diff --git a/docs/source/products/data/external_ace_swepam_timeseries.rst b/docs/source/products/data/external_ace_swepam_timeseries.rst index cd21da0ca29dd6d195572dec610b344fa8913201..4be227ea4bddcfbe8e01d48b11e1f47cb4571427 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 52fe3ff541bead24f9e0361d3330db2c52274a87..766cd96eba8891d7d67672139e6a63cb96bb27ec 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 ee4b7f357593e817fecb8834859aa7bdbf0dc64d..f179e8fb904b05ef6b65cbdb3aef81cd3ed50b33 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 569606bfcdee89936d7127acceec0816f045de98..e6f11622b2ea65f9527bc76920fd85724cca6933 100644 --- a/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst +++ b/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst @@ -1,52 +1,200 @@ -======================================== -INAF SuperDARN Cross 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 -~~~~~~~~~~~~~~~~ - -| **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 - +============================= +SuperDARN Polar Cap Potential +============================= + +.. 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 +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 + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 0e0ebb7875443ec1d624a3d4fa4436adcc1bbe2c..0000000000000000000000000000000000000000 --- 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 c303fa2f45522a643dfd431cf446320c5ac70108..b7d8d36e65884000536ec2a84acb48773eba8d0e 100644 --- a/docs/source/products/data/inaf_data_solopas_timeseries.rst +++ b/docs/source/products/data/inaf_data_solopas_timeseries.rst @@ -1,61 +1,126 @@ -========================================= -INAF Solar Orbiter-PAS data -========================================= +================================ +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. +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) +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. 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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 377192f2954970efbbaa0156fab2684ea0b74487..0000000000000000000000000000000000000000 --- 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 c88d3de33373147e204f408ba89269f34250ac80..3542b5cce86bf33329a9789a26015f8a93894bec 100644 --- a/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst +++ b/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst @@ -1,46 +1,82 @@ -========================================= -INAF SVIRCO neutron monitor (1h) -========================================= - -.. 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: 1h. - -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**: timeseries - -| **Data formats**: - ASCII - - -| **Sample**: https://drive.google.com/file/d/17ahUkpirH-DUWnqBr731ExAgjMBGNeJ4/view?usp=sharing - -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 - +============================================= +SVIRCO Observatory - the Rome neutron monitor +============================================= + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 56a72c4d0e71bbf772a1cbf950630b4ef95ecbdf..0000000000000000000000000000000000000000 --- 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 274a7e9cead0be49d093250b9ad14204496de65c..8e7960b4a4ca6168eef6d57cddf4918edec7ec5a 100644 --- a/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst +++ b/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst @@ -1,43 +1,92 @@ -========================================= -INAF SVIRCO neutron monitor (5m) -========================================= - -.. 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% - -**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**: https://drive.google.com/file/d/1U4o3cRHggf7_9f8V_qCVvgRt0RufDxIw/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 - +============================================== +SVIRCO Obser vatory - the Rome neutron monitor +============================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 218f8b4d2537da163f7dc1638457f060af9372e4..0000000000000000000000000000000000000000 --- 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 da5f93918251c5562849821a4da2f5a4ff5c7193..1867a25fbc0cb6c13ad51958e44d7bc50c5b89b7 100644 --- a/docs/source/products/data/inaf_gsmaps_datacube.rst +++ b/docs/source/products/data/inaf_gsmaps_datacube.rst @@ -1,53 +1,92 @@ ===================================================== -INAF Grad-Shafranov Reconstruction of Magnetic Clouds +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. -**Providers**: - -- **Wind** - sources: - - - MFI - - SWE -- **Solar Orbiter** - sources: - - - SWA - - MAG -- **Small Scale Magnetic Flux Rope Database** - source: - - - http://fluxrope.info/ - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T12:00:39+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: spectral-cubes - -| **Data formats**: - mat - - -| **Sample**: https://drive.google.com/file/d/1Sij8YjsMeCS_vVwOxHzTDreAHYNy6p0r/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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 e6ffa7554a3127073cec41dde722c3cadf7a7d52..b7baee1975cd9338c0bfd2aa3fd80a483f0eac9b 100644 --- a/docs/source/products/data/inaf_m2flare_tableset.rst +++ b/docs/source/products/data/inaf_m2flare_tableset.rst @@ -1,49 +1,132 @@ -========================================= -INAF > 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. - -**Providers**: - -- **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 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 - +============================== +IAPS ≥M2 SXR Flare Catalogue +============================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 82363faf1ede439a47b5f0d4b9c0c221387f8196..c580787ea7e2696a7a0ef2aebf2643c5e5ce7209 100644 --- a/docs/source/products/data/inaf_na_mercexo_image.rst +++ b/docs/source/products/data/inaf_na_mercexo_image.rst @@ -1,38 +1,157 @@ =============================================== -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). - -**Providers**: - -- **THEMIS solar telescope** - - -| **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 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 - +.. 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 +~~~~~~~~~~ + +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. + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 2f2e0fcbd0d1ed56f679c0fcaad7f5394018ed4d..0000000000000000000000000000000000000000 --- 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 268b27c6024329b80f0ac3ccce81a3265d898d66..f60fb579494d9614b0a5e45a4c90d79274f77204 100644 --- a/docs/source/products/data/inaf_s1sep_tableset.rst +++ b/docs/source/products/data/inaf_s1sep_tableset.rst @@ -1,53 +1,207 @@ -========================================= -INAF S1 SEP Catalogue -========================================= +============================ +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. -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 3346c00593d0336cdbf7175c018f031799336e9f..0963e5ab3958144d73032121e120a6b42e9c64aa 100644 --- a/docs/source/products/data/inaf_s2sep_tableset.rst +++ b/docs/source/products/data/inaf_s2sep_tableset.rst @@ -1,53 +1,207 @@ -========================================= -INAF S2 SEP Catalogue -========================================= +============================ +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. -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 d2d0b9dc2ce5698dff856393587d22cf7f813255..0000000000000000000000000000000000000000 --- 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 3080e9a4c1e94a016f95f768e6500197d8106f35..7777305761bda3574b940fc062193e693f907ec0 100644 --- a/docs/source/products/data/inaf_tps_datacube.rst +++ b/docs/source/products/data/inaf_tps_datacube.rst @@ -1,48 +1,92 @@ ================================================ -INAF Test Particle Simulation on Magnetic Clouds +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. -**Providers**: - -- **Solar Modulation Parameter Table Oulu NM** - source: - - - https://cosmicrays.oulu.fi/phi/phi.html -- **Grad-Shafranov reconstruction maps** - source: - - - in ASPIS - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T12:00:39+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: spectral-cubes - -| **Data formats**: - mat - - -| **Sample**: https://drive.google.com/file/d/1DueJgqzWtUO3-ptb1AmgaotZuIaPYEzY/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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 c64a4f95b4619d0234dd0233b11ac21552d0547f..0000000000000000000000000000000000000000 --- 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 e4ca620ec389f59b8d1bd709df938515cb8cdb38..0000000000000000000000000000000000000000 --- 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 267f837a200c764007549ca7e49b12736c528788..46cb275230e05001532763fc09cf463e95980c3c 100644 --- a/docs/source/products/data/inaf_vbcorr_wind_tableset.rst +++ b/docs/source/products/data/inaf_vbcorr_wind_tableset.rst @@ -1,47 +1,98 @@ -==================================================================================== -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 +.. 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. -**Providers**: - -- **WIND** - sources: - - - 3-D Plasma and Energetic Particle Investigation (3DP) - - Magnetic Field Instrument (MFI) - - -| **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 - +References +~~~~~~~~~~ + +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 + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 bab6560a656f8dbf869bd0bdbf95799f1969a6c5..0000000000000000000000000000000000000000 --- 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 1bf9ec856001533b9f7cea48eea4bfeaa40b9d0e..0000000000000000000000000000000000000000 --- 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 7adac1878e2feec8f6ddfbc4990bd070b838ce9d..0000000000000000000000000000000000000000 --- 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_cses_hepd_spectrum.rst b/docs/source/products/data/infn_cses_hepd_spectrum.rst index c52aa746445a6c3e7704849e4239b62cdff299f0..101557c299850c16766057dbdd2cd427af73f62f 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 fc1c94f081660fd35f5ee12e7944dcb305ee3833..9fc615e84ed6c9f28dc34fa6e5745b4204a12e92 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 6573397d674d84ddbc8fd45cb70407ed5b59d061..1d9f643431302241e82030de449dbfd522f22589 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 806906d4a9dca2a5225b7f2a6add95e11f306842..036958f43eed827a5cc00a41e2364e2cf94d1200 100644 --- a/docs/source/products/data/infn_saandose_samadha_timeseries.rst +++ b/docs/source/products/data/infn_saandose_samadha_timeseries.rst @@ -1,38 +1,87 @@ -================================================== -INFN SAMADHA neutron dose rate at Mount Chacaltaya -================================================== +============================================= +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. -**Providers**: - -- **SAMADHA project** - source: - - - neutron dosimeter (rem counter) - - -| **Product Type**: data - -| **Status**: Inactive - -| **Creation date**: 2022-04-29T16:11:31+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text - - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -ND - +References +~~~~~~~~~~ + +http://samadha.to.infn.it + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 e5c5bd3751dfbfd74ce0a4268f39c33b7fe84e94..e1a2431261658845ab4a16e89966adf91040310f 100644 --- a/docs/source/products/data/infn_tgndose_samadha_timeseries.rst +++ b/docs/source/products/data/infn_tgndose_samadha_timeseries.rst @@ -1,37 +1,87 @@ -============================================== -INFN SAMADHA neutron dose rate at Testa Grigia -============================================== +========================================= +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. -**Providers**: - -- **SAMADHA** - source: - - - neutron detector (rem counter) - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-29T16:11:31+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - text - - -| **Sample**: ND - -Capabilities -~~~~~~~~~~~~ - -ND +References +~~~~~~~~~~ + +http://samadha.to.infn.it + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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/ingv_alert_aqu_timeseries.rst b/docs/source/products/data/ingv_alert_aqu_timeseries.rst index 34d644b3d6918dd01584961da47143666adcffc1..03fd83b68173f900cee0ab437e7604e7d639ab31 100644 --- a/docs/source/products/data/ingv_alert_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_alert_aqu_timeseries.rst @@ -1,51 +1,135 @@ -========================================= -INGV L'Aquila GIC level alert -========================================= - -.. 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) - -**Providers**: - -- **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 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 - +====================================================== +INGV geomagnetic data, GIC indices and alert: L'Aquila +====================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 12f6c1c9cc9d7ac93deac3690942f9eaf6c232d7..fe23a673281bfb5e3f9557ee43a195b00898b670 100644 --- a/docs/source/products/data/ingv_alert_cts_timeseries.rst +++ b/docs/source/products/data/ingv_alert_cts_timeseries.rst @@ -1,51 +1,132 @@ -==================================== -INGV Castello Tesino GIC level alert -==================================== +============================================================= +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) -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 1428320cb60a3fe0059cb3fcf6426c8d316dac26..3f667530123fb0edb31f4814e2a583c6eebb7f31 100644 --- a/docs/source/products/data/ingv_alert_dur_timeseries.rst +++ b/docs/source/products/data/ingv_alert_dur_timeseries.rst @@ -1,51 +1,132 @@ -============================ -INGV Duronia GIC level alert -============================ +===================================================== +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) -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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_int_timeseries.rst b/docs/source/products/data/ingv_alert_int_timeseries.rst index 129b61e8812a85af0f6b78a14d6d18a61686d8ba..f3d991b67ad43ebd44a187ae51bfd1208a1898a0 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 b1848ada74ff5d3b11ac7db39f7b9a8dfae2cae8..c2feed37f52fa9df9d0385ed85f9ad61e33fad72 100644 --- a/docs/source/products/data/ingv_alert_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_alert_lmp_timeseries.rst @@ -1,51 +1,132 @@ -========================================= -INGV Lampedusa GIC level alert -========================================= +======================================================= +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) -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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_wdc_timeseries.rst b/docs/source/products/data/ingv_alert_wdc_timeseries.rst index f6a5db5f711bd858e714e48715a9f006626ae179..1675fc8e4d8cff79f25c7ffc8d64424bb3eb7acb 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 2f767c08bf50cda1d6051e0f0fa6929a859a46d7..ac14a8b268e250b17b89151d3f621c6642abe9fd 100644 --- a/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst @@ -1,48 +1,117 @@ -=========================================== -INGV Autoscaled data Bahia Blanca Ionosonde -=========================================== +====================================== +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 -**Providers**: - -- **AIS-INGV ionosonde** - - -| **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 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 - +References +~~~~~~~~~~ + +http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 7b5cdf3d4273ff3fc05352623b748693fe712bc0..a8a85d6a4c81b75fd4bdd9c90328b9c5b5040fe2 100644 --- a/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst @@ -1,48 +1,117 @@ -========================================= -INGV Autoscaled data Gibilmanna Ionosonde -========================================= +==================================== +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 -**Providers**: - -- **AIS-INGV ionosonde** - - -| **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 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 - +References +~~~~~~~~~~ + +http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 687e4d19f6515a31e6a49b8ea1255ab14631794f..287c30e8277b743c59ee7a1179e366c6ec95bf66 100644 --- a/docs/source/products/data/ingv_autoiono_rome_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_rome_timeseries.rst @@ -1,48 +1,117 @@ -========================================= -INGV Autoscaled data Rome Ionosonde -========================================= +============================== +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 -**Providers**: - -- **AIS-INGV ionosonde** - - -| **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 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 - +References +~~~~~~~~~~ + +http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 c09ff8064dee0365a655134e1cc00767e4b6a56f..10e5a97b862e23bf44f3539c487b91a4ea8ef407 100644 --- a/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst @@ -1,48 +1,117 @@ -====================================== -INGV Autoscaled data Tucuman Ionosonde -====================================== +================================= +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 -**Providers**: - -- **AIS-INGV ionosonde** - - -| **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 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 - +References +~~~~~~~~~~ + +http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 dd738cecc21abb6217b4c585438be6adfe480a14..3dbf61d258b3e75d97ff6497f8e29948cc9acb2d 100644 --- a/docs/source/products/data/ingv_b_swarm_image.rst +++ b/docs/source/products/data/ingv_b_swarm_image.rst @@ -1,39 +1,107 @@ -========================================= -INGV Swarm vector magnetic field maps -========================================= +================================ +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. -**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/1hyNQW6Gk_AaqXG3KGbKtRZ7c1KCAjTZu/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.3: Download: Web GUI -- ext2230.3: Download: ASPIS.py - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 d21f0903f0f2ecb8adbebcd570927d4820d4fc74..4a8ca4566d72cd42f5aac67279558d910722022d 100644 --- a/docs/source/products/data/ingv_b_swarm_timeseries.rst +++ b/docs/source/products/data/ingv_b_swarm_timeseries.rst @@ -1,41 +1,147 @@ -=========================================================== -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 +.. 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 -**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/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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 4c9b27ddd5c5232dc08546fc1bb891ae597ff325..0000000000000000000000000000000000000000 --- 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 edd78f6d3b8d3940b819d22688362bf9e06ba71a..0000000000000000000000000000000000000000 --- 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 80ef7cb9c2e5e8588f9eae9d970d9b33aa5fcc00..0000000000000000000000000000000000000000 --- 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 5471af79cfcf0bc41cdff168e1494519b71920a7..0000000000000000000000000000000000000000 --- 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 661fedd1587ec3cc6885e31678a185ffa8e22a8d..f2f2a564ea8017ca3c14cf0b529341ff7bde1ae8 100644 --- a/docs/source/products/data/ingv_bvect_cses_tableset.rst +++ b/docs/source/products/data/ingv_bvect_cses_tableset.rst @@ -1,69 +1,102 @@ -===================================================== -INGV 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). - -Each file contains 6 columns: - -#. 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. - -Sub-Sub-folders: - -* “csv”: Yearly .csv data. - -* “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. - -* “nc”: Yearly netCDF data. - -* “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. - -**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 `_ - -**Providers**: - -- **CSES-01 mission** - source: - - - High Precision 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/1Pw-9K9iSgmShWu5faeYLAA_xnNYJJji1/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 - +================================================ +CSES-01 on track values of vector magnetic field +================================================ + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 2d02669ce72509125e4ba5e985f057756898d3da..ed8d81ba3137c165ce9ddd586865ea1a04fa7609 100644 --- a/docs/source/products/data/ingv_evect_cses_tableset.rst +++ b/docs/source/products/data/ingv_evect_cses_tableset.rst @@ -1,66 +1,102 @@ -===================================================== -INGV 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). - -Each file contains 6 columns: - -#. 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. - -#. electric field vector time series (Ez) with a 0.5 Hz sampling in NEC coordinates and units mV/m. - -Sub-Sub-folders: - -* “csv”: Yearly and orbital .csv data. - -* “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. - -* “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. - - -**References:** - -**Providers**: - -- **CSES-01 mission** - source: - - - 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**: tableset - -| **Data formats**: - text file - - -| **Sample**: https://drive.google.com/file/d/1xPLSlHW3WSOFR7NRzvoQQD2YXKeEagEl/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 - +================================================ +CSES-01 on track values of vector electric field +================================================ + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 a37df460f93fee559220d8e3af270b3a5d5395ec..0000000000000000000000000000000000000000 --- 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 fa4261a509ca3edafdcec866fc5c8dc7f1ac2e06..65ef3f8f903446d0f43c5313c2c2e3df8653337e 100644 --- a/docs/source/products/data/ingv_gic_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_gic_aqu_timeseries.rst @@ -1,49 +1,132 @@ -========================================= -INGV L'Aquila GIC index -========================================= - -.. 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. - -**Providers**: - -- **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 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 - +====================================================== +INGV geomagnetic data, GIC indices and alert: L'Aquila +====================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 ab61cfd35c59e874b7285694d47caf0f5197abe9..ab407a60e4021de239839ce4a52897b1f9b18fa9 100644 --- a/docs/source/products/data/ingv_gic_cts_timeseries.rst +++ b/docs/source/products/data/ingv_gic_cts_timeseries.rst @@ -1,49 +1,132 @@ -========================================= -INGV Castello Tesino GIC index -========================================= - -.. 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. - -**Providers**: - -- **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 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 - +============================================================= +INGV geomagnetic data, GIC indices and alert: Castello Tesino +============================================================= + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 03e718ae1b470bd544cdd77934385f73c219e269..d1025184ac4e44f0dda1ea1f5f6e9433b306f758 100644 --- a/docs/source/products/data/ingv_gic_dur_timeseries.rst +++ b/docs/source/products/data/ingv_gic_dur_timeseries.rst @@ -1,49 +1,132 @@ -========================================= -INGV Duronia GIC index -========================================= - -.. 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. - -**Providers**: - -- **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 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 - +===================================================== +INGV geomagnetic data, GIC indices and alert: Duronia +===================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 c6a23fb824963f6a2d9a2dee43104c6d5a88dcd7..47efee6190e55abc61f013edfd2d4742b2e6cf5a 100644 --- a/docs/source/products/data/ingv_gic_int_timeseries.rst +++ b/docs/source/products/data/ingv_gic_int_timeseries.rst @@ -1,49 +1,137 @@ -============================================ -INGV GIC index for 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. - -**Providers**: - -- **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 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 - +============================================================================ +Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories +============================================================================ + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 7ac40160b00abb270d7905f955ba72d39ee1c87a..e7cbb63b23d68662b595e490bf915e7a40e3921a 100644 --- a/docs/source/products/data/ingv_gic_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_gic_lmp_timeseries.rst @@ -1,49 +1,132 @@ -========================================= -INGV Lampedusa GIC index -========================================= - -.. 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. - -**Providers**: - -- **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 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 - +======================================================= +INGV geomagnetic data, GIC indices and alert: Lampedusa +======================================================= + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 e3c974ef44ea66a1936adb0076377d3331d859bb..a150198ca0bb3599e3b5bd983a3048351af33263 100644 --- a/docs/source/products/data/ingv_gic_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_gic_wdc_timeseries.rst @@ -1,49 +1,137 @@ -======================================================================= -INGV GIC index for 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. - -**Providers**: - -- **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 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 - +======================================================================================================== +Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories +======================================================================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 9dcf9147eab7a3527cab78425e0b261ccf9ad80d..0000000000000000000000000000000000000000 --- 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 8cb547fb32dfca11c37c9f3f0195f64bfdd76611..0000000000000000000000000000000000000000 --- 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 8bfffe6f406b4f750a904215e6ccb06d4cf25fb3..227feeb0a77148e72d227039f7c854c6f1d59345 100644 --- a/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst @@ -1,38 +1,107 @@ -============================================ -INGV Long Term MUF maps centered on Cagliari -============================================ +======================================= +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. -**Providers**: - -- **INGV model** - - -| **Product Type**: lookup-table - -| **Status**: Inactive - -| **Creation date**: 2022-04-27T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - png - - -| **Sample**: https://drive.google.com/file/d/1OlmXoC8dVV9COHgbs_Nuv7egePhEMVaF/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 adea00fd8688e28ec40c1bc03f6e4221e95dcebe..1fa87b3ef73db3047633ccaec999506d80e8a898 100644 --- a/docs/source/products/data/ingv_ltmuf_catania_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_catania_tableset.rst @@ -1,38 +1,107 @@ -=========================================== -INGV Long Term MUF maps centered on Catania -=========================================== +====================================== +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. -**Providers**: - -- **INGV model** - - -| **Product Type**: lookup-table - -| **Status**: Inactive - -| **Creation date**: 2022-04-27T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - png - - -| **Sample**: https://drive.google.com/file/d/15P1zVVveGqEHLFJzTcSwwpELDv9J-nqR/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 9166bc99e4774dd4d1d402c7efa304a56b5ef3a1..8e4b51e486eee85f6e03cd3d51b0c3fc1fb41ee0 100644 --- a/docs/source/products/data/ingv_ltmuf_milan_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_milan_tableset.rst @@ -1,38 +1,107 @@ -========================================= -INGV Long Term MUF maps centered on Milan -========================================= +===================================== +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. -**Providers**: - -- **INGV model** - - -| **Product Type**: lookup-table - -| **Status**: Inactive - -| **Creation date**: 2022-04-27T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - png - - -| **Sample**: https://drive.google.com/file/d/1fFM0mShvAoHlf_HlOVh7rjvQ5Ai5dyV3/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 21b20d2af13af49623956b68059bd334e9f0c3bc..fdc73e1052b0512259360fa2511a83332fffa560 100644 --- a/docs/source/products/data/ingv_ltmuf_rome_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_rome_tableset.rst @@ -1,38 +1,107 @@ -========================================= -INGV Long Term MUF maps centered on Rome -========================================= +=================================== +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. -**Providers**: - -- **INGV model** - - -| **Product Type**: lookup-table - -| **Status**: Inactive - -| **Creation date**: 2022-04-26T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - png - - -| **Sample**: https://drive.google.com/file/d/1reQwlgS-qA36yenYJyp9Ch8NJ_nKfjq4/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 8669ef5a4de14a3659cceea20055c1491754bea5..a47bd7eadf4a94e85ff9d99364e0b76d02c81f80 100644 --- a/docs/source/products/data/ingv_mag_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_mag_aqu_timeseries.rst @@ -1,49 +1,132 @@ -========================================= -INGV Preliminary L'Aquila magnetic data -========================================= - -.. 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. - -**Providers**: - -- **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 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 - +====================================================== +INGV geomagnetic data, GIC indices and alert: L'Aquila +====================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 d4b0d82ce0739cc1f2ffb4744ada3b450d1ab05c..a544bfc382bb9929849c38b32718f36e0802e531 100644 --- a/docs/source/products/data/ingv_mag_cts_timeseries.rst +++ b/docs/source/products/data/ingv_mag_cts_timeseries.rst @@ -1,49 +1,132 @@ -============================================== -INGV Preliminary Castello Tesino magnetic data -============================================== - -.. 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. - -**Providers**: - -- **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 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 - +============================================================= +INGV geomagnetic data, GIC indices and alert: Castello Tesino +============================================================= + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 c4acd8a6277f2d0f8e7085c7741a013e20aa33c9..84229117b4afcb3b5c95618eb90f1d189ecade12 100644 --- a/docs/source/products/data/ingv_mag_dmc_timeseries.rst +++ b/docs/source/products/data/ingv_mag_dmc_timeseries.rst @@ -1,49 +1,132 @@ -========================================= -INGV Preliminary Dome C magnetic data -========================================= - -.. 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. - -**Providers**: - -- **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 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 - +==================================================== +INGV geomagnetic data, GIC indices and alert: Dome C +==================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 6241743407912154007ddda4436e7e28fd322368..c4c3054c5b54869755c59d82b33791d1f5b684a3 100644 --- a/docs/source/products/data/ingv_mag_dur_timeseries.rst +++ b/docs/source/products/data/ingv_mag_dur_timeseries.rst @@ -1,49 +1,132 @@ -========================================= -INGV Preliminary Duronia magnetic data -========================================= - -.. 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. - -**Providers**: - -- **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 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 - +===================================================== +INGV geomagnetic data, GIC indices and alert: Duronia +===================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 e144d2114c74f0f33ec3341a1b8e1315751b4d9a..06f912f8ada46d7b68f4a76188707f5384e65cfa 100644 --- a/docs/source/products/data/ingv_mag_int_timeseries.rst +++ b/docs/source/products/data/ingv_mag_int_timeseries.rst @@ -1,46 +1,137 @@ -================================================= -INGV Magnetic data from 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 - -**Providers**: - -- **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 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 - +============================================================================ +Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories +============================================================================ + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 0c12fb0defa2199888661f6a763563dfa2969fe9..afb19d813ec23d44357542154418a251923d15e2 100644 --- a/docs/source/products/data/ingv_mag_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_mag_lmp_timeseries.rst @@ -1,49 +1,132 @@ -========================================= -INGV Preliminary Lampedusa magnetic data -========================================= - -.. 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. - -**Providers**: - -- **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 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 - +======================================================= +INGV geomagnetic data, GIC indices and alert: Lampedusa +======================================================= + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 d0213d8fc1cb96dd94a4aa7777557bc26503fa2e..2988f79e6ee991aeba674cb6e57af2e3a67da8a4 100644 --- a/docs/source/products/data/ingv_mag_tnb_timeseries.rst +++ b/docs/source/products/data/ingv_mag_tnb_timeseries.rst @@ -1,49 +1,132 @@ -============================================= -INGV Preliminary Terra Nova Bay magnetic data -============================================= - -.. 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. - -**Providers**: - -- **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 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 - +============================================================ +INGV geomagnetic data, GIC indices and alert: Terra Nova Bay +============================================================ + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 aad7747cfb85a222663dfcd5eeebe73adedbdda8..fc9c041bc7890c1e4e435ac741d03041e15a980b 100644 --- a/docs/source/products/data/ingv_mag_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_mag_wdc_timeseries.rst @@ -1,49 +1,137 @@ -============================================================================= -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 +.. 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. -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 dacaf8d8d4abaa8c51bb288c4e98ead28d88ac12..3ab56612f174a35ebf070167ddf8615d38a54aa4 100644 --- a/docs/source/products/data/ingv_magdef_cts_timeseries.rst +++ b/docs/source/products/data/ingv_magdef_cts_timeseries.rst @@ -1,50 +1,133 @@ -============================================= -INGV Definitive Castello Tesino magnetic data -============================================= - -.. 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. - -**Providers**: - -- **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 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 - +============================================================= +INGV geomagnetic data, GIC indices and alert: Castello Tesino +============================================================= + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 fe91a09f018c1f4b5a28d2f914238e02847e04da..9d8e7e3ff95e8732b77ed33f9180786e0cb22b27 100644 --- a/docs/source/products/data/ingv_magdef_dur_timeseries.rst +++ b/docs/source/products/data/ingv_magdef_dur_timeseries.rst @@ -1,50 +1,133 @@ -========================================= -INGV Definitive Duronia magnetic data -========================================= - -.. 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. - -**Providers**: - -- **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 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 - +===================================================== +INGV geomagnetic data, GIC indices and alert: Duronia +===================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 ad3cd733c8cc3e9eb3a99a6a3a25f13358af9c1c..0e2a819f3b2c623d5348cd68f620b1a7c42c95d4 100644 --- a/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst @@ -1,42 +1,107 @@ -============================================ -INGV Nowcasting MUF map centered on Cagliari -============================================ - -.. contents:: The tiny table of contents - - -~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ +======================================= +Nowcasting MUF map centered on Cagliari +======================================= +.. 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. -**Providers**: - -- **INGV model** - - -| **Product Type**: lookup-table - -| **Status**: Inactive - -| **Creation date**: 2022-04-26T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - png - - -| **Sample**: https://drive.google.com/file/d/1OlmXoC8dVV9COHgbs_Nuv7egePhEMVaF/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 7f29d73545f54c6ce19dd3957864de54eaabd4e0..f720d9b5965c2f9a23d412f088913ebd64dabafc 100644 --- a/docs/source/products/data/ingv_ncmuf_catania_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_catania_tableset.rst @@ -1,38 +1,107 @@ -=========================================== -INGV Nowcasting MUF map centered on Catania -=========================================== +====================================== +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. -**Providers**: - -- **INGV model** - - -| **Product Type**: lookup-table - -| **Status**: Inactive - -| **Creation date**: 2022-04-26T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - png - - -| **Sample**: https://drive.google.com/file/d/15P1zVVveGqEHLFJzTcSwwpELDv9J-nqR/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 cfceabf349cad192a5e43c51d16a9c385292159a..96508c160f6427bafc5c6cf3876a24116913ab00 100644 --- a/docs/source/products/data/ingv_ncmuf_milan_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_milan_tableset.rst @@ -1,38 +1,107 @@ -========================================= -INGV Nowcasting MUF map centered on Milan -========================================= +===================================== +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. -**Providers**: - -- **INGV model** - - -| **Product Type**: lookup-table - -| **Status**: Inactive - -| **Creation date**: 2022-04-26T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - png - - -| **Sample**: https://drive.google.com/file/d/1fFM0mShvAoHlf_HlOVh7rjvQ5Ai5dyV3/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 32c22ea91692c9447e74d429fdf4a0288e326a8f..7f3deb453863da606524dae06b270e4fc0836b4b 100644 --- a/docs/source/products/data/ingv_ncmuf_rome_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_rome_tableset.rst @@ -1,38 +1,107 @@ -========================================= -INGV Nowcasting MUF map centered on Rome -========================================= +=================================== +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. -**Providers**: - -- **INGV model** - - -| **Product Type**: lookup-table - -| **Status**: Inactive - -| **Creation date**: 2022-04-26T06:26:08+00:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: image - -| **Data formats**: - png - - -| **Sample**: https://drive.google.com/file/d/1reQwlgS-qA36yenYJyp9Ch8NJ_nKfjq4/view?usp=sharing - -Capabilities -~~~~~~~~~~~~ - -- ext2220.1: Standard Visualisation: Web GUI -- int2130.1: Product ingestion -- int2130.2: Mirroring: synchronised - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 faed328368c3160c536ffabd784d1b3fbfa4a3c5..0000000000000000000000000000000000000000 --- 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 6ad488454c2a3cae5a85b496517fdca5f2ceea0a..0000000000000000000000000000000000000000 --- 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 25022172e895edd5909143457e38093d02f25310..0000000000000000000000000000000000000000 --- 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 806e67dbe2df89c92de8af925994219b30fb94db..0000000000000000000000000000000000000000 --- 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 f3e0c9b1d639f7167e7df898b6ff6103acdb619c..0000000000000000000000000000000000000000 --- 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 7876c4075633c7a59ae970a3dd6500efc219288d..0000000000000000000000000000000000000000 --- 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 6043b1d91e50b346ad43ab9db89a595132379935..0000000000000000000000000000000000000000 --- 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 ea64b3818c7e1456308f4d4b4f7d39b99d05f135..0000000000000000000000000000000000000000 --- 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 8bc6c2e7017bb4304d80455620c683b313dc2863..0000000000000000000000000000000000000000 --- 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 275a2c058fe9a7b647233785c1e677d5202cd057..0000000000000000000000000000000000000000 --- 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 b8430da6c1eb35735374b54e4fc04721b0f2dc93..0000000000000000000000000000000000000000 --- 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 4c0441e25391e171724fd95b9d5176c70d56c576..0000000000000000000000000000000000000000 --- 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 f85252c7248d9e26879259e16ed44c50287e1991..0000000000000000000000000000000000000000 --- 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 23d5320ba25cad3ceff13afeaa9d987c2de7f44c..0000000000000000000000000000000000000000 --- 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 1f0e8c2453d2cbc1a9f5eca231a98bd781059f3d..5090e8b7a9a68c3c03993e45de29e811211da442 100644 --- a/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst +++ b/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst @@ -1,48 +1,147 @@ -========================================= -INGV Validated data Gibilmanna Ionosonde -========================================= +=================================== +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 -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 b0a1d816e57a410fd302ae2e5a06026681e8aa64..71ec3843a88113dd6658d48e8d04e5dbf3a3a412 100644 --- a/docs/source/products/data/ingv_valiiono_rome_timeseries.rst +++ b/docs/source/products/data/ingv_valiiono_rome_timeseries.rst @@ -1,48 +1,147 @@ -========================================= -INGV Validated data Rome Ionosonde -========================================= +============================= +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 -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 2fbc4fb8b03d8d2a7eb2ca3100aef3646a448308..0000000000000000000000000000000000000000 --- 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 138203b3cd29cbe140fe9439c2747ff736afa02f..9933cf02210db52457c2ec1048c7423c9156e561 100644 --- a/docs/source/products/data/uniaq_curr_maigic_tableset.rst +++ b/docs/source/products/data/uniaq_curr_maigic_tableset.rst @@ -1,44 +1,127 @@ -======================================================================== -UNIAQ 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. - - -**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**: 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 - +================================================================== +Magnetospheric-Ionospheric-Ground Induced Current model - currents +================================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 497f227db6c58d0646ef5e80e947ae8a33044764..5e1c4e8231128acdc1f822e9813741d447cb1cff 100644 --- a/docs/source/products/data/uniaq_epmde_emma_timeseries.rst +++ b/docs/source/products/data/uniaq_epmde_emma_timeseries.rst @@ -1,38 +1,117 @@ -============================================================== -UNIAQ Equatorial Plasma Mass Density estimates in Plasmasphere -============================================================== +======================================================== +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. -**Providers**: - -- **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 type**: tableset - -| **Data formats**: - -- json - - -| **Sample**: https://drive.google.com/file/d/1ORb-g1JGbSmf0h0IbzkMXnWQgwV3aSvb/view?usp=share_link - -Capabilities -~~~~~~~~~~~~ - -- int2130.1: Product ingestion - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 51db6d0d2df3da00972c4037e810de949b567251..0000000000000000000000000000000000000000 --- 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 d87cc8a3d13d3c84d6fb42a4184d32e2cedfc734..99dc51e6d035a6fc2cdaf731e3eba6c13fb6ca70 100644 --- a/docs/source/products/data/uniaq_field_maigic_tableset.rst +++ b/docs/source/products/data/uniaq_field_maigic_tableset.rst @@ -1,46 +1,132 @@ -================================================================================= -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**: 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 - +========================================================================== +Magnetospheric-Ionospheric-Gound Induced Current model - Geoelectric Field +========================================================================== + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 26c6dcce2eed913687dc3e8e30468f00d0d54e1f..1fafe6cadeb890c591d14ab66844224dc15891ac 100644 --- a/docs/source/products/data/uniaq_mag_emma_timeseries.rst +++ b/docs/source/products/data/uniaq_mag_emma_timeseries.rst @@ -1,67 +1,127 @@ -========================================= -UNIAQ EMMA Geomagnetic field data -========================================= +=========================== +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. -**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**: - -- 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 9244f1f6d062422e2146ef9a2cdf156501ab964e..eb692b89f71f87f49c4450da4291cc2c9f6da438 100644 --- a/docs/source/products/data/unical_espseptransport_tableset.rst +++ b/docs/source/products/data/unical_espseptransport_tableset.rst @@ -1,62 +1,117 @@ -========================================== -UNICAL 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 - - -Data Description ----------------- - -| **Data type**: tableset - -| **Data formats**: - csv - - -| **Version**: v2.0 - -Data Provider -------------- - -Data are collected by the following instruments: - -- **ACE** - source: - - - EPAM - -Data Coverage -------------- -The product cover measurements for the ND messangers. - -Data coverage is listed below: - -| **Spatial** IP - -| **Temporal** - time_start: 2009-01-01T00:00:00+01:00 - -- time_stop: 2022-03-31T00:00:00+02:00 - - - -| **Spectral** range: ND ND - ND ND - -Product Status --------------- - -| **Status**: Active - -| **Creation date**: 2022-04-27T09:47:00+02:00 - -| **Last Update**: 2023-10-31T12:00:00+01:00 - -Data Policy ------------ - -This product contains public data. Public access to the data. - -Example -------- - -Example is not yet provided . +=================================== +Energetic particle spectral indices +=================================== + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 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 3e71eeb417c5cf5112d813988a420b51853ed13c..e341290f364c50cec2f9da79ef32f861cf7e1052 100644 --- a/docs/source/products/data/unical_sep_ace_spectrum.rst +++ b/docs/source/products/data/unical_sep_ace_spectrum.rst @@ -1,45 +1,107 @@ -================================================ -UNICAL SEP Proton Spectra for the ACE spacecraft -================================================ +========================================= +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. -**Providers**: - -- **Ace** - source: - - - EPAM - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T11:51:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - txt - - -| **Sample**: https://drive.google.com/file/d/1jIQGdVMZImhyC24Aoe-lvbrdgGpoFIeh/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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 f2fa5918a34dc0c516a862c5fc456c3714023bd5..db1f85a9014daa2ba9dc900ee288774d74bd2677 100644 --- a/docs/source/products/data/unical_sep_psp_spectrum.rst +++ b/docs/source/products/data/unical_sep_psp_spectrum.rst @@ -1,45 +1,107 @@ -================================================ -UNICAL SEP Proton Spectra for the PSP spacecraft -================================================ +========================================= +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. -**Providers**: - -- **PSP** - source: - - - ISOIS - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-28T13:34:40+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - txt - - -| **Sample**: https://drive.google.com/file/d/1U6Am0CfJXaEqI_5gAJdaV85bp4U5pRX5/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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 a6e6e61ed6f96a2804a7b8f67d03116de9c06ae3..540262dd0667a5d13801c5711d2fdf3eb8f4f2c4 100644 --- a/docs/source/products/data/unical_sep_soho_spectrum.rst +++ b/docs/source/products/data/unical_sep_soho_spectrum.rst @@ -1,45 +1,107 @@ -================================================= -UNICAL SEP Proton Spectra for the SoHO spacecraft -================================================= +========================================== +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. -**Providers**: - -- **SoHO** - source: - - - ERNE - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T11:51:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - txt - - -| **Sample**: https://drive.google.com/file/d/1IwOQPDq4HZ9j0Say9Yh5CY18LV9lWhXr/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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 07e199945aad66d8ceb198e8dd6604109e499fa6..b3474e49fdcb40f2ba16ab862396d672bb551e19 100644 --- a/docs/source/products/data/unical_sep_solo_spectrum.rst +++ b/docs/source/products/data/unical_sep_solo_spectrum.rst @@ -1,45 +1,107 @@ -================================================= -UNICAL SEP Proton Spectra for the SolO spacecraft -================================================= +========================================== +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. -**Providers**: - -- **SolO** - source: - - - EPD - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T11:51:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - txt - - -| **Sample**: ND - -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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 c01b65b90bc42781f2aba2b86745b4999b4d49d3..6fcd665648dd0bd9cabbdee680b615432088e7b3 100644 --- a/docs/source/products/data/unical_sep_stra_spectrum.rst +++ b/docs/source/products/data/unical_sep_stra_spectrum.rst @@ -1,45 +1,107 @@ -===================================================== -UNICAL SEP Proton Spectra for the STEREO A spacecraft -===================================================== +============================================== +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. -**Providers**: - -- **STEREO A** - source: - - - IMPACT - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T11:51:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - txt - - -| **Sample**: https://drive.google.com/file/d/1bT1Y7NyXrVFg_oAdZWjas_x2w6lBn9uE/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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 9a7dcd6732d3ee8c8c095b27085ea7da7907a54d..104d36ada67638b3f88970c1b1c490ec4e1f8f62 100644 --- a/docs/source/products/data/unical_sep_wind_spectrum.rst +++ b/docs/source/products/data/unical_sep_wind_spectrum.rst @@ -1,46 +1,107 @@ -================================================= -UNICAL SEP Proton Spectra for the WIND spacecraft -================================================= +========================================== +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. -**Providers**: - -- **WIND** - sources: - - - 3DP - - EPACT - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-04-26T11:51:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: tableset - -| **Data formats**: - txt - - -| **Sample**: https://drive.google.com/file/d/17K170-oRokV3BeEZKaHrgCtmLkq1NhsF/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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 1f4affe74d83a97eabd62ce672a27b01a93e63e5..9e2c06776466958b8403f1555d9bb8f0b42377a7 100644 --- a/docs/source/products/data/unical_shockpar_tableset.rst +++ b/docs/source/products/data/unical_shockpar_tableset.rst @@ -1,159 +1,217 @@ -====================================================== -UNICAL 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: - -Jian et al. Interplanetary Shock list -(URL: https://stereo-ssc.nascom.nasa.gov/data/ins_data/impact/level3/IPs.pdf ) - -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. - -:download:`Further readings (pdf) <../../private/unical_shockpar_tableset-Description_ESP_STEREOA.pdf>`. - -: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 . +=============================================== +Parameters of shocks associated with ESP events +=============================================== + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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_facula_image.rst b/docs/source/products/data/unict_facula_image.rst index 15404278bdd2bf5c4ddb846ab519beea03944200..7a7b2b9027e1fb35e8122f1db9955549af3c0581 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 492e8175fb28e4c0057d8dbadfabb39e97e5d8fc..d35694794c328831fdd80dc837d6bf19ad5aac1a 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 ddf5412cdf7db39641bf84205ae7c52f96f0c136..6298a66491117ca500bab5bf361e6a53cbe5f83c 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_promin_ws.rst b/docs/source/products/data/unict_promin_ws.rst deleted file mode 100644 index 897d8d47135fd0bed5774d762353de7d7fa0e9ee..0000000000000000000000000000000000000000 --- 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/unict_sunspot_image.rst b/docs/source/products/data/unict_sunspot_image.rst index c1a96b03dc57bf917f5443130b8b9af48a609336..9a89ea74478306926483b48b4d1f08929e0309ae 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/unipg_gcr_model.rst b/docs/source/products/data/unipg_gcr_model.rst deleted file mode 100644 index 405b1cfdce346329790203e057ce9e50c601dab9..0000000000000000000000000000000000000000 --- 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 b01870b07f0797ba1111f9f2c167f9be0e6e3f91..d92ca63f8134e5b5d28e22884e7090ae7144177c 100644 --- a/docs/source/products/data/unitn_flux_cses_timeseries.rst +++ b/docs/source/products/data/unitn_flux_cses_timeseries.rst @@ -1,43 +1,97 @@ -========================================= -UNITN CSES satellite particle flux data -========================================= +================================= +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. -**Providers**: - -- **CSES satellite HEPP electron and proton data** - - -| **Product Type**: data - -| **Status**: Active - -| **Creation date**: 2022-05-03T09:00:00+02:00 - -| **Last Update**: 2023-10-01T12:00:00+02:00 - -Data Description -~~~~~~~~~~~~~~~~ - -| **Data type**: timeseries - -| **Data formats**: - .mat - - -| **Sample**: https://drive.google.com/file/d/1PBiyD4KIxWKtFyMF-vn5Eaau4tFxofIk/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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 7c45499d099687510cf47f46b896becf62a8800b..da9827f855b089bcc924086e90fa6caa98410f0d 100644 --- a/docs/source/products/data/unitov_halpha_tsst_image.rst +++ b/docs/source/products/data/unitov_halpha_tsst_image.rst @@ -1,45 +1,137 @@ -========================================= -UNITOV 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. - -**Providers**: - -- **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 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 - +============================= +TSST H-alpha Full Disk Images +============================= + +.. 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 +~~~~~~~~~~ + + + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 65b2cf0b3c329ef5c72bb9a602c4b7e8edee989e..c8b0204eab7cf0c34ea1c9204dfdbb5aea87147a 100644 --- a/docs/source/products/data/unitov_icme_tableset.rst +++ b/docs/source/products/data/unitov_icme_tableset.rst @@ -2,49 +2,231 @@ 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. -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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_iss_lidal_timeseries.rst b/docs/source/products/data/unitov_iss_lidal_timeseries.rst index 1b70ce921d0b6899ee07bfa9ea5e2135ea7cb9e9..9ee9f05d6888eb4b92b31849dd4d43904782f6db 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 acac8a1080772e7406ec226308f2fd5a3de12d6f..e409bc7e70b74f2786d44d3421a65559ea74a605 100644 --- a/docs/source/products/data/unitov_mag_tsst_image.rst +++ b/docs/source/products/data/unitov_mag_tsst_image.rst @@ -1,45 +1,137 @@ -========================================= -UNITOV TSST Full Disk LoS magnetic maps -========================================= +================================ +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. -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 4b550d1858520aa0822d584b2d25ba663bd54be0..0000000000000000000000000000000000000000 --- 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 ff7ebb8c624e3571955697a5e9088e60894b8ea6..e35cf84311cec65a377c8b894656803d744be570 100644 --- a/docs/source/products/data/unitov_rdparameter_tableset.rst +++ b/docs/source/products/data/unitov_rdparameter_tableset.rst @@ -1,45 +1,127 @@ -========================================= -UNITOV R and D Active Region parameters -========================================= +================================ +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 -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 d2979da52791dc420aae2edd5e995bd90662a253..fb7b19000c7a2220258da2d60ef9d842a2c5e5d3 100644 --- a/docs/source/products/data/unitov_vel_tsst_image.rst +++ b/docs/source/products/data/unitov_vel_tsst_image.rst @@ -1,45 +1,137 @@ -========================================= -UNITOV TSST Full Disk Velocity Maps -========================================= +============================ +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. -**Providers**: - -- **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 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 - +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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