROTEI ionospheric index global maps from ESA Swarm satellites -================================================================== - -.. contents:: The tiny table of contents - -Global maps of ROTEI (Rate Of change of electron TEmperature Index) ionospheric index, as derived by in-situ electron temperature observations from the Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2020. - -Data for ionospheric indices calculation are collected by the ESA Swarm satellites mission. Swarm is a constellation constituted by three low-Earth-orbit satellites launched at the end of 2013, and still operating, in a circular near-polar orbit. Two of them (Swarm A and C) have the same orbit configuration (inclination of 87.4°, initial altitude of about 460 km, east-west separation of about 1°–1.5° in longitude). The third (Swarm B) has a different orbital configuration (inclination of 88°, initial altitude of about 520 km) compared to the couple Swarm A and C. In-situ electron density (Ne) and electron temperature (Te) observations are collected by Langmuir Probes (LP). Precise Orbit Determination (POD) antennas are GPS receivers from which the TEC is determined, both vertical and slant, for each GPS satellite in view. Swarm’s data are freely downloadable at ftp://swarm-diss.eo.esa.int. - -**References:** - -De Michelis et al. (2020), Journal of Geophysical Research: Space Physics, 125, e2020JA027934. https://doi.org/10.1029/2020JA027934 - -De Michelis, et al. (2021a), Remote Sensing, 13, 759. https://doi.org/10.3390/rs13040759 - -De Michelis, et al. (2021b), Scientific Reports, 11, 6183, https://doi.org/10.1038/s41598-021-84985-1 - -De Michelis et al. (2022), Remote Sensing, 14, 918. https://doi.org/10.3390/rs14040918 - -Pignalberi (2021), Computers and Geosciences, 48, 104675, https://doi.org/10.1016/j.cageo.2020.104675 - -Pignalberi et al. (2021), Universe, 7, 290. https://doi.org/10.3390/universe7080290 - - -**Providers**: - -- **Swarm A satellite** - source: - - - ESA Swarm A Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ -- **Swarm B satellite** - source: - - - ESA Swarm B Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ -- **Swarm C satellite** - source: - - - ESA Swarm C Electric Field Instrument - Langmuir Probe, https://swarm-diss.eo.esa.int/ - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - text files - - -| **Sample**: https://drive.google.com/file/d/1Nwy-7S5zlhHRQfUyhcYvBxUkiJr5xF4d/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_roti1hz_swarm_timeseries.rst b/docs/source/products/data/ingv_roti1hz_swarm_timeseries.rst deleted file mode 100644 index 8bc6c2e..0000000 --- a/docs/source/products/data/ingv_roti1hz_swarm_timeseries.rst +++ /dev/null @@ -1,66 +0,0 @@ -====================================================================================== -INGV ROTI ionospheric index time series at 1Hz from ESA Swarm satellites (A, B, and C) -====================================================================================== - -.. contents:: The tiny table of contents - -Time series of ROTI (Rate Of change of Total electron content Index) ionospheric index, as derived by total electron content observations from the Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2021, for each of the 32 GPS satellites. Along with ROTI values, time and position of the satellite, flags, and some quantities related to ROTI calculation are also provided. - -Data for ionospheric indices calculation are collected by the ESA Swarm satellites mission. Swarm is a constellation constituted by three low-Earth-orbit satellites launched at the end of 2013, and still operating, in a circular near-polar orbit. Two of them (Swarm A and C) have the same orbit configuration (inclination of 87.4°, initial altitude of about 460 km, east-west separation of about 1°–1.5° in longitude). The third (Swarm B) has a different orbital configuration (inclination of 88°, initial altitude of about 520 km) compared to the couple Swarm A and C. In-situ electron density (Ne) and electron temperature (Te) observations are collected by Langmuir Probes (LP). Precise Orbit Determination (POD) antennas are GPS receivers from which the TEC is determined, both vertical and slant, for each GPS satellite in view. Swarm’s data are freely downloadable at ftp://swarm-diss.eo.esa.int. - -**References:** - -De Michelis et al. (2020), Journal of Geophysical Research: Space Physics, 125, e2020JA027934. https://doi.org/10.1029/2020JA027934 - -De Michelis, et al. (2021a), Remote Sensing, 13, 759. https://doi.org/10.3390/rs13040759 - -De Michelis, et al. (2021b), Scientific Reports, 11, 6183, https://doi.org/10.1038/s41598-021-84985-1 - -De Michelis et al. (2022), Remote Sensing, 14, 918. https://doi.org/10.3390/rs14040918 - -Pignalberi (2021), Computers and Geosciences, 48, 104675, https://doi.org/10.1016/j.cageo.2020.104675 - -Pignalberi et al. (2021), Universe, 7, 290. https://doi.org/10.3390/universe7080290 - - - - -**Providers**: - -- **Swarm A satellite** - source: - - - ESA Swarm A Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ -- **Swarm B satellite** - source: - - - ESA Swarm B Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ -- **Swarm C satellite** - source: - - - ESA Swarm C Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text files - - -| **Sample**: https://drive.google.com/file/d/1k649G6k1RrBaK4BGl-hwJXvMyJ5GoDcN/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_roti_swarm_image.rst b/docs/source/products/data/ingv_roti_swarm_image.rst deleted file mode 100644 index 275a2c0..0000000 --- a/docs/source/products/data/ingv_roti_swarm_image.rst +++ /dev/null @@ -1,62 +0,0 @@ -================================================================= -INGV ROTI ionospheric index global maps from ESA Swarm satellites -================================================================= - -.. contents:: The tiny table of contents - -Global maps of ROTI (Rate Of change of Total electron content Index) ionospheric index, as derived by total electron content observations from the Swarm satellites (A, B, and C) at 1Hz rate, from 1 January 2014 to 31 December 2020. - -Data for ionospheric indices calculation are collected by the ESA Swarm satellites mission. Swarm is a constellation constituted by three low-Earth-orbit satellites launched at the end of 2013, and still operating, in a circular near-polar orbit. Two of them (Swarm A and C) have the same orbit configuration (inclination of 87.4°, initial altitude of about 460 km, east-west separation of about 1°–1.5° in longitude). The third (Swarm B) has a different orbital configuration (inclination of 88°, initial altitude of about 520 km) compared to the couple Swarm A and C. In-situ electron density (Ne) and electron temperature (Te) observations are collected by Langmuir Probes (LP). Precise Orbit Determination (POD) antennas are GPS receivers from which the TEC is determined, both vertical and slant, for each GPS satellite in view. Swarm’s data are freely downloadable at ftp://swarm-diss.eo.esa.int. - -**References:** - -De Michelis et al. (2020), Journal of Geophysical Research: Space Physics, 125, e2020JA027934. https://doi.org/10.1029/2020JA027934 - -De Michelis, et al. (2021a), Remote Sensing, 13, 759. https://doi.org/10.3390/rs13040759 - -De Michelis, et al. (2021b), Scientific Reports, 11, 6183, https://doi.org/10.1038/s41598-021-84985-1 - -De Michelis et al. (2022), Remote Sensing, 14, 918. https://doi.org/10.3390/rs14040918 - -Pignalberi (2021), Computers and Geosciences, 48, 104675, https://doi.org/10.1016/j.cageo.2020.104675 - -Pignalberi et al. (2021), Universe, 7, 290. https://doi.org/10.3390/universe7080290 - - -**Providers**: - -- **Swarm A satellite** - source: - - - ESA Swarm A Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ -- **Swarm B satellite** - source: - - - ESA Swarm B Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ -- **Swarm C satellite** - source: - - - ESA Swarm C Precise Orbit Determination (POD) antenna, https://swarm-diss.eo.esa.int/ - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - text files - - -| **Sample**: https://drive.google.com/file/d/1g1HI_eMy4ZQHtCoyxHu1j3mEYINe5xlY/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_sigma_swarm_image.rst b/docs/source/products/data/ingv_sigma_swarm_image.rst deleted file mode 100644 index b8430da..0000000 --- a/docs/source/products/data/ingv_sigma_swarm_image.rst +++ /dev/null @@ -1,47 +0,0 @@ -================================================ -INGV Swarm parallel electrical conductivity maps -================================================ - -.. contents:: The tiny table of contents - -Parallel electrical conductivity maps from LP instruments onboard the Swarm constellation (Alpha, Bravo and Charlie satellites) obtained from data between 1 January 2014 and 31 December 2022. - -**References:** - -* `F. Giannattasio, P. De Michelis, A. Pignalberi, I. Coco, G. Consolini, M. Pezzopane, R. Tozzi, Parallel Electrical Conductivity in the Topside Ionosphere Derived From Swarm Measurements, JGR Space Physics, Volume126, Issue2 February 2021, https://doi.org/10.1029/2020JA028452 `_ - -* `F. Giannattasio, A. Pignalberi, P. De Michelis, I. Coco, G. Consolini, M. Pezzopane, R. Tozzi, Dependence of Parallel Electrical Conductivity in the Topside Ionosphere on Solar and Geomagnetic Activity, JGR Space Physics, Volume126, Issue6 June 2021, https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2021JA029138 `_ - - - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Electric Field Instrument - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - .jpg/.png - - -| **Sample**: https://drive.google.com/file/d/14AktJhqFyzBtUKL2HHP9lk4jg5iwHsZF/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_sigma_swarm_timeseries.rst b/docs/source/products/data/ingv_sigma_swarm_timeseries.rst deleted file mode 100644 index 4c0441e..0000000 --- a/docs/source/products/data/ingv_sigma_swarm_timeseries.rst +++ /dev/null @@ -1,41 +0,0 @@ -=================================================================== -INGV 1 Hz Swarm on track values of parallel electrical conductivity -=================================================================== - -.. contents:: The tiny table of contents - -In situ time series of parallel electrical conductivity derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of which has a size of about 12 GB. The sample file attached is extracted from one month of data acquired by Swarm A - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Electric Field Instrument - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text file - - -| **Sample**: https://drive.google.com/file/d/1tTE0N9t2gWYGR-lUR_GyypyMAaFZoBVZ/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_te_swarm_image.rst b/docs/source/products/data/ingv_te_swarm_image.rst deleted file mode 100644 index f85252c..0000000 --- a/docs/source/products/data/ingv_te_swarm_image.rst +++ /dev/null @@ -1,39 +0,0 @@ -==================================== -INGV Swarm electron temperature maps -==================================== - -.. contents:: The tiny table of contents - -Electron temperature maps in quasi-dipole latitude vs magnetic local time coordinates derived from the Swarm constellation data acquired at 1 second cadence from 1 January 2014 to 31 December 2020. The output consists in three .jpg or .png files mapping electron temperature in polar and equatorial projections (3 images) for each of the 3 satellites of the Swarm constellation. Each map has a size of about 280 kB. The sample file attached is a map from the Swarm A satellite in the Northern hemisphere polar projection. - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Electric Field Instrument - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - .jpg/.png - - -| **Sample**: https://drive.google.com/file/d/1BfHVrah0MI3DrvZ-wTc_BfgVAP240vJn/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_te_swarm_timeseries.rst b/docs/source/products/data/ingv_te_swarm_timeseries.rst deleted file mode 100644 index 23d5320..0000000 --- a/docs/source/products/data/ingv_te_swarm_timeseries.rst +++ /dev/null @@ -1,41 +0,0 @@ -======================================================= -INGV 1 Hz Swarm on track values of electron temperature -======================================================= - -.. contents:: The tiny table of contents - -In situ time series of electron temperature derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of one has a size of about 9 GB. The sample file attached is extracted from one year of data acquired by Swarm A - -**Providers**: - -- **ESA's Swarm constellation** - source: - - - Electric Field Instrument - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-13T16:16:20+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text file - - -| **Sample**: https://drive.google.com/file/d/1_QoiKXfcSwFcnQ1yLvu-bsQWZ16vBC7k/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst b/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst index 1f0e8c2..ed243cc 100644 --- a/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst +++ b/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst @@ -1,48 +1,143 @@ -========================================= -INGV Validated data Gibilmanna Ionosonde -========================================= +=================================== +Validated data Gibilmanna Ionosonde +=================================== .. contents:: The tiny table of contents Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna -**Providers**: +**References** -- **AIS-INGV ionosonde** -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-22T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1u62OdH0NV_ZSV_FN9wyfTjuSwJRldPKu/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- http://ws-eswua.rm.ingv.it/ais.\php/records/gm037_rev: Web service endpoint -- int2130.1: Product ingestion -- int2130.3: Mirroring: bulk static - +**internal_name:** ingv_valiiono_gibi_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 13A + +**id_tmp:** 31 + +**short_name:** ValiIonoGibi + +**identifier:** aspis://ingv/valiiono_gibi_timeseries + +**dynamic:** The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 1463 + +**time_start:** 2012-03-07 + +**time_stop:** 2015-06-30 + +**spatial:** IONO + +**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** + +**latest update:** 2024-03-28 05:08:14 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of the sounding + * - 2 + - Geo_Lat + - deg + - float + - latitude + * - 3 + - Geo_Lon + - deg + - float + - longitude + * - 4 + - foF2 + - MHz + - float + - (MHz) maximum frequency reflected by the F2 layer + * - 5 + - muf3000f2 + - MHz + - float + - (MHz) maximum usable frequency for a distance of 3000 km centered over the ionosonde site + * - 6 + - m3000f2 + - dimensionless + - float + - (adimensional) propagation factor + * - 7 + - fof1 + - MHz + - float + - (MHz) maximum frequency reflected by the F1 layer + * - 8 + - h_f2 + - km + - integer + - (km) virtual height of the F2 layer + * - 9 + - h_f + - km + - integer + - (km) virtual height of the F2 region + * - 10 + - h_e + - km + - integer + - (km) virtual height of the E region + * - 11 + - foe + - MHz + - float + - (MHz) maximum frequency reflected by the E layer + * - 12 + - h_es + - km + - integer + - (km) virtual height of the sporadic E layer + * - 13 + - foes + - MHz + - float + - (MHz) maximum frequency reflected by the sporadic E layer + * - 14 + - fbes + - MHz + - float + - (MHz) blanketing frequency of the sporadic E layer + * - 15 + - fmin + - MHz + - float + - (MHz) minimum frequency reflected by the ionosphere diff --git a/docs/source/products/data/ingv_valiiono_rome_timeseries.rst b/docs/source/products/data/ingv_valiiono_rome_timeseries.rst index b0a1d81..2b46496 100644 --- a/docs/source/products/data/ingv_valiiono_rome_timeseries.rst +++ b/docs/source/products/data/ingv_valiiono_rome_timeseries.rst @@ -1,48 +1,143 @@ -========================================= -INGV Validated data Rome Ionosonde -========================================= +============================= +Validated data Rome Ionosonde +============================= .. contents:: The tiny table of contents Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Rome -**Providers**: +**References** -- **AIS-INGV ionosonde** -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-22T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/14Z8q5lhjzQMjxJiy8YG9vqwL4SQaKDdl/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- http://ws-eswua.rm.ingv.it/ais.\php/records/rm041_rev: Web service endpoint -- int2130.1: Product ingestion -- int2130.3: Mirroring: bulk static - +**internal_name:** ingv_valiiono_rome_timeseries + +**publisher:** INGV + +**alphanumeric_code:** 13B + +**id_tmp:** 32 + +**short_name:** ValiIonoRome + +**identifier:** aspis://ingv/valiiono_rome_timeseries + +**dynamic:** The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated + +**size:** 10MB + +**format:** csv + +**type:** timeseries + +**records_number:** 1727 + +**time_start:** 2012-03-07 + +**time_stop:** 2017-09-15 + +**spatial:** IONO + +**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** + +**latest update:** 2024-03-28 05:08:14 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time of the sounding + * - 2 + - Geo_Lat + - deg + - float + - latitude + * - 3 + - Geo_Lon + - deg + - float + - longitude + * - 4 + - foF2 + - MHz + - float + - (MHz) maximum frequency reflected by the F2 layer + * - 5 + - muf3000f2 + - MHz + - float + - (MHz) maximum usable frequency for a distance of 3000 km centered over the ionosonde site + * - 6 + - m3000f2 + - dimensionless + - float + - (adimensional) propagation factor + * - 7 + - fof1 + - MHz + - float + - (MHz) maximum frequency reflected by the F1 layer + * - 8 + - h_f2 + - km + - integer + - (km) virtual height of the F2 layer + * - 9 + - h_F + - km + - integer + - (km) virtual height of the F2 region + * - 10 + - h_e + - km + - integer + - (km) virtual height of the E region + * - 11 + - foe + - MHz + - float + - (MHz) maximum frequency reflected by the E layer + * - 12 + - h_es + - km + - integer + - (km) virtual height of the sporadic E layer + * - 13 + - foes + - MHz + - float + - (MHz) maximum frequency reflected by the sporadic E layer + * - 14 + - fbes + - MHz + - float + - (MHz) blanketing frequency of the sporadic E layer + * - 15 + - fmin + - MHz + - float + - (MHz) minimum frequency reflected by the ionosphere diff --git a/docs/source/products/data/uniaq_curr_maigic_image.rst b/docs/source/products/data/uniaq_curr_maigic_image.rst deleted file mode 100644 index 2fbc4fb..0000000 --- a/docs/source/products/data/uniaq_curr_maigic_image.rst +++ /dev/null @@ -1,44 +0,0 @@ -======================================================================= -UNIAQ Magnetospheric-Ionospheric-Gound Induced Current model - currents -======================================================================= - -.. contents:: The tiny table of contents - -The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. -To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. - - -**Providers**: - -- **Ground magnetometer data** - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-19T18:00:27+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - .pdf - - -| **Sample**: `sample ` - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.5: On demand computation -- ext2230.1: Advanced Visualisation: ASPIS.py - diff --git a/docs/source/products/data/uniaq_curr_maigic_tableset.rst b/docs/source/products/data/uniaq_curr_maigic_tableset.rst index 138203b..3fe7a42 100644 --- a/docs/source/products/data/uniaq_curr_maigic_tableset.rst +++ b/docs/source/products/data/uniaq_curr_maigic_tableset.rst @@ -1,44 +1,123 @@ -======================================================================== -UNIAQ Magnetospheric-Ionospheric-Ground Induced Current model - currents -======================================================================== +================================================================== +Magnetospheric-Ionospheric-Ground Induced Current model - currents +================================================================== .. contents:: The tiny table of contents -The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. -To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. +The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. +**References** -**Providers**: -- **Ground magnetometer data** - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-19T18:00:27+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - .mat - - -| **Sample**: https://drive.google.com/file/d/1-r3xmlIn9n8bDpwr3LE071uB-9utQlDF/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.5: On demand computation -- ext2230.1: Advanced Visualisation: ASPIS.py - +**internal_name:** uniaq_curr_maigic_tableset + +**publisher:** Mirko Piersanti + +**alphanumeric_code:** 40B + +**id_tmp:** 86 + +**short_name:** MA.I.GIC. current + +**identifier:** aspis://uniaq//curr_maigic_tableset + +**dynamic:** Static and depending on the length of the input data + +**size:** 5MB + +**format:** .mat + +**type:** tableset + +**records_number:** 8641 + +**time_start:** 2021-04-12 + +**time_stop:** 2021-04-13 + +**spatial:** GEOMAG + +**messenger:** magnetic field + +**spectral_min:** 0 + +**spectral_max:** 0 + +**spectral_units:** 0 + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:14 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - Time (2022-09-14T03:00:03) - UTC Time + * - 2 + - GEI_lon + - deg + - float + - Geographic Longitude (deg) + * - 3 + - GEI_lat + - deg + - float + - Geographic Latitude (deg) + * - 4 + - year + - year + - int + - no description + * - 5 + - month + - month + - int + - no description + * - 6 + - day + - day + - int + - no description + * - 7 + - hour + - hour + - int + - no description + * - 8 + - min + - min + - int + - no description + * - 9 + - sec + - sec + - int + - no description + * - 10 + - GICN + - mV/km + - float + - geomagnetically induced current N (mV/km) + * - 11 + - GICE + - mV/km + - float + - geomagnetically induced current E (mV/km) diff --git a/docs/source/products/data/uniaq_epmde_emma_timeseries.rst b/docs/source/products/data/uniaq_epmde_emma_timeseries.rst index 497f227..72509e5 100644 --- a/docs/source/products/data/uniaq_epmde_emma_timeseries.rst +++ b/docs/source/products/data/uniaq_epmde_emma_timeseries.rst @@ -1,38 +1,113 @@ -============================================================== -UNIAQ Equatorial Plasma Mass Density estimates in Plasmasphere -============================================================== +======================================================== +Equatorial Plasma Mass Density estimates in Plasmasphere +======================================================== .. contents:: The tiny table of contents Equatorial plasma mass density estimates in plasmasphere (2 < L < 6) are derived from the the EMMA magnetometers network, updated every 15 minutes. -**Providers**: +**References** -- **EMMA Network** -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-05-07T10:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1ORb-g1JGbSmf0h0IbzkMXnWQgwV3aSvb/view?usp=share_link - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion - +**internal_name:** uniaq_epmde_emma_timeseries + +**publisher:** University of L'Aquila Dept. of Physical and Chemical Sciences + +**alphanumeric_code:** 29 + +**id_tmp:** 33 + +**short_name:** EPMDP-Estimates + +**identifier:** aspis:///uniaq/epmdp + +**dynamic:** Static + +**size:** 200kB + +**format:** csv + +**type:** timeseries + +**records_number:** 1951 + +**time_start:** 2022-01-01 + +**time_stop:** 2023-12-21 + +**spatial:** GEOMAG + +**messenger:** MHD waves + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** ESP + +**latest update:** 2024-03-28 05:08:14 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC time of the estimation in the format YYYY-MM-DDThh:mm:ss + * - 2 + - gsm_lat + - deg + - float + - The latitude of the position of the magnetic field line foot used for the estimation in the geocentric solar magnetic (GSM) reference frame + * - 3 + - gsm_lon + - deg + - float + - The longitude of the position of the magnetic field line foot used for the estimation in the geocentric solar magnetic (GSM) reference frame + * - 4 + - gsm_z + - m + - float + - The radial distance (meters) from the Earth's center of the magnetic field line foot used for the estimation in the geocentric solar magnetic (GSM) reference frame + * - 5 + - rho_si + - Kg/m^3 + - float + - Estimation of the plasmaspheric mass density in Kg/m^3 (SI) + * - 6 + - rho + - amu/cc + - float + - Estimation of the plasmaspheric mass density in amu/cc + * - 7 + - distance + - R_E + - float + - The radial distance (Earth radii) from the Earth's center of the magnetic field line foot used for the estimation in the geocentric solar magnetic (GSM) reference frame + * - 8 + - lt + - hour + - float + - Local Time in fraction of hours of the day + * - 9 + - mlt + - hour + - float + - Magnetic Local Time in fraction of hours of the day diff --git a/docs/source/products/data/uniaq_field_maigic_image.rst b/docs/source/products/data/uniaq_field_maigic_image.rst deleted file mode 100644 index 51db6d0..0000000 --- a/docs/source/products/data/uniaq_field_maigic_image.rst +++ /dev/null @@ -1,46 +0,0 @@ -================================================================================= -UNIAQ Magnetospheric-Ionospheric-Ground Induced Current model - Geoelectric Field -================================================================================= - -.. contents:: The tiny table of contents - -The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. -To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. - - -**Providers**: - -- **Ground magnetometer data** - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-19T18:00:27+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - .fig - - -| **Sample**: https://drive.google.com/file/d/1De2kR3bGaJJGDQ55VXPLKDYtC6mqIHbd/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.5: On demand computation -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/uniaq_field_maigic_tableset.rst b/docs/source/products/data/uniaq_field_maigic_tableset.rst index d87cc8a..0838e28 100644 --- a/docs/source/products/data/uniaq_field_maigic_tableset.rst +++ b/docs/source/products/data/uniaq_field_maigic_tableset.rst @@ -1,46 +1,128 @@ -================================================================================= -UNIAQ Magnetospheric-Ionospheric-Ground Induced Current model - Geoelectric Field -================================================================================= +========================================================================== +Magnetospheric-Ionospheric-Gound Induced Current model - Geoelectric Field +========================================================================== .. contents:: The tiny table of contents -The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. -To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. +The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. +**References** -**Providers**: -- **Ground magnetometer data** - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-19T18:00:27+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - .mat - - -| **Sample**: https://drive.google.com/file/d/1AGdix2SXqN5sXaisH3FXPPi0vXKsjWdz/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.5: On demand computation -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** uniaq_field_maigic_tableset + +**publisher:** Mirko Piersanti + +**alphanumeric_code:** 41B + +**id_tmp:** 87 + +**short_name:** MA.I.GIC. Geoelectric Field + +**identifier:** aspis:///univaq/field_maigic_tableset + +**dynamic:** Static and depending on the length of the input data + +**size:** 5MB + +**format:** .mat + +**type:** tableset + +**records_number:** 8641 + +**time_start:** 2021-04-12 + +**time_stop:** 2021-04-13 + +**spatial:** GEOMAG + +**messenger:** Electric Field + +**spectral_min:** 0 + +**spectral_max:** 0 + +**spectral_units:** 0 + +**observable:** GIC,GEOINDEX + +**latest update:** 2024-03-28 05:08:14 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - Time (2022-09-14T03:00:03) - UTC Time + * - 2 + - GEI_lon + - deg + - float + - Geographic Longitude (deg) + * - 3 + - GEI_lat + - deg + - float + - Geographic Latitude (deg) + * - 4 + - year + - year + - int + - no description + * - 5 + - month + - month + - int + - no description + * - 6 + - day + - day + - int + - no description + * - 7 + - hour + - hour + - int + - no description + * - 8 + - min + - min + - int + - no description + * - 9 + - sec + - sec + - int + - no description + * - 10 + - HF_component + - nT + - float + - the high-frequency contribution (nT) + * - 11 + - Iono_component + - nT + - float + - the ionospheric contribution (nT) + * - 12 + - Magn_component + - nT + - float + - the magnetospheric contribution (nT) diff --git a/docs/source/products/data/uniaq_mag_emma_timeseries.rst b/docs/source/products/data/uniaq_mag_emma_timeseries.rst index 26c6dcc..3fbc633 100644 --- a/docs/source/products/data/uniaq_mag_emma_timeseries.rst +++ b/docs/source/products/data/uniaq_mag_emma_timeseries.rst @@ -1,67 +1,123 @@ -========================================= -UNIAQ EMMA Geomagnetic field data -========================================= +=========================== +EMMA Geomagnetic field data +=========================== .. contents:: The tiny table of contents 1-minute averages of the magnetic field variations recorded at 27 ground stations located in Italy and Europe along a meridional chain covering a large range in geographical latitude (from 70 to 42 degrees). The data are automatically collected in near real-time and updated every 15 minutes. -**Providers**: - -- **EMMA - European quasi-Meridional Magnetometer Array** - sources: - - - Masi (MAS) Station - Finnish Meteorological Institute (FMI) - - Kevo (KEV) Station - Finnish Meteorological Institute (FMI) - - Kilpisjärvi (KIL) Station - Finnish Meteorological Institute (FMI) - - Ivalo (IVA) Station - Finnish Meteorological Institute (FMI) - - Muonio (MUO) Station - Finnish Meteorological Institute (FMI) - - Sodankylä (SOD) Station - Sodankylä Geophysical Observatory (SGO) - - Pello (PEL) Station - Finnish Meteorological Institute (FMI) - - Ranua (RAN) Station - Finnish Meteorological Institute (FMI) - - Oulujärvi (OUJ) Station - Finnish Meteorological Institute (FMI) - - Mekrijärvi (MEK) Station - Finnish Meteorological Institute (FMI) - - Hankasalmi (HAN) Station - Finnish Meteorological Institute (FMI) - - Nurmijärvi (NUR) Station - Finnish Meteorological Institute (FMI) - - Nurmijärvi (NU2) Station - Finnish Meteorological Institute (FMI) - - Tartu (TAR) Station - Finnish Meteorological Institute (FMI) - - Birzai (BRZ) Station - Institute of Geophysics Polish Academy of Sciences (IGF-PAN) - - Hel (HLP) Station - Institute of Geophysics Polish Academy of Sciences (IGF-PAN) - - Suwałki (SUW) Station - Institute of Geophysics Polish Academy of Sciences (IGF-PAN) - - Belsk (BEL) Station - Institute of Geophysics Polish Academy of Sciences (IGF-PAN) - - Polesie (PPN) Station - Institute of Geophysics Polish Academy of Sciences (IGF-PAN) - - Zagorzyce (ZAG) Station - Institute of Geophysics Polish Academy of Sciences (IGF-PAN) - - Vyhne (VYH) Station - Division of Geophysics Earth Science Institute Slovak Academy of Sciences - - Nagycenk (NCK) Station - Geodetic and Geophysical Research Institute Hungarian Academy of Sciences - - Tihany (THY) Station - Geodetic and Geophysical Research Institute Hungarian Academy of Sciences - - Castello Tesino (CST) Station - Department of Physical and Chemical Sciences University of L'Aquila - - Lonjsko Polje (LOP) Station - Geodetic and Geophysical Research Institute Hungarian Academy of Sciences - - Ranchio (RNC) Station - Department of Physical and Chemical Sciences University of L'Aquila - - L'Aquila (AQU) Station - Department of Physical and Chemical Sciences University of L'Aquila - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-05-07T09:30:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: +**References** -- json -| **Sample**: https://drive.google.com/file/d/1jsMpdfuNosno09IpvGh_MRhANASaTJ4v/view?usp=share_link - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- ext2220.1: Standard Visualisation: Web GUI +Data description +~~~~~~~~~~~~~~~~ +**internal_name:** uniaq_mag_emma_timeseries + +**publisher:** University of L'Aquila Dept. of Physical and Chemical Sciences + +**alphanumeric_code:** 10 + +**id_tmp:** 34 + +**short_name:** EMMA-data + +**identifier:** aspis://uniaq/emma + +**dynamic:** For each day, there is one master dataset containing the general information of each station and related dataset and n (maximum value 27) datasets containing the 1-minute averages of the individual stations. + +**size:** 2MB + +**format:** csv + +**type:** tableset + +**records_number:** 277 + +**time_start:** 2022-01-01 + +**time_stop:** 2023-12-21 + +**spatial:** GROUND + +**messenger:** MHD waves + +**spectral_min:** 0 + +**spectral_max:** 0 + +**spectral_units:** + +**observable:** GLE + +**latest update:** 2024-03-28 05:08:15 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - Initial UTC time of the dataset in the format YYYY-MM-DDThh:mm:ss + * - 2 + - Code + - - + - string + - The code of the station (three capital letters according the the INTERMAGNET standards) + * - 3 + - filename + - - + - string + - name of the station dataset + * - 4 + - Reference Frame + - - + - string + - coordinate system used to record geomagnetic field values + * - 5 + - data ratio + - - + - float + - valid data percentage in a daily dataset + * - 6 + - var_1 + - pT + - float + - range of variation of component 1 of the geomagnetic field computed on the whole period + * - 7 + - STD_1 + - pT + - float + - standard deviation of component 1 of the geomagnetic field variations computed on the whole period + * - 8 + - var_2 + - pT + - float + - range of variation of component 2 of the geomagnetic field computed on the whole period + * - 9 + - STD_2 + - pT + - float + - standard deviation of component 2 of the geomagnetic field variations computed on the whole period + * - 10 + - var_3 + - pT + - float + - range of variation of component 3 of the geomagnetic field computed on the whole period + * - 11 + - STD_3 + - pT + - float + - standard deviation of component 3 of the geomagnetic field variations computed on the whole period diff --git a/docs/source/products/data/unical_espseptransport_tableset.rst b/docs/source/products/data/unical_espseptransport_tableset.rst index 9244f1f..fdf662b 100644 --- a/docs/source/products/data/unical_espseptransport_tableset.rst +++ b/docs/source/products/data/unical_espseptransport_tableset.rst @@ -1,62 +1,113 @@ -========================================== -UNICAL Energetic particle spectral indices -========================================== +=================================== +Energetic particle spectral indices +=================================== .. contents:: The tiny table of contents -The differential energy spectral index is listed for all the SEP/ESP events analyzed and a pointer to the relevant transport parameter files +not available in DBF +**References** -Data Description ----------------- +not available in DBF -| **Data type**: tableset +Data description +~~~~~~~~~~~~~~~~ -| **Data formats**: - csv +**internal_name:** unical_espseptransport_tableset +**publisher:** not available in DBF -| **Version**: v2.0 +**alphanumeric_code:** 20B -Data Provider -------------- +**id_tmp:** 57 -Data are collected by the following instruments: +**short_name:** SEP+ESP-spectral -- **ACE** - source: +**identifier:** aspis:///unical/espseptransport_tableset_old - - EPAM +**dynamic:** Static collection -Data Coverage -------------- -The product cover measurements for the ND messangers. +**size:** 1kB -Data coverage is listed below: +**format:** csv -| **Spatial** IP +**type:** tableset -| **Temporal** - time_start: 2009-01-01T00:00:00+01:00 +**records_number:** 59 -- time_stop: 2022-03-31T00:00:00+02:00 +**time_start:** 2009-01-01 +**time_stop:** 2022-03-31 +**spatial:** IP -| **Spectral** range: ND ND - ND ND +**messenger:** protons -Product Status --------------- +**spectral_min:** 0.01 -| **Status**: Active +**spectral_max:** 100 -| **Creation date**: 2022-04-27T09:47:00+02:00 +**spectral_units:** MeV -| **Last Update**: 2023-10-31T12:00:00+01:00 +**observable:** SEP,ESP,IPS,CME -Data Policy ------------ +**latest update:** 2024-03-28 05:08:15 -This product contains public data. Public access to the data. +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -Example -------- +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 -Example is not yet provided . + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime (2010-01-01 01:30:05.500) (time.epoch) - Start time of the event + * - 2 + - start_time + - UTC + - datetime + - datetime (2010-01-01 01:30:05.500) (time.epoch) - Start time of the event + * - 3 + - end_time + - UTC + - datetime + - datetime (2010-01-01 01:30:05.500) (time.epoch) - End time of the event + * - 4 + - alpha + - spectral index + - float + - rreal number between [1-2] (1.4) - exponent of the mean square displacement as a function of time of energetic particle in each energy channel + * - 5 + - spacecraft + - char + - string + - Spacecraft + * - 6 + - energy_min + - MeV + - float + - MeV (0.580) - min value of the selected energy channel + * - 7 + - energy_max + - MeV + - float + - MeV (1.000) - max value of the selected energy channel + * - 8 + - d_diff + - km^2/s^alpha + - float + - km^2/s or km^2/s^(alpha) (220000000) - diffusion coefficient of energetic particles in each energy channel (unit of measure depends upon the transport- diffusive or superdiffusive) + * - 9 + - t_acc + - hr + - float + - hr (12) - acceleration time of energetic particles in each energy channel diff --git a/docs/source/products/data/unical_sep_ace_spectrum.rst b/docs/source/products/data/unical_sep_ace_spectrum.rst index 3e71eeb..89b5ab3 100644 --- a/docs/source/products/data/unical_sep_ace_spectrum.rst +++ b/docs/source/products/data/unical_sep_ace_spectrum.rst @@ -1,45 +1,103 @@ -================================================ -UNICAL SEP Proton Spectra for the ACE spacecraft -================================================ +========================================= +SEP Proton Spectra for the ACE spacecraft +========================================= .. contents:: The tiny table of contents Proton spectra for geoeffective target SWE events (at L1) from ACE spacecraft. -**Providers**: +**References** -- **Ace** - source: - - EPAM +Data description +~~~~~~~~~~~~~~~~ -| **Product Type**: data +**internal_name:** unical_sep_ace_spectrum -| **Status**: Active +**publisher:** University of Calabria Dept. of Physics -| **Creation date**: 2022-04-26T11:51:00+02:00 +**alphanumeric_code:** 20C -| **Last Update**: 2023-10-01T12:00:00+02:00 +**id_tmp:** 36 -Data Description -~~~~~~~~~~~~~~~~ +**short_name:** SEP-spectrum-Ace + +**identifier:** aspis://unical/unical_sep_ace_spectrum + +**dynamic:** +1 kb updated every SEP event + +**size:** 10kB + +**format:** csv + +**type:** spectrum + +**records_number:** 8 + +**time_start:** 2009-01-01 + +**time_stop:** 2022-03-31 + +**spatial:** L1 + +**messenger:** Protons + +**spectral_min:** 0.04 -| **Data type**: tableset +**spectral_max:** 5 -| **Data formats**: - txt +**spectral_units:** MeV +**observable:** SEP,CME -| **Sample**: https://drive.google.com/file/d/1jIQGdVMZImhyC24Aoe-lvbrdgGpoFIeh/view?usp=sharing +**latest update:** 2024-03-28 05:08:15 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - datetime - reference time of the SEP event + * - 2 + - start_time + - UTC + - datetime + - UTC - datetime - start time of the time average + * - 3 + - end_time + - UTC + - datetime + - UTC - datetime - end time of the time average + * - 4 + - spacecraft + - char + - string + - the name of the spacecraft + * - 5 + - data_name + - char + - string + - the name of the file with the data + * - 6 + - prew_name + - char + - string + - the name of the full preview file + * - 7 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/unical_sep_psp_spectrum.rst b/docs/source/products/data/unical_sep_psp_spectrum.rst index f2fa591..cf69c7e 100644 --- a/docs/source/products/data/unical_sep_psp_spectrum.rst +++ b/docs/source/products/data/unical_sep_psp_spectrum.rst @@ -1,45 +1,103 @@ -================================================ -UNICAL SEP Proton Spectra for the PSP spacecraft -================================================ +========================================= +SEP Proton Spectra for the PSP spacecraft +========================================= .. contents:: The tiny table of contents Proton spectra for widespread target SWE events from PSP spacecraft. -**Providers**: +**References** -- **PSP** - source: - - ISOIS +Data description +~~~~~~~~~~~~~~~~ -| **Product Type**: data +**internal_name:** unical_sep_psp_spectrum -| **Status**: Active +**publisher:** University of Calabria Dept. of Physics -| **Creation date**: 2022-04-28T13:34:40+02:00 +**alphanumeric_code:** 20E -| **Last Update**: 2023-10-01T12:00:00+02:00 +**id_tmp:** 37 -Data Description -~~~~~~~~~~~~~~~~ +**short_name:** SEP-spectrum-PSP + +**identifier:** aspis://unical/unical_sep_psp_spectrum + +**dynamic:** +5 kb updated every SEP event + +**size:** 5kB + +**format:** csv + +**type:** spectrum + +**records_number:** 1 + +**time_start:** 2020-01-01 + +**time_stop:** 2022-03-31 + +**spatial:** IP + +**messenger:** Protons + +**spectral_min:** 0.6 -| **Data type**: tableset +**spectral_max:** 95 -| **Data formats**: - txt +**spectral_units:** MeV +**observable:** SEP,CME -| **Sample**: https://drive.google.com/file/d/1U6Am0CfJXaEqI_5gAJdaV85bp4U5pRX5/view?usp=sharing +**latest update:** 2024-03-28 05:08:15 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - datetime - reference time of the SEP event + * - 2 + - start_time + - UTC + - datetime + - UTC - datetime - start time of the time average + * - 3 + - end_time + - UTC + - datetime + - UTC - datetime - end time of the time average + * - 4 + - spacecraft + - char + - string + - the name of the spacecraft + * - 5 + - data_name + - char + - string + - the name of the file with the data + * - 6 + - prew_name + - char + - string + - the name of the full preview file + * - 7 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/unical_sep_soho_spectrum.rst b/docs/source/products/data/unical_sep_soho_spectrum.rst index a6e6e61..901d35c 100644 --- a/docs/source/products/data/unical_sep_soho_spectrum.rst +++ b/docs/source/products/data/unical_sep_soho_spectrum.rst @@ -1,45 +1,103 @@ -================================================= -UNICAL SEP Proton Spectra for the SoHO spacecraft -================================================= +========================================== +SEP Proton Spectra for the SoHO spacecraft +========================================== .. contents:: The tiny table of contents Proton spectra for: geoeffective target SWE events (at L1) from SoHO spacecraft. -**Providers**: +**References** -- **SoHO** - source: - - ERNE +Data description +~~~~~~~~~~~~~~~~ -| **Product Type**: data +**internal_name:** unical_sep_soho_spectrum -| **Status**: Active +**publisher:** University of Calabria Dept. of Physics -| **Creation date**: 2022-04-26T11:51:00+02:00 +**alphanumeric_code:** 20F -| **Last Update**: 2023-10-01T12:00:00+02:00 +**id_tmp:** 58 -Data Description -~~~~~~~~~~~~~~~~ +**short_name:** SEP-spectrum-Soho + +**identifier:** aspis://unical/unical_sep_soho_spectrum + +**dynamic:** +1 kb updated every SEP event + +**size:** 10kB + +**format:** csv + +**type:** spectrum + +**records_number:** 7 + +**time_start:** 2009-01-01 + +**time_stop:** 2022-03-31 + +**spatial:** L1 + +**messenger:** Protons + +**spectral_min:** 1.3 -| **Data type**: tableset +**spectral_max:** 130 -| **Data formats**: - txt +**spectral_units:** MeV +**observable:** SEP,CME -| **Sample**: https://drive.google.com/file/d/1IwOQPDq4HZ9j0Say9Yh5CY18LV9lWhXr/view?usp=sharing +**latest update:** 2024-03-28 05:08:15 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - datetime - reference time of the SEP event + * - 2 + - start_time + - UTC + - datetime + - UTC - datetime - start time of the time average + * - 3 + - end_time + - UTC + - datetime + - UTC - datetime - end time of the time average + * - 4 + - spacecraft + - char + - string + - the name of the spacecraft + * - 5 + - data_name + - char + - string + - the name of the file with the data + * - 6 + - prew_name + - char + - string + - the name of the full preview file + * - 7 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/unical_sep_solo_spectrum.rst b/docs/source/products/data/unical_sep_solo_spectrum.rst index 07e1999..799fa66 100644 --- a/docs/source/products/data/unical_sep_solo_spectrum.rst +++ b/docs/source/products/data/unical_sep_solo_spectrum.rst @@ -1,45 +1,103 @@ -================================================= -UNICAL SEP Proton Spectra for the SolO spacecraft -================================================= +========================================== +SEP Proton Spectra for the SolO spacecraft +========================================== .. contents:: The tiny table of contents Proton spectra for widespread target SWE events from SolO spacecraft. -**Providers**: +**References** -- **SolO** - source: - - EPD +Data description +~~~~~~~~~~~~~~~~ -| **Product Type**: data +**internal_name:** unical_sep_solo_spectrum -| **Status**: Active +**publisher:** University of Calabria Dept. of Physics -| **Creation date**: 2022-04-26T11:51:00+02:00 +**alphanumeric_code:** 20G -| **Last Update**: 2023-10-01T12:00:00+02:00 +**id_tmp:** 39 -Data Description -~~~~~~~~~~~~~~~~ +**short_name:** SEP-spectrum-SolO + +**identifier:** aspis://unical/unical_sep_solo_spectrum + +**dynamic:** +2 kb updated every SEP event + +**size:** 5kB + +**format:** csv + +**type:** spectrum + +**records_number:** 2 + +**time_start:** 2020-03-01 + +**time_stop:** 2022-03-31 + +**spatial:** IP + +**messenger:** Protons + +**spectral_min:** 0.03 -| **Data type**: tableset +**spectral_max:** 90 -| **Data formats**: - txt +**spectral_units:** MeV +**observable:** SEP,CME -| **Sample**: ND +**latest update:** 2024-03-28 05:08:15 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - datetime - reference time of the SEP event + * - 2 + - start_time + - UTC + - datetime + - UTC - datetime - start time of the time average + * - 3 + - end_time + - UTC + - datetime + - UTC - datetime - end time of the time average + * - 4 + - spacecraft + - char + - string + - the name of the spacecraft + * - 5 + - data_name + - char + - string + - the name of the file with the data + * - 6 + - prew_name + - char + - string + - the name of the full preview file + * - 7 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/unical_sep_stra_spectrum.rst b/docs/source/products/data/unical_sep_stra_spectrum.rst index c01b65b..d9716a2 100644 --- a/docs/source/products/data/unical_sep_stra_spectrum.rst +++ b/docs/source/products/data/unical_sep_stra_spectrum.rst @@ -1,45 +1,103 @@ -===================================================== -UNICAL SEP Proton Spectra for the STEREO A spacecraft -===================================================== +============================================== +SEP Proton Spectra for the STEREO A spacecraft +============================================== .. contents:: The tiny table of contents Proton spectra for widespread target SWE events from STEREO A spacecraft. -**Providers**: +**References** -- **STEREO A** - source: - - IMPACT +Data description +~~~~~~~~~~~~~~~~ -| **Product Type**: data +**internal_name:** unical_sep_stra_spectrum -| **Status**: Active +**publisher:** University of Calabria Dept. of Physics -| **Creation date**: 2022-04-26T11:51:00+02:00 +**alphanumeric_code:** 20H -| **Last Update**: 2023-10-01T12:00:00+02:00 +**id_tmp:** 40 -Data Description -~~~~~~~~~~~~~~~~ +**short_name:** SEP-spectrum-StereoA + +**identifier:** aspis://unical/unical_sep_stra_spectrum + +**dynamic:** +1 kb updated every SEP event + +**size:** 10kB + +**format:** csv + +**type:** spectrum + +**records_number:** 2 + +**time_start:** 2020-01-01 + +**time_stop:** 2022-03-31 + +**spatial:** IP + +**messenger:** Protons + +**spectral_min:** 0.08 -| **Data type**: tableset +**spectral_max:** 100 -| **Data formats**: - txt +**spectral_units:** MeV +**observable:** SEP,CME -| **Sample**: https://drive.google.com/file/d/1bT1Y7NyXrVFg_oAdZWjas_x2w6lBn9uE/view?usp=sharing +**latest update:** 2024-03-28 05:08:16 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime (2010-01-01 01:30:05.500) (time.epoch) - Start time of the time average + * - 2 + - start_time + - UTC + - datetime + - datetime (2010-01-01 01:30:05.500) (time.epoch) - Start time of the time average + * - 3 + - end_time + - UTC + - datetime + - datetime (2010-01-01 01:30:05.500) (time.epoch) - End time of the time average + * - 4 + - spacecraft + - char + - string + - the name of the spacecraft + * - 5 + - data_name + - char + - string + - the name of the file with the data + * - 6 + - prew_name + - char + - string + - the name of the full preview file + * - 7 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/unical_sep_wind_spectrum.rst b/docs/source/products/data/unical_sep_wind_spectrum.rst index 9a7dcd6..ad4bfb6 100644 --- a/docs/source/products/data/unical_sep_wind_spectrum.rst +++ b/docs/source/products/data/unical_sep_wind_spectrum.rst @@ -1,46 +1,103 @@ -================================================= -UNICAL SEP Proton Spectra for the WIND spacecraft -================================================= +========================================== +SEP Proton Spectra for the WIND spacecraft +========================================== .. contents:: The tiny table of contents Proton spectra for: geoeffective target SWE events (at L1) from Wind spacecraft. -**Providers**: +**References** -- **WIND** - sources: - - 3DP - - EPACT +Data description +~~~~~~~~~~~~~~~~ -| **Product Type**: data +**internal_name:** unical_sep_wind_spectrum -| **Status**: Active +**publisher:** University of Calabria Dept. of Physics -| **Creation date**: 2022-04-26T11:51:00+02:00 +**alphanumeric_code:** 20I -| **Last Update**: 2023-10-01T12:00:00+02:00 +**id_tmp:** 41 -Data Description -~~~~~~~~~~~~~~~~ +**short_name:** SEP-spectrum-Wind + +**identifier:** aspis://unical/unical_sep_wind_spectrum + +**dynamic:** +1 kb updated every SEP event + +**size:** 10kB + +**format:** csv + +**type:** spectrum + +**records_number:** 8 + +**time_start:** 2009-01-01 + +**time_stop:** 2022-03-31 + +**spatial:** L1 + +**messenger:** Protons + +**spectral_min:** 0.07 -| **Data type**: tableset +**spectral_max:** 80 -| **Data formats**: - txt +**spectral_units:** MeV +**observable:** SEP,CME -| **Sample**: https://drive.google.com/file/d/17K170-oRokV3BeEZKaHrgCtmLkq1NhsF/view?usp=sharing +**latest update:** 2024-03-28 05:08:16 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime (2010-01-01 01:30:05.500) (time.epoch) - Start time of the time average + * - 2 + - start_time + - UTC + - datetime + - datetime (2010-01-01 01:30:05.500) (time.epoch) - Start time of the time average + * - 3 + - end_time + - UTC + - datetime + - datetime (2010-01-01 01:30:05.500) (time.epoch) - End time of the time average + * - 4 + - spacecraft + - char + - string + - the name of the spacecraft + * - 5 + - data_name + - char + - string + - the name of the file with the data + * - 6 + - prew_name + - char + - string + - the name of the full preview file + * - 7 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/unical_shockpar_tableset.rst b/docs/source/products/data/unical_shockpar_tableset.rst index 1f4affe..c7ee3f0 100644 --- a/docs/source/products/data/unical_shockpar_tableset.rst +++ b/docs/source/products/data/unical_shockpar_tableset.rst @@ -1,159 +1,213 @@ -====================================================== -UNICAL Parameters of shocks associated with ESP events -====================================================== +=============================================== +Parameters of shocks associated with ESP events +=============================================== .. contents:: The tiny table of contents -The table contains a list -of shocks (and their parameters) associated with ESP and SEP events, observed from Stereo -A, Wind, ACE spacecraft from 2009. The shock parameters (the plasma beta, the angle -between the mean magnetic field and the normal to the shock, the magnetosonic Mach -number) for Stereo A spacecraft were taken from: +not available in DBF -Jian et al. Interplanetary Shock list -(URL: https://stereo-ssc.nascom.nasa.gov/data/ins_data/impact/level3/IPs.pdf ) +**References** -and the -related ESP spectra are presented in detail in the paper Chiappetta et al. (2021) ApJ 915, 8 -DOI: 10.3847/1538-4357/abfe09. -The shock parameters (the plasma beta, the angle between the mean magnetic field and the -normal to the shock, the magnetosonic Mach number, compression ratio) for Wind and ACE, -have been calculated using upstream and downstream time intervals of [tshock – 9min, tshock – -1min] and [tshock + 2min, tshock + 10min], respectively. In these cases the normal vector of the -shock (and therefore the angle θBn) is calculated using the Mixed Mode 3 method. When the -plasma data for the event is not available, the magnetic coplanarity method is used to -determine the shock normal vector. -The table also contains information relating to the ESP and SEP spectra files, and to the -turbulence analysis upstream and downstream of the shocks, if available. +not available in DBF -:download:`Further readings (pdf) <../../private/unical_shockpar_tableset-Description_ESP_STEREOA.pdf>`. +Data description +~~~~~~~~~~~~~~~~ -:download:`Further readings (pdf) <../../private/unical_shockpar_tableset-Description_product22-1.pdf>`. - -Data Description ----------------- - -| **Data type**: tableset - -| **Data formats**: - csv - - -| **Version**: v1.0 - -**Columns:** - -1. time and date of the shock arrival at spacecraft; - -2. the plasma beta (β); - -3. the angle (θBn) between the mean magnetic field and the normal to the shock; - -4. the magnetosonic Mach number (Mms); - -5. the compression ratio (r); - -6. the name of the spacecraft; - -7. a flag which indicates if there is a SEP in progress or not; - -8. the name of the SEP spectrum file (if available); - -9. the starting time of the range used to calculate the SEP energy spectrum; - -10. the ending time of the range used to calculate the SEP energy spectrum; - -11. a flag indicating whether ESP spectrum is available; - -12. the name of the ESP spectrum file (if available); - -13. a flag to indicate if the data calibration procedure has been performed or if it has not been necessary; - -14. the starting time of the range used to calculate the ESP energy spectrum; - -15. the ending time of the range used to calculate the ESP energy spectrum; - -16. a flag to indicate whether the PSD is available; - -17. the name of the PSD file calculated in the upstream region of the shock (if available); - -18. the starting time of the range used to calculate the PSD in the upstream region; - -19. the ending time of the range used to calculate the PSD in the upstream region; - -20. the name of the PSD file calculated in the downstream region of the shock (if available); - -21. the starting time of the range used to calculate the PSD in the downstream region; - -22. the ending time of the range used to calculate the PSD in the downstream region; - -23. a flag to indicate whether the Structure Functions are available; - -24. the name of the Structure Functions file calculated in the upstream region of the shock (if available); - -25. the starting time of the range used to calculate the Structure Functions in the upstream region; - -26. the ending time of the range used to calculate the Structure Functions in the upstream region; - -27. the name of the Structure Functions file calculated in the downstream region of the shock (if available); - -28. the starting time of the range used to calculate the Structure Functions in the downstream region; - -29. the ending time of the range used to calculate the Structure Functions in the downstream region. - -Data Provider ---------------- - -Data are collected by the following instruments: - -- **ACE** - sources: - - - EPAM - - MAG - - SWEPAM -- **WIND** - sources: - - - 3DP - - EPACT - - MFI - - SWE -- **STEREO A** - source: - - - IMPACT -- **Jian et al. Interplanetary Shock list at STEREO A** - source: - - - https://stereo-ssc.nascom.nasa.gov/data/ins_data/impact/level3/IPs.pdf - -Data Coverage ------------------ -The product cover measurements for the ND messangers. - -Data coverage is listed below: - -| **Spatial** IP - -| **Temporal** - time_start: 2009-01-01T00:00:36+01:00 - -- time_stop: 2022-03-31T23:00:00+02:00 - - - -| **Spectral** range: ND ND - ND ND - -Product Status ---------------- - -| **Status**: Active - -| **Creation date**: 2023-10-22T17:40:00+02:00 - -| **Last Update**: 2023-10-22T17:40:00+02:00 - -Data Policy --------------- - -This product contains public data. Other. - -Example ------------- - -Example is not yet provided . +**internal_name:** unical_shockpar_tableset + +**publisher:** not available in DBF + +**alphanumeric_code:** 22A + +**id_tmp:** 49 + +**short_name:** Shocks-parameters + +**identifier:** aspis://unical/unical_shockpar_tableset + +**dynamic:** +300 byte updated every event + +**size:** 20kB + +**format:** csv + +**type:** tableset + +**records_number:** 65 + +**time_start:** 2009-01-01 + +**time_stop:** 2022-03-31 + +**spatial:** IP + +**messenger:** Protons,Magnetic field + +**spectral_min:** 0.01 + +**spectral_max:** 100 + +**spectral_units:** MeV + +**observable:** IPS,SW,SEP,ESP,IMF + +**latest update:** 2024-03-28 05:08:16 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - time and date of the shock arrival at spacecraft + * - 2 + - Beta_plasma + - + - float + - the plasma beta (β) + * - 3 + - Theta_Bn + - deg + - float + - the angle (θ_Bn) between the mean magnetic field and the normal to the shock + * - 4 + - M_ms + - + - float + - the magnetosonic Mach number (M_ms) + * - 5 + - r + - + - float + - the compression ratio (r) + * - 6 + - SC + - + - string + - the name of the spacecraft + * - 7 + - SEP + - + - integer + - a flag which indicates if there is a SEP in progress or not + * - 8 + - Filename_SEP_spectrum + - + - string + - the name of the SEP spectrum file (if available) + * - 9 + - SEP_spectrum_start + - UTC + - datetime + - the starting time of the range used to calculate the SEP energy spectrum + * - 10 + - SEP_spectrum_end + - UTC + - datetime + - the ending time of the range used to calculate the SEP energy spectrum + * - 11 + - ESP_spectrum + - + - integer + - a flag indicating whether ESP spectrum is available + * - 12 + - Filename_ESP_spectrum + - + - string + - the name of the ESP spectrum file (if available) + * - 13 + - Calibration_ESP + - + - integer + - a flag to indicate if the data calibration procedure has been performed or if it has not been necessary + * - 14 + - ESP_spectrum_start + - UTC + - datetime + - the starting time of the range used to calculate the ESP energy spectrum + * - 15 + - ESP_spectrum_end + - UTC + - datetime + - the ending time of the range used to calculate the ESP energy spectrum + * - 16 + - PSD + - + - integer + - a flag to indicate whether the PSD is available + * - 17 + - Filename_PSD_upstream + - + - string + - the name of the PSD file calculated in the upstream region of the shock (if available) + * - 18 + - PSD_upstream_start + - UTC + - datetime + - the starting time of the range used to calculate the PSD in the upstream region + * - 19 + - PSD_upstream_end + - UTC + - datetime + - the ending time of the range used to calculate the PSD in the upstream region + * - 20 + - Filename_PSD_downstream + - + - string + - the name of the PSD file calculated in the downstream region of the shock (if available) + * - 21 + - PSD_downstream_start + - UTC + - datetime + - the starting time of the range used to calculate the PSD in the downstream region + * - 22 + - PSD_downstream_end + - UTC + - datetime + - the ending time of the range used to calculate the PSD in the downstream region + * - 23 + - Structure_functions + - + - integer + - a flag to indicate whether the Structure Functions are available + * - 24 + - Filename_SFs_upstream + - + - string + - the name of the Structure Functions file calculated in the upstream region of the shock (if available) + * - 25 + - SFs_upstream_start + - UTC + - datetime + - the starting time of the range used to calculate the Structure Functions in the upstream region + * - 26 + - SFs_upstream_end + - UTC + - datetime + - the ending time of the range used to calculate the Structure Functions in the upstream region + * - 27 + - Filename_SFs_downstream + - + - string + - the name of the Structure Functions file calculated in the downstream region of the shock (if available) + * - 28 + - SFs_downstream_start + - UTC + - datetime + - the starting time of the range used to calculate the Structure Functions in the downstream region + * - 29 + - SFs_downstream_end + - UTC + - datetime + - the ending time of the range used to calculate the Structure Functions in the downstream region diff --git a/docs/source/products/data/unict_promin_ws.rst b/docs/source/products/data/unict_promin_ws.rst deleted file mode 100644 index 897d8d4..0000000 --- a/docs/source/products/data/unict_promin_ws.rst +++ /dev/null @@ -1,40 +0,0 @@ -============================================================ -UNICT Geometry and location of prominences on the solar limb -============================================================ - -.. contents:: The tiny table of contents - -Software devoted to the automated determination of the prominences position and geometrical characteristics using real-time H-alpha images acquired at Catania Solar Telescope. These data have a spatial resolution of 2 arcsec and a cadence of 1 image/day. - -**Providers**: - -ND - -| **Product Type**: software - -| **Status**: Active - -| **Creation date**: 2022-04-28T06:16:26+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: ND - -| **Data formats**: ND - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.4: Scheduled computation -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py -- int2320.1: Data conversion - diff --git a/docs/source/products/data/unipg_gcr_model.rst b/docs/source/products/data/unipg_gcr_model.rst deleted file mode 100644 index 405b1cf..0000000 --- a/docs/source/products/data/unipg_gcr_model.rst +++ /dev/null @@ -1,34 +0,0 @@ -========================================= -UNIPG GCRs long-term modulation -========================================= - -.. contents:: The tiny table of contents - -The software is aimed at implementing a physical model for the so-called solar modulation effect, that is, the long-term influence of solar activity on the intensity and energy spectra of Galactic cosmic rays (GCRs). The physical mechanisms governing solar modulation are diffusion, convection, adiabatic energy losses and drifts of energetic charged particles through the solar wind and its embedded magnetic field. The interplay among the various mechanisms at the different timescales and energy depends on the level of solar activity and interplanetary conditions. The model is based on numerical integration of differential equation for the transport of Galactic cosmic rays (GCR) in the heliosphere. The model output is the differential flux intensity J=J(t,E), evaluated near-Earth, which is defined as the number of GCR particles per unit of time, solid angle, area, and energy. Such an output is provided as a time series within a user-specified range [t_1,t_2], or for a given input epoch t. The input options to be specified by the user may include: an arbitrary past epoch t, the GCR particle type (e.g. proton, helium, light nuclei), and the value of kinetic energy E (between 100 MeV and 100 GeV). - -**Providers**: - -ND - -| **Product Type**: software - -| **Status**: Active - -| **Creation date**: 2022-05-03T17:05:10+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: ND - -| **Data formats**: ND - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI - diff --git a/docs/source/products/data/unitn_flux_cses_timeseries.rst b/docs/source/products/data/unitn_flux_cses_timeseries.rst index b01870b..f1172c7 100644 --- a/docs/source/products/data/unitn_flux_cses_timeseries.rst +++ b/docs/source/products/data/unitn_flux_cses_timeseries.rst @@ -1,43 +1,93 @@ -========================================= -UNITN CSES satellite particle flux data -========================================= +================================= +CSES satellite particle flux data +================================= .. contents:: The tiny table of contents Particle flux in the Lshell – pitch reference frame. Lshell will be calculated using the IGRF model for the internal origin field and Tsyganenko model for the external origin field. -**Providers**: +**References** -- **CSES satellite HEPP electron and proton data** -| **Product Type**: data +Data description +~~~~~~~~~~~~~~~~ -| **Status**: Active +**internal_name:** unitn_flux_cses_timeseries -| **Creation date**: 2022-05-03T09:00:00+02:00 +**publisher:** Roberto Battiston -| **Last Update**: 2023-10-01T12:00:00+02:00 +**alphanumeric_code:** 44 -Data Description -~~~~~~~~~~~~~~~~ +**id_tmp:** 42 + +**short_name:** CSES Flux + +**identifier:** aspis://unitn/flux_cses_timeseries + +**dynamic:** Static and depending on the length of the input data + +**size:** 5MB + +**format:** .mat + +**type:** timeseries + +**records_number:** 18129 + +**time_start:** 2021-04-12 + +**time_stop:** 2021-04-13 + +**spatial:** IONO + +**messenger:** phys.flux + +**spectral_min:** 0 -| **Data type**: timeseries +**spectral_max:** 0 -| **Data formats**: - .mat +**spectral_units:** 0 +**observable:** GCR,ESP,SEP -| **Sample**: https://drive.google.com/file/d/1PBiyD4KIxWKtFyMF-vn5Eaau4tFxofIk/view?usp=sharing +**latest update:** 2024-03-28 05:08:17 -Capabilities -~~~~~~~~~~~~ +Columns specification +~~~~~~~~~~~~~~~~~~~~~ -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime (2012-03-01T12:00:00) - time UTC of the data-taking + * - 2 + - L + - R_E + - float + - R_E Lshell – pitch reference frame + * - 3 + - En00 + - cm^-2s^-1sr^-1 + - float + - cm^-2s^-1sr^-1 electron and proton flux above 100 KeV + * - 4 + - En01 + - cm^-2s^-1sr^-1 + - float + - cm^-2s^-1sr^-1 electron and proton flux above 150 KeV + * - 5 + - En02 + - cm^-2s^-1sr^-1 + - float + - cm^-2s^-1sr^-1 electron and proton flux above 250 KeV diff --git a/docs/source/products/data/unitov_halpha_tsst_image.rst b/docs/source/products/data/unitov_halpha_tsst_image.rst index 7c45499..52acbd5 100644 --- a/docs/source/products/data/unitov_halpha_tsst_image.rst +++ b/docs/source/products/data/unitov_halpha_tsst_image.rst @@ -1,45 +1,133 @@ -========================================= -UNITOV TSST H-alpha Full Disk Images -========================================= +============================= +TSST H-alpha Full Disk Images +============================= .. contents:: The tiny table of contents -The Hα channel of the TSST is a Daystar SR-127 QT, an achromatic refractor with 127 mm aperture and a focal length of 2667 mm. The telescope features a narrow band filter with a passband of 0.04 nm centered at the Hα line. The filter is a temperature stabilized etalon in collimated configuration, and it is the same filter used in the GONG network for the Hα channel to monitor the chromospheric transients (Giersch, 2013). The Hα channel is equipped with a focal reducer, acting also as a field curvature corrector, to match the Dalsa Pantera 1M60 pixel scale of the MOF channel (2.6 arcsec/pixel). The main goal of this TSST channel is the real time detection of flaring region (Piazzesi et al., 2012; Pötzi et al., 2015, 2018) during the impulsive and flash phases when the intensity reaches its maximum (Benz, 2017). Hα images are extremely important for ground based SWe monitoring (see, e.g. Veronig & Potzi, 2016) and to automatically detect and track structures in the solar chromosphere, as filaments (Bernasconi et al., 2005; Fuller et al., 2005; Bonnin et al., 2013) and prominences (Wang et al., 2010), that can be associated with flare and coronal mass ejections. +The Hα channel of the TSST is a Daystar SR-127 QT, an achromatic refractor with 127 mm aperture and a focal length of 2667 mm. The telescope features a narrow band filter with a passband of 0.04 nm centered at the Hα line. The filter is a temperature stabilized etalon in collimated configuration, and it is the same filter used in the GONG network for the Hα channel to monitor the chromospheric transients (Giersch, 2013). The Hα channel is equipped with a focal reducer, acting also as a field curvature corrector, to match the Dalsa Pantera 1M60 pixel scale of the MOF channel (2.6 arcsec/pixel). The main goal of this TSST channel is the real time detection of flaring region (Piazzesi et al., 2012, Pötzi et al., 2015, 2018) during the impulsive and flash phases when the intensity reaches its maximum (Benz, 2017). Hα images are extremely important for ground based SWe monitoring (see, e.g. Veronig & Potzi, 2016) and to automatically detect and track structures in the solar chromosphere, as filaments (Bernasconi et al., 2005, Fuller et al., 2005, Bonnin et al., 2013) and prominences (Wang et al., 2010), that can be associated with flare and coronal mass ejections. -**Providers**: +**References** -- **TSST** - source: - - H-alpha - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-29T12:32:27+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: image - -| **Data formats**: - .fits - - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** unitov_halpha_tsst_image + +**publisher:** University of Rome Tor Vergata + +**alphanumeric_code:** 2 + +**id_tmp:** 59 + +**short_name:** TSST-halpha + +**identifier:** aspis:///unitov/halpha_tsst_image + +**dynamic:** data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares + +**size:** 20GB + +**format:** .fits + +**type:** image + +**records_number:** 9 + +**time_start:** 2022-09-01 + +**time_stop:** 2023-05-01 + +**spatial:** SUN + +**messenger:** photons + +**spectral_min:** 656.26 + +**spectral_max:** 656.34 + +**spectral_units:** nm + +**observable:** spect.line.intensity,AR,flare + +**latest update:** 2024-03-28 05:08:17 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - datetime - Acquisition time + * - 2 + - Quality + - 0-1 + - float + - Quality of the image 0-1 0=bad, 1=OK + * - 3 + - X_cen + - pixel + - int + - Position of the Solar centre on the X image axis [pixels] + * - 4 + - Y_cen + - pixel + - int + - Position of the Solar centre on the Y image axis [pixels] + * - 5 + - R_sun + - pixel + - int + - Radius of the Solar disk [pixels] + * - 6 + - min + - ADU + - float + - minimum value of the image [ADU] + * - 7 + - Max + - ADU + - float + - maximum value of the image [ADU] + * - 8 + - mean + - ADU + - float + - average value of the image [ADU] + * - 9 + - std + - ADU + - float + - standard deviation value of the image [ADU] + * - 10 + - B0 + - deg + - float + - apparent tilt of the sun's axis of rotation with respect to the ecliptic [degrees] + * - 11 + - data_name + - char + - string + - the name of the file with the data + * - 12 + - prew_name + - char + - string + - the name of the full preview file + * - 13 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/unitov_icme_tableset.rst b/docs/source/products/data/unitov_icme_tableset.rst index 65b2cf0..0697ea9 100644 --- a/docs/source/products/data/unitov_icme_tableset.rst +++ b/docs/source/products/data/unitov_icme_tableset.rst @@ -6,45 +6,223 @@ UNITOV Catalogue of geoeffective CMEs A database associating L1 Time of Arrival and Speed of an interplanetary CME to the kinematic characteristics of the corresponding CME, covering the period 1996-2020. -**Providers**: +**References** -- **SDO** - source: - - AIA -- **SOHO** - source: - - LASCO -- **Richardson & Cane CME List** -- **ACE** - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-08T11:24:13+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - csv - - -| **Sample**: `here `_ - - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** unitov_icme_tableset + +**publisher:** University of Rome Tor Vergata Dept. of Physics + +**alphanumeric_code:** 15 + +**id_tmp:** 44 + +**short_name:** UNITOV-ICME + +**identifier:** aspis:/unitov/icme_tableset + +**dynamic:** +10kB updated every year + +**size:** 100kB + +**format:** csv + +**type:** tableset + +**records_number:** 213 + +**time_start:** 1997-01-01 + +**time_stop:** 2019-12-31 + +**spatial:** IP + +**messenger:** Photons,Protons + +**spectral_min:** 0 + +**spectral_max:** 0 + +**spectral_units:** + +**observable:** + +**latest update:** 2024-03-28 05:08:17 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime (1997-01-06T16:23:38) - time of the first detection of the CME in LASCO FoV + * - 2 + - HPC_Tx + - arcsec + - float + - arcsec (25.21) - Helioprojective Cartesian Longitutude: the angle relative to the plane containing the Sun-observer line and the Sun’s rotation axis, with positive values in the direction of the Sun’s west limb + * - 3 + - HPC_Ty + - arcsec + - float + - arcsec (-3.22) - Helioprojective Cartesian Latitude: the angle relative to the Sun’s equatorial plane, with positive values in the direction of the Sun’s north pole + * - 4 + - HPC_distance + - AU + - float + - AU (0.98) - the Sun-observer distance + * - 5 + - CME_num + - index + - int + - index (1) - progressive number + * - 6 + - Start_Date + - UTC + - datetime + - datetime (1997-01-06 16:23:38.000) - extimated time of the CME passage at 20 R_Sun + * - 7 + - Arrival_Date + - UTC + - datetime + - datetime (1997-01-06 16:23:38.000) - time of the CME passage at L1 + * - 8 + - PE_duration + - hours + - float + - hours (22.0) - ICME Plasma Event duration at L1 + * - 9 + - Arrival_v + - km/s + - int + - km/s (450) - measured velocity of the CME at L1 + * - 10 + - Transit_time + - hours + - float + - hours (98.3) - time elapsed from the Start_Date and Arrival_Date + * - 11 + - Transit_time_err + - hours + - float + - hours (98.3) - error associated to the extimated transit time + * - 12 + - LASCO_Date + - UTC + - datetime + - datetime (1997-01-06 16:23:38.000) - time of the first detection of the CME in LASCO FoV + * - 13 + - LASCO_v + - km/s + - int + - km/s (459.5) - plane-of-sky velocity of the CME from LASCO images + * - 14 + - LASCO_pa + - deg + - int + - deg (263.0) - CME principal angle, counterclockwise from North + * - 15 + - LASCO_da + - deg + - int + - deg (165.0) - CME angular width + * - 16 + - LASCO_halo + - char + - char + - string (N/PH/HH/FH) - indicating halo/partial halo CME + * - 17 + - v_r + - km/s + - float + - km/s (705.35) - estimated radial velocity of the CME + * - 18 + - v_r_err + - km/s + - float + - km/s (104.89) - error associated to the radial velocity of the CME + * - 19 + - Theta_source + - arcsec + - float + - arcsec (14.92) - longitude of the most probable source of the CME on the solar disk + * - 20 + - Phi_source + - arcsec + - float + - arcsec (-25.97) - co-latitude of the most probable source of the CME on the solar disk + * - 21 + - source_err + - arcsec + - float + - arcsec (20.0) - uncertainty on the source location on the solar disk + * - 22 + - POS_source_angle + - deg + - float + - deg (64.60) - plane-of-sky angle of the source region of the CME + * - 23 + - rel_wid + - rad + - float + - rad (0.5585) - estimated deprojected CME angular width + * - 24 + - Mass + - g + - float + - g (1.8e+16) - Estimated mass of the CME + * - 25 + - SW_type + - char + - char + - char (F/S) - Solar wind type (Fast/Slow) for the ICME propagation + * - 26 + - Bz + - nT + - int + - nT (16) - z-component of the ICME magnetic field at L1 + * - 27 + - DST + - nT + - int + - nT (-68.0) - minimum DST during ICME event at L1 + * - 28 + - v_r_stat + - km/s + - float + - km/s (544.73) - statistical de-projection of the CME POS speed + * - 29 + - Accel. + - m/s^2 + - float + - m/s^2 (8.9076) - CME acceleration between the lift-off and 20 solar radii + * - 30 + - Analyitic_w + - km/s + - float + - km/s (395.56) - solar wind value obtained via analytic inversion of the DBM equations + * - 31 + - Analyitic_gamma + - km^-1 + - float + - km^-1 (3.5029e-06) -value of the drag parameter obtained via analytic inversion of the DBM equations + * - 32 + - filename + - char + - char + - string (CME_0111_param_inv.txt ) - name of the file containing PDBM information from the statistical inversion procedure diff --git a/docs/source/products/data/unitov_mag_tsst_image.rst b/docs/source/products/data/unitov_mag_tsst_image.rst index acac8a1..4e8cddb 100644 --- a/docs/source/products/data/unitov_mag_tsst_image.rst +++ b/docs/source/products/data/unitov_mag_tsst_image.rst @@ -1,45 +1,133 @@ -========================================= -UNITOV TSST Full Disk LoS magnetic maps -========================================= +================================ +TSST Full Disk LoS magnetic maps +================================ .. contents:: The tiny table of contents The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. -**Providers**: +**References** -- **TSST** - source: - - MOF - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-29T12:32:27+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: image - -| **Data formats**: - .fits - - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** unitov_mag_tsst_image + +**publisher:** University of Rome Tor Vergata + +**alphanumeric_code:** 1A + +**id_tmp:** 60 + +**short_name:** TSST-mag + +**identifier:** aspis:///unitov/mag_tsst_image + +**dynamic:** data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares + +**size:** 300GB + +**format:** .fits + +**type:** image + +**records_number:** 10 + +**time_start:** 2022-09-01 + +**time_stop:** 2023-05-01 + +**spatial:** SUN + +**messenger:** photons + +**spectral_min:** 769.88 + +**spectral_max:** 769.92 + +**spectral_units:** nm + +**observable:** phys.magField,AR + +**latest update:** 2024-03-28 05:08:17 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - datetime - Acquisition time + * - 2 + - Quality + - 0-1 + - float + - Quality of the image 0-1 0=bad, 1=OK + * - 3 + - X_cen + - pixel + - int + - Position of the Solar centre on the X image axis [pixels] + * - 4 + - Y_cen + - pixel + - int + - Position of the Solar centre on the Y image axis [pixels] + * - 5 + - R_sun + - pixel + - int + - Radius of the Solar disk [pixels] + * - 6 + - min + - Gauss + - float + - minimum value of the image [ADU] + * - 7 + - Max + - Gauss + - float + - maximum value of the image [ADU] + * - 8 + - mean + - Gauss + - float + - average value of the image [ADU] + * - 9 + - std + - Gauss + - float + - standard deviation value of the image [ADU] + * - 10 + - B0 + - deg + - float + - apparent tilt of the sun's axis of rotation with respect to the ecliptic [degrees] + * - 11 + - data_name + - char + - string + - the name of the file with the data + * - 12 + - prew_name + - char + - string + - the name of the full preview file + * - 13 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/data/unitov_pdb_model.rst b/docs/source/products/data/unitov_pdb_model.rst deleted file mode 100644 index 4b550d1..0000000 --- a/docs/source/products/data/unitov_pdb_model.rst +++ /dev/null @@ -1,40 +0,0 @@ -========================================= -UNITOV P-DBM CME propagation model -========================================= - -.. contents:: The tiny table of contents - -The CME propagation is modeled by using probability distribution functions. This allows us to evaluate the ICME arrival times and velocities along with the uncertainties on the forecast. - -**Providers**: - -ND - -| **Product Type**: software - -| **Status**: Active - -| **Creation date**: 2022-04-14T10:45:06+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: ND - -| **Data formats**: ND - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2130.4: Scheduled computation -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.5: On demand computation -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.3: Download: ASPIS.py - diff --git a/docs/source/products/data/unitov_rdparameter_tableset.rst b/docs/source/products/data/unitov_rdparameter_tableset.rst index ff7ebb8..ccdb3bb 100644 --- a/docs/source/products/data/unitov_rdparameter_tableset.rst +++ b/docs/source/products/data/unitov_rdparameter_tableset.rst @@ -1,45 +1,123 @@ -========================================= -UNITOV R and D Active Region parameters -========================================= +================================ +R and D Active Region parameters +================================ .. contents:: The tiny table of contents Parameters for flare-forecasting applications, representing the complexity of a solar active region -**Providers**: +**References** -- **SDO** - source: - - HMI - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-05-11T10:59:38+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: tableset - -| **Data formats**: - csv - - -| **Sample**: https://drive.google.com/file/d/1U8NIiVtR19sSaxDMGgz5pgWLMV4ISCk7/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- int2320.1: Data conversion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** unitov_rdparameter_tableset + +**publisher:** University of Rome Tor Vergata Dept. of Physics + +**alphanumeric_code:** 3 + +**id_tmp:** 46 + +**short_name:** AR-parameters + +**identifier:** aspis:///unitov/rdparameter_tableset + +**dynamic:** +1MB updated every month + +**size:** 20MB + +**format:** csv + +**type:** tableset + +**records_number:** 35998 + +**time_start:** 2012-09-14 + +**time_stop:** 2016-04-13 + +**spatial:** SUN + +**messenger:** Photons + +**spectral_min:** + +**spectral_max:** + +**spectral_units:** + +**observable:** AR,flare + +**latest update:** 2024-03-28 05:08:18 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - Time (2012-09-14T03:00:03) - UTC Time of the HMI image + * - 2 + - HGS_Lon + - deg + - float + - HGS_Lon (93.03142277) - HeliographicStonyhurst Longitude + * - 3 + - HGS_Lat + - deg + - float + - HGS_Lat (23.61954406) - HeliographicStonyhurst Latitide + * - 4 + - HGS_distance + - AU + - float + - HGS_distance (0.004484606346) - HeliographicStonyhurst distance in Astronomical Units + * - 5 + - HARP_number + - index + - int + - HARP number - Number associated to the Active Region + * - 6 + - datetime + - UTC + - datetime + - datetime (2012-09-14T03:00:03+00:00) - Time of the HMI image + * - 7 + - R_UTOV + - + - float + - R_UTOV (3.3818) - Value of the R parameter + * - 8 + - D + - + - int + - D (1) - Value of the D parameter + * - 9 + - X_pos + - pixel + - float + - X_pos (1612.9648) - Solar X position of the AR centre in HMI image pixels + * - 10 + - Y_pos + - pixel + - float + - Y_pos (720.9119) - Solar Y position of the AR centre in HMI image pixels + * - 11 + - R_Sun + - pixel + - float + - R_Sun (1891.4001) - Solar radius in HMI image pixels diff --git a/docs/source/products/data/unitov_vel_tsst_image.rst b/docs/source/products/data/unitov_vel_tsst_image.rst index d2979da..e534529 100644 --- a/docs/source/products/data/unitov_vel_tsst_image.rst +++ b/docs/source/products/data/unitov_vel_tsst_image.rst @@ -1,45 +1,133 @@ -========================================= -UNITOV TSST Full Disk Velocity Maps -========================================= +============================ +TSST Full Disk Velocity Maps +============================ .. contents:: The tiny table of contents The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. -**Providers**: +**References** -- **TSST** - source: - - MOF - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-29T12:32:27+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description +Data description ~~~~~~~~~~~~~~~~ -| **Data type**: image - -| **Data formats**: - .fits - - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion -- ext2220.1: Standard Visualisation: Web GUI -- ext2220.2: Standard Query: Web GUI -- ext2220.3: Download: Web GUI -- ext2220.4: NRT Visualisation: Web GUI -- ext2230.1: Advanced Visualisation: ASPIS.py -- ext2230.2: Advanced Query: ASPIS.py -- ext2230.3: Download: ASPIS.py - +**internal_name:** unitov_vel_tsst_image + +**publisher:** University of Rome Tor Vergata + +**alphanumeric_code:** 1B + +**id_tmp:** 61 + +**short_name:** TSST-vel + +**identifier:** aspis:///unitov/vel_tsst_image + +**dynamic:** data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares + +**size:** 300GB + +**format:** .fits + +**type:** image + +**records_number:** 10 + +**time_start:** 2022-09-01 + +**time_stop:** 2023-05-01 + +**spatial:** SUN + +**messenger:** photons + +**spectral_min:** 769.88 + +**spectral_max:** 769.92 + +**spectral_units:** nm + +**observable:** phys.veloc,AR + +**latest update:** 2024-03-28 05:08:18 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC - datetime - Acquisition time + * - 2 + - Quality + - 0-1 + - float + - Quality of the image 0-1 0=bad, 1=OK + * - 3 + - X_cen + - pixel + - int + - Position of the Solar centre on the X image axis [pixels] + * - 4 + - Y_cen + - pixel + - int + - Position of the Solar centre on the Y image axis [pixels] + * - 5 + - R_sun + - pixel + - int + - Radius of the Solar disk [pixels] + * - 6 + - min + - m/s + - float + - minimum value of the image [ADU] + * - 7 + - Max + - m/s + - float + - maximum value of the image [ADU] + * - 8 + - mean + - m/s + - float + - average value of the image [ADU] + * - 9 + - std + - m/s + - float + - standard deviation value of the image [ADU] + * - 10 + - B0 + - deg + - float + - apparent tilt of the sun's axis of rotation with respect to the ecliptic [degrees] + * - 11 + - data_name + - char + - string + - the name of the file with the data + * - 12 + - prew_name + - char + - string + - the name of the full preview file + * - 13 + - thumb_name + - char + - string + - the name of the thumbnail file -- GitLab From 3068206d211f6f92940576e1b93b9bfae8e0e820 Mon Sep 17 00:00:00 2001 From: stefano scardigli Date: Wed, 10 Apr 2024 12:54:24 +0200 Subject: [PATCH 2/2] yes yes yes... --- .../data/external_ace_swepam_timeseries.rst | 92 ++++++++--------- .../data/external_flux_goes_timeseries.rst | 92 ++++++++--------- .../data/external_part_goes_timeseries.rst | 92 ++++++++--------- .../data/inaf_cpcp_superdarn_datacube.rst | 92 ++++++++--------- .../data/inaf_data_solopas_timeseries.rst | 92 ++++++++--------- .../data/inaf_flux1h_svirco_timeseries.rst | 98 ++++++++++--------- .../data/inaf_flux5m_svirco_timeseries.rst | 98 ++++++++++--------- .../products/data/inaf_gsmaps_datacube.rst | 98 ++++++++++--------- .../products/data/inaf_m2flare_tableset.rst | 98 ++++++++++--------- .../products/data/inaf_na_mercexo_image.rst | 92 ++++++++--------- .../products/data/inaf_s1sep_tableset.rst | 98 ++++++++++--------- .../products/data/inaf_s2sep_tableset.rst | 98 ++++++++++--------- .../products/data/inaf_tps_datacube.rst | 98 ++++++++++--------- .../data/inaf_vbcorr_wind_tableset.rst | 92 ++++++++--------- .../products/data/infn_cses_hepd_spectrum.rst | 92 ++++++++--------- .../data/infn_iss_ams_flux_timeseries.rst | 92 ++++++++--------- .../data/infn_pamela_flux_timeseries.rst | 92 ++++++++--------- .../data/infn_saandose_samadha_timeseries.rst | 92 ++++++++--------- .../data/infn_tgndose_samadha_timeseries.rst | 92 ++++++++--------- .../data/ingv_alert_aqu_timeseries.rst | 98 ++++++++++--------- .../data/ingv_alert_cts_timeseries.rst | 98 ++++++++++--------- .../data/ingv_alert_dur_timeseries.rst | 98 ++++++++++--------- .../data/ingv_alert_int_timeseries.rst | 92 ++++++++--------- .../data/ingv_alert_lmp_timeseries.rst | 98 ++++++++++--------- .../data/ingv_alert_wdc_timeseries.rst | 92 ++++++++--------- .../data/ingv_autoiono_bbla_timeseries.rst | 92 ++++++++--------- .../data/ingv_autoiono_gibi_timeseries.rst | 92 ++++++++--------- .../data/ingv_autoiono_rome_timeseries.rst | 92 ++++++++--------- .../data/ingv_autoiono_tucu_timeseries.rst | 92 ++++++++--------- .../products/data/ingv_b_swarm_image.rst | 98 ++++++++++--------- .../products/data/ingv_b_swarm_timeseries.rst | 98 ++++++++++--------- .../data/ingv_bvect_cses_tableset.rst | 98 ++++++++++--------- .../data/ingv_evect_cses_tableset.rst | 98 ++++++++++--------- .../products/data/ingv_gic_aqu_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_cts_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_dur_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_int_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_lmp_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_wdc_timeseries.rst | 98 ++++++++++--------- .../data/ingv_ltmuf_cagliari_tableset.rst | 98 ++++++++++--------- .../data/ingv_ltmuf_catania_tableset.rst | 98 ++++++++++--------- .../data/ingv_ltmuf_milan_tableset.rst | 98 ++++++++++--------- .../data/ingv_ltmuf_rome_tableset.rst | 98 ++++++++++--------- .../products/data/ingv_mag_aqu_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_cts_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_dmc_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_dur_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_int_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_lmp_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_tnb_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_wdc_timeseries.rst | 98 ++++++++++--------- .../data/ingv_magdef_cts_timeseries.rst | 98 ++++++++++--------- .../data/ingv_magdef_dur_timeseries.rst | 98 ++++++++++--------- .../data/ingv_ncmuf_cagliari_tableset.rst | 98 ++++++++++--------- .../data/ingv_ncmuf_catania_tableset.rst | 98 ++++++++++--------- .../data/ingv_ncmuf_milan_tableset.rst | 98 ++++++++++--------- .../data/ingv_ncmuf_rome_tableset.rst | 98 ++++++++++--------- .../data/ingv_valiiono_gibi_timeseries.rst | 98 ++++++++++--------- .../data/ingv_valiiono_rome_timeseries.rst | 98 ++++++++++--------- .../data/uniaq_curr_maigic_tableset.rst | 98 ++++++++++--------- .../data/uniaq_epmde_emma_timeseries.rst | 98 ++++++++++--------- .../data/uniaq_field_maigic_tableset.rst | 98 ++++++++++--------- .../data/uniaq_mag_emma_timeseries.rst | 98 ++++++++++--------- .../data/unical_espseptransport_tableset.rst | 92 ++++++++--------- .../products/data/unical_sep_ace_spectrum.rst | 98 ++++++++++--------- .../products/data/unical_sep_psp_spectrum.rst | 98 ++++++++++--------- .../data/unical_sep_soho_spectrum.rst | 98 ++++++++++--------- .../data/unical_sep_solo_spectrum.rst | 98 ++++++++++--------- .../data/unical_sep_stra_spectrum.rst | 98 ++++++++++--------- .../data/unical_sep_wind_spectrum.rst | 98 ++++++++++--------- .../data/unical_shockpar_tableset.rst | 92 ++++++++--------- .../products/data/unict_facula_image.rst | 92 ++++++++--------- .../products/data/unict_filament_image.rst | 92 ++++++++--------- .../products/data/unict_offlimb_image.rst | 92 ++++++++--------- .../products/data/unict_sunspot_image.rst | 92 ++++++++--------- .../data/unitn_flux_cses_timeseries.rst | 98 ++++++++++--------- .../data/unitov_halpha_tsst_image.rst | 98 ++++++++++--------- .../products/data/unitov_icme_tableset.rst | 98 ++++++++++--------- .../data/unitov_iss_lidal_timeseries.rst | 92 ++++++++--------- .../products/data/unitov_mag_tsst_image.rst | 98 ++++++++++--------- .../data/unitov_rdparameter_tableset.rst | 98 ++++++++++--------- .../products/data/unitov_vel_tsst_image.rst | 98 ++++++++++--------- 82 files changed, 4107 insertions(+), 3779 deletions(-) diff --git a/docs/source/products/data/external_ace_swepam_timeseries.rst b/docs/source/products/data/external_ace_swepam_timeseries.rst index cd21da0..4be227e 100644 --- a/docs/source/products/data/external_ace_swepam_timeseries.rst +++ b/docs/source/products/data/external_ace_swepam_timeseries.rst @@ -2,56 +2,60 @@ ACE Solar Wind 1 min ==================== -.. contents:: The tiny table of contents +.. contents:: Table of contents qui dovra' esserci la descrizione del prodotto -**References** +References +~~~~~~~~~~ qui invece la bibliografia -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** external_ace_swepam_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 101A - -**id_tmp:** 101 - -**short_name:** ace_1minute - -**identifier:** aspis:///external/ace_swepam_timeseries - -**dynamic:** Approx 2MB every week - -**size:** 100kB - -**format:** csv - -**type:** timeseries - -**records_number:** 21599 - -**time_start:** 2016-12-14 - -**time_stop:** 2020-12-31 - -**spatial:** L1 - -**messenger:** protons,electrons - -**spectral_min:** 0.26 - -**spectral_max:** 36 - -**spectral_units:** keV - -**observable:** CME,SW,SEP - -**latest update:** 2024-03-29 12:01:32 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - external_ace_swepam_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 101A + * - **id_tmp:** + - 101 + * - **short_name:** + - ace_1minute + * - **identifier:** + - aspis:///external/ace_swepam_timeseries + * - **dynamic:** + - Approx 2MB every week + * - **size:** + - 100kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 21599 + * - **time_start:** + - 2016-12-14 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - L1 + * - **messenger:** + - protons,electrons + * - **spectral_min:** + - 0.26 + * - **spectral_max:** + - 36 + * - **spectral_units:** + - keV + * - **observable:** + - CME,SW,SEP + * - **latest update:** + - 2024-03-29 12:01:32 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/external_flux_goes_timeseries.rst b/docs/source/products/data/external_flux_goes_timeseries.rst index 52fe3ff..766cd96 100644 --- a/docs/source/products/data/external_flux_goes_timeseries.rst +++ b/docs/source/products/data/external_flux_goes_timeseries.rst @@ -2,56 +2,60 @@ GOES X-ray Flux =============== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** external_flux_goes_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 102A - -**id_tmp:** 102 - -**short_name:** goesx1min - -**identifier:** aspis:///external/flux_goes_timeseries - -**dynamic:** Approx 1MB every week - -**size:** 5MB - -**format:** csv - -**type:** timeseries - -**records_number:** 21599 - -**time_start:** 2016-12-14 - -**time_stop:** 2020-12-31 - -**spatial:** L1 - -**messenger:** photons - -**spectral_min:** 1 - -**spectral_max:** 8 - -**spectral_units:** Angstrom - -**observable:** flare - -**latest update:** 2024-03-28 05:08:04 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - external_flux_goes_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 102A + * - **id_tmp:** + - 102 + * - **short_name:** + - goesx1min + * - **identifier:** + - aspis:///external/flux_goes_timeseries + * - **dynamic:** + - Approx 1MB every week + * - **size:** + - 5MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 21599 + * - **time_start:** + - 2016-12-14 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - L1 + * - **messenger:** + - photons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 8 + * - **spectral_units:** + - Angstrom + * - **observable:** + - flare + * - **latest update:** + - 2024-03-28 05:08:04 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/external_part_goes_timeseries.rst b/docs/source/products/data/external_part_goes_timeseries.rst index ee4b7f3..f179e8f 100644 --- a/docs/source/products/data/external_part_goes_timeseries.rst +++ b/docs/source/products/data/external_part_goes_timeseries.rst @@ -2,56 +2,60 @@ GOES proton Flux ================ -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** external_part_goes_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 103A - -**id_tmp:** 103 - -**short_name:** GOES_particle1min - -**identifier:** aspis:///external/part_goes_timeseries - -**dynamic:** Approx 2MB every week - -**size:** 2MB - -**format:** csv - -**type:** timeseries - -**records_number:** 4319 - -**time_start:** 2016-12-14 - -**time_stop:** 2020-12-31 - -**spatial:** L1 - -**messenger:** protons,electrons - -**spectral_min:** 1 - -**spectral_max:** 100 - -**spectral_units:** MeV - -**observable:** flare,SEP,CME,ESP,SW - -**latest update:** 2024-03-28 05:08:04 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - external_part_goes_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 103A + * - **id_tmp:** + - 103 + * - **short_name:** + - GOES_particle1min + * - **identifier:** + - aspis:///external/part_goes_timeseries + * - **dynamic:** + - Approx 2MB every week + * - **size:** + - 2MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 4319 + * - **time_start:** + - 2016-12-14 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - L1 + * - **messenger:** + - protons,electrons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - flare,SEP,CME,ESP,SW + * - **latest update:** + - 2024-03-28 05:08:04 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst b/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst index 8e2d31c..e6f1162 100644 --- a/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst +++ b/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst @@ -2,7 +2,7 @@ SuperDARN Polar Cap Potential ============================= -.. contents:: The tiny table of contents +.. contents:: Table of contents The Super Dual Auroral Radar Network (SuperDARN) is an international network of High Frequency coherent scatter radars. A map of the fields of view of the radars @@ -22,7 +22,8 @@ As ionospheric irregularities are dragged in the large scale convection at high allows to infer the velocity of the ambient plasma with respect to the sounded direction and gate. -**References** +References +~~~~~~~~~~ https://www.sciencedirect.com/science/article/abs/pii/S136468260600263X @@ -48,48 +49,51 @@ https://doi.org/10.1002/2018JA025280 and Functional Approximations, J. Geophys. Res., Space Physics, 119(9), 7501-7521 (2014). https://doi.org/10.1002/2014JA020264 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_cpcp_superdarn_datacube - -**publisher:** INAF - -**alphanumeric_code:** 31 - -**id_tmp:** 71 - -**short_name:** SuperDARN CPCP - -**identifier:** aspis://inaf/cpcp_superdarn_datacube - -**dynamic:** static - -**size:** 200MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1515672 - -**time_start:** 2015-06-21 - -**time_stop:** 2017-09-11 - -**spatial:** IONO - -**messenger:** electrons, - -**spectral_min:** 0 - -**spectral_max:** 1 - -**spectral_units:** dimensionless - -**observable:** IMF,GEOINDEX - -**latest update:** 2024-04-04 01:53:25 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_cpcp_superdarn_datacube + * - **publisher:** + - INAF + * - **alph_code:** + - 31 + * - **id_tmp:** + - 71 + * - **short_name:** + - SuperDARN CPCP + * - **identifier:** + - aspis://inaf/cpcp_superdarn_datacube + * - **dynamic:** + - static + * - **size:** + - 200MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1515672 + * - **time_start:** + - 2015-06-21 + * - **time_stop:** + - 2017-09-11 + * - **spatial:** + - IONO + * - **messenger:** + - electrons, + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - dimensionless + * - **observable:** + - IMF,GEOINDEX + * - **latest update:** + - 2024-04-04 01:53:25 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_data_solopas_timeseries.rst b/docs/source/products/data/inaf_data_solopas_timeseries.rst index cb30f8d..b7d8d36 100644 --- a/docs/source/products/data/inaf_data_solopas_timeseries.rst +++ b/docs/source/products/data/inaf_data_solopas_timeseries.rst @@ -2,14 +2,15 @@ INAF-IAPS Solar Orbiter-PAS data ================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The product contains density N, speed vector V, pressure tensor P, temperature components (Tx, Ty, Tz), and the velocity of the satellite V_solo, computed using the data collected by the Proton-Alpha Sensor (PAS) onboard Solar Orbiter. PAS measures the 3D distribution functions of the dominant ions of the solar wind, from 200 eV to 20 KeV, without mass and charge selection. In practice, this concerns mostly the proton and alfa populations (unseparated). At full resolution, PAS collects the 3D ion distribution function in about 1 second, even though the moments have a cadence of 4 seconds, while in “snapshot” mode the phase space sampling is reduced, allowing a greater cadence for the moments. Data is hosted on http://soar.esac.esa.int/soar/ -**References** +References +~~~~~~~~~~ R. D’Amicis et al, Astronomy &Astrophysics 656, A21 (2021) @@ -19,48 +20,51 @@ D. Perrone et al, Astronomy &Astrophysics 668, A189 (2022) R. De Marco et al, Astronomy &Astrophysics, 669, A108 (2023) -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_data_solopas_timeseries - -**publisher:** INAF-IAPS, Plasma & Space Weather Group - -**alphanumeric_code:** 14 - -**id_tmp:** 72 - -**short_name:** SolO-PAS_data - -**identifier:** aspis://inaf/data_solopas_timeseries - -**dynamic:** a file each day (file size between 3 and 4 Mb). As a general rule, one month of data is uploaded each month, generally relating to 3 months before the upload date - -**size:** 2GB - -**format:** dsv - -**type:** timeseries - -**records_number:** 38653 - -**time_start:** 2020-07-06 - -**time_stop:** 2022-01-31 - -**spatial:** IP - -**messenger:** Protons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** SW,SEP - -**latest update:** 2024-04-04 01:54:59 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_data_solopas_timeseries + * - **publisher:** + - INAF-IAPS, Plasma & Space Weather Group + * - **alph_code:** + - 14 + * - **id_tmp:** + - 72 + * - **short_name:** + - SolO-PAS_data + * - **identifier:** + - aspis://inaf/data_solopas_timeseries + * - **dynamic:** + - a file each day (file size between 3 and 4 Mb). As a general rule, one month of data is uploaded each month, generally relating to 3 months before the upload date + * - **size:** + - 2GB + * - **format:** + - dsv + * - **type:** + - timeseries + * - **records_number:** + - 38653 + * - **time_start:** + - 2020-07-06 + * - **time_stop:** + - 2022-01-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - SW,SEP + * - **latest update:** + - 2024-04-04 01:54:59 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst b/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst index ece0c56..3542b5c 100644 --- a/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst +++ b/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst @@ -2,56 +2,60 @@ SVIRCO Observatory - the Rome neutron monitor ============================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 1h. Average intensity of January-February 1997 = 100% -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_flux1h_svirco_timeseries - -**publisher:** INAF - -**alphanumeric_code:** 42C - -**id_tmp:** 73 - -**short_name:** flux1h_SVIRCO - -**identifier:** inaf_flux1h_svirco_timeseries - -**dynamic:** Data collection grows in time. - -**size:** 13MB - -**format:** CSV - -**type:** timeseries - -**records_number:** 479976 - -**time_start:** 1966-04-01 - -**time_stop:** 2020-12-31 - -**spatial:** GROUND - -**messenger:** Nucleons - -**spectral_min:** 6.3 - -**spectral_max:** 9999 - -**spectral_units:** GeV - -**observable:** GLE,GCR - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_flux1h_svirco_timeseries + * - **publisher:** + - INAF + * - **alph_code:** + - 42C + * - **id_tmp:** + - 73 + * - **short_name:** + - flux1h_SVIRCO + * - **identifier:** + - inaf_flux1h_svirco_timeseries + * - **dynamic:** + - Data collection grows in time. + * - **size:** + - 13MB + * - **format:** + - CSV + * - **type:** + - timeseries + * - **records_number:** + - 479976 + * - **time_start:** + - 1966-04-01 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - GROUND + * - **messenger:** + - Nucleons + * - **spectral_min:** + - 6.3 + * - **spectral_max:** + - 9999 + * - **spectral_units:** + - GeV + * - **observable:** + - GLE,GCR + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst b/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst index 3248096..8e7960b 100644 --- a/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst +++ b/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst @@ -2,56 +2,60 @@ SVIRCO Obser vatory - the Rome neutron monitor ============================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 5min Average intensity of January-February 1997 = 100% -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_flux5m_svirco_timeseries - -**publisher:** INAF - -**alphanumeric_code:** 42B - -**id_tmp:** 74 - -**short_name:** flux5m_SVIRCO - -**identifier:** inaf_flux5m_svirco_timeseries - -**dynamic:** Data collection grows in time. - -**size:** 80MB - -**format:** CSV - -**type:** timeseries - -**records_number:** 2007072 - -**time_start:** 1997-05-21 - -**time_stop:** 2017-01-01 - -**spatial:** GROUND - -**messenger:** Neutrons - -**spectral_min:** 6.3 - -**spectral_max:** 9999 - -**spectral_units:** GeV - -**observable:** GLE,GCR - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_flux5m_svirco_timeseries + * - **publisher:** + - INAF + * - **alph_code:** + - 42B + * - **id_tmp:** + - 74 + * - **short_name:** + - flux5m_SVIRCO + * - **identifier:** + - inaf_flux5m_svirco_timeseries + * - **dynamic:** + - Data collection grows in time. + * - **size:** + - 80MB + * - **format:** + - CSV + * - **type:** + - timeseries + * - **records_number:** + - 2007072 + * - **time_start:** + - 1997-05-21 + * - **time_stop:** + - 2017-01-01 + * - **spatial:** + - GROUND + * - **messenger:** + - Neutrons + * - **spectral_min:** + - 6.3 + * - **spectral_max:** + - 9999 + * - **spectral_units:** + - GeV + * - **observable:** + - GLE,GCR + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_gsmaps_datacube.rst b/docs/source/products/data/inaf_gsmaps_datacube.rst index 60bd736..1867a25 100644 --- a/docs/source/products/data/inaf_gsmaps_datacube.rst +++ b/docs/source/products/data/inaf_gsmaps_datacube.rst @@ -2,56 +2,60 @@ IAPS Grad-Shafranov Reconstruction of Magnetic Clouds ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Quasi 3-d magnetic field maps of magnetic field configuration within magnetic clouds for geoeffective target SWE events. Such maps will be estimated through the Grad-Shafranov reconstruction from single-spacecraft plasma and magnetic field data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_gsmaps_datacube - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 25 - -**id_tmp:** 96 - -**short_name:** gsmaps-cubes - -**identifier:** aspis://inaf/gsmaps_datacube - -**dynamic:** static - -**size:** 300kB - -**format:** nc - -**type:** spectrum - -**records_number:** 3 - -**time_start:** 1997-01-01 - -**time_stop:** 2022-01-01 - -**spatial:** IP - -**messenger:** Magnetic field,Magnetic vector potential,Flux rope coordinates - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** phys.magField,phys.potential,phys.size - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_gsmaps_datacube + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 25 + * - **id_tmp:** + - 96 + * - **short_name:** + - gsmaps-cubes + * - **identifier:** + - aspis://inaf/gsmaps_datacube + * - **dynamic:** + - static + * - **size:** + - 300kB + * - **format:** + - nc + * - **type:** + - spectrum + * - **records_number:** + - 3 + * - **time_start:** + - 1997-01-01 + * - **time_stop:** + - 2022-01-01 + * - **spatial:** + - IP + * - **messenger:** + - Magnetic field,Magnetic vector potential,Flux rope coordinates + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - phys.magField,phys.potential,phys.size + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_m2flare_tableset.rst b/docs/source/products/data/inaf_m2flare_tableset.rst index 5511286..b7baee1 100644 --- a/docs/source/products/data/inaf_m2flare_tableset.rst +++ b/docs/source/products/data/inaf_m2flare_tableset.rst @@ -2,56 +2,60 @@ IAPS ≥M2 SXR Flare Catalogue ============================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The catalogue will contain the > M2 Soft X- Ray (SXR) flares from 1995 to 2017. The columns in the table are defined as follows: (1) event number (2) date of the SXR flare (3) peak time of SXR flare (4) peak SXR classification (saturated events flagged with an S in which case (3) refers to the onset of saturation), (5) flare location, (6) time-integrated SXR intensity (nominally between the 1/3 power points on rise and fall), (7) time-integrated 1 MHz Wind/WAVES intensity from 10 minutes before the onset of integration for the SXR burst to 10 minutes after the SXR burst peak, (8) Waves frequency used. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_m2flare_tableset - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 7 - -**id_tmp:** 75 - -**short_name:** IAPS-M2SXR - -**identifier:** aspis://inaf/m2flare_tableset - -**dynamic:** static - -**size:** 100kB - -**format:** xlsx - -**type:** tableset - -**records_number:** 1040 - -**time_start:** 1995-01-01 - -**time_stop:** 2017-05-03 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** phys.flux - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_m2flare_tableset + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 7 + * - **id_tmp:** + - 75 + * - **short_name:** + - IAPS-M2SXR + * - **identifier:** + - aspis://inaf/m2flare_tableset + * - **dynamic:** + - static + * - **size:** + - 100kB + * - **format:** + - xlsx + * - **type:** + - tableset + * - **records_number:** + - 1040 + * - **time_start:** + - 1995-01-01 + * - **time_stop:** + - 2017-05-03 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - phys.flux + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_na_mercexo_image.rst b/docs/source/products/data/inaf_na_mercexo_image.rst index 3c2ad68..c580787 100644 --- a/docs/source/products/data/inaf_na_mercexo_image.rst +++ b/docs/source/products/data/inaf_na_mercexo_image.rst @@ -2,11 +2,12 @@ INAF-bidimensional maps of Mercury Na exosphere =============================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Dataset of observations of Mercury's exosphere in the sodium D lines. Data are taken from the ground-based solar telescope THEMIS (years 2009-2013). They have been produced in both D1 and D2 lines (when both available) and converted into bi-dimensional maps of Rayleigh emission. Estimation of the “seeing” parameter is included in the jpeg files. Here the original fits files are given too for the whole data base (2007-2014), and it may be expanded to the most recent data from 2021 and 2022 (TBC). Data can be provided both uncalibrated and/or calibrated (TBD). -**References** +References +~~~~~~~~~~ Leblanc, F., Doressoundiram, A., Schneider, N., Mangano, V., López Ariste, A., Lemen, C., Gelly, B., Barbieri, C. and Cremonese, G., 2008. High latitude peaks in Mercury's sodium exosphere: Spectral signature using THEMIS solar telescope. Geophysical Research Letters, 35(18). @@ -20,48 +21,51 @@ Massetti, S., Mangano, V., Milillo, A., Mura, A., Orsini, S. and Plainaki, C., 2 Orsini, S., Mangano, V., Milillo, A., Plainaki, C., Mura, A., Raines, J.M., De Angelis, E., Rispoli, R., Lazzarotto, F. and Aronica, A., 2018. Mercury sodium exospheric emission as a proxy for solar perturbations transit. Scientific reports, 8(1), p.928. -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_na_mercexo_image - -**publisher:** Valeria Mangano, INAF-IAPS - -**alphanumeric_code:** 57 - -**id_tmp:** 76 - -**short_name:** Merc_exos_Na_fts - -**identifier:** aspis://inaf/na_mercexo_image - -**dynamic:** period 2009-2013 is static, but if we decide to include also most recent data, it will grow in time. - -**size:** 1GB - -**format:** fits - -**type:** image - -**records_number:** 7 - -**time_start:** 2009-04-17 - -**time_stop:** 2013-05-25 - -**spatial:** Mercury - -**messenger:** photons - -**spectral_min:** 5890 - -**spectral_max:** 5896 - -**spectral_units:** Angstrom - -**observable:** IMF,SW,CME - -**latest update:** 2024-04-04 01:59:34 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_na_mercexo_image + * - **publisher:** + - Valeria Mangano, INAF-IAPS + * - **alph_code:** + - 57 + * - **id_tmp:** + - 76 + * - **short_name:** + - Merc_exos_Na_fts + * - **identifier:** + - aspis://inaf/na_mercexo_image + * - **dynamic:** + - period 2009-2013 is static, but if we decide to include also most recent data, it will grow in time. + * - **size:** + - 1GB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 7 + * - **time_start:** + - 2009-04-17 + * - **time_stop:** + - 2013-05-25 + * - **spatial:** + - Mercury + * - **messenger:** + - photons + * - **spectral_min:** + - 5890 + * - **spectral_max:** + - 5896 + * - **spectral_units:** + - Angstrom + * - **observable:** + - IMF,SW,CME + * - **latest update:** + - 2024-04-04 01:59:34 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_s1sep_tableset.rst b/docs/source/products/data/inaf_s1sep_tableset.rst index 1e164d2..f60fb57 100644 --- a/docs/source/products/data/inaf_s1sep_tableset.rst +++ b/docs/source/products/data/inaf_s1sep_tableset.rst @@ -2,56 +2,60 @@ IAPS S1 SEP events Catalogue ============================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The catalogue contains SEP events observed at the Earth of class S1, i.e. with flux in the range [10, 100) pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux >= 100 pfu at > 10 MeV are listed in the companion table S2 SEP Catalogue. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_s1sep_tableset - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 16A - -**id_tmp:** 77 - -**short_name:** IAPS-S1 SEP events - -**identifier:** aspis://inaf/s1sep_tableset - -**dynamic:** static - -**size:** 100kB - -**format:** csv - -**type:** tableset - -**records_number:** 68 - -**time_start:** 1995-01-01 - -**time_stop:** 2014-09-10 - -**spatial:** Earth - -**messenger:** Protons,Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** flare,CME,SEP - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_s1sep_tableset + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 16A + * - **id_tmp:** + - 77 + * - **short_name:** + - IAPS-S1 SEP events + * - **identifier:** + - aspis://inaf/s1sep_tableset + * - **dynamic:** + - static + * - **size:** + - 100kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 68 + * - **time_start:** + - 1995-01-01 + * - **time_stop:** + - 2014-09-10 + * - **spatial:** + - Earth + * - **messenger:** + - Protons,Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - flare,CME,SEP + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_s2sep_tableset.rst b/docs/source/products/data/inaf_s2sep_tableset.rst index 717b419..0963e5a 100644 --- a/docs/source/products/data/inaf_s2sep_tableset.rst +++ b/docs/source/products/data/inaf_s2sep_tableset.rst @@ -2,56 +2,60 @@ IAPS S2 SEP events Catalogue ============================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The catalogue contains SEP events observed at the Earth of class S2, i.e. with flux >100 pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux in the interval [10, 100) pfu at > 10 MeV are listed in the companion table S1 SEP Catalogue. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_s2sep_tableset - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 16B - -**id_tmp:** 78 - -**short_name:** IAPS-S2 SEP events - -**identifier:** aspis://inaf/s1sep_tableset - -**dynamic:** static - -**size:** 100kB - -**format:** csv - -**type:** tableset - -**records_number:** 60 - -**time_start:** 1995-01-01 - -**time_stop:** 2014-09-10 - -**spatial:** Earth - -**messenger:** Protons,Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** flare,CME,SEP - -**latest update:** 2024-03-28 05:08:06 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_s2sep_tableset + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 16B + * - **id_tmp:** + - 78 + * - **short_name:** + - IAPS-S2 SEP events + * - **identifier:** + - aspis://inaf/s1sep_tableset + * - **dynamic:** + - static + * - **size:** + - 100kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 60 + * - **time_start:** + - 1995-01-01 + * - **time_stop:** + - 2014-09-10 + * - **spatial:** + - Earth + * - **messenger:** + - Protons,Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - flare,CME,SEP + * - **latest update:** + - 2024-03-28 05:08:06 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_tps_datacube.rst b/docs/source/products/data/inaf_tps_datacube.rst index 8e6184b..7777305 100644 --- a/docs/source/products/data/inaf_tps_datacube.rst +++ b/docs/source/products/data/inaf_tps_datacube.rst @@ -2,56 +2,60 @@ IAPS Test Particle Simulation on Magnetic Clouds ================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents Galactic cosmic ray intensity variations associated to the passage of magnetic clouds. The particle intensity variation is estimated through a dedicated full-orbit test-particle simulation. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_tps_datacube - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 51 - -**id_tmp:** 97 - -**short_name:** IAPS-TPS - -**identifier:** aspis://inaf/tps_datacube - -**dynamic:** static - -**size:** 300kB - -**format:** nc - -**type:** spectrum - -**records_number:** 3 - -**time_start:** 1997-01-01 - -**time_stop:** 2022-01-01 - -**spatial:** Interplanetary Space (not L1 and Planets),Sun-Earth L1 - -**messenger:** Particle intensity variation - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** phys.flux,phys.particle.proton - -**latest update:** 2024-03-28 05:08:06 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_tps_datacube + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 51 + * - **id_tmp:** + - 97 + * - **short_name:** + - IAPS-TPS + * - **identifier:** + - aspis://inaf/tps_datacube + * - **dynamic:** + - static + * - **size:** + - 300kB + * - **format:** + - nc + * - **type:** + - spectrum + * - **records_number:** + - 3 + * - **time_start:** + - 1997-01-01 + * - **time_stop:** + - 2022-01-01 + * - **spatial:** + - Interplanetary Space (not L1 and Planets),Sun-Earth L1 + * - **messenger:** + - Particle intensity variation + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - phys.flux,phys.particle.proton + * - **latest update:** + - 2024-03-28 05:08:06 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_vbcorr_wind_tableset.rst b/docs/source/products/data/inaf_vbcorr_wind_tableset.rst index ad9a0c6..46cb275 100644 --- a/docs/source/products/data/inaf_vbcorr_wind_tableset.rst +++ b/docs/source/products/data/inaf_vbcorr_wind_tableset.rst @@ -2,11 +2,12 @@ IAPS - Wind velocity-magnetic field correlation coefficient data of solar wind streams ====================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The velocity - magnetic field (v-b) correlation coefficient unables to identify Alfvénic solar wind intervals (along with almost constant magnetic field magnitude and proton number density). It is derived as the ratio between the covariance of velocity and magnetic field (in Alfvén units) components and the product of their standard deviations, in a time window ranging between tens of minutes to hours. In principle, this formula should be applied to every component of the velocity (V_i) and magnetic fields (B_i) (with i = R, T, N in RTN coordinate system or i = X, Y, Z in GSE coordinate system). The total correlation coefficient is then derived as the average from the three components. However, for the sake of simplicity, we consider only the N component since more Alfvénic than the other two. -**References** +References +~~~~~~~~~~ D’Amicis et al, GRL, 34, L05108, 2007; Frontiers in Physics, 8, 541, 2020 @@ -16,48 +17,51 @@ D’Amicis et al, A&A, 656, A21, 2021 Tu et al., JGR, 94, 11739, 1989 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_vbcorr_wind_tableset - -**publisher:** INAF-IAPS, Fisica dei Plasmi Spaziali e Space Weather - -**alphanumeric_code:** 24C - -**id_tmp:** 98 - -**short_name:** wind_v-b_corr - -**identifier:** aspis://inaf/vbcorr_wind_tableset - -**dynamic:** static - -**size:** 35MB - -**format:** csv - -**type:** tableset - -**records_number:** 538 - -**time_start:** 1998-10-01 - -**time_stop:** 2022-05-06 - -**spatial:** L1 - -**messenger:** protons - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - - -**observable:** SW - -**latest update:** 2024-04-04 02:05:02 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_vbcorr_wind_tableset + * - **publisher:** + - INAF-IAPS, Fisica dei Plasmi Spaziali e Space Weather + * - **alph_code:** + - 24C + * - **id_tmp:** + - 98 + * - **short_name:** + - wind_v-b_corr + * - **identifier:** + - aspis://inaf/vbcorr_wind_tableset + * - **dynamic:** + - static + * - **size:** + - 35MB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 538 + * - **time_start:** + - 1998-10-01 + * - **time_stop:** + - 2022-05-06 + * - **spatial:** + - L1 + * - **messenger:** + - protons + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - - + * - **observable:** + - SW + * - **latest update:** + - 2024-04-04 02:05:02 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_cses_hepd_spectrum.rst b/docs/source/products/data/infn_cses_hepd_spectrum.rst index c52aa74..101557c 100644 --- a/docs/source/products/data/infn_cses_hepd_spectrum.rst +++ b/docs/source/products/data/infn_cses_hepd_spectrum.rst @@ -2,56 +2,60 @@ HEPD-01 time-integrated proton spectrum during the Ground-Level Enhancement of October 28, 2021 =============================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Time-integrated spectrum of solar protons measured by the HEPD-01 detector from space during the Ground-Level Enhancement of October 28, 2021 -**References** +References +~~~~~~~~~~ https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2022SW003191 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_cses_hepd_spectrum - -**publisher:** not available in DBF - -**alphanumeric_code:** 44C - -**id_tmp:** 106 - -**short_name:** HEPD-proton - -**identifier:** aspis://infn/infn_cses_hepd_spectrum - -**dynamic:** - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 1 - -**time_start:** 2021-10-28 - -**time_stop:** 2021-11-03 - -**spatial:** GEOMAG - -**messenger:** protons - -**spectral_min:** 55 - -**spectral_max:** 250 - -**spectral_units:** MeV - -**observable:** GLE,flare,SEP,GCR,CME - -**latest update:** 2024-04-04 02:08:35 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_cses_hepd_spectrum + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 44C + * - **id_tmp:** + - 106 + * - **short_name:** + - HEPD-proton + * - **identifier:** + - aspis://infn/infn_cses_hepd_spectrum + * - **dynamic:** + - + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 1 + * - **time_start:** + - 2021-10-28 + * - **time_stop:** + - 2021-11-03 + * - **spatial:** + - GEOMAG + * - **messenger:** + - protons + * - **spectral_min:** + - 55 + * - **spectral_max:** + - 250 + * - **spectral_units:** + - MeV + * - **observable:** + - GLE,flare,SEP,GCR,CME + * - **latest update:** + - 2024-04-04 02:08:35 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_iss_ams_flux_timeseries.rst b/docs/source/products/data/infn_iss_ams_flux_timeseries.rst index fc1c94f..9fc615e 100644 --- a/docs/source/products/data/infn_iss_ams_flux_timeseries.rst +++ b/docs/source/products/data/infn_iss_ams_flux_timeseries.rst @@ -2,56 +2,60 @@ INFN AMS daily proton time dependent fluxes =========================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Daily proton fluxes in cosmic rays were measured with the Alpha Magnetic Spectrometer aboard the International Space Station, from May 20, 2011 to October 29, 2019 (a total of 2824 days or 114 Bartels rotations) in the rigidity interval from 1 to 100 GV, based on 5.5×10^9 protons collected. Several Forbush decreases were also observed during the whole period, in connection with transient magnetic perturbations. The product provides these data as time-profiles from May 20, 2011 to October 29 2019 as a function of rigidity. In particular the daily proton fluxes are measured in 30 bins from 1.00 to 100 GV. The errors include statistics, time-dependent systematic errors and the total systematic error. -**References** +References +~~~~~~~~~~ https://doi.org/10.1103/PhysRevLett.127.271102 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_iss_ams_flux_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 50A - -**id_tmp:** 89 - -**short_name:** AMS_daily_H - -**identifier:** aspis:///infn/ams_protons - -**dynamic:** static - -**size:** 4.1MB - -**format:** csv - -**type:** timeseries - -**records_number:** 83757 - -**time_start:** 2011-05-20 - -**time_stop:** 2019-10-29 - -**spatial:** GEOMAG - -**messenger:** Protons - -**spectral_min:** 1 - -**spectral_max:** 100 - -**spectral_units:** GV - -**observable:** GCR - -**latest update:** 2024-04-04 02:10:23 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_iss_ams_flux_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 50A + * - **id_tmp:** + - 89 + * - **short_name:** + - AMS_daily_H + * - **identifier:** + - aspis:///infn/ams_protons + * - **dynamic:** + - static + * - **size:** + - 4.1MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 83757 + * - **time_start:** + - 2011-05-20 + * - **time_stop:** + - 2019-10-29 + * - **spatial:** + - GEOMAG + * - **messenger:** + - Protons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - GV + * - **observable:** + - GCR + * - **latest update:** + - 2024-04-04 02:10:23 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_pamela_flux_timeseries.rst b/docs/source/products/data/infn_pamela_flux_timeseries.rst index 6573397..1d9f643 100644 --- a/docs/source/products/data/infn_pamela_flux_timeseries.rst +++ b/docs/source/products/data/infn_pamela_flux_timeseries.rst @@ -2,56 +2,60 @@ PAMELA time-profiles of protons during 4 Forbush Decreases ========================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Time-profiles of galactic cosmic-ray protons measured by the PAMELA detector in space during 4 Forbush Decreases from March 2012 to June 2015 in various rigidity intervals. Each profile is scaled for a suitable period of quiet Sun, estimated about 10 days before each Forbush Decrease -**References** +References +~~~~~~~~~~ https://iopscience.iop.org/article/10.3847/1538-4357/aaa0c8 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_pamela_flux_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 50B - -**id_tmp:** 90 - -**short_name:** PAMELA-proton - -**identifier:** aspis://INFN-PAMELA/proton - -**dynamic:** Data collected starts on March 1, 2012 and is increasing with a daily resolution up until July 17, 2015 - -**size:** 200kB - -**format:** csv - -**type:** timeseries - -**records_number:** 2394 - -**time_start:** 2012-03-01 - -**time_stop:** 2015-07-17 - -**spatial:** GEOMAG - -**messenger:** protons - -**spectral_min:** 0.85 - -**spectral_max:** 8.68 - -**spectral_units:** GV - -**observable:** GCR - -**latest update:** 2024-04-04 02:12:29 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_pamela_flux_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 50B + * - **id_tmp:** + - 90 + * - **short_name:** + - PAMELA-proton + * - **identifier:** + - aspis://INFN-PAMELA/proton + * - **dynamic:** + - Data collected starts on March 1, 2012 and is increasing with a daily resolution up until July 17, 2015 + * - **size:** + - 200kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 2394 + * - **time_start:** + - 2012-03-01 + * - **time_stop:** + - 2015-07-17 + * - **spatial:** + - GEOMAG + * - **messenger:** + - protons + * - **spectral_min:** + - 0.85 + * - **spectral_max:** + - 8.68 + * - **spectral_units:** + - GV + * - **observable:** + - GCR + * - **latest update:** + - 2024-04-04 02:12:29 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_saandose_samadha_timeseries.rst b/docs/source/products/data/infn_saandose_samadha_timeseries.rst index b46635f..036958f 100644 --- a/docs/source/products/data/infn_saandose_samadha_timeseries.rst +++ b/docs/source/products/data/infn_saandose_samadha_timeseries.rst @@ -2,56 +2,60 @@ SAMADHA neutron dose rate at Mount Chacaltaya ============================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) is an INFN project aimed to monitor the neutron dose rate due to cosmic rays at the Chacaltaya Station (Bolivia, 5200 m) inside the South Atlantic Anomaly region, to study possible correlation between space weather events and dose rate at the ground, considering the proximity of the Van Allen Belts to the Earth's surface in the SAA region. -**References** +References +~~~~~~~~~~ http://samadha.to.infn.it -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_saandose_samadha_timeseries - -**publisher:** SAMADHA - -**alphanumeric_code:** 75A - -**id_tmp:** 99 - -**short_name:** SAA_Ndose - -**identifier:** aspis://infn/saandose_samadha_timeseries - -**dynamic:** one dataset per day (50 kB/day) - -**size:** 50kB - -**format:** text - -**type:** tableset - -**records_number:** 2358 - -**time_start:** 2022-10-01 - -**time_stop:** 2023-12-31 - -**spatial:** Earth's Ground - -**messenger:** neutrons - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** - -**latest update:** 2024-04-04 02:14:12 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_saandose_samadha_timeseries + * - **publisher:** + - SAMADHA + * - **alph_code:** + - 75A + * - **id_tmp:** + - 99 + * - **short_name:** + - SAA_Ndose + * - **identifier:** + - aspis://infn/saandose_samadha_timeseries + * - **dynamic:** + - one dataset per day (50 kB/day) + * - **size:** + - 50kB + * - **format:** + - text + * - **type:** + - tableset + * - **records_number:** + - 2358 + * - **time_start:** + - 2022-10-01 + * - **time_stop:** + - 2023-12-31 + * - **spatial:** + - Earth's Ground + * - **messenger:** + - neutrons + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - + * - **latest update:** + - 2024-04-04 02:14:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_tgndose_samadha_timeseries.rst b/docs/source/products/data/infn_tgndose_samadha_timeseries.rst index 674c0e3..e1a2431 100644 --- a/docs/source/products/data/infn_tgndose_samadha_timeseries.rst +++ b/docs/source/products/data/infn_tgndose_samadha_timeseries.rst @@ -2,56 +2,60 @@ SAMADHA neutron dose rate at Testa Grigia ========================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Monitoring of the neutron dose rate due to cosmic rays at the Testa Grigia Station (3480 m, Cervinia, Italy), to study possible correlation between space weather events and dose rate at the ground. This measurement is part of the INFN project SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) aimed to monitor the neutron dose inside the South Atlantic Anomaly (SAA) region in Bolivia. The data taken at Testa Grigia are a term of comparison for those collected in the SAA region. -**References** +References +~~~~~~~~~~ http://samadha.to.infn.it -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_tgndose_samadha_timeseries - -**publisher:** samadha - -**alphanumeric_code:** 75B - -**id_tmp:** 79 - -**short_name:** TG_Ndose - -**identifier:** aspis://infn/tgndose_samadha_timeseries - -**dynamic:** one dataset per day (50 kB/day) - -**size:** 50kB - -**format:** text - -**type:** timeseries - -**records_number:** 2835 - -**time_start:** 2021-09-01 - -**time_stop:** 2023-12-31 - -**spatial:** Earth's Ground - -**messenger:** neutrons - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** - -**latest update:** 2024-04-04 02:15:39 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_tgndose_samadha_timeseries + * - **publisher:** + - samadha + * - **alph_code:** + - 75B + * - **id_tmp:** + - 79 + * - **short_name:** + - TG_Ndose + * - **identifier:** + - aspis://infn/tgndose_samadha_timeseries + * - **dynamic:** + - one dataset per day (50 kB/day) + * - **size:** + - 50kB + * - **format:** + - text + * - **type:** + - timeseries + * - **records_number:** + - 2835 + * - **time_start:** + - 2021-09-01 + * - **time_stop:** + - 2023-12-31 + * - **spatial:** + - Earth's Ground + * - **messenger:** + - neutrons + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - + * - **latest update:** + - 2024-04-04 02:15:39 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_aqu_timeseries.rst b/docs/source/products/data/ingv_alert_aqu_timeseries.rst index 47abb7a..03fd83b 100644 --- a/docs/source/products/data/ingv_alert_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_alert_aqu_timeseries.rst @@ -2,59 +2,63 @@ INGV geomagnetic data, GIC indices and alert: L'Aquila ====================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents From both components of GIC index for L'Aquila observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) This tableset contains a set of data corresponding to products with ids 8, 47 and 48. In detail it contains the definitive values of the X,Y and Z components (in NEC coordinates) and of total intensity F of the geomagnetic field recorded at ground magnetic observatories managed by INGV. Besides, it contains the values of the GicX and GicY indices calculated from the Y and X components, respectively. To finish it contains values of the risk (i.e. alertX and alertY) , corresponding to the estimated values of the GicX and GicY indices. Data sampling is of 1-minute. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_aqu_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 48A - -**id_tmp:** 80 - -**short_name:** INGV_AQU_alert - -**identifier:** aspis:///ingv/INGV_AQU_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-04-04 02:27:54 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_aqu_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 48A + * - **id_tmp:** + - 80 + * - **short_name:** + - INGV_AQU_alert + * - **identifier:** + - aspis:///ingv/INGV_AQU_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-04-04 02:27:54 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_cts_timeseries.rst b/docs/source/products/data/ingv_alert_cts_timeseries.rst index 9c7018c..fe23a67 100644 --- a/docs/source/products/data/ingv_alert_cts_timeseries.rst +++ b/docs/source/products/data/ingv_alert_cts_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Castello Tesino ============================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents From both components of GIC index for Castello Tesino observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_cts_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 48B - -**id_tmp:** 81 - -**short_name:** INGV_CTS_alert - -**identifier:** aspis:///ingv/INGV_CTS_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:07 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_cts_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 48B + * - **id_tmp:** + - 81 + * - **short_name:** + - INGV_CTS_alert + * - **identifier:** + - aspis:///ingv/INGV_CTS_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:07 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_dur_timeseries.rst b/docs/source/products/data/ingv_alert_dur_timeseries.rst index 76388d4..3f66753 100644 --- a/docs/source/products/data/ingv_alert_dur_timeseries.rst +++ b/docs/source/products/data/ingv_alert_dur_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Duronia ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents From both components of GIC index for Duronia observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_dur_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 48C - -**id_tmp:** 82 - -**short_name:** INGV_DUR_alert - -**identifier:** aspis:///ingv/INGV_DUR_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:07 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_dur_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 48C + * - **id_tmp:** + - 82 + * - **short_name:** + - INGV_DUR_alert + * - **identifier:** + - aspis:///ingv/INGV_DUR_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:07 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_int_timeseries.rst b/docs/source/products/data/ingv_alert_int_timeseries.rst index 129b61e..f3d991b 100644 --- a/docs/source/products/data/ingv_alert_int_timeseries.rst +++ b/docs/source/products/data/ingv_alert_int_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories ============================================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_int_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 48E - -**id_tmp:** 88 - -**short_name:** INGV_INT_alert - -**identifier:** aspis:///ingv/INGV_INT_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:07 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_int_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 48E + * - **id_tmp:** + - 88 + * - **short_name:** + - INGV_INT_alert + * - **identifier:** + - aspis:///ingv/INGV_INT_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:07 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_lmp_timeseries.rst b/docs/source/products/data/ingv_alert_lmp_timeseries.rst index a13abd8..c2feed3 100644 --- a/docs/source/products/data/ingv_alert_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_alert_lmp_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Lampedusa ======================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents From both components of GIC index for Lampedusa observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_lmp_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 48D - -**id_tmp:** 83 - -**short_name:** INGV_LMP_alert - -**identifier:** aspis:///ingv/INGV_LMP_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:08 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_lmp_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 48D + * - **id_tmp:** + - 83 + * - **short_name:** + - INGV_LMP_alert + * - **identifier:** + - aspis:///ingv/INGV_LMP_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:08 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_wdc_timeseries.rst b/docs/source/products/data/ingv_alert_wdc_timeseries.rst index f6a5db5..1675fc8 100644 --- a/docs/source/products/data/ingv_alert_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_alert_wdc_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories ======================================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_wdc_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 48F - -**id_tmp:** 48 - -**short_name:** INGV_WDC_alert - -**identifier:** aspis:///ingv/INGV_WDC_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:08 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_wdc_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 48F + * - **id_tmp:** + - 48 + * - **short_name:** + - INGV_WDC_alert + * - **identifier:** + - aspis:///ingv/INGV_WDC_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:08 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst b/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst index 80a2ba5..ac14a8b 100644 --- a/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst @@ -2,56 +2,60 @@ Autoscaled data Bahia Blanca Ionosonde ====================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Bahia Blanca -**References** +References +~~~~~~~~~~ http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_autoiono_bbla_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 12A - -**id_tmp:** 1 - -**short_name:** AutoIonoBBla - -**identifier:** aspis://ingv/autoiono_bbla_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Bahia Blanca AIS-INGV ionosonde started sounding in September 2016, this is why in the Number of datasets field you will find the number 7 (years 2016-2022). This collection grows in real time, because th - -**size:** 15MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1558 - -**time_start:** 2016-09-26 - -**time_stop:** 2022-04-14 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-04-04 05:53:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_autoiono_bbla_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 12A + * - **id_tmp:** + - 1 + * - **short_name:** + - AutoIonoBBla + * - **identifier:** + - aspis://ingv/autoiono_bbla_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Bahia Blanca AIS-INGV ionosonde started sounding in September 2016, this is why in the Number of datasets field you will find the number 7 (years 2016-2022). This collection grows in real time, because th + * - **size:** + - 15MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1558 + * - **time_start:** + - 2016-09-26 + * - **time_stop:** + - 2022-04-14 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-04-04 05:53:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst b/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst index 59b1916..a8a85d6 100644 --- a/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst @@ -2,56 +2,60 @@ Autoscaled data Gibilmanna Ionosonde ==================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna -**References** +References +~~~~~~~~~~ http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_autoiono_gibi_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 12B - -**id_tmp:** 2 - -**short_name:** AutoIonoGibi - -**identifier:** aspis://ingv/autoiono_gibi_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Gibilmanna AIS-INGV ionosonde started sounding in November 2002, this is why in the Number of datasets field you will find the number 21 (years 2002-2022). This collection grows in real time, because the - -**size:** 15MB - -**format:** csv - -**type:** timeseries - -**records_number:** 5793 - -**time_start:** 2002-11-26 - -**time_stop:** 2022-04-14 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-04-04 05:55:21 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_autoiono_gibi_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 12B + * - **id_tmp:** + - 2 + * - **short_name:** + - AutoIonoGibi + * - **identifier:** + - aspis://ingv/autoiono_gibi_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Gibilmanna AIS-INGV ionosonde started sounding in November 2002, this is why in the Number of datasets field you will find the number 21 (years 2002-2022). This collection grows in real time, because the + * - **size:** + - 15MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 5793 + * - **time_start:** + - 2002-11-26 + * - **time_stop:** + - 2022-04-14 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-04-04 05:55:21 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_autoiono_rome_timeseries.rst b/docs/source/products/data/ingv_autoiono_rome_timeseries.rst index e31ce5a..287c30e 100644 --- a/docs/source/products/data/ingv_autoiono_rome_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_rome_timeseries.rst @@ -2,56 +2,60 @@ Autoscaled data Rome Ionosonde ============================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Rome -**References** +References +~~~~~~~~~~ http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_autoiono_rome_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 12C - -**id_tmp:** 3 - -**short_name:** AutoIonoRome - -**identifier:** aspis://ingv/autoiono_rome_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Rome AIS-INGV ionosonde started sounding in November 2004, this is why in the Number of datasets field you will find the number 19 (years 2004-2022). This collection grows in real time, because the ionoso - -**size:** 15MB - -**format:** csv - -**type:** timeseries - -**records_number:** 7303 - -**time_start:** 2004-11-25 - -**time_stop:** 2022-04-14 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-04-04 05:56:30 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_autoiono_rome_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 12C + * - **id_tmp:** + - 3 + * - **short_name:** + - AutoIonoRome + * - **identifier:** + - aspis://ingv/autoiono_rome_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Rome AIS-INGV ionosonde started sounding in November 2004, this is why in the Number of datasets field you will find the number 19 (years 2004-2022). This collection grows in real time, because the ionoso + * - **size:** + - 15MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 7303 + * - **time_start:** + - 2004-11-25 + * - **time_stop:** + - 2022-04-14 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-04-04 05:56:30 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst b/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst index bf95bc7..10e5a97 100644 --- a/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst @@ -2,56 +2,60 @@ Autoscaled data Tucuman Ionosonde ================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Tucuman -**References** +References +~~~~~~~~~~ http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_autoiono_tucu_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 12D - -**id_tmp:** 4 - -**short_name:** AutoIonoTucu - -**identifier:** aspis://ingv/autoiono_tucu_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Tucuman AIS-INGV ionosonde started sounding in August 2007, this is why in the Number of datasets field you will find the number 16 (years 2007-2022). This collection grows in real time, because the ionos - -**size:** 15MB - -**format:** csv - -**type:** timeseries - -**records_number:** 6283 - -**time_start:** 2007-08-04 - -**time_stop:** 2022-04-14 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-04-04 05:57:34 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_autoiono_tucu_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 12D + * - **id_tmp:** + - 4 + * - **short_name:** + - AutoIonoTucu + * - **identifier:** + - aspis://ingv/autoiono_tucu_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Tucuman AIS-INGV ionosonde started sounding in August 2007, this is why in the Number of datasets field you will find the number 16 (years 2007-2022). This collection grows in real time, because the ionos + * - **size:** + - 15MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 6283 + * - **time_start:** + - 2007-08-04 + * - **time_stop:** + - 2022-04-14 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-04-04 05:57:34 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_b_swarm_image.rst b/docs/source/products/data/ingv_b_swarm_image.rst index c01e835..3dbf61d 100644 --- a/docs/source/products/data/ingv_b_swarm_image.rst +++ b/docs/source/products/data/ingv_b_swarm_image.rst @@ -2,56 +2,60 @@ Swarm vector magnetic field maps ================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents Vector magnetic field maps in quasi-dipole latitude vs magnetic local time coordinates derived from the Swarm constellation data acquired at 1 second cadence from 1 January 2014 to 31 December 2020. The output consists in nine .jpg or .png files mapping the three components of the vector magnetic field in polar and equatorial projections (3 images for the three components) for each of the 3 satellites of the Swarm constellation. Each map has a size of about 300 kB. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_b_swarm_image - -**publisher:** INGV group - -**alphanumeric_code:** 35B - -**id_tmp:** 62 - -**short_name:** Swarm_B_maps - -**identifier:** aspis://ingv/b_swarm_image - -**dynamic:** static - -**size:** 300kB - -**format:** FITS - -**type:** image - -**records_number:** 24 - -**time_start:** 2014-01-01 - -**time_stop:** 2020-12-31 - -**spatial:** Earth's Ionosphere - -**messenger:** - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** phys.magField - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_b_swarm_image + * - **publisher:** + - INGV group + * - **alph_code:** + - 35B + * - **id_tmp:** + - 62 + * - **short_name:** + - Swarm_B_maps + * - **identifier:** + - aspis://ingv/b_swarm_image + * - **dynamic:** + - static + * - **size:** + - 300kB + * - **format:** + - FITS + * - **type:** + - image + * - **records_number:** + - 24 + * - **time_start:** + - 2014-01-01 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - Earth's Ionosphere + * - **messenger:** + - + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - phys.magField + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_b_swarm_timeseries.rst b/docs/source/products/data/ingv_b_swarm_timeseries.rst index a50603e..4a8ca45 100644 --- a/docs/source/products/data/ingv_b_swarm_timeseries.rst +++ b/docs/source/products/data/ingv_b_swarm_timeseries.rst @@ -2,56 +2,60 @@ 1 Hz Swarm on track values of observed, external and projected vector geomagnetic field ======================================================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents In situ time series of vector geomagnetic field derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of one has a size of about 14.5 GB. The sample file attached is extracted from one month of data acquired by Swarm A -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_b_swarm_timeseries - -**publisher:** INGV group - -**alphanumeric_code:** 35A - -**id_tmp:** 52 - -**short_name:** Swarm_B_tseries - -**identifier:** aspis://ingv/b_swarm_timeseries - -**dynamic:** static - -**size:** 20GB - -**format:** text file - -**type:** tableset - -**records_number:** 2634060 - -**time_start:** 2014-01-01 - -**time_stop:** 2022-12-31 - -**spatial:** Earth's Ionosphere - -**messenger:** - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** phys.magField - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_b_swarm_timeseries + * - **publisher:** + - INGV group + * - **alph_code:** + - 35A + * - **id_tmp:** + - 52 + * - **short_name:** + - Swarm_B_tseries + * - **identifier:** + - aspis://ingv/b_swarm_timeseries + * - **dynamic:** + - static + * - **size:** + - 20GB + * - **format:** + - text file + * - **type:** + - tableset + * - **records_number:** + - 2634060 + * - **time_start:** + - 2014-01-01 + * - **time_stop:** + - 2022-12-31 + * - **spatial:** + - Earth's Ionosphere + * - **messenger:** + - + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - phys.magField + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_bvect_cses_tableset.rst b/docs/source/products/data/ingv_bvect_cses_tableset.rst index 7bdb335..f2f2a56 100644 --- a/docs/source/products/data/ingv_bvect_cses_tableset.rst +++ b/docs/source/products/data/ingv_bvect_cses_tableset.rst @@ -2,56 +2,60 @@ CSES-01 on track values of vector magnetic field ================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents In situ time series of vector magnetic field derived from the CSES-01 satellite from 1 January 2019 to 30 September 2021. The output is a single .txt formatted file for both diurnal and nocturnal orbits, each of which has a size of about 3 GB. The sample file attached is extracted from one minute acquired by CSES-01 -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_bvect_cses_tableset - -**publisher:** INGV group - -**alphanumeric_code:** 46B - -**id_tmp:** 84 - -**short_name:** CSES_Bvect_ts - -**identifier:** aspis://ingv/bvect_cses_tableset - -**dynamic:** static - -**size:** 3GB - -**format:** csv - -**type:** timeseries - -**records_number:** 10356758 - -**time_start:** 2019-01-01 - -**time_stop:** 2021-09-30 - -**spatial:** Earth's Ionosphere - -**messenger:** - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** phys.density,phys.electron - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_bvect_cses_tableset + * - **publisher:** + - INGV group + * - **alph_code:** + - 46B + * - **id_tmp:** + - 84 + * - **short_name:** + - CSES_Bvect_ts + * - **identifier:** + - aspis://ingv/bvect_cses_tableset + * - **dynamic:** + - static + * - **size:** + - 3GB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 10356758 + * - **time_start:** + - 2019-01-01 + * - **time_stop:** + - 2021-09-30 + * - **spatial:** + - Earth's Ionosphere + * - **messenger:** + - + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - phys.density,phys.electron + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_evect_cses_tableset.rst b/docs/source/products/data/ingv_evect_cses_tableset.rst index 11760ed..ed8d81b 100644 --- a/docs/source/products/data/ingv_evect_cses_tableset.rst +++ b/docs/source/products/data/ingv_evect_cses_tableset.rst @@ -2,56 +2,60 @@ CSES-01 on track values of vector electric field ================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents In situ time series of vector electric field derived from the CSES-01 satellite from 1 January 2019 to 30 September 2021. The output is a single .txt formatted file for both diurnal and nocturnal orbits, each of which has a size of about 3 GB. The sample file attached is extracted from about ten minutes acquired by CSES-01 -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_evect_cses_tableset - -**publisher:** INGV group - -**alphanumeric_code:** 46A - -**id_tmp:** 85 - -**short_name:** CSES_Evec_ts - -**identifier:** aspis://ingv/evect_cses_tableset - -**dynamic:** static - -**size:** 3GB - -**format:** csv - -**type:** tableset - -**records_number:** 9769594 - -**time_start:** 2019-01-01 - -**time_stop:** 2021-09-30 - -**spatial:** Earth's Ionosphere - -**messenger:** - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** phys.density,phys.electron - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_evect_cses_tableset + * - **publisher:** + - INGV group + * - **alph_code:** + - 46A + * - **id_tmp:** + - 85 + * - **short_name:** + - CSES_Evec_ts + * - **identifier:** + - aspis://ingv/evect_cses_tableset + * - **dynamic:** + - static + * - **size:** + - 3GB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 9769594 + * - **time_start:** + - 2019-01-01 + * - **time_stop:** + - 2021-09-30 + * - **spatial:** + - Earth's Ionosphere + * - **messenger:** + - + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - phys.density,phys.electron + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_aqu_timeseries.rst b/docs/source/products/data/ingv_gic_aqu_timeseries.rst index 96a9dfa..65ef3f8 100644 --- a/docs/source/products/data/ingv_gic_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_gic_aqu_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: L'Aquila ====================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents GIC index for L'Aquila observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. Since for L'Aquila observatory only preliminary data are available, before obtaining GICxy index it will be necessary to estimate X and Y from H and D preliminary data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_aqu_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47A - -**id_tmp:** 7 - -**short_name:** INGV_AQU_gic - -**identifier:** aspis:///ingv/INGV_AQU_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_aqu_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47A + * - **id_tmp:** + - 7 + * - **short_name:** + - INGV_AQU_gic + * - **identifier:** + - aspis:///ingv/INGV_AQU_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_cts_timeseries.rst b/docs/source/products/data/ingv_gic_cts_timeseries.rst index 8c4523e..ab407a6 100644 --- a/docs/source/products/data/ingv_gic_cts_timeseries.rst +++ b/docs/source/products/data/ingv_gic_cts_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Castello Tesino ============================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents GIC index for Castello Tesino observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. If definitive values for Castello Tesino are available GICxy indices will calculates directly from X and Y 1-minute data, otherwise an estimate of X and Y will be first obtained from H and D preliminary data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_cts_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47B - -**id_tmp:** 8 - -**short_name:** INGV_CTS_gic - -**identifier:** aspis:///ingv/INGV_CTS_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_cts_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47B + * - **id_tmp:** + - 8 + * - **short_name:** + - INGV_CTS_gic + * - **identifier:** + - aspis:///ingv/INGV_CTS_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_dur_timeseries.rst b/docs/source/products/data/ingv_gic_dur_timeseries.rst index 997436d..d102518 100644 --- a/docs/source/products/data/ingv_gic_dur_timeseries.rst +++ b/docs/source/products/data/ingv_gic_dur_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Duronia ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents GIC index for Duronia observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. If definitive values for Duronia are available GICxy indices will calculates directly from X and Y 1-minute data, otherwise an estimate of X and Y will be first obtained from H and D preliminary data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_dur_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47C - -**id_tmp:** 9 - -**short_name:** INGV_DUR_gic - -**identifier:** aspis:///ingv/INGV_DUR_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_dur_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47C + * - **id_tmp:** + - 9 + * - **short_name:** + - INGV_DUR_gic + * - **identifier:** + - aspis:///ingv/INGV_DUR_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_int_timeseries.rst b/docs/source/products/data/ingv_gic_int_timeseries.rst index c12f5a3..47efee6 100644 --- a/docs/source/products/data/ingv_gic_int_timeseries.rst +++ b/docs/source/products/data/ingv_gic_int_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories ============================================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents As specified for product INTmag, data from INTERMAGNET observatories will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. For the selected observatories GIC index (specifically GICx and GICy) will be calculated. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_int_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47E - -**id_tmp:** 10 - -**short_name:** INGV_INT_gic - -**identifier:** aspis:///ingv/INGV_INT_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_int_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47E + * - **id_tmp:** + - 10 + * - **short_name:** + - INGV_INT_gic + * - **identifier:** + - aspis:///ingv/INGV_INT_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_lmp_timeseries.rst b/docs/source/products/data/ingv_gic_lmp_timeseries.rst index 3e501e2..e7cbb63 100644 --- a/docs/source/products/data/ingv_gic_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_gic_lmp_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Lampedusa ======================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents GIC index for Lampedusa observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. Since for Lampedusa observatory only preliminary data are available, before obtaining GICxy index it will be necessary to estimate X and Y from H and D preliminary data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_lmp_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47D - -**id_tmp:** 11 - -**short_name:** INGV_LMP_gic - -**identifier:** aspis:///ingv/INGV_LMP_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_lmp_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47D + * - **id_tmp:** + - 11 + * - **short_name:** + - INGV_LMP_gic + * - **identifier:** + - aspis:///ingv/INGV_LMP_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_wdc_timeseries.rst b/docs/source/products/data/ingv_gic_wdc_timeseries.rst index d86724c..a150198 100644 --- a/docs/source/products/data/ingv_gic_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_gic_wdc_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories ======================================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents As specified for product WDCmag, data from World Data Center of Geomagnetism observatories will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. For the selected observatories GIC index (specifically GICx and GICy) will be calculated. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_wdc_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47F - -**id_tmp:** 12 - -**short_name:** INGV_WDC_gic - -**identifier:** aspis:///ingv/INGV_WDC_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_wdc_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47F + * - **id_tmp:** + - 12 + * - **short_name:** + - INGV_WDC_gic + * - **identifier:** + - aspis:///ingv/INGV_WDC_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst b/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst index c5d0e4a..227feeb 100644 --- a/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst @@ -2,56 +2,60 @@ Long Term MUF maps centered on Cagliari ======================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Cagliari over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ltmuf_cagliari_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28A - -**id_tmp:** 63 - -**short_name:** LTMUFCagliari - -**identifier:** aspis://ingv/ltmuf_cagliari_tableset - -**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. - -**size:** 1MB - -**format:** dat,png - -**type:** tableset - -**records_number:** 48 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ltmuf_cagliari_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28A + * - **id_tmp:** + - 63 + * - **short_name:** + - LTMUFCagliari + * - **identifier:** + - aspis://ingv/ltmuf_cagliari_tableset + * - **dynamic:** + - The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + * - **size:** + - 1MB + * - **format:** + - dat,png + * - **type:** + - tableset + * - **records_number:** + - 48 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ltmuf_catania_tableset.rst b/docs/source/products/data/ingv_ltmuf_catania_tableset.rst index e65976e..1fa87b3 100644 --- a/docs/source/products/data/ingv_ltmuf_catania_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_catania_tableset.rst @@ -2,56 +2,60 @@ Long Term MUF maps centered on Catania ====================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ltmuf_catania_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28B - -**id_tmp:** 70 - -**short_name:** LTMUFCatania - -**identifier:** aspis://ingv/ltmuf_catania_tableset - -**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. - -**size:** 1MB - -**format:** dat,png - -**type:** tableset - -**records_number:** 48 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ltmuf_catania_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28B + * - **id_tmp:** + - 70 + * - **short_name:** + - LTMUFCatania + * - **identifier:** + - aspis://ingv/ltmuf_catania_tableset + * - **dynamic:** + - The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + * - **size:** + - 1MB + * - **format:** + - dat,png + * - **type:** + - tableset + * - **records_number:** + - 48 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ltmuf_milan_tableset.rst b/docs/source/products/data/ingv_ltmuf_milan_tableset.rst index 325f463..8e4b51e 100644 --- a/docs/source/products/data/ingv_ltmuf_milan_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_milan_tableset.rst @@ -2,56 +2,60 @@ Long Term MUF maps centered on Milano ===================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ltmuf_milan_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28C - -**id_tmp:** 68 - -**short_name:** LTMUFMilano - -**identifier:** aspis://ingv/ltmuf_milano_tableset - -**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. - -**size:** 1MB - -**format:** dat,png - -**type:** tableset - -**records_number:** 48 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ltmuf_milan_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28C + * - **id_tmp:** + - 68 + * - **short_name:** + - LTMUFMilano + * - **identifier:** + - aspis://ingv/ltmuf_milano_tableset + * - **dynamic:** + - The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + * - **size:** + - 1MB + * - **format:** + - dat,png + * - **type:** + - tableset + * - **records_number:** + - 48 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ltmuf_rome_tableset.rst b/docs/source/products/data/ingv_ltmuf_rome_tableset.rst index 061f2e1..fdc73e1 100644 --- a/docs/source/products/data/ingv_ltmuf_rome_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_rome_tableset.rst @@ -2,56 +2,60 @@ Long Term MUF maps centered on Roma =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ltmuf_rome_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28D - -**id_tmp:** 69 - -**short_name:** LTMUFRoma - -**identifier:** aspis://ingv/ltmuf_roma_tableset - -**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. - -**size:** 1MB - -**format:** dat,png - -**type:** tableset - -**records_number:** 48 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ltmuf_rome_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28D + * - **id_tmp:** + - 69 + * - **short_name:** + - LTMUFRoma + * - **identifier:** + - aspis://ingv/ltmuf_roma_tableset + * - **dynamic:** + - The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + * - **size:** + - 1MB + * - **format:** + - dat,png + * - **type:** + - tableset + * - **records_number:** + - 48 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_aqu_timeseries.rst b/docs/source/products/data/ingv_mag_aqu_timeseries.rst index 7032fc4..a47bd7e 100644 --- a/docs/source/products/data/ingv_mag_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_mag_aqu_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: L'Aquila ====================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at L'Aquila magnetic observatory (IAGA code: AQU Latitude: 42.383000° Longitude: 13.316000° Altitude: 682.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_aqu_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8A - -**id_tmp:** 17 - -**short_name:** INGV_AQU_mag - -**identifier:** aspis:///ingv/INGV_AQU_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_aqu_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8A + * - **id_tmp:** + - 17 + * - **short_name:** + - INGV_AQU_mag + * - **identifier:** + - aspis:///ingv/INGV_AQU_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_cts_timeseries.rst b/docs/source/products/data/ingv_mag_cts_timeseries.rst index db53559..a544bfc 100644 --- a/docs/source/products/data/ingv_mag_cts_timeseries.rst +++ b/docs/source/products/data/ingv_mag_cts_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Castello Tesino ============================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino (TN) magnetic observatory (IAGA code: CTS Latitude: 46.047000° Longitude: 11.649000° Altitude : 1175.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. For this observatory also definitive data are available. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_cts_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8B - -**id_tmp:** 18 - -**short_name:** INGV_CTS_mag - -**identifier:** aspis:///ingv/INGV_CTS_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_cts_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8B + * - **id_tmp:** + - 18 + * - **short_name:** + - INGV_CTS_mag + * - **identifier:** + - aspis:///ingv/INGV_CTS_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_dmc_timeseries.rst b/docs/source/products/data/ingv_mag_dmc_timeseries.rst index a810c5b..8422911 100644 --- a/docs/source/products/data/ingv_mag_dmc_timeseries.rst +++ b/docs/source/products/data/ingv_mag_dmc_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Dome C ==================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Dome C magnetic observatory(AGA code: DMC Latitude: -75.250000° Longitude: 124.167000° Altitude: 3250.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_dmc_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8D - -**id_tmp:** 19 - -**short_name:** INGV_DMC_mag - -**identifier:** aspis:///ingv/INGV_DMC_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_dmc_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8D + * - **id_tmp:** + - 19 + * - **short_name:** + - INGV_DMC_mag + * - **identifier:** + - aspis:///ingv/INGV_DMC_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_dur_timeseries.rst b/docs/source/products/data/ingv_mag_dur_timeseries.rst index f598575..c4c3054 100644 --- a/docs/source/products/data/ingv_mag_dur_timeseries.rst +++ b/docs/source/products/data/ingv_mag_dur_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Duronia ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Duronia magnetic observatory (IAGA code: DUR Latitude: 41.650000° Longitude: 14.466000° Altitude: 895.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. For this observatory also definitive data are available. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_dur_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8E - -**id_tmp:** 20 - -**short_name:** INGV_DUR_mag - -**identifier:** aspis:///ingv/INGV_DUR_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_dur_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8E + * - **id_tmp:** + - 20 + * - **short_name:** + - INGV_DUR_mag + * - **identifier:** + - aspis:///ingv/INGV_DUR_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_int_timeseries.rst b/docs/source/products/data/ingv_mag_int_timeseries.rst index 84e5be3..06f912f 100644 --- a/docs/source/products/data/ingv_mag_int_timeseries.rst +++ b/docs/source/products/data/ingv_mag_int_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories ============================================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The INTERMAGNET programme exists to establish a global network of cooperating digital magnetic observatories, adopting modern standard specifications for measuring and recording equipment, in order to facilitate data exchanges and the production of geomagnetic products in close to real time. From the INTERMAGNET website it is possible to download 1-minute averages (in daily files) of vector components in either (H, D, Z) or (X, Y, Z) reference frame from world wide magnetic observatories. For this reason, it is not possible to exhaustively fill this form. For instance, the time window of data availability changes from observatory to observatory as well as the tern provided (either (H, D, Z) or (X, Y, Z)) . Data from INTERMAGNET will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. Data can be downloaded as .gz files from an ftp (ftp://ftp.seismo.nrcan.gc.ca/intermagnet/). Each file contains 1 day of 1-minute magnetic data for a single INTERMAGNET observatory -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_int_timeseries - -**publisher:** INTERMAGNET - -**alphanumeric_code:** 9A - -**id_tmp:** 21 - -**short_name:** INGV_INT_mag - -**identifier:** aspis:///ingv/INGV_INT_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_int_timeseries + * - **publisher:** + - INTERMAGNET + * - **alph_code:** + - 9A + * - **id_tmp:** + - 21 + * - **short_name:** + - INGV_INT_mag + * - **identifier:** + - aspis:///ingv/INGV_INT_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_lmp_timeseries.rst b/docs/source/products/data/ingv_mag_lmp_timeseries.rst index cdf193b..afb19d8 100644 --- a/docs/source/products/data/ingv_mag_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_mag_lmp_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Lampedusa ======================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Lampedusa magnetic observatory (IAGA code: LMP Latitude: 35.517000° Longitude: 12.545000° Altitude: 93.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_lmp_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8G - -**id_tmp:** 22 - -**short_name:** INGV_LMP_mag - -**identifier:** aspis:///ingv/INGV_LMP_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_lmp_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8G + * - **id_tmp:** + - 22 + * - **short_name:** + - INGV_LMP_mag + * - **identifier:** + - aspis:///ingv/INGV_LMP_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_tnb_timeseries.rst b/docs/source/products/data/ingv_mag_tnb_timeseries.rst index 97a05bb..2988f79 100644 --- a/docs/source/products/data/ingv_mag_tnb_timeseries.rst +++ b/docs/source/products/data/ingv_mag_tnb_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Terra Nova Bay ============================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Terra Nova Bay magnetic observatory (IAGA code: TNB Latitude: -74.693000° Longitude: 164.099000° Altitude: 59.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_tnb_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8H - -**id_tmp:** 23 - -**short_name:** INGV_TNB_mag - -**identifier:** aspis:///ingv/INGV_TNB_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_tnb_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8H + * - **id_tmp:** + - 23 + * - **short_name:** + - INGV_TNB_mag + * - **identifier:** + - aspis:///ingv/INGV_TNB_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_wdc_timeseries.rst b/docs/source/products/data/ingv_mag_wdc_timeseries.rst index fa9c8ab..fc9c041 100644 --- a/docs/source/products/data/ingv_mag_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_mag_wdc_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories ======================================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The mission of the World Data Center for Geomagnetism is to provide geomagnetic field data supplied from a worldwide network of magnetic observatories, as well as geomagnetic indices (AE index, ASY/SYM index, and Dst index) derived in this data center to researchers specializing mostly in solar terrestrial physics, and geomagnetism in order to facilitate the global exchange of the geomagnetic field data including the geomagnetic indices. From the WDC websites it is possible to download 1-minute averages (in daily files) of vector components in either (H, D, Z) or (X, Y, Z) reference frame from world wide magnetic observatories. For this reason, it is not possible to exhaustively fill this form. For instance, the time window of data availability changes from observatory to observatory as well as the tern provided (either (H, D, Z) or (X, Y, Z)) . Data from WDC will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. The set of WDC observatories well overlap to the set of INTERMAGNET observatories. WDC data can be retrieved through queries to a web service (http://www.wdc.bgs.ac.uk/dataportal/webservice_doc.html). At the present moment, however, the service and the website are not working properly and it is not possible to download a sample file. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_wdc_timeseries - -**publisher:** World Data Center for Geomagnetism - -**alphanumeric_code:** 9B - -**id_tmp:** 24 - -**short_name:** INGV_WDC_mag - -**identifier:** aspis:///ingv/INGV_WDC_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_wdc_timeseries + * - **publisher:** + - World Data Center for Geomagnetism + * - **alph_code:** + - 9B + * - **id_tmp:** + - 24 + * - **short_name:** + - INGV_WDC_mag + * - **identifier:** + - aspis:///ingv/INGV_WDC_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_magdef_cts_timeseries.rst b/docs/source/products/data/ingv_magdef_cts_timeseries.rst index 187adac..3ab5661 100644 --- a/docs/source/products/data/ingv_magdef_cts_timeseries.rst +++ b/docs/source/products/data/ingv_magdef_cts_timeseries.rst @@ -2,57 +2,61 @@ INGV geomagnetic data, GIC indices and alert: Castello Tesino ============================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of the components (X, Y, Z in the NEC, i.e. North-East-Center frame) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino magnetic observatory (IAGA code: CTS Latitude: 46.047000° Longitude: 11.649000° Altitude: 1175.000 m). These are the definitive values that will be used to calculate GICx and GICy indices. These data are definitive, new definitive data are added yearly. They can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_magdef_cts_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8C - -**id_tmp:** 25 - -**short_name:** INGV_CTS_magdef - -**identifier:** aspis:///ingv/INGV_CTS_magdef - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_magdef_cts_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8C + * - **id_tmp:** + - 25 + * - **short_name:** + - INGV_CTS_magdef + * - **identifier:** + - aspis:///ingv/INGV_CTS_magdef + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_magdef_dur_timeseries.rst b/docs/source/products/data/ingv_magdef_dur_timeseries.rst index 40d43f6..9d8e7e3 100644 --- a/docs/source/products/data/ingv_magdef_dur_timeseries.rst +++ b/docs/source/products/data/ingv_magdef_dur_timeseries.rst @@ -2,57 +2,61 @@ INGV geomagnetic data, GIC indices and alert: Duronia ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of the components (X, Y, Z in the NEC, i.e. North-East-Center frame) and of total intensity (F) of the Earth's geomagnetic field measured at Duronia magnetic observatory (IAGA code: DUR Latitude: 41.650000° Longitude: 14.466000° Altitude: 895.000 m). These are the definitive values that will be used to calculate GICx and GICy indices. These data are definitive, new definitive data are added yearly. They can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_magdef_dur_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8F - -**id_tmp:** 26 - -**short_name:** INGV_DUR_magdef - -**identifier:** aspis:///ingv/INGV_DUR_magdef - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_magdef_dur_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8F + * - **id_tmp:** + - 26 + * - **short_name:** + - INGV_DUR_magdef + * - **identifier:** + - aspis:///ingv/INGV_DUR_magdef + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst b/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst index 053d383..0e2a819 100644 --- a/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst @@ -2,56 +2,60 @@ Nowcasting MUF map centered on Cagliari ======================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Cagliari over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ncmuf_cagliari_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28E - -**id_tmp:** 27 - -**short_name:** NCMUFCagliari - -**identifier:** aspis://ingv/ncmuf_cagliari_tableset - -**dynamic:** The map is a nowcasting map, generated every 15 minutes. - -**size:** 1MB - -**format:** png,dat - -**type:** tableset - -**records_number:** 192 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:13 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ncmuf_cagliari_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28E + * - **id_tmp:** + - 27 + * - **short_name:** + - NCMUFCagliari + * - **identifier:** + - aspis://ingv/ncmuf_cagliari_tableset + * - **dynamic:** + - The map is a nowcasting map, generated every 15 minutes. + * - **size:** + - 1MB + * - **format:** + - png,dat + * - **type:** + - tableset + * - **records_number:** + - 192 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:13 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ncmuf_catania_tableset.rst b/docs/source/products/data/ingv_ncmuf_catania_tableset.rst index e257ba3..f720d9b 100644 --- a/docs/source/products/data/ingv_ncmuf_catania_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_catania_tableset.rst @@ -2,56 +2,60 @@ Nowcasting MUF map centered on Catania ====================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ncmuf_catania_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28F - -**id_tmp:** 28 - -**short_name:** NCMUFCatania - -**identifier:** aspis://ingv/ncmuf_catania_tableset - -**dynamic:** The map is a nowcasting map, generated every 15 minutes. - -**size:** 1MB - -**format:** png,dat - -**type:** tableset - -**records_number:** 192 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:13 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ncmuf_catania_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28F + * - **id_tmp:** + - 28 + * - **short_name:** + - NCMUFCatania + * - **identifier:** + - aspis://ingv/ncmuf_catania_tableset + * - **dynamic:** + - The map is a nowcasting map, generated every 15 minutes. + * - **size:** + - 1MB + * - **format:** + - png,dat + * - **type:** + - tableset + * - **records_number:** + - 192 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:13 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ncmuf_milan_tableset.rst b/docs/source/products/data/ingv_ncmuf_milan_tableset.rst index 6a29c09..96508c1 100644 --- a/docs/source/products/data/ingv_ncmuf_milan_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_milan_tableset.rst @@ -2,56 +2,60 @@ Nowcasting MUF map centered on Milano ===================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ncmuf_milan_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28G - -**id_tmp:** 29 - -**short_name:** NCMUFMilano - -**identifier:** aspis://ingv/ncmuf_milano_tableset - -**dynamic:** The map is a nowcasting map, generated every 15 minutes. - -**size:** 1MB - -**format:** png,dat - -**type:** tableset - -**records_number:** 192 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:13 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ncmuf_milan_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28G + * - **id_tmp:** + - 29 + * - **short_name:** + - NCMUFMilano + * - **identifier:** + - aspis://ingv/ncmuf_milano_tableset + * - **dynamic:** + - The map is a nowcasting map, generated every 15 minutes. + * - **size:** + - 1MB + * - **format:** + - png,dat + * - **type:** + - tableset + * - **records_number:** + - 192 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:13 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ncmuf_rome_tableset.rst b/docs/source/products/data/ingv_ncmuf_rome_tableset.rst index acf8ec2..7f3deb4 100644 --- a/docs/source/products/data/ingv_ncmuf_rome_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_rome_tableset.rst @@ -2,56 +2,60 @@ Nowcasting MUF map centered on Roma =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ncmuf_rome_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28H - -**id_tmp:** 30 - -**short_name:** NCMUFCatania - -**identifier:** aspis://ingv/ncmuf_roma_tableset - -**dynamic:** The map is a nowcasting map, generated every 15 minutes. - -**size:** 1MB - -**format:** png,dat - -**type:** tableset - -**records_number:** 192 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ncmuf_rome_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28H + * - **id_tmp:** + - 30 + * - **short_name:** + - NCMUFCatania + * - **identifier:** + - aspis://ingv/ncmuf_roma_tableset + * - **dynamic:** + - The map is a nowcasting map, generated every 15 minutes. + * - **size:** + - 1MB + * - **format:** + - png,dat + * - **type:** + - tableset + * - **records_number:** + - 192 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst b/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst index ed243cc..5090e8b 100644 --- a/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst +++ b/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst @@ -2,56 +2,60 @@ Validated data Gibilmanna Ionosonde =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_valiiono_gibi_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 13A - -**id_tmp:** 31 - -**short_name:** ValiIonoGibi - -**identifier:** aspis://ingv/valiiono_gibi_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1463 - -**time_start:** 2012-03-07 - -**time_stop:** 2015-06-30 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_valiiono_gibi_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 13A + * - **id_tmp:** + - 31 + * - **short_name:** + - ValiIonoGibi + * - **identifier:** + - aspis://ingv/valiiono_gibi_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1463 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2015-06-30 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_valiiono_rome_timeseries.rst b/docs/source/products/data/ingv_valiiono_rome_timeseries.rst index 2b46496..71ec384 100644 --- a/docs/source/products/data/ingv_valiiono_rome_timeseries.rst +++ b/docs/source/products/data/ingv_valiiono_rome_timeseries.rst @@ -2,56 +2,60 @@ Validated data Rome Ionosonde ============================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Rome -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_valiiono_rome_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 13B - -**id_tmp:** 32 - -**short_name:** ValiIonoRome - -**identifier:** aspis://ingv/valiiono_rome_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1727 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_valiiono_rome_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 13B + * - **id_tmp:** + - 32 + * - **short_name:** + - ValiIonoRome + * - **identifier:** + - aspis://ingv/valiiono_rome_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1727 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/uniaq_curr_maigic_tableset.rst b/docs/source/products/data/uniaq_curr_maigic_tableset.rst index 3fe7a42..9933cf0 100644 --- a/docs/source/products/data/uniaq_curr_maigic_tableset.rst +++ b/docs/source/products/data/uniaq_curr_maigic_tableset.rst @@ -2,56 +2,60 @@ Magnetospheric-Ionospheric-Ground Induced Current model - currents ================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** uniaq_curr_maigic_tableset - -**publisher:** Mirko Piersanti - -**alphanumeric_code:** 40B - -**id_tmp:** 86 - -**short_name:** MA.I.GIC. current - -**identifier:** aspis://uniaq//curr_maigic_tableset - -**dynamic:** Static and depending on the length of the input data - -**size:** 5MB - -**format:** .mat - -**type:** tableset - -**records_number:** 8641 - -**time_start:** 2021-04-12 - -**time_stop:** 2021-04-13 - -**spatial:** GEOMAG - -**messenger:** magnetic field - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - uniaq_curr_maigic_tableset + * - **publisher:** + - Mirko Piersanti + * - **alph_code:** + - 40B + * - **id_tmp:** + - 86 + * - **short_name:** + - MA.I.GIC. current + * - **identifier:** + - aspis://uniaq//curr_maigic_tableset + * - **dynamic:** + - Static and depending on the length of the input data + * - **size:** + - 5MB + * - **format:** + - .mat + * - **type:** + - tableset + * - **records_number:** + - 8641 + * - **time_start:** + - 2021-04-12 + * - **time_stop:** + - 2021-04-13 + * - **spatial:** + - GEOMAG + * - **messenger:** + - magnetic field + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/uniaq_epmde_emma_timeseries.rst b/docs/source/products/data/uniaq_epmde_emma_timeseries.rst index 72509e5..5e1c4e8 100644 --- a/docs/source/products/data/uniaq_epmde_emma_timeseries.rst +++ b/docs/source/products/data/uniaq_epmde_emma_timeseries.rst @@ -2,56 +2,60 @@ Equatorial Plasma Mass Density estimates in Plasmasphere ======================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Equatorial plasma mass density estimates in plasmasphere (2 < L < 6) are derived from the the EMMA magnetometers network, updated every 15 minutes. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** uniaq_epmde_emma_timeseries - -**publisher:** University of L'Aquila Dept. of Physical and Chemical Sciences - -**alphanumeric_code:** 29 - -**id_tmp:** 33 - -**short_name:** EPMDP-Estimates - -**identifier:** aspis:///uniaq/epmdp - -**dynamic:** Static - -**size:** 200kB - -**format:** csv - -**type:** timeseries - -**records_number:** 1951 - -**time_start:** 2022-01-01 - -**time_stop:** 2023-12-21 - -**spatial:** GEOMAG - -**messenger:** MHD waves - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** ESP - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - uniaq_epmde_emma_timeseries + * - **publisher:** + - University of L'Aquila Dept. of Physical and Chemical Sciences + * - **alph_code:** + - 29 + * - **id_tmp:** + - 33 + * - **short_name:** + - EPMDP-Estimates + * - **identifier:** + - aspis:///uniaq/epmdp + * - **dynamic:** + - Static + * - **size:** + - 200kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1951 + * - **time_start:** + - 2022-01-01 + * - **time_stop:** + - 2023-12-21 + * - **spatial:** + - GEOMAG + * - **messenger:** + - MHD waves + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - ESP + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/uniaq_field_maigic_tableset.rst b/docs/source/products/data/uniaq_field_maigic_tableset.rst index 0838e28..99dc51e 100644 --- a/docs/source/products/data/uniaq_field_maigic_tableset.rst +++ b/docs/source/products/data/uniaq_field_maigic_tableset.rst @@ -2,56 +2,60 @@ Magnetospheric-Ionospheric-Gound Induced Current model - Geoelectric Field ========================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** uniaq_field_maigic_tableset - -**publisher:** Mirko Piersanti - -**alphanumeric_code:** 41B - -**id_tmp:** 87 - -**short_name:** MA.I.GIC. Geoelectric Field - -**identifier:** aspis:///univaq/field_maigic_tableset - -**dynamic:** Static and depending on the length of the input data - -**size:** 5MB - -**format:** .mat - -**type:** tableset - -**records_number:** 8641 - -**time_start:** 2021-04-12 - -**time_stop:** 2021-04-13 - -**spatial:** GEOMAG - -**messenger:** Electric Field - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - uniaq_field_maigic_tableset + * - **publisher:** + - Mirko Piersanti + * - **alph_code:** + - 41B + * - **id_tmp:** + - 87 + * - **short_name:** + - MA.I.GIC. Geoelectric Field + * - **identifier:** + - aspis:///univaq/field_maigic_tableset + * - **dynamic:** + - Static and depending on the length of the input data + * - **size:** + - 5MB + * - **format:** + - .mat + * - **type:** + - tableset + * - **records_number:** + - 8641 + * - **time_start:** + - 2021-04-12 + * - **time_stop:** + - 2021-04-13 + * - **spatial:** + - GEOMAG + * - **messenger:** + - Electric Field + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/uniaq_mag_emma_timeseries.rst b/docs/source/products/data/uniaq_mag_emma_timeseries.rst index 3fbc633..1fafe6c 100644 --- a/docs/source/products/data/uniaq_mag_emma_timeseries.rst +++ b/docs/source/products/data/uniaq_mag_emma_timeseries.rst @@ -2,56 +2,60 @@ EMMA Geomagnetic field data =========================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of the magnetic field variations recorded at 27 ground stations located in Italy and Europe along a meridional chain covering a large range in geographical latitude (from 70 to 42 degrees). The data are automatically collected in near real-time and updated every 15 minutes. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** uniaq_mag_emma_timeseries - -**publisher:** University of L'Aquila Dept. of Physical and Chemical Sciences - -**alphanumeric_code:** 10 - -**id_tmp:** 34 - -**short_name:** EMMA-data - -**identifier:** aspis://uniaq/emma - -**dynamic:** For each day, there is one master dataset containing the general information of each station and related dataset and n (maximum value 27) datasets containing the 1-minute averages of the individual stations. - -**size:** 2MB - -**format:** csv - -**type:** tableset - -**records_number:** 277 - -**time_start:** 2022-01-01 - -**time_stop:** 2023-12-21 - -**spatial:** GROUND - -**messenger:** MHD waves - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** GLE - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - uniaq_mag_emma_timeseries + * - **publisher:** + - University of L'Aquila Dept. of Physical and Chemical Sciences + * - **alph_code:** + - 10 + * - **id_tmp:** + - 34 + * - **short_name:** + - EMMA-data + * - **identifier:** + - aspis://uniaq/emma + * - **dynamic:** + - For each day, there is one master dataset containing the general information of each station and related dataset and n (maximum value 27) datasets containing the 1-minute averages of the individual stations. + * - **size:** + - 2MB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 277 + * - **time_start:** + - 2022-01-01 + * - **time_stop:** + - 2023-12-21 + * - **spatial:** + - GROUND + * - **messenger:** + - MHD waves + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - GLE + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_espseptransport_tableset.rst b/docs/source/products/data/unical_espseptransport_tableset.rst index fdf662b..eb692b8 100644 --- a/docs/source/products/data/unical_espseptransport_tableset.rst +++ b/docs/source/products/data/unical_espseptransport_tableset.rst @@ -2,56 +2,60 @@ Energetic particle spectral indices =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_espseptransport_tableset - -**publisher:** not available in DBF - -**alphanumeric_code:** 20B - -**id_tmp:** 57 - -**short_name:** SEP+ESP-spectral - -**identifier:** aspis:///unical/espseptransport_tableset_old - -**dynamic:** Static collection - -**size:** 1kB - -**format:** csv - -**type:** tableset - -**records_number:** 59 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** protons - -**spectral_min:** 0.01 - -**spectral_max:** 100 - -**spectral_units:** MeV - -**observable:** SEP,ESP,IPS,CME - -**latest update:** 2024-03-28 05:08:15 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_espseptransport_tableset + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 20B + * - **id_tmp:** + - 57 + * - **short_name:** + - SEP+ESP-spectral + * - **identifier:** + - aspis:///unical/espseptransport_tableset_old + * - **dynamic:** + - Static collection + * - **size:** + - 1kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 59 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - protons + * - **spectral_min:** + - 0.01 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,ESP,IPS,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_ace_spectrum.rst b/docs/source/products/data/unical_sep_ace_spectrum.rst index 89b5ab3..e341290 100644 --- a/docs/source/products/data/unical_sep_ace_spectrum.rst +++ b/docs/source/products/data/unical_sep_ace_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the ACE spacecraft ========================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for geoeffective target SWE events (at L1) from ACE spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_ace_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20C - -**id_tmp:** 36 - -**short_name:** SEP-spectrum-Ace - -**identifier:** aspis://unical/unical_sep_ace_spectrum - -**dynamic:** +1 kb updated every SEP event - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 8 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** L1 - -**messenger:** Protons - -**spectral_min:** 0.04 - -**spectral_max:** 5 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_ace_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20C + * - **id_tmp:** + - 36 + * - **short_name:** + - SEP-spectrum-Ace + * - **identifier:** + - aspis://unical/unical_sep_ace_spectrum + * - **dynamic:** + - +1 kb updated every SEP event + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 8 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - L1 + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.04 + * - **spectral_max:** + - 5 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_psp_spectrum.rst b/docs/source/products/data/unical_sep_psp_spectrum.rst index cf69c7e..db1f85a 100644 --- a/docs/source/products/data/unical_sep_psp_spectrum.rst +++ b/docs/source/products/data/unical_sep_psp_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the PSP spacecraft ========================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for widespread target SWE events from PSP spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_psp_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20E - -**id_tmp:** 37 - -**short_name:** SEP-spectrum-PSP - -**identifier:** aspis://unical/unical_sep_psp_spectrum - -**dynamic:** +5 kb updated every SEP event - -**size:** 5kB - -**format:** csv - -**type:** spectrum - -**records_number:** 1 - -**time_start:** 2020-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** Protons - -**spectral_min:** 0.6 - -**spectral_max:** 95 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_psp_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20E + * - **id_tmp:** + - 37 + * - **short_name:** + - SEP-spectrum-PSP + * - **identifier:** + - aspis://unical/unical_sep_psp_spectrum + * - **dynamic:** + - +5 kb updated every SEP event + * - **size:** + - 5kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 1 + * - **time_start:** + - 2020-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.6 + * - **spectral_max:** + - 95 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_soho_spectrum.rst b/docs/source/products/data/unical_sep_soho_spectrum.rst index 901d35c..540262d 100644 --- a/docs/source/products/data/unical_sep_soho_spectrum.rst +++ b/docs/source/products/data/unical_sep_soho_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the SoHO spacecraft ========================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for: geoeffective target SWE events (at L1) from SoHO spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_soho_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20F - -**id_tmp:** 58 - -**short_name:** SEP-spectrum-Soho - -**identifier:** aspis://unical/unical_sep_soho_spectrum - -**dynamic:** +1 kb updated every SEP event - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 7 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** L1 - -**messenger:** Protons - -**spectral_min:** 1.3 - -**spectral_max:** 130 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_soho_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20F + * - **id_tmp:** + - 58 + * - **short_name:** + - SEP-spectrum-Soho + * - **identifier:** + - aspis://unical/unical_sep_soho_spectrum + * - **dynamic:** + - +1 kb updated every SEP event + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 7 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - L1 + * - **messenger:** + - Protons + * - **spectral_min:** + - 1.3 + * - **spectral_max:** + - 130 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_solo_spectrum.rst b/docs/source/products/data/unical_sep_solo_spectrum.rst index 799fa66..b3474e4 100644 --- a/docs/source/products/data/unical_sep_solo_spectrum.rst +++ b/docs/source/products/data/unical_sep_solo_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the SolO spacecraft ========================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for widespread target SWE events from SolO spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_solo_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20G - -**id_tmp:** 39 - -**short_name:** SEP-spectrum-SolO - -**identifier:** aspis://unical/unical_sep_solo_spectrum - -**dynamic:** +2 kb updated every SEP event - -**size:** 5kB - -**format:** csv - -**type:** spectrum - -**records_number:** 2 - -**time_start:** 2020-03-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** Protons - -**spectral_min:** 0.03 - -**spectral_max:** 90 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_solo_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20G + * - **id_tmp:** + - 39 + * - **short_name:** + - SEP-spectrum-SolO + * - **identifier:** + - aspis://unical/unical_sep_solo_spectrum + * - **dynamic:** + - +2 kb updated every SEP event + * - **size:** + - 5kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 2 + * - **time_start:** + - 2020-03-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.03 + * - **spectral_max:** + - 90 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_stra_spectrum.rst b/docs/source/products/data/unical_sep_stra_spectrum.rst index d9716a2..6fcd665 100644 --- a/docs/source/products/data/unical_sep_stra_spectrum.rst +++ b/docs/source/products/data/unical_sep_stra_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the STEREO A spacecraft ============================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for widespread target SWE events from STEREO A spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_stra_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20H - -**id_tmp:** 40 - -**short_name:** SEP-spectrum-StereoA - -**identifier:** aspis://unical/unical_sep_stra_spectrum - -**dynamic:** +1 kb updated every SEP event - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 2 - -**time_start:** 2020-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** Protons - -**spectral_min:** 0.08 - -**spectral_max:** 100 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:16 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_stra_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20H + * - **id_tmp:** + - 40 + * - **short_name:** + - SEP-spectrum-StereoA + * - **identifier:** + - aspis://unical/unical_sep_stra_spectrum + * - **dynamic:** + - +1 kb updated every SEP event + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 2 + * - **time_start:** + - 2020-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.08 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_wind_spectrum.rst b/docs/source/products/data/unical_sep_wind_spectrum.rst index ad4bfb6..104d36a 100644 --- a/docs/source/products/data/unical_sep_wind_spectrum.rst +++ b/docs/source/products/data/unical_sep_wind_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the WIND spacecraft ========================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for: geoeffective target SWE events (at L1) from Wind spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_wind_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20I - -**id_tmp:** 41 - -**short_name:** SEP-spectrum-Wind - -**identifier:** aspis://unical/unical_sep_wind_spectrum - -**dynamic:** +1 kb updated every SEP event - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 8 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** L1 - -**messenger:** Protons - -**spectral_min:** 0.07 - -**spectral_max:** 80 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:16 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_wind_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20I + * - **id_tmp:** + - 41 + * - **short_name:** + - SEP-spectrum-Wind + * - **identifier:** + - aspis://unical/unical_sep_wind_spectrum + * - **dynamic:** + - +1 kb updated every SEP event + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 8 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - L1 + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.07 + * - **spectral_max:** + - 80 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_shockpar_tableset.rst b/docs/source/products/data/unical_shockpar_tableset.rst index c7ee3f0..9e2c067 100644 --- a/docs/source/products/data/unical_shockpar_tableset.rst +++ b/docs/source/products/data/unical_shockpar_tableset.rst @@ -2,56 +2,60 @@ Parameters of shocks associated with ESP events =============================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_shockpar_tableset - -**publisher:** not available in DBF - -**alphanumeric_code:** 22A - -**id_tmp:** 49 - -**short_name:** Shocks-parameters - -**identifier:** aspis://unical/unical_shockpar_tableset - -**dynamic:** +300 byte updated every event - -**size:** 20kB - -**format:** csv - -**type:** tableset - -**records_number:** 65 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** Protons,Magnetic field - -**spectral_min:** 0.01 - -**spectral_max:** 100 - -**spectral_units:** MeV - -**observable:** IPS,SW,SEP,ESP,IMF - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_shockpar_tableset + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 22A + * - **id_tmp:** + - 49 + * - **short_name:** + - Shocks-parameters + * - **identifier:** + - aspis://unical/unical_shockpar_tableset + * - **dynamic:** + - +300 byte updated every event + * - **size:** + - 20kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 65 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons,Magnetic field + * - **spectral_min:** + - 0.01 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - IPS,SW,SEP,ESP,IMF + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_facula_image.rst b/docs/source/products/data/unict_facula_image.rst index 1540427..7a7b2b9 100644 --- a/docs/source/products/data/unict_facula_image.rst +++ b/docs/source/products/data/unict_facula_image.rst @@ -2,56 +2,60 @@ Faculae geometrical characteristics =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_facula_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 5B - -**id_tmp:** 91 - -**short_name:** Facular area - -**identifier:** aspis:///unict/unict_facula_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-10-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_facula_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 5B + * - **id_tmp:** + - 91 + * - **short_name:** + - Facular area + * - **identifier:** + - aspis:///unict/unict_facula_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-10-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_filament_image.rst b/docs/source/products/data/unict_filament_image.rst index 492e817..d356947 100644 --- a/docs/source/products/data/unict_filament_image.rst +++ b/docs/source/products/data/unict_filament_image.rst @@ -2,56 +2,60 @@ Filament position and geometrical characteristics ================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_filament_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 5C - -**id_tmp:** 92 - -**short_name:** Solar Filaments - -**identifier:** aspis:///unict/unict_filament_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 36 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-10-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_filament_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 5C + * - **id_tmp:** + - 92 + * - **short_name:** + - Solar Filaments + * - **identifier:** + - aspis:///unict/unict_filament_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 36 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-10-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_offlimb_image.rst b/docs/source/products/data/unict_offlimb_image.rst index ddf5412..6298a66 100644 --- a/docs/source/products/data/unict_offlimb_image.rst +++ b/docs/source/products/data/unict_offlimb_image.rst @@ -2,56 +2,60 @@ Geometry and location of prominences on the solar limb ====================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_offlimb_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 6B - -**id_tmp:** 93 - -**short_name:** Prominences location and geometry - -**identifier:** aspis:///unict/unict_offlimb_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 3 - -**time_start:** 2022-12-15 - -**time_stop:** 2023-10-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_offlimb_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 6B + * - **id_tmp:** + - 93 + * - **short_name:** + - Prominences location and geometry + * - **identifier:** + - aspis:///unict/unict_offlimb_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 3 + * - **time_start:** + - 2022-12-15 + * - **time_stop:** + - 2023-10-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_sunspot_image.rst b/docs/source/products/data/unict_sunspot_image.rst index c1a96b0..9a89ea7 100644 --- a/docs/source/products/data/unict_sunspot_image.rst +++ b/docs/source/products/data/unict_sunspot_image.rst @@ -2,56 +2,60 @@ Sunspots Zurich and McIntosh class ================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_sunspot_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 4B - -**id_tmp:** 94 - -**short_name:** Sunspots class - -**identifier:** aspis:///unict/unict_sunspot_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-12-15 - -**time_stop:** 2023-02-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:17 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_sunspot_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 4B + * - **id_tmp:** + - 94 + * - **short_name:** + - Sunspots class + * - **identifier:** + - aspis:///unict/unict_sunspot_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-12-15 + * - **time_stop:** + - 2023-02-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitn_flux_cses_timeseries.rst b/docs/source/products/data/unitn_flux_cses_timeseries.rst index f1172c7..d92ca63 100644 --- a/docs/source/products/data/unitn_flux_cses_timeseries.rst +++ b/docs/source/products/data/unitn_flux_cses_timeseries.rst @@ -2,56 +2,60 @@ CSES satellite particle flux data ================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Particle flux in the Lshell – pitch reference frame. Lshell will be calculated using the IGRF model for the internal origin field and Tsyganenko model for the external origin field. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitn_flux_cses_timeseries - -**publisher:** Roberto Battiston - -**alphanumeric_code:** 44 - -**id_tmp:** 42 - -**short_name:** CSES Flux - -**identifier:** aspis://unitn/flux_cses_timeseries - -**dynamic:** Static and depending on the length of the input data - -**size:** 5MB - -**format:** .mat - -**type:** timeseries - -**records_number:** 18129 - -**time_start:** 2021-04-12 - -**time_stop:** 2021-04-13 - -**spatial:** IONO - -**messenger:** phys.flux - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** GCR,ESP,SEP - -**latest update:** 2024-03-28 05:08:17 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitn_flux_cses_timeseries + * - **publisher:** + - Roberto Battiston + * - **alph_code:** + - 44 + * - **id_tmp:** + - 42 + * - **short_name:** + - CSES Flux + * - **identifier:** + - aspis://unitn/flux_cses_timeseries + * - **dynamic:** + - Static and depending on the length of the input data + * - **size:** + - 5MB + * - **format:** + - .mat + * - **type:** + - timeseries + * - **records_number:** + - 18129 + * - **time_start:** + - 2021-04-12 + * - **time_stop:** + - 2021-04-13 + * - **spatial:** + - IONO + * - **messenger:** + - phys.flux + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - GCR,ESP,SEP + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_halpha_tsst_image.rst b/docs/source/products/data/unitov_halpha_tsst_image.rst index 52acbd5..da9827f 100644 --- a/docs/source/products/data/unitov_halpha_tsst_image.rst +++ b/docs/source/products/data/unitov_halpha_tsst_image.rst @@ -2,56 +2,60 @@ TSST H-alpha Full Disk Images ============================= -.. contents:: The tiny table of contents +.. contents:: Table of contents The Hα channel of the TSST is a Daystar SR-127 QT, an achromatic refractor with 127 mm aperture and a focal length of 2667 mm. The telescope features a narrow band filter with a passband of 0.04 nm centered at the Hα line. The filter is a temperature stabilized etalon in collimated configuration, and it is the same filter used in the GONG network for the Hα channel to monitor the chromospheric transients (Giersch, 2013). The Hα channel is equipped with a focal reducer, acting also as a field curvature corrector, to match the Dalsa Pantera 1M60 pixel scale of the MOF channel (2.6 arcsec/pixel). The main goal of this TSST channel is the real time detection of flaring region (Piazzesi et al., 2012, Pötzi et al., 2015, 2018) during the impulsive and flash phases when the intensity reaches its maximum (Benz, 2017). Hα images are extremely important for ground based SWe monitoring (see, e.g. Veronig & Potzi, 2016) and to automatically detect and track structures in the solar chromosphere, as filaments (Bernasconi et al., 2005, Fuller et al., 2005, Bonnin et al., 2013) and prominences (Wang et al., 2010), that can be associated with flare and coronal mass ejections. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_halpha_tsst_image - -**publisher:** University of Rome Tor Vergata - -**alphanumeric_code:** 2 - -**id_tmp:** 59 - -**short_name:** TSST-halpha - -**identifier:** aspis:///unitov/halpha_tsst_image - -**dynamic:** data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares - -**size:** 20GB - -**format:** .fits - -**type:** image - -**records_number:** 9 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-05-01 - -**spatial:** SUN - -**messenger:** photons - -**spectral_min:** 656.26 - -**spectral_max:** 656.34 - -**spectral_units:** nm - -**observable:** spect.line.intensity,AR,flare - -**latest update:** 2024-03-28 05:08:17 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_halpha_tsst_image + * - **publisher:** + - University of Rome Tor Vergata + * - **alph_code:** + - 2 + * - **id_tmp:** + - 59 + * - **short_name:** + - TSST-halpha + * - **identifier:** + - aspis:///unitov/halpha_tsst_image + * - **dynamic:** + - data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares + * - **size:** + - 20GB + * - **format:** + - .fits + * - **type:** + - image + * - **records_number:** + - 9 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-05-01 + * - **spatial:** + - SUN + * - **messenger:** + - photons + * - **spectral_min:** + - 656.26 + * - **spectral_max:** + - 656.34 + * - **spectral_units:** + - nm + * - **observable:** + - spect.line.intensity,AR,flare + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_icme_tableset.rst b/docs/source/products/data/unitov_icme_tableset.rst index 0697ea9..c8b0204 100644 --- a/docs/source/products/data/unitov_icme_tableset.rst +++ b/docs/source/products/data/unitov_icme_tableset.rst @@ -2,56 +2,60 @@ UNITOV Catalogue of geoeffective CMEs ===================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents A database associating L1 Time of Arrival and Speed of an interplanetary CME to the kinematic characteristics of the corresponding CME, covering the period 1996-2020. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_icme_tableset - -**publisher:** University of Rome Tor Vergata Dept. of Physics - -**alphanumeric_code:** 15 - -**id_tmp:** 44 - -**short_name:** UNITOV-ICME - -**identifier:** aspis:/unitov/icme_tableset - -**dynamic:** +10kB updated every year - -**size:** 100kB - -**format:** csv - -**type:** tableset - -**records_number:** 213 - -**time_start:** 1997-01-01 - -**time_stop:** 2019-12-31 - -**spatial:** IP - -**messenger:** Photons,Protons - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:17 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_icme_tableset + * - **publisher:** + - University of Rome Tor Vergata Dept. of Physics + * - **alph_code:** + - 15 + * - **id_tmp:** + - 44 + * - **short_name:** + - UNITOV-ICME + * - **identifier:** + - aspis:/unitov/icme_tableset + * - **dynamic:** + - +10kB updated every year + * - **size:** + - 100kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 213 + * - **time_start:** + - 1997-01-01 + * - **time_stop:** + - 2019-12-31 + * - **spatial:** + - IP + * - **messenger:** + - Photons,Protons + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_iss_lidal_timeseries.rst b/docs/source/products/data/unitov_iss_lidal_timeseries.rst index 1b70ce9..9ee9f05 100644 --- a/docs/source/products/data/unitov_iss_lidal_timeseries.rst +++ b/docs/source/products/data/unitov_iss_lidal_timeseries.rst @@ -2,56 +2,60 @@ LIDAL Flux and Dose timeseries ============================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_iss_lidal_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 64A - -**id_tmp:** 50 - -**short_name:** LIDAL_values - -**identifier:** aspis:///unitov/lidal - -**dynamic:** LIDAL is foreseen to be acquiring data utnil 2028. Estimation is 1 MB per year - -**size:** 60kB - -**format:** csv - -**type:** timeseries - -**records_number:** 1096 - -**time_start:** 2020-01-19 - -**time_stop:** 2022-12-31 - -**spatial:** GEOMAG - -**messenger:** charged nuclei - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** SEP,ESP,GCR - -**latest update:** 2024-03-28 05:08:17 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_iss_lidal_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 64A + * - **id_tmp:** + - 50 + * - **short_name:** + - LIDAL_values + * - **identifier:** + - aspis:///unitov/lidal + * - **dynamic:** + - LIDAL is foreseen to be acquiring data utnil 2028. Estimation is 1 MB per year + * - **size:** + - 60kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1096 + * - **time_start:** + - 2020-01-19 + * - **time_stop:** + - 2022-12-31 + * - **spatial:** + - GEOMAG + * - **messenger:** + - charged nuclei + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - SEP,ESP,GCR + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_mag_tsst_image.rst b/docs/source/products/data/unitov_mag_tsst_image.rst index 4e8cddb..e409bc7 100644 --- a/docs/source/products/data/unitov_mag_tsst_image.rst +++ b/docs/source/products/data/unitov_mag_tsst_image.rst @@ -2,56 +2,60 @@ TSST Full Disk LoS magnetic maps ================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_mag_tsst_image - -**publisher:** University of Rome Tor Vergata - -**alphanumeric_code:** 1A - -**id_tmp:** 60 - -**short_name:** TSST-mag - -**identifier:** aspis:///unitov/mag_tsst_image - -**dynamic:** data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares - -**size:** 300GB - -**format:** .fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-05-01 - -**spatial:** SUN - -**messenger:** photons - -**spectral_min:** 769.88 - -**spectral_max:** 769.92 - -**spectral_units:** nm - -**observable:** phys.magField,AR - -**latest update:** 2024-03-28 05:08:17 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_mag_tsst_image + * - **publisher:** + - University of Rome Tor Vergata + * - **alph_code:** + - 1A + * - **id_tmp:** + - 60 + * - **short_name:** + - TSST-mag + * - **identifier:** + - aspis:///unitov/mag_tsst_image + * - **dynamic:** + - data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares + * - **size:** + - 300GB + * - **format:** + - .fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-05-01 + * - **spatial:** + - SUN + * - **messenger:** + - photons + * - **spectral_min:** + - 769.88 + * - **spectral_max:** + - 769.92 + * - **spectral_units:** + - nm + * - **observable:** + - phys.magField,AR + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_rdparameter_tableset.rst b/docs/source/products/data/unitov_rdparameter_tableset.rst index ccdb3bb..e35cf84 100644 --- a/docs/source/products/data/unitov_rdparameter_tableset.rst +++ b/docs/source/products/data/unitov_rdparameter_tableset.rst @@ -2,56 +2,60 @@ R and D Active Region parameters ================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents Parameters for flare-forecasting applications, representing the complexity of a solar active region -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_rdparameter_tableset - -**publisher:** University of Rome Tor Vergata Dept. of Physics - -**alphanumeric_code:** 3 - -**id_tmp:** 46 - -**short_name:** AR-parameters - -**identifier:** aspis:///unitov/rdparameter_tableset - -**dynamic:** +1MB updated every month - -**size:** 20MB - -**format:** csv - -**type:** tableset - -**records_number:** 35998 - -**time_start:** 2012-09-14 - -**time_stop:** 2016-04-13 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR,flare - -**latest update:** 2024-03-28 05:08:18 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_rdparameter_tableset + * - **publisher:** + - University of Rome Tor Vergata Dept. of Physics + * - **alph_code:** + - 3 + * - **id_tmp:** + - 46 + * - **short_name:** + - AR-parameters + * - **identifier:** + - aspis:///unitov/rdparameter_tableset + * - **dynamic:** + - +1MB updated every month + * - **size:** + - 20MB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 35998 + * - **time_start:** + - 2012-09-14 + * - **time_stop:** + - 2016-04-13 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR,flare + * - **latest update:** + - 2024-03-28 05:08:18 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_vel_tsst_image.rst b/docs/source/products/data/unitov_vel_tsst_image.rst index e534529..fb7b190 100644 --- a/docs/source/products/data/unitov_vel_tsst_image.rst +++ b/docs/source/products/data/unitov_vel_tsst_image.rst @@ -2,56 +2,60 @@ TSST Full Disk Velocity Maps ============================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_vel_tsst_image - -**publisher:** University of Rome Tor Vergata - -**alphanumeric_code:** 1B - -**id_tmp:** 61 - -**short_name:** TSST-vel - -**identifier:** aspis:///unitov/vel_tsst_image - -**dynamic:** data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares - -**size:** 300GB - -**format:** .fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-05-01 - -**spatial:** SUN - -**messenger:** photons - -**spectral_min:** 769.88 - -**spectral_max:** 769.92 - -**spectral_units:** nm - -**observable:** phys.veloc,AR - -**latest update:** 2024-03-28 05:08:18 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_vel_tsst_image + * - **publisher:** + - University of Rome Tor Vergata + * - **alph_code:** + - 1B + * - **id_tmp:** + - 61 + * - **short_name:** + - TSST-vel + * - **identifier:** + - aspis:///unitov/vel_tsst_image + * - **dynamic:** + - data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares + * - **size:** + - 300GB + * - **format:** + - .fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-05-01 + * - **spatial:** + - SUN + * - **messenger:** + - photons + * - **spectral_min:** + - 769.88 + * - **spectral_max:** + - 769.92 + * - **spectral_units:** + - nm + * - **observable:** + - phys.veloc,AR + * - **latest update:** + - 2024-03-28 05:08:18 Columns specification ~~~~~~~~~~~~~~~~~~~~~ -- GitLab