From f77f83d329113af534260d3132cfe5728ef64ad1 Mon Sep 17 00:00:00 2001 From: stefano scardigli Date: Fri, 12 Apr 2024 12:47:48 +0200 Subject: [PATCH 1/2] Updated products divided by spatial --- .../data/external_ace_swepam_timeseries.rst | 92 ------- .../data/external_flux_goes_timeseries.rst | 87 ------- .../data/external_part_goes_timeseries.rst | 122 --------- .../data/inaf_cpcp_superdarn_datacube.rst | 200 --------------- .../data/inaf_data_solopas_timeseries.rst | 126 ---------- .../data/inaf_flux1h_svirco_timeseries.rst | 82 ------- .../data/inaf_flux5m_svirco_timeseries.rst | 92 ------- .../products/data/inaf_gsmaps_datacube.rst | 92 ------- .../products/data/inaf_m2flare_tableset.rst | 132 ---------- .../products/data/inaf_na_mercexo_image.rst | 157 ------------ .../products/data/inaf_s1sep_tableset.rst | 207 ---------------- .../products/data/inaf_s2sep_tableset.rst | 207 ---------------- .../products/data/inaf_tps_datacube.rst | 92 ------- .../data/inaf_vbcorr_wind_tableset.rst | 98 -------- .../products/data/infn_cses_hepd_spectrum.rst | 107 -------- .../data/infn_iss_ams_flux_timeseries.rst | 107 -------- .../data/infn_pamela_flux_timeseries.rst | 102 -------- .../data/infn_saandose_samadha_timeseries.rst | 87 ------- .../data/infn_tgndose_samadha_timeseries.rst | 87 ------- .../data/ingv_alert_aqu_timeseries.rst | 135 ---------- .../data/ingv_alert_cts_timeseries.rst | 132 ---------- .../data/ingv_alert_dur_timeseries.rst | 132 ---------- .../data/ingv_alert_int_timeseries.rst | 137 ----------- .../data/ingv_alert_lmp_timeseries.rst | 132 ---------- .../data/ingv_alert_wdc_timeseries.rst | 137 ----------- .../data/ingv_autoiono_bbla_timeseries.rst | 117 --------- .../data/ingv_autoiono_gibi_timeseries.rst | 117 --------- .../data/ingv_autoiono_rome_timeseries.rst | 117 --------- .../data/ingv_autoiono_tucu_timeseries.rst | 117 --------- .../products/data/ingv_b_swarm_image.rst | 107 -------- .../products/data/ingv_b_swarm_timeseries.rst | 147 ----------- .../data/ingv_bvect_cses_tableset.rst | 102 -------- .../data/ingv_evect_cses_tableset.rst | 102 -------- .../products/data/ingv_gic_aqu_timeseries.rst | 132 ---------- .../products/data/ingv_gic_cts_timeseries.rst | 132 ---------- .../products/data/ingv_gic_dur_timeseries.rst | 132 ---------- .../products/data/ingv_gic_int_timeseries.rst | 137 ----------- .../products/data/ingv_gic_lmp_timeseries.rst | 132 ---------- .../products/data/ingv_gic_wdc_timeseries.rst | 137 ----------- .../data/ingv_ltmuf_cagliari_tableset.rst | 107 -------- .../data/ingv_ltmuf_catania_tableset.rst | 107 -------- .../data/ingv_ltmuf_milan_tableset.rst | 107 -------- .../data/ingv_ltmuf_rome_tableset.rst | 107 -------- .../products/data/ingv_mag_aqu_timeseries.rst | 132 ---------- .../products/data/ingv_mag_cts_timeseries.rst | 132 ---------- .../products/data/ingv_mag_dmc_timeseries.rst | 132 ---------- .../products/data/ingv_mag_dur_timeseries.rst | 132 ---------- .../products/data/ingv_mag_int_timeseries.rst | 137 ----------- .../products/data/ingv_mag_lmp_timeseries.rst | 132 ---------- .../products/data/ingv_mag_tnb_timeseries.rst | 132 ---------- .../products/data/ingv_mag_wdc_timeseries.rst | 137 ----------- .../data/ingv_magdef_cts_timeseries.rst | 133 ---------- .../data/ingv_magdef_dur_timeseries.rst | 133 ---------- .../data/ingv_ncmuf_cagliari_tableset.rst | 107 -------- .../data/ingv_ncmuf_catania_tableset.rst | 107 -------- .../data/ingv_ncmuf_milan_tableset.rst | 107 -------- .../data/ingv_ncmuf_rome_tableset.rst | 107 -------- .../data/ingv_valiiono_gibi_timeseries.rst | 147 ----------- .../data/ingv_valiiono_rome_timeseries.rst | 147 ----------- .../data/uniaq_curr_maigic_tableset.rst | 127 ---------- .../data/uniaq_epmde_emma_timeseries.rst | 117 --------- .../data/uniaq_field_maigic_tableset.rst | 132 ---------- .../data/uniaq_mag_emma_timeseries.rst | 127 ---------- .../data/unical_espseptransport_tableset.rst | 117 --------- .../products/data/unical_sep_ace_spectrum.rst | 107 -------- .../products/data/unical_sep_psp_spectrum.rst | 107 -------- .../data/unical_sep_soho_spectrum.rst | 107 -------- .../data/unical_sep_solo_spectrum.rst | 107 -------- .../data/unical_sep_stra_spectrum.rst | 107 -------- .../data/unical_sep_wind_spectrum.rst | 107 -------- .../data/unical_shockpar_tableset.rst | 217 ---------------- .../products/data/unict_facula_image.rst | 127 ---------- .../products/data/unict_filament_image.rst | 122 --------- .../products/data/unict_offlimb_image.rst | 122 --------- .../products/data/unict_sunspot_image.rst | 197 --------------- .../data/unitn_flux_cses_timeseries.rst | 97 -------- .../data/unitov_halpha_tsst_image.rst | 137 ----------- .../products/data/unitov_icme_tableset.rst | 232 ------------------ .../data/unitov_iss_lidal_timeseries.rst | 92 ------- .../products/data/unitov_mag_tsst_image.rst | 137 ----------- .../data/unitov_rdparameter_tableset.rst | 127 ---------- .../products/data/unitov_vel_tsst_image.rst | 137 ----------- docs/source/products/data_products.rst | 92 ++++++- docs/source/products/main.rst | 2 +- 84 files changed, 91 insertions(+), 10300 deletions(-) delete mode 100644 docs/source/products/data/external_ace_swepam_timeseries.rst delete mode 100644 docs/source/products/data/external_flux_goes_timeseries.rst delete mode 100644 docs/source/products/data/external_part_goes_timeseries.rst delete mode 100644 docs/source/products/data/inaf_cpcp_superdarn_datacube.rst delete mode 100644 docs/source/products/data/inaf_data_solopas_timeseries.rst delete mode 100644 docs/source/products/data/inaf_flux1h_svirco_timeseries.rst delete mode 100644 docs/source/products/data/inaf_flux5m_svirco_timeseries.rst delete mode 100644 docs/source/products/data/inaf_gsmaps_datacube.rst delete mode 100644 docs/source/products/data/inaf_m2flare_tableset.rst delete mode 100644 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- -References -~~~~~~~~~~ - -qui invece la bibliografia - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. list-table:: - :widths: 7 20 15 10 48 - :align: right - :header-rows: 1 - - * - progr - - column - - units - - type - - description - * - 1 - - time - - UTC - - datetime - - UTC - * - 2 - - ProtonDensity - - p/cc - - double - - p/cm^3 - * - 3 - - BulkSpeed - - km/s - - double - - km/s - * - 4 - - IonTemperature - - K - - double - - K diff --git a/docs/source/products/data/external_flux_goes_timeseries.rst b/docs/source/products/data/external_flux_goes_timeseries.rst deleted file mode 100644 index 766cd96..0000000 --- a/docs/source/products/data/external_flux_goes_timeseries.rst +++ /dev/null @@ -1,87 +0,0 @@ -=============== -GOES X-ray Flux -=============== - -.. contents:: Table of contents - -not available in DBF - -References -~~~~~~~~~~ - -not available in DBF - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. list-table:: - :widths: 7 20 15 10 48 - :align: right - :header-rows: 1 - - * - progr - - column - - units - - type - - description - * - 1 - - time - - UTC - - datetime - - UTC - * - 2 - - Short_Wave - - Watts/m^2 - - double - - W/m^2 - * - 3 - - Long_Wave - - Watts/m^2 - - double - - W/m^2 diff --git a/docs/source/products/data/external_part_goes_timeseries.rst b/docs/source/products/data/external_part_goes_timeseries.rst deleted file mode 100644 index f179e8f..0000000 --- a/docs/source/products/data/external_part_goes_timeseries.rst +++ /dev/null @@ -1,122 +0,0 @@ -================ -GOES proton Flux -================ - -.. contents:: Table of contents - -not available in DBF - -References -~~~~~~~~~~ - -not available in DBF - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. list-table:: - :widths: 7 20 15 10 48 - :align: right - :header-rows: 1 - - * - progr - - column - - units - - type - - description - * - 1 - - time - - UTC - - datetime - - UTC - * - 2 - - P1 - - Protons/cm^2 - s^-1 - sr - - double - - >=1Mev integral proton flux 5min average - * - 3 - - P5 - - Protons/cm^2 - s^-1 - sr - - double - - >=5Mev integral proton flux 5min average - * - 4 - - P10 - - Protons/cm^2 - s^-1 - sr - - double - - >=10Mev integral proton flux 5min average - * - 5 - - P30 - - Protons/cm^2 - s^-1 - sr - - double - - >=30Mev integral proton flux 5min average - * - 6 - - P50 - - Protons/cm^2 - s^-1 - sr - - double - - >=50Mev integral proton flux 5min average - * - 7 - - P100 - - Protons/cm^2 - s^-1 - sr - - double - - >=100Mev integral proton flux 5min average - * - 8 - - E_8 - - Electrons/cm^2 - s^-1 - sr - - double - - >=0.8Mev integral electron flux 5min average - * - 9 - - E2_0 - - Electrons/cm^2 - s^-1 - sr - - double - - >=2Mev integral electron flux 5min average - * - 10 - - E4_0 - - Electrons/cm^2 - s^-1 - sr - - double - - >=4Mev integral electron flux 5min average diff --git a/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst b/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst deleted file mode 100644 index e6f1162..0000000 --- a/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst +++ /dev/null @@ -1,200 +0,0 @@ -============================= -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_data_solopas_timeseries.rst b/docs/source/products/data/inaf_data_solopas_timeseries.rst deleted file mode 100644 index b7d8d36..0000000 --- a/docs/source/products/data/inaf_data_solopas_timeseries.rst +++ /dev/null @@ -1,126 +0,0 @@ -================================ -INAF-IAPS Solar Orbiter-PAS data -================================ - -.. contents:: Table of contents - -The product contains density N, speed vector V, pressure tensor P, temperature components (Tx, Ty, Tz), and the velocity of the satellite V_solo, computed using the data collected by the Proton-Alpha Sensor (PAS) onboard Solar Orbiter. -PAS measures the 3D distribution functions of the dominant ions of the solar wind, from 200 eV to 20 KeV, without mass and charge selection. In practice, this concerns mostly the proton and alfa populations (unseparated). At full resolution, PAS collects the 3D ion distribution function in about 1 second, even though the moments have a cadence of 4 seconds, while in “snapshot” mode the phase space sampling is reduced, allowing a greater cadence for the moments. - -Data is hosted on http://soar.esac.esa.int/soar/ - -References -~~~~~~~~~~ - -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) - -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_flux1h_svirco_timeseries.rst b/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst deleted file mode 100644 index 3542b5c..0000000 --- a/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst +++ /dev/null @@ -1,82 +0,0 @@ -============================================= -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_flux5m_svirco_timeseries.rst b/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst deleted file mode 100644 index 8e7960b..0000000 --- a/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst +++ /dev/null @@ -1,92 +0,0 @@ -============================================== -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_gsmaps_datacube.rst b/docs/source/products/data/inaf_gsmaps_datacube.rst deleted file mode 100644 index 1867a25..0000000 --- a/docs/source/products/data/inaf_gsmaps_datacube.rst +++ /dev/null @@ -1,92 +0,0 @@ -===================================================== -IAPS Grad-Shafranov Reconstruction of Magnetic Clouds -===================================================== - -.. contents:: Table of contents - -Quasi 3-d magnetic field maps of magnetic field configuration within magnetic clouds for geoeffective target SWE events. Such maps will be estimated through the Grad-Shafranov reconstruction from single-spacecraft plasma and magnetic field data. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index b7baee1..0000000 --- a/docs/source/products/data/inaf_m2flare_tableset.rst +++ /dev/null @@ -1,132 +0,0 @@ -============================== -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 deleted file mode 100644 index c580787..0000000 --- a/docs/source/products/data/inaf_na_mercexo_image.rst +++ /dev/null @@ -1,157 +0,0 @@ -=============================================== -INAF-bidimensional maps of Mercury Na exosphere -=============================================== - -.. 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_s1sep_tableset.rst b/docs/source/products/data/inaf_s1sep_tableset.rst deleted file mode 100644 index f60fb57..0000000 --- a/docs/source/products/data/inaf_s1sep_tableset.rst +++ /dev/null @@ -1,207 +0,0 @@ -============================ -IAPS S1 SEP events Catalogue -============================ - -.. contents:: Table of contents - -The catalogue contains SEP events observed at the Earth of class S1, i.e. with flux in the range [10, 100) pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux >= 100 pfu at > 10 MeV are listed in the companion table S2 SEP Catalogue. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 0963e5a..0000000 --- a/docs/source/products/data/inaf_s2sep_tableset.rst +++ /dev/null @@ -1,207 +0,0 @@ -============================ -IAPS S2 SEP events Catalogue -============================ - -.. contents:: Table of contents - -The catalogue contains SEP events observed at the Earth of class S2, i.e. with flux >100 pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux in the interval [10, 100) pfu at > 10 MeV are listed in the companion table S1 SEP Catalogue. - -References -~~~~~~~~~~ - - - -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_tps_datacube.rst b/docs/source/products/data/inaf_tps_datacube.rst deleted file mode 100644 index 7777305..0000000 --- a/docs/source/products/data/inaf_tps_datacube.rst +++ /dev/null @@ -1,92 +0,0 @@ -================================================ -IAPS Test Particle Simulation on Magnetic Clouds -================================================ - -.. contents:: Table of contents - -Galactic cosmic ray intensity variations associated to the passage of magnetic clouds. The particle intensity variation is estimated through a dedicated full-orbit test-particle simulation. - -References -~~~~~~~~~~ - - - -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_wind_tableset.rst b/docs/source/products/data/inaf_vbcorr_wind_tableset.rst deleted file mode 100644 index 46cb275..0000000 --- a/docs/source/products/data/inaf_vbcorr_wind_tableset.rst +++ /dev/null @@ -1,98 +0,0 @@ -====================================================================================== -IAPS - Wind velocity-magnetic field correlation coefficient data of solar wind streams -====================================================================================== - -.. contents:: Table of contents - -The velocity - magnetic field (v-b) correlation coefficient unables to identify Alfvénic solar wind intervals (along with almost constant magnetic field magnitude and proton number density). It is derived as the ratio between the covariance of velocity and magnetic field (in Alfvén units) components and the product of their standard deviations, in a time window ranging between tens of minutes to hours. In principle, this formula should be applied to every component of the velocity (V_i) and magnetic fields (B_i) (with i = R, T, N in RTN coordinate system or i = X, Y, Z in GSE coordinate system). The total correlation coefficient is then derived as the average from the three components. However, for the sake of simplicity, we consider only the N component since more Alfvénic than the other two. - -References -~~~~~~~~~~ - -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/infn_cses_hepd_spectrum.rst b/docs/source/products/data/infn_cses_hepd_spectrum.rst deleted file mode 100644 index 101557c..0000000 --- a/docs/source/products/data/infn_cses_hepd_spectrum.rst +++ /dev/null @@ -1,107 +0,0 @@ -=============================================================================================== -HEPD-01 time-integrated proton spectrum during the Ground-Level Enhancement of October 28, 2021 -=============================================================================================== - -.. 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 -~~~~~~~~~~ - -https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2022SW003191 - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. list-table:: - :widths: 7 20 15 10 48 - :align: right - :header-rows: 1 - - * - progr - - column - - units - - type - - description - * - 1 - - time - - UTC - - datetime - - datetime (2021-10-28T00:00:00.000) (time.epoch) - Reference time of the event - * - 2 - - start_time - - UTC - - datetime - - datetime (2021-10-28T00:00:00.000) (time.epoch) - Start time of the data integration - * - 3 - - end_time - - UTC - - datetime - - datetime (2021-11-03T23:59:59.000) (time.epoch) - End time of the data integration - * - 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/infn_iss_ams_flux_timeseries.rst b/docs/source/products/data/infn_iss_ams_flux_timeseries.rst deleted file mode 100644 index 9fc615e..0000000 --- a/docs/source/products/data/infn_iss_ams_flux_timeseries.rst +++ /dev/null @@ -1,107 +0,0 @@ -=========================================== -INFN AMS daily proton time dependent fluxes -=========================================== - -.. 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 -~~~~~~~~~~ - -https://doi.org/10.1103/PhysRevLett.127.271102 - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. list-table:: - :widths: 7 20 15 10 48 - :align: right - :header-rows: 1 - - * - progr - - column - - units - - type - - description - * - 1 - - time - - UTC - - datetime - - datetime (2011-05-20T12:00:00) - time UTC of the data-taking - * - 2 - - rigidity_min - - GV - - float - - GV (10.1) - lower edge of the rigidity interval - * - 3 - - rigidity_max - - GV - - float - - GV (16.6) - upper edge of the rigidity interval - * - 4 - - proton_flux - - m^-2sr^-1s^-1GV^-1 - - float - - m^-2sr^-1s^-1GV^-1 (259.9) - daily proton flux - * - 5 - - proton_flux_error_statistical - - m^-2sr^-1s^-1GV^-1 - - float - - m^-2sr^-1s^-1GV^-1 (0.11) - total statistical error - * - 6 - - proton_flux_error_timedependent - - m^-2sr^-1s^-1GV^-1 - - float - - m^-2sr^-1s^-1GV^-1 (0.07) - systematic error from the trigger and reconstruction efficiencies - * - 7 - - proton_flux_error_systematic_total - - m^-2sr^-1s^-1GV^-1 - - float - - m^-2sr^-1s^-1GV^-1 (0.24) - total systematic error (sum in quadrature of the time-indep and the time-dep systematic errors) diff --git a/docs/source/products/data/infn_pamela_flux_timeseries.rst b/docs/source/products/data/infn_pamela_flux_timeseries.rst deleted file mode 100644 index 1d9f643..0000000 --- a/docs/source/products/data/infn_pamela_flux_timeseries.rst +++ /dev/null @@ -1,102 +0,0 @@ -========================================================== -PAMELA time-profiles of protons during 4 Forbush Decreases -========================================================== - -.. 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 -~~~~~~~~~~ - -https://iopscience.iop.org/article/10.3847/1538-4357/aaa0c8 - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. 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 - - rig_min - - GV - - float - - GV (0.85) - lower edge of the rigidity interval - * - 3 - - rig_max - - GV - - float - - GV (1.04) - upper edge of the rigidity interval - * - 4 - - flux - - none - - float - - none (0.949654) - cosmic-ray flux, normalized for a quiet period before the event generating the decrease - * - 5 - - error_flux - - none - - float - - none (0.0326884) - error on the proton measurement (stat + syst) - * - 6 - - num_event - - none - - int - - none (0) - Forbush decrease number diff --git a/docs/source/products/data/infn_saandose_samadha_timeseries.rst b/docs/source/products/data/infn_saandose_samadha_timeseries.rst deleted file mode 100644 index 036958f..0000000 --- a/docs/source/products/data/infn_saandose_samadha_timeseries.rst +++ /dev/null @@ -1,87 +0,0 @@ -============================================= -SAMADHA neutron dose rate at Mount Chacaltaya -============================================= - -.. contents:: Table of contents - -SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) is an INFN project aimed to monitor the neutron dose rate due to cosmic rays at the Chacaltaya Station (Bolivia, 5200 m) inside the South Atlantic Anomaly region, to study possible correlation between space weather events and dose rate at the ground, considering the proximity of the Van Allen Belts to the Earth's surface in the SAA region. - -References -~~~~~~~~~~ - -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 deleted file mode 100644 index e1a2431..0000000 --- a/docs/source/products/data/infn_tgndose_samadha_timeseries.rst +++ /dev/null @@ -1,87 +0,0 @@ -========================================= -SAMADHA neutron dose rate at Testa Grigia -========================================= - -.. contents:: Table of contents - -Monitoring of the neutron dose rate due to cosmic rays at the Testa Grigia Station (3480 m, Cervinia, Italy), to study possible correlation between space weather events and dose rate at the ground. This measurement is part of the INFN project SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) aimed to monitor the neutron dose inside the South Atlantic Anomaly (SAA) region in Bolivia. The data taken at Testa Grigia are a term of comparison for those collected in the SAA region. - -References -~~~~~~~~~~ - -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 deleted file mode 100644 index 03fd83b..0000000 --- a/docs/source/products/data/ingv_alert_aqu_timeseries.rst +++ /dev/null @@ -1,135 +0,0 @@ -====================================================== -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 deleted file mode 100644 index fe23a67..0000000 --- a/docs/source/products/data/ingv_alert_cts_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -============================================================= -INGV geomagnetic data, GIC indices and alert: Castello Tesino -============================================================= - -.. contents:: Table of contents - -From both components of GIC index for Castello Tesino observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 3f66753..0000000 --- a/docs/source/products/data/ingv_alert_dur_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -===================================================== -INGV geomagnetic data, GIC indices and alert: Duronia -===================================================== - -.. contents:: Table of contents - -From both components of GIC index for Duronia observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index f3d991b..0000000 --- a/docs/source/products/data/ingv_alert_int_timeseries.rst +++ /dev/null @@ -1,137 +0,0 @@ -============================================================================ -Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories -============================================================================ - -.. contents:: Table of contents - -not available in DBF - -References -~~~~~~~~~~ - -not available in DBF - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. 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_alert_lmp_timeseries.rst b/docs/source/products/data/ingv_alert_lmp_timeseries.rst deleted file mode 100644 index c2feed3..0000000 --- a/docs/source/products/data/ingv_alert_lmp_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -======================================================= -INGV geomagnetic data, GIC indices and alert: Lampedusa -======================================================= - -.. contents:: Table of contents - -From both components of GIC index for Lampedusa observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 1675fc8..0000000 --- a/docs/source/products/data/ingv_alert_wdc_timeseries.rst +++ /dev/null @@ -1,137 +0,0 @@ -======================================================================================================== -Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories -======================================================================================================== - -.. contents:: Table of contents - -not available in DBF - -References -~~~~~~~~~~ - -not available in DBF - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. 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_autoiono_bbla_timeseries.rst b/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst deleted file mode 100644 index ac14a8b..0000000 --- a/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst +++ /dev/null @@ -1,117 +0,0 @@ -====================================== -Autoscaled data Bahia Blanca Ionosonde -====================================== - -.. contents:: Table of contents - -Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Bahia Blanca - -References -~~~~~~~~~~ - -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 deleted file mode 100644 index a8a85d6..0000000 --- a/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst +++ /dev/null @@ -1,117 +0,0 @@ -==================================== -Autoscaled data Gibilmanna Ionosonde -==================================== - -.. contents:: Table of contents - -Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna - -References -~~~~~~~~~~ - -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 deleted file mode 100644 index 287c30e..0000000 --- a/docs/source/products/data/ingv_autoiono_rome_timeseries.rst +++ /dev/null @@ -1,117 +0,0 @@ -============================== -Autoscaled data Rome Ionosonde -============================== - -.. contents:: Table of contents - -Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Rome - -References -~~~~~~~~~~ - -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 deleted file mode 100644 index 10e5a97..0000000 --- a/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst +++ /dev/null @@ -1,117 +0,0 @@ -================================= -Autoscaled data Tucuman Ionosonde -================================= - -.. contents:: Table of contents - -Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Tucuman - -References -~~~~~~~~~~ - -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 deleted file mode 100644 index 3dbf61d..0000000 --- a/docs/source/products/data/ingv_b_swarm_image.rst +++ /dev/null @@ -1,107 +0,0 @@ -================================ -Swarm vector magnetic field maps -================================ - -.. contents:: Table of contents - -Vector magnetic field maps in quasi-dipole latitude vs magnetic local time coordinates derived from the Swarm constellation data acquired at 1 second cadence from 1 January 2014 to 31 December 2020. The output consists in nine .jpg or .png files mapping the three components of the vector magnetic field in polar and equatorial projections (3 images for the three components) for each of the 3 satellites of the Swarm constellation. Each map has a size of about 300 kB. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 4a8ca45..0000000 --- a/docs/source/products/data/ingv_b_swarm_timeseries.rst +++ /dev/null @@ -1,147 +0,0 @@ -======================================================================================= -1 Hz Swarm on track values of observed, external and projected vector geomagnetic field -======================================================================================= - -.. contents:: Table of contents - -In situ time series of vector geomagnetic field derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of one has a size of about 14.5 GB. The sample file attached is extracted from one month of data acquired by Swarm A - -References -~~~~~~~~~~ - - - -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_bvect_cses_tableset.rst b/docs/source/products/data/ingv_bvect_cses_tableset.rst deleted file mode 100644 index f2f2a56..0000000 --- a/docs/source/products/data/ingv_bvect_cses_tableset.rst +++ /dev/null @@ -1,102 +0,0 @@ -================================================ -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 deleted file mode 100644 index ed8d81b..0000000 --- a/docs/source/products/data/ingv_evect_cses_tableset.rst +++ /dev/null @@ -1,102 +0,0 @@ -================================================ -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_gic_aqu_timeseries.rst b/docs/source/products/data/ingv_gic_aqu_timeseries.rst deleted file mode 100644 index 65ef3f8..0000000 --- a/docs/source/products/data/ingv_gic_aqu_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -====================================================== -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 deleted file mode 100644 index ab407a6..0000000 --- a/docs/source/products/data/ingv_gic_cts_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -============================================================= -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 deleted file mode 100644 index d102518..0000000 --- a/docs/source/products/data/ingv_gic_dur_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -===================================================== -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 deleted file mode 100644 index 47efee6..0000000 --- a/docs/source/products/data/ingv_gic_int_timeseries.rst +++ /dev/null @@ -1,137 +0,0 @@ -============================================================================ -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 deleted file mode 100644 index e7cbb63..0000000 --- a/docs/source/products/data/ingv_gic_lmp_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -======================================================= -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 deleted file mode 100644 index a150198..0000000 --- a/docs/source/products/data/ingv_gic_wdc_timeseries.rst +++ /dev/null @@ -1,137 +0,0 @@ -======================================================================================================== -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_ltmuf_cagliari_tableset.rst b/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst deleted file mode 100644 index 227feeb..0000000 --- a/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst +++ /dev/null @@ -1,107 +0,0 @@ -======================================= -Long Term MUF maps centered on Cagliari -======================================= - -.. contents:: Table of contents - -Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Cagliari over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 1fa87b3..0000000 --- a/docs/source/products/data/ingv_ltmuf_catania_tableset.rst +++ /dev/null @@ -1,107 +0,0 @@ -====================================== -Long Term MUF maps centered on Catania -====================================== - -.. contents:: Table of contents - -Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 8e4b51e..0000000 --- a/docs/source/products/data/ingv_ltmuf_milan_tableset.rst +++ /dev/null @@ -1,107 +0,0 @@ -===================================== -Long Term MUF maps centered on Milano -===================================== - -.. contents:: Table of contents - -Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index fdc73e1..0000000 --- a/docs/source/products/data/ingv_ltmuf_rome_tableset.rst +++ /dev/null @@ -1,107 +0,0 @@ -=================================== -Long Term MUF maps centered on Roma -=================================== - -.. contents:: Table of contents - -Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index a47bd7e..0000000 --- a/docs/source/products/data/ingv_mag_aqu_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -====================================================== -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 deleted file mode 100644 index a544bfc..0000000 --- a/docs/source/products/data/ingv_mag_cts_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -============================================================= -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 deleted file mode 100644 index 8422911..0000000 --- a/docs/source/products/data/ingv_mag_dmc_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -==================================================== -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 deleted file mode 100644 index c4c3054..0000000 --- a/docs/source/products/data/ingv_mag_dur_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -===================================================== -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 deleted file mode 100644 index 06f912f..0000000 --- a/docs/source/products/data/ingv_mag_int_timeseries.rst +++ /dev/null @@ -1,137 +0,0 @@ -============================================================================ -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 deleted file mode 100644 index afb19d8..0000000 --- a/docs/source/products/data/ingv_mag_lmp_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -======================================================= -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 deleted file mode 100644 index 2988f79..0000000 --- a/docs/source/products/data/ingv_mag_tnb_timeseries.rst +++ /dev/null @@ -1,132 +0,0 @@ -============================================================ -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 deleted file mode 100644 index fc9c041..0000000 --- a/docs/source/products/data/ingv_mag_wdc_timeseries.rst +++ /dev/null @@ -1,137 +0,0 @@ -======================================================================================================== -Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories -======================================================================================================== - -.. contents:: Table of contents - -The mission of the World Data Center for Geomagnetism is to provide geomagnetic field data supplied from a worldwide network of magnetic observatories, as well as geomagnetic indices (AE index, ASY/SYM index, and Dst index) derived in this data center to researchers specializing mostly in solar terrestrial physics, and geomagnetism in order to facilitate the global exchange of the geomagnetic field data including the geomagnetic indices. From the WDC websites it is possible to download 1-minute averages (in daily files) of vector components in either (H, D, Z) or (X, Y, Z) reference frame from world wide magnetic observatories. For this reason, it is not possible to exhaustively fill this form. For instance, the time window of data availability changes from observatory to observatory as well as the tern provided (either (H, D, Z) or (X, Y, Z)) . Data from WDC will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. The set of WDC observatories well overlap to the set of INTERMAGNET observatories. WDC data can be retrieved through queries to a web service (http://www.wdc.bgs.ac.uk/dataportal/webservice_doc.html). At the present moment, however, the service and the website are not working properly and it is not possible to download a sample file. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 3ab5661..0000000 --- a/docs/source/products/data/ingv_magdef_cts_timeseries.rst +++ /dev/null @@ -1,133 +0,0 @@ -============================================================= -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 deleted file mode 100644 index 9d8e7e3..0000000 --- a/docs/source/products/data/ingv_magdef_dur_timeseries.rst +++ /dev/null @@ -1,133 +0,0 @@ -===================================================== -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 deleted file mode 100644 index 0e2a819..0000000 --- a/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst +++ /dev/null @@ -1,107 +0,0 @@ -======================================= -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. - -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 deleted file mode 100644 index f720d9b..0000000 --- a/docs/source/products/data/ingv_ncmuf_catania_tableset.rst +++ /dev/null @@ -1,107 +0,0 @@ -====================================== -Nowcasting MUF map centered on Catania -====================================== - -.. contents:: Table of contents - -Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 96508c1..0000000 --- a/docs/source/products/data/ingv_ncmuf_milan_tableset.rst +++ /dev/null @@ -1,107 +0,0 @@ -===================================== -Nowcasting MUF map centered on Milano -===================================== - -.. contents:: Table of contents - -Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 7f3deb4..0000000 --- a/docs/source/products/data/ingv_ncmuf_rome_tableset.rst +++ /dev/null @@ -1,107 +0,0 @@ -=================================== -Nowcasting MUF map centered on Roma -=================================== - -.. contents:: Table of contents - -Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. - -References -~~~~~~~~~~ - - - -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_valiiono_gibi_timeseries.rst b/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst deleted file mode 100644 index 5090e8b..0000000 --- a/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst +++ /dev/null @@ -1,147 +0,0 @@ -=================================== -Validated data Gibilmanna Ionosonde -=================================== - -.. contents:: Table of contents - -Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 71ec384..0000000 --- a/docs/source/products/data/ingv_valiiono_rome_timeseries.rst +++ /dev/null @@ -1,147 +0,0 @@ -============================= -Validated data Rome Ionosonde -============================= - -.. contents:: Table of contents - -Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Rome - -References -~~~~~~~~~~ - - - -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_tableset.rst b/docs/source/products/data/uniaq_curr_maigic_tableset.rst deleted file mode 100644 index 9933cf0..0000000 --- a/docs/source/products/data/uniaq_curr_maigic_tableset.rst +++ /dev/null @@ -1,127 +0,0 @@ -================================================================== -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 deleted file mode 100644 index 5e1c4e8..0000000 --- a/docs/source/products/data/uniaq_epmde_emma_timeseries.rst +++ /dev/null @@ -1,117 +0,0 @@ -======================================================== -Equatorial Plasma Mass Density estimates in Plasmasphere -======================================================== - -.. contents:: Table of contents - -Equatorial plasma mass density estimates in plasmasphere (2 < L < 6) are derived from the the EMMA magnetometers network, updated every 15 minutes. - -References -~~~~~~~~~~ - - - -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_tableset.rst b/docs/source/products/data/uniaq_field_maigic_tableset.rst deleted file mode 100644 index 99dc51e..0000000 --- a/docs/source/products/data/uniaq_field_maigic_tableset.rst +++ /dev/null @@ -1,132 +0,0 @@ -========================================================================== -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 deleted file mode 100644 index 1fafe6c..0000000 --- a/docs/source/products/data/uniaq_mag_emma_timeseries.rst +++ /dev/null @@ -1,127 +0,0 @@ -=========================== -EMMA Geomagnetic field data -=========================== - -.. contents:: Table of contents - -1-minute averages of the magnetic field variations recorded at 27 ground stations located in Italy and Europe along a meridional chain covering a large range in geographical latitude (from 70 to 42 degrees). The data are automatically collected in near real-time and updated every 15 minutes. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index eb692b8..0000000 --- a/docs/source/products/data/unical_espseptransport_tableset.rst +++ /dev/null @@ -1,117 +0,0 @@ -=================================== -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 deleted file mode 100644 index e341290..0000000 --- a/docs/source/products/data/unical_sep_ace_spectrum.rst +++ /dev/null @@ -1,107 +0,0 @@ -========================================= -SEP Proton Spectra for the ACE spacecraft -========================================= - -.. contents:: Table of contents - -Proton spectra for geoeffective target SWE events (at L1) from ACE spacecraft. - -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 deleted file mode 100644 index db1f85a..0000000 --- a/docs/source/products/data/unical_sep_psp_spectrum.rst +++ /dev/null @@ -1,107 +0,0 @@ -========================================= -SEP Proton Spectra for the PSP spacecraft -========================================= - -.. contents:: Table of contents - -Proton spectra for widespread target SWE events from PSP spacecraft. - -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 deleted file mode 100644 index 540262d..0000000 --- a/docs/source/products/data/unical_sep_soho_spectrum.rst +++ /dev/null @@ -1,107 +0,0 @@ -========================================== -SEP Proton Spectra for the SoHO spacecraft -========================================== - -.. contents:: Table of contents - -Proton spectra for: geoeffective target SWE events (at L1) from SoHO spacecraft. - -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 deleted file mode 100644 index b3474e4..0000000 --- a/docs/source/products/data/unical_sep_solo_spectrum.rst +++ /dev/null @@ -1,107 +0,0 @@ -========================================== -SEP Proton Spectra for the SolO spacecraft -========================================== - -.. contents:: Table of contents - -Proton spectra for widespread target SWE events from SolO spacecraft. - -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 deleted file mode 100644 index 6fcd665..0000000 --- a/docs/source/products/data/unical_sep_stra_spectrum.rst +++ /dev/null @@ -1,107 +0,0 @@ -============================================== -SEP Proton Spectra for the STEREO A spacecraft -============================================== - -.. contents:: Table of contents - -Proton spectra for widespread target SWE events from STEREO A spacecraft. - -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 deleted file mode 100644 index 104d36a..0000000 --- a/docs/source/products/data/unical_sep_wind_spectrum.rst +++ /dev/null @@ -1,107 +0,0 @@ -========================================== -SEP Proton Spectra for the WIND spacecraft -========================================== - -.. contents:: Table of contents - -Proton spectra for: geoeffective target SWE events (at L1) from Wind spacecraft. - -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 deleted file mode 100644 index 9e2c067..0000000 --- a/docs/source/products/data/unical_shockpar_tableset.rst +++ /dev/null @@ -1,217 +0,0 @@ -=============================================== -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 deleted file mode 100644 index 7a7b2b9..0000000 --- a/docs/source/products/data/unict_facula_image.rst +++ /dev/null @@ -1,127 +0,0 @@ -=================================== -Faculae geometrical characteristics -=================================== - -.. contents:: Table of contents - -not available in DBF - -References -~~~~~~~~~~ - -not available in DBF - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. 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 of the associated image - * - 2 - - Fac_index - - index - - int - - index of the facular feature - * - 3 - - Width of Contour - - arcsec - - float - - Width of contoured feature in arcseconds - * - 4 - - Height of Contour - - arcsec - - float - - Height of contoured feature in arcseconds - * - 5 - - HGS_Lon - - deg - - float - - Latitude of contoured Sunspot in Stonyhurst Heliographic Coordinates - * - 6 - - HGS_Lat - - deg - - float - - Longitude of contoured Sunspot in Stonyhurst Heliographic Coordinates - * - 7 - - Area of Contour - - arcsec**2 - - float - - Area of contoured feature in arcseconds squared - * - 8 - - Average Magnetic Field - - Gauss - - float - - Average Magnetic Field in Gauss - * - 9 - - data_name - - char - - string - - the name of the calibrated halpha image - * - 10 - - prew_name - - char - - string - - the name of the full preview file - * - 11 - - thumb_name - - char - - string - - the name of the thumbnail file diff --git a/docs/source/products/data/unict_filament_image.rst b/docs/source/products/data/unict_filament_image.rst deleted file mode 100644 index d356947..0000000 --- a/docs/source/products/data/unict_filament_image.rst +++ /dev/null @@ -1,122 +0,0 @@ -================================================= -Filament position and geometrical characteristics -================================================= - -.. contents:: Table of contents - -not available in DBF - -References -~~~~~~~~~~ - -not available in DBF - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. 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 of the associated image - * - 2 - - Fil_index - - index - - int - - index of the filament feature - * - 3 - - Width of Contour - - arcsec - - float - - Width of contoured feature in arcseconds - * - 4 - - Height of Contour - - arcsec - - float - - Height of contoured feature in arcseconds - * - 5 - - HGS_Lon - - deg - - float - - Latitude of contoured Sunspot in Stonyhurst Heliographic Coordinates - * - 6 - - HGS_Lat - - deg - - float - - Longitude of contoured Sunspot in Stonyhurst Heliographic Coordinates - * - 7 - - Area of Contour - - arcsec**2 - - float - - Area of contoured feature in arcseconds squared - * - 8 - - data_name - - char - - string - - the name of the calibrated halpha image - * - 9 - - prew_name - - char - - string - - the name of the full preview file - * - 10 - - thumb_name - - char - - string - - the name of the thumbnail file diff --git a/docs/source/products/data/unict_offlimb_image.rst b/docs/source/products/data/unict_offlimb_image.rst deleted file mode 100644 index 6298a66..0000000 --- a/docs/source/products/data/unict_offlimb_image.rst +++ /dev/null @@ -1,122 +0,0 @@ -====================================================== -Geometry and location of prominences on the solar limb -====================================================== - -.. contents:: Table of contents - -not available in DBF - -References -~~~~~~~~~~ - -not available in DBF - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. 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 of the associated image - * - 2 - - feature_index - - index - - int - - index of the offlimb feature - * - 3 - - Width of Contour - - arcsec - - float - - Width of contoured feature in arcseconds - * - 4 - - Height of Contour - - arcsec - - float - - Height of contoured feature in arcseconds - * - 5 - - HGS_Lat - - arcsec - - float - - Latitude of contoured Sunspot in Stonyhurst Heliographic Coordinates - * - 6 - - HGS_Lon - - arcsec - - float - - Longitude of contoured Sunspot in Stonyhurst Heliographic Coordinates - * - 7 - - Area of Contour - - arcsec**2 - - float - - Area of contoured feature in arcseconds squared - * - 8 - - data_name - - char - - string - - the name of the calibrated halpha image - * - 9 - - prew_name - - char - - string - - the name of the full preview file - * - 10 - - thumb_name - - char - - string - - the name of the thumbnail file diff --git a/docs/source/products/data/unict_sunspot_image.rst b/docs/source/products/data/unict_sunspot_image.rst deleted file mode 100644 index 9a89ea7..0000000 --- a/docs/source/products/data/unict_sunspot_image.rst +++ /dev/null @@ -1,197 +0,0 @@ -================================== -Sunspots Zurich and McIntosh class -================================== - -.. contents:: Table of contents - -not available in DBF - -References -~~~~~~~~~~ - -not available in DBF - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. 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 of the associated image - * - 2 - - S_index - - index - - int - - index of the Sunspot - * - 3 - - Width of Contour - - arcsec - - float - - Width of contoured Sunspot in arcseconds - * - 4 - - Height of Contour - - arcsec - - float - - Height of contoured Sunspot in arcseconds - * - 5 - - HGS_Lon - - deg - - float - - Latitude of contoured Sunspot in Stonyhurst Heliographic Coordinates - * - 6 - - HGS_Lat - - deg - - float - - Longitude of contoured Sunspot in Stonyhurst Heliographic Coordinates - * - 7 - - Area of Contour - - arcsec**2 - - float - - Area of contoured Sunspot in arcseconds squared - * - 8 - - HMI_HGS_Lon - - deg - - float - - Latitude of contoured HMI magnetic field element in Stonyhurst Helio- graphic Coordinates - * - 9 - - HMI_HGS_Lat - - deg - - float - - Longitude of contoured HMI magnetic field element in Stonyhurst Helio- graphic Coordinates - * - 10 - - Average Magnetic Field - - Gauss - - float - - Average Magnetic Field in Gauss - * - 11 - - Lat_Distance_sunspot - - arcsec - - float - - Latitude difference between the contoured Sunspot and HMI magnetic field element - * - 12 - - Lon_Distance_sunspot - - arcsec - - float - - Longitude difference between the contoured Sunspot and HMI magnetic field element - * - 13 - - NOAA number - - index - - int - - NOAA number - * - 14 - - Center Latitude_hmi - - deg - - int - - Sunspot group latitude in heliographic degrees (mea- sured in degrees north or south) - * - 15 - - Center Longitude_hmi - - deg - - int - - Sunspot group longitude in heliographic degrees (mea- sured in degrees east or west). It provides the east-west position of the region on the Sun’s surface - * - 16 - - Area - - uSun - - int - - Total estimated area of the sunspot group in millionths of the solar hemisphere. This field quantifies the size or area covered by the entire sunspot group - * - 17 - - Z - - char - - string - - McIntosh classification of the sunspot group. The McIntosh classification is a system used to categorize sunspot groups based on their visual characteristics, including the arrangement and com- plexity of sunspots and magnetic fields. It provides informa - * - 18 - - LL - - deg - - int - - Longitudinal extent of the sunspot group in he- liographic degrees. This field indicates the east-west extent of the sunspot group on the solar surface - * - 19 - - NN - - index - - int - - Total number of individual sunspots visible in the sunspot group. This field specifies how many individual sunspots are part of the sunspot group - * - 20 - - Mag Type - - char - - string - - Modified Mount Wil- son classification of the sunspot group. The Mount Wilson classification is a system used to categorize sunspot groups based on their magnetic prop- erties. The ”Modified” classification may indicate a variation or adapta- tion of the - * - 21 - - Lon_Distance_hmi - - arcsec - - float - - Latitude difference between the HMI magnetic field element and Solar- monitor data - * - 22 - - Lat_Distance_hmi - - arcsec - - float - - Longitude difference between the HMI magnetic field element and Solar- monitor data - * - 23 - - data_name - - char - - string - - the name of the calibrated halpha image - * - 24 - - prew_name - - char - - string - - the name of the full preview file - * - 25 - - thumb_name - - char - - string - - the name of the thumbnail file diff --git a/docs/source/products/data/unitn_flux_cses_timeseries.rst b/docs/source/products/data/unitn_flux_cses_timeseries.rst deleted file mode 100644 index d92ca63..0000000 --- a/docs/source/products/data/unitn_flux_cses_timeseries.rst +++ /dev/null @@ -1,97 +0,0 @@ -================================= -CSES satellite particle flux data -================================= - -.. contents:: Table of contents - -Particle flux in the Lshell – pitch reference frame. Lshell will be calculated using the IGRF model for the internal origin field and Tsyganenko model for the external origin field. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index da9827f..0000000 --- a/docs/source/products/data/unitov_halpha_tsst_image.rst +++ /dev/null @@ -1,137 +0,0 @@ -============================= -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 deleted file mode 100644 index c8b0204..0000000 --- a/docs/source/products/data/unitov_icme_tableset.rst +++ /dev/null @@ -1,232 +0,0 @@ -===================================== -UNITOV Catalogue of geoeffective CMEs -===================================== - -.. contents:: Table of contents - -A database associating L1 Time of Arrival and Speed of an interplanetary CME to the kinematic characteristics of the corresponding CME, covering the period 1996-2020. - -References -~~~~~~~~~~ - - - -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 deleted file mode 100644 index 9ee9f05..0000000 --- a/docs/source/products/data/unitov_iss_lidal_timeseries.rst +++ /dev/null @@ -1,92 +0,0 @@ -============================== -LIDAL Flux and Dose timeseries -============================== - -.. contents:: Table of contents - -not available in DBF - -References -~~~~~~~~~~ - -not available in DBF - -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 -~~~~~~~~~~~~~~~~~~~~~ - -.. 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 - - Flux - - counts/s/cm^2/sterad - - float - - Flux (0.184981454) - Total particle flux daily average - * - 3 - - Dose - - muG/h - - float - - Dose (0.184981454) - Dose rate daily average - * - 4 - - Orientation - - index - - int - - Orientation (1) - Orientation wrt ISS axes, 1=x, 2=y, 3=z diff --git a/docs/source/products/data/unitov_mag_tsst_image.rst b/docs/source/products/data/unitov_mag_tsst_image.rst deleted file mode 100644 index e409bc7..0000000 --- a/docs/source/products/data/unitov_mag_tsst_image.rst +++ /dev/null @@ -1,137 +0,0 @@ -================================ -TSST Full Disk LoS magnetic maps -================================ - -.. contents:: Table of contents - -The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. - -References -~~~~~~~~~~ - - - -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_rdparameter_tableset.rst b/docs/source/products/data/unitov_rdparameter_tableset.rst deleted file mode 100644 index e35cf84..0000000 --- a/docs/source/products/data/unitov_rdparameter_tableset.rst +++ /dev/null @@ -1,127 +0,0 @@ -================================ -R and D Active Region parameters -================================ - -.. contents:: Table of contents - -Parameters for flare-forecasting applications, representing the complexity of a solar active region - -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 deleted file mode 100644 index fb7b190..0000000 --- a/docs/source/products/data/unitov_vel_tsst_image.rst +++ /dev/null @@ -1,137 +0,0 @@ -============================ -TSST Full Disk Velocity Maps -============================ - -.. contents:: Table of contents - -The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. - -References -~~~~~~~~~~ - - - -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 diff --git a/docs/source/products/data_products.rst b/docs/source/products/data_products.rst index 74f252a..7210268 100644 --- a/docs/source/products/data_products.rst +++ b/docs/source/products/data_products.rst @@ -1,8 +1,96 @@ -Data Products +Atmosphere +---------- + +.. toctree:: + :titlesonly: + :glob: + + filerst_ATMO/* + +Earth image/map +--------------- + +.. toctree:: + :titlesonly: + :glob: + + filerst_Earth/* + +Geomagnetosphere +---------------- + +.. toctree:: + :titlesonly: + :glob: + + filerst_GEOMAG/* + +Ground +------ + +.. toctree:: + :titlesonly: + :glob: + + filerst_GROUND/* + +Ionosphere +---------- + +.. toctree:: + :titlesonly: + :glob: + + filerst_IONO/* + +Data Acquired in the interplanetary space +----------------------------------------- + +.. toctree:: + :titlesonly: + :glob: + + filerst_IP/* + +Data Acquired at Lagrange 1 position +------------------------------------ + +.. toctree:: + :titlesonly: + :glob: + + filerst_L1/* + +Mercury image/map +----------------- + +.. toctree:: + :titlesonly: + :glob: + + filerst_Mercury/* + +Sun image/map ------------- .. toctree:: :titlesonly: :glob: - data/* + filerst_SUN/* + +Venus image/map +--------------- + +.. toctree:: + :titlesonly: + :glob: + + filerst_Venus/* + + + + + + + diff --git a/docs/source/products/main.rst b/docs/source/products/main.rst index eafa591..e7d14ec 100644 --- a/docs/source/products/main.rst +++ b/docs/source/products/main.rst @@ -1,4 +1,4 @@ -Product Catalogue +Products Catalogue ================== .. include:: intro.rst -- GitLab From b03d354a55693a9b74f61db6cdb0bd1a638a764a Mon Sep 17 00:00:00 2001 From: stefano scardigli Date: Fri, 12 Apr 2024 12:55:19 +0200 Subject: [PATCH 2/2] second attemp.... --- .../filerst_Earth/inaf_s1sep_tableset.rst | 207 ++++++++++++++++ .../filerst_Earth/inaf_s2sep_tableset.rst | 207 ++++++++++++++++ .../infn_cses_hepd_spectrum.rst | 107 ++++++++ .../infn_iss_ams_flux_timeseries.rst | 107 ++++++++ .../infn_pamela_flux_timeseries.rst | 102 ++++++++ .../uniaq_curr_maigic_tableset.rst | 127 ++++++++++ .../uniaq_epmde_emma_timeseries.rst | 117 +++++++++ .../uniaq_field_maigic_tableset.rst | 132 ++++++++++ .../unitov_iss_lidal_timeseries.rst | 92 +++++++ .../inaf_flux1h_svirco_timeseries.rst | 82 +++++++ .../inaf_flux5m_svirco_timeseries.rst | 92 +++++++ .../infn_saandose_samadha_timeseries.rst | 87 +++++++ .../infn_tgndose_samadha_timeseries.rst | 87 +++++++ .../ingv_alert_aqu_timeseries.rst | 135 ++++++++++ .../ingv_alert_cts_timeseries.rst | 132 ++++++++++ .../ingv_alert_dur_timeseries.rst | 132 ++++++++++ .../ingv_alert_int_timeseries.rst | 137 +++++++++++ .../ingv_alert_lmp_timeseries.rst | 132 ++++++++++ .../ingv_alert_wdc_timeseries.rst | 137 +++++++++++ .../ingv_gic_aqu_timeseries.rst | 132 ++++++++++ .../ingv_gic_cts_timeseries.rst | 132 ++++++++++ .../ingv_gic_dur_timeseries.rst | 132 ++++++++++ .../ingv_gic_int_timeseries.rst | 137 +++++++++++ .../ingv_gic_lmp_timeseries.rst | 132 ++++++++++ .../ingv_gic_wdc_timeseries.rst | 137 +++++++++++ .../ingv_mag_aqu_timeseries.rst | 132 ++++++++++ .../ingv_mag_cts_timeseries.rst | 132 ++++++++++ .../ingv_mag_dmc_timeseries.rst | 132 ++++++++++ .../ingv_mag_dur_timeseries.rst | 132 ++++++++++ .../ingv_mag_int_timeseries.rst | 137 +++++++++++ .../ingv_mag_lmp_timeseries.rst | 132 ++++++++++ .../ingv_mag_tnb_timeseries.rst | 132 ++++++++++ .../ingv_mag_wdc_timeseries.rst | 137 +++++++++++ .../ingv_magdef_cts_timeseries.rst | 133 ++++++++++ .../ingv_magdef_dur_timeseries.rst | 133 ++++++++++ .../uniaq_mag_emma_timeseries.rst | 127 ++++++++++ .../inaf_cpcp_superdarn_datacube.rst | 200 +++++++++++++++ .../ingv_autoiono_bbla_timeseries.rst | 117 +++++++++ .../ingv_autoiono_gibi_timeseries.rst | 117 +++++++++ .../ingv_autoiono_rome_timeseries.rst | 117 +++++++++ .../ingv_autoiono_tucu_timeseries.rst | 117 +++++++++ .../filerst_IONO/ingv_b_swarm_image.rst | 107 ++++++++ .../filerst_IONO/ingv_b_swarm_timeseries.rst | 147 +++++++++++ .../filerst_IONO/ingv_bvect_cses_tableset.rst | 102 ++++++++ .../filerst_IONO/ingv_evect_cses_tableset.rst | 102 ++++++++ .../ingv_ltmuf_cagliari_tableset.rst | 107 ++++++++ .../ingv_ltmuf_catania_tableset.rst | 107 ++++++++ .../ingv_ltmuf_milan_tableset.rst | 107 ++++++++ .../filerst_IONO/ingv_ltmuf_rome_tableset.rst | 107 ++++++++ .../ingv_ncmuf_cagliari_tableset.rst | 107 ++++++++ .../ingv_ncmuf_catania_tableset.rst | 107 ++++++++ .../ingv_ncmuf_milan_tableset.rst | 107 ++++++++ .../filerst_IONO/ingv_ncmuf_rome_tableset.rst | 107 ++++++++ .../ingv_valiiono_gibi_timeseries.rst | 147 +++++++++++ .../ingv_valiiono_rome_timeseries.rst | 147 +++++++++++ .../unitn_flux_cses_timeseries.rst | 97 ++++++++ .../inaf_data_solopas_timeseries.rst | 126 ++++++++++ .../filerst_IP/inaf_gsmaps_datacube.rst | 92 +++++++ .../products/filerst_IP/inaf_tps_datacube.rst | 92 +++++++ .../unical_espseptransport_tableset.rst | 117 +++++++++ .../filerst_IP/unical_sep_psp_spectrum.rst | 107 ++++++++ .../filerst_IP/unical_sep_solo_spectrum.rst | 107 ++++++++ .../filerst_IP/unical_sep_stra_spectrum.rst | 107 ++++++++ .../filerst_IP/unical_shockpar_tableset.rst | 217 ++++++++++++++++ .../filerst_IP/unitov_icme_tableset.rst | 232 ++++++++++++++++++ .../external_ace_swepam_timeseries.rst | 92 +++++++ .../external_flux_goes_timeseries.rst | 87 +++++++ .../external_part_goes_timeseries.rst | 122 +++++++++ .../filerst_L1/inaf_vbcorr_wind_tableset.rst | 98 ++++++++ .../filerst_L1/unical_sep_ace_spectrum.rst | 107 ++++++++ .../filerst_L1/unical_sep_soho_spectrum.rst | 107 ++++++++ .../filerst_L1/unical_sep_wind_spectrum.rst | 107 ++++++++ .../filerst_Mercury/inaf_na_mercexo_image.rst | 157 ++++++++++++ .../filerst_SUN/inaf_m2flare_tableset.rst | 132 ++++++++++ .../filerst_SUN/unict_facula_image.rst | 127 ++++++++++ .../filerst_SUN/unict_filament_image.rst | 122 +++++++++ .../filerst_SUN/unict_offlimb_image.rst | 122 +++++++++ .../filerst_SUN/unict_sunspot_image.rst | 197 +++++++++++++++ .../filerst_SUN/unitov_halpha_tsst_image.rst | 137 +++++++++++ .../filerst_SUN/unitov_mag_tsst_image.rst | 137 +++++++++++ .../unitov_rdparameter_tableset.rst | 127 ++++++++++ .../filerst_SUN/unitov_vel_tsst_image.rst | 137 +++++++++++ 82 files changed, 10297 insertions(+) create mode 100644 docs/source/products/filerst_Earth/inaf_s1sep_tableset.rst create mode 100644 docs/source/products/filerst_Earth/inaf_s2sep_tableset.rst create mode 100644 docs/source/products/filerst_GEOMAG/infn_cses_hepd_spectrum.rst create mode 100644 docs/source/products/filerst_GEOMAG/infn_iss_ams_flux_timeseries.rst create mode 100644 docs/source/products/filerst_GEOMAG/infn_pamela_flux_timeseries.rst create mode 100644 docs/source/products/filerst_GEOMAG/uniaq_curr_maigic_tableset.rst create mode 100644 docs/source/products/filerst_GEOMAG/uniaq_epmde_emma_timeseries.rst create mode 100644 docs/source/products/filerst_GEOMAG/uniaq_field_maigic_tableset.rst create mode 100644 docs/source/products/filerst_GEOMAG/unitov_iss_lidal_timeseries.rst create mode 100644 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docs/source/products/filerst_SUN/unitov_mag_tsst_image.rst create mode 100644 docs/source/products/filerst_SUN/unitov_rdparameter_tableset.rst create mode 100644 docs/source/products/filerst_SUN/unitov_vel_tsst_image.rst diff --git a/docs/source/products/filerst_Earth/inaf_s1sep_tableset.rst b/docs/source/products/filerst_Earth/inaf_s1sep_tableset.rst new file mode 100644 index 0000000..f60fb57 --- /dev/null +++ b/docs/source/products/filerst_Earth/inaf_s1sep_tableset.rst @@ -0,0 +1,207 @@ +============================ +IAPS S1 SEP events Catalogue +============================ + +.. contents:: Table of contents + +The catalogue contains SEP events observed at the Earth of class S1, i.e. with flux in the range [10, 100) pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux >= 100 pfu at > 10 MeV are listed in the companion table S2 SEP Catalogue. + +References +~~~~~~~~~~ + + + +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/filerst_Earth/inaf_s2sep_tableset.rst b/docs/source/products/filerst_Earth/inaf_s2sep_tableset.rst new file mode 100644 index 0000000..0963e5a --- /dev/null +++ b/docs/source/products/filerst_Earth/inaf_s2sep_tableset.rst @@ -0,0 +1,207 @@ +============================ +IAPS S2 SEP events Catalogue +============================ + +.. contents:: Table of contents + +The catalogue contains SEP events observed at the Earth of class S2, i.e. with flux >100 pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux in the interval [10, 100) pfu at > 10 MeV are listed in the companion table S1 SEP Catalogue. + +References +~~~~~~~~~~ + + + +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/filerst_GEOMAG/infn_cses_hepd_spectrum.rst b/docs/source/products/filerst_GEOMAG/infn_cses_hepd_spectrum.rst new file mode 100644 index 0000000..101557c --- /dev/null +++ b/docs/source/products/filerst_GEOMAG/infn_cses_hepd_spectrum.rst @@ -0,0 +1,107 @@ +=============================================================================================== +HEPD-01 time-integrated proton spectrum during the Ground-Level Enhancement of October 28, 2021 +=============================================================================================== + +.. 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 +~~~~~~~~~~ + +https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2022SW003191 + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime (2021-10-28T00:00:00.000) (time.epoch) - Reference time of the event + * - 2 + - start_time + - UTC + - datetime + - datetime (2021-10-28T00:00:00.000) (time.epoch) - Start time of the data integration + * - 3 + - end_time + - UTC + - datetime + - datetime (2021-11-03T23:59:59.000) (time.epoch) - End time of the data integration + * - 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/filerst_GEOMAG/infn_iss_ams_flux_timeseries.rst b/docs/source/products/filerst_GEOMAG/infn_iss_ams_flux_timeseries.rst new file mode 100644 index 0000000..9fc615e --- /dev/null +++ b/docs/source/products/filerst_GEOMAG/infn_iss_ams_flux_timeseries.rst @@ -0,0 +1,107 @@ +=========================================== +INFN AMS daily proton time dependent fluxes +=========================================== + +.. 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 +~~~~~~~~~~ + +https://doi.org/10.1103/PhysRevLett.127.271102 + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - datetime (2011-05-20T12:00:00) - time UTC of the data-taking + * - 2 + - rigidity_min + - GV + - float + - GV (10.1) - lower edge of the rigidity interval + * - 3 + - rigidity_max + - GV + - float + - GV (16.6) - upper edge of the rigidity interval + * - 4 + - proton_flux + - m^-2sr^-1s^-1GV^-1 + - float + - m^-2sr^-1s^-1GV^-1 (259.9) - daily proton flux + * - 5 + - proton_flux_error_statistical + - m^-2sr^-1s^-1GV^-1 + - float + - m^-2sr^-1s^-1GV^-1 (0.11) - total statistical error + * - 6 + - proton_flux_error_timedependent + - m^-2sr^-1s^-1GV^-1 + - float + - m^-2sr^-1s^-1GV^-1 (0.07) - systematic error from the trigger and reconstruction efficiencies + * - 7 + - proton_flux_error_systematic_total + - m^-2sr^-1s^-1GV^-1 + - float + - m^-2sr^-1s^-1GV^-1 (0.24) - total systematic error (sum in quadrature of the time-indep and the time-dep systematic errors) diff --git a/docs/source/products/filerst_GEOMAG/infn_pamela_flux_timeseries.rst b/docs/source/products/filerst_GEOMAG/infn_pamela_flux_timeseries.rst new file mode 100644 index 0000000..1d9f643 --- /dev/null +++ b/docs/source/products/filerst_GEOMAG/infn_pamela_flux_timeseries.rst @@ -0,0 +1,102 @@ +========================================================== +PAMELA time-profiles of protons during 4 Forbush Decreases +========================================================== + +.. 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 +~~~~~~~~~~ + +https://iopscience.iop.org/article/10.3847/1538-4357/aaa0c8 + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 + - rig_min + - GV + - float + - GV (0.85) - lower edge of the rigidity interval + * - 3 + - rig_max + - GV + - float + - GV (1.04) - upper edge of the rigidity interval + * - 4 + - flux + - none + - float + - none (0.949654) - cosmic-ray flux, normalized for a quiet period before the event generating the decrease + * - 5 + - error_flux + - none + - float + - none (0.0326884) - error on the proton measurement (stat + syst) + * - 6 + - num_event + - none + - int + - none (0) - Forbush decrease number diff --git a/docs/source/products/filerst_GEOMAG/uniaq_curr_maigic_tableset.rst b/docs/source/products/filerst_GEOMAG/uniaq_curr_maigic_tableset.rst new file mode 100644 index 0000000..9933cf0 --- /dev/null +++ b/docs/source/products/filerst_GEOMAG/uniaq_curr_maigic_tableset.rst @@ -0,0 +1,127 @@ +================================================================== +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/filerst_GEOMAG/uniaq_epmde_emma_timeseries.rst b/docs/source/products/filerst_GEOMAG/uniaq_epmde_emma_timeseries.rst new file mode 100644 index 0000000..5e1c4e8 --- /dev/null +++ b/docs/source/products/filerst_GEOMAG/uniaq_epmde_emma_timeseries.rst @@ -0,0 +1,117 @@ +======================================================== +Equatorial Plasma Mass Density estimates in Plasmasphere +======================================================== + +.. contents:: Table of contents + +Equatorial plasma mass density estimates in plasmasphere (2 < L < 6) are derived from the the EMMA magnetometers network, updated every 15 minutes. + +References +~~~~~~~~~~ + + + +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/filerst_GEOMAG/uniaq_field_maigic_tableset.rst b/docs/source/products/filerst_GEOMAG/uniaq_field_maigic_tableset.rst new file mode 100644 index 0000000..99dc51e --- /dev/null +++ b/docs/source/products/filerst_GEOMAG/uniaq_field_maigic_tableset.rst @@ -0,0 +1,132 @@ +========================================================================== +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/filerst_GEOMAG/unitov_iss_lidal_timeseries.rst b/docs/source/products/filerst_GEOMAG/unitov_iss_lidal_timeseries.rst new file mode 100644 index 0000000..9ee9f05 --- /dev/null +++ b/docs/source/products/filerst_GEOMAG/unitov_iss_lidal_timeseries.rst @@ -0,0 +1,92 @@ +============================== +LIDAL Flux and Dose timeseries +============================== + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 + - Flux + - counts/s/cm^2/sterad + - float + - Flux (0.184981454) - Total particle flux daily average + * - 3 + - Dose + - muG/h + - float + - Dose (0.184981454) - Dose rate daily average + * - 4 + - Orientation + - index + - int + - Orientation (1) - Orientation wrt ISS axes, 1=x, 2=y, 3=z diff --git a/docs/source/products/filerst_GROUND/inaf_flux1h_svirco_timeseries.rst b/docs/source/products/filerst_GROUND/inaf_flux1h_svirco_timeseries.rst new file mode 100644 index 0000000..3542b5c --- /dev/null +++ b/docs/source/products/filerst_GROUND/inaf_flux1h_svirco_timeseries.rst @@ -0,0 +1,82 @@ +============================================= +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/filerst_GROUND/inaf_flux5m_svirco_timeseries.rst b/docs/source/products/filerst_GROUND/inaf_flux5m_svirco_timeseries.rst new file mode 100644 index 0000000..8e7960b --- /dev/null +++ b/docs/source/products/filerst_GROUND/inaf_flux5m_svirco_timeseries.rst @@ -0,0 +1,92 @@ +============================================== +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/filerst_GROUND/infn_saandose_samadha_timeseries.rst b/docs/source/products/filerst_GROUND/infn_saandose_samadha_timeseries.rst new file mode 100644 index 0000000..da89444 --- /dev/null +++ b/docs/source/products/filerst_GROUND/infn_saandose_samadha_timeseries.rst @@ -0,0 +1,87 @@ +============================================= +SAMADHA neutron dose rate at Mount Chacaltaya +============================================= + +.. contents:: Table of contents + +SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) is an INFN project aimed to monitor the neutron dose rate due to cosmic rays at the Chacaltaya Station (Bolivia, 5200 m) inside the South Atlantic Anomaly region, to study possible correlation between space weather events and dose rate at the ground, considering the proximity of the Van Allen Belts to the Earth's surface in the SAA region. + +References +~~~~~~~~~~ + +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:** + - 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/filerst_GROUND/infn_tgndose_samadha_timeseries.rst b/docs/source/products/filerst_GROUND/infn_tgndose_samadha_timeseries.rst new file mode 100644 index 0000000..a392c0e --- /dev/null +++ b/docs/source/products/filerst_GROUND/infn_tgndose_samadha_timeseries.rst @@ -0,0 +1,87 @@ +========================================= +SAMADHA neutron dose rate at Testa Grigia +========================================= + +.. contents:: Table of contents + +Monitoring of the neutron dose rate due to cosmic rays at the Testa Grigia Station (3480 m, Cervinia, Italy), to study possible correlation between space weather events and dose rate at the ground. This measurement is part of the INFN project SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) aimed to monitor the neutron dose inside the South Atlantic Anomaly (SAA) region in Bolivia. The data taken at Testa Grigia are a term of comparison for those collected in the SAA region. + +References +~~~~~~~~~~ + +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:** + - 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/filerst_GROUND/ingv_alert_aqu_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_alert_aqu_timeseries.rst new file mode 100644 index 0000000..03fd83b --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_alert_aqu_timeseries.rst @@ -0,0 +1,135 @@ +====================================================== +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/filerst_GROUND/ingv_alert_cts_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_alert_cts_timeseries.rst new file mode 100644 index 0000000..fe23a67 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_alert_cts_timeseries.rst @@ -0,0 +1,132 @@ +============================================================= +INGV geomagnetic data, GIC indices and alert: Castello Tesino +============================================================= + +.. contents:: Table of contents + +From both components of GIC index for Castello Tesino observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) + +References +~~~~~~~~~~ + + + +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/filerst_GROUND/ingv_alert_dur_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_alert_dur_timeseries.rst new file mode 100644 index 0000000..3f66753 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_alert_dur_timeseries.rst @@ -0,0 +1,132 @@ +===================================================== +INGV geomagnetic data, GIC indices and alert: Duronia +===================================================== + +.. contents:: Table of contents + +From both components of GIC index for Duronia observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) + +References +~~~~~~~~~~ + + + +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/filerst_GROUND/ingv_alert_int_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_alert_int_timeseries.rst new file mode 100644 index 0000000..f3d991b --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_alert_int_timeseries.rst @@ -0,0 +1,137 @@ +============================================================================ +Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories +============================================================================ + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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/filerst_GROUND/ingv_alert_lmp_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_alert_lmp_timeseries.rst new file mode 100644 index 0000000..c2feed3 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_alert_lmp_timeseries.rst @@ -0,0 +1,132 @@ +======================================================= +INGV geomagnetic data, GIC indices and alert: Lampedusa +======================================================= + +.. contents:: Table of contents + +From both components of GIC index for Lampedusa observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) + +References +~~~~~~~~~~ + + + +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/filerst_GROUND/ingv_alert_wdc_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_alert_wdc_timeseries.rst new file mode 100644 index 0000000..1675fc8 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_alert_wdc_timeseries.rst @@ -0,0 +1,137 @@ +======================================================================================================== +Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories +======================================================================================================== + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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/filerst_GROUND/ingv_gic_aqu_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_gic_aqu_timeseries.rst new file mode 100644 index 0000000..65ef3f8 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_gic_aqu_timeseries.rst @@ -0,0 +1,132 @@ +====================================================== +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/filerst_GROUND/ingv_gic_cts_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_gic_cts_timeseries.rst new file mode 100644 index 0000000..ab407a6 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_gic_cts_timeseries.rst @@ -0,0 +1,132 @@ +============================================================= +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/filerst_GROUND/ingv_gic_dur_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_gic_dur_timeseries.rst new file mode 100644 index 0000000..d102518 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_gic_dur_timeseries.rst @@ -0,0 +1,132 @@ +===================================================== +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/filerst_GROUND/ingv_gic_int_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_gic_int_timeseries.rst new file mode 100644 index 0000000..47efee6 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_gic_int_timeseries.rst @@ -0,0 +1,137 @@ +============================================================================ +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/filerst_GROUND/ingv_gic_lmp_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_gic_lmp_timeseries.rst new file mode 100644 index 0000000..e7cbb63 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_gic_lmp_timeseries.rst @@ -0,0 +1,132 @@ +======================================================= +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/filerst_GROUND/ingv_gic_wdc_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_gic_wdc_timeseries.rst new file mode 100644 index 0000000..a150198 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_gic_wdc_timeseries.rst @@ -0,0 +1,137 @@ +======================================================================================================== +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/filerst_GROUND/ingv_mag_aqu_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_mag_aqu_timeseries.rst new file mode 100644 index 0000000..a47bd7e --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_mag_aqu_timeseries.rst @@ -0,0 +1,132 @@ +====================================================== +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/filerst_GROUND/ingv_mag_cts_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_mag_cts_timeseries.rst new file mode 100644 index 0000000..a544bfc --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_mag_cts_timeseries.rst @@ -0,0 +1,132 @@ +============================================================= +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/filerst_GROUND/ingv_mag_dmc_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_mag_dmc_timeseries.rst new file mode 100644 index 0000000..8422911 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_mag_dmc_timeseries.rst @@ -0,0 +1,132 @@ +==================================================== +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/filerst_GROUND/ingv_mag_dur_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_mag_dur_timeseries.rst new file mode 100644 index 0000000..c4c3054 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_mag_dur_timeseries.rst @@ -0,0 +1,132 @@ +===================================================== +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/filerst_GROUND/ingv_mag_int_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_mag_int_timeseries.rst new file mode 100644 index 0000000..06f912f --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_mag_int_timeseries.rst @@ -0,0 +1,137 @@ +============================================================================ +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/filerst_GROUND/ingv_mag_lmp_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_mag_lmp_timeseries.rst new file mode 100644 index 0000000..afb19d8 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_mag_lmp_timeseries.rst @@ -0,0 +1,132 @@ +======================================================= +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/filerst_GROUND/ingv_mag_tnb_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_mag_tnb_timeseries.rst new file mode 100644 index 0000000..2988f79 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_mag_tnb_timeseries.rst @@ -0,0 +1,132 @@ +============================================================ +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/filerst_GROUND/ingv_mag_wdc_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_mag_wdc_timeseries.rst new file mode 100644 index 0000000..fc9c041 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_mag_wdc_timeseries.rst @@ -0,0 +1,137 @@ +======================================================================================================== +Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories +======================================================================================================== + +.. contents:: Table of contents + +The mission of the World Data Center for Geomagnetism is to provide geomagnetic field data supplied from a worldwide network of magnetic observatories, as well as geomagnetic indices (AE index, ASY/SYM index, and Dst index) derived in this data center to researchers specializing mostly in solar terrestrial physics, and geomagnetism in order to facilitate the global exchange of the geomagnetic field data including the geomagnetic indices. From the WDC websites it is possible to download 1-minute averages (in daily files) of vector components in either (H, D, Z) or (X, Y, Z) reference frame from world wide magnetic observatories. For this reason, it is not possible to exhaustively fill this form. For instance, the time window of data availability changes from observatory to observatory as well as the tern provided (either (H, D, Z) or (X, Y, Z)) . Data from WDC will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. The set of WDC observatories well overlap to the set of INTERMAGNET observatories. WDC data can be retrieved through queries to a web service (http://www.wdc.bgs.ac.uk/dataportal/webservice_doc.html). At the present moment, however, the service and the website are not working properly and it is not possible to download a sample file. + +References +~~~~~~~~~~ + + + +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/filerst_GROUND/ingv_magdef_cts_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_magdef_cts_timeseries.rst new file mode 100644 index 0000000..3ab5661 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_magdef_cts_timeseries.rst @@ -0,0 +1,133 @@ +============================================================= +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/filerst_GROUND/ingv_magdef_dur_timeseries.rst b/docs/source/products/filerst_GROUND/ingv_magdef_dur_timeseries.rst new file mode 100644 index 0000000..9d8e7e3 --- /dev/null +++ b/docs/source/products/filerst_GROUND/ingv_magdef_dur_timeseries.rst @@ -0,0 +1,133 @@ +===================================================== +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/filerst_GROUND/uniaq_mag_emma_timeseries.rst b/docs/source/products/filerst_GROUND/uniaq_mag_emma_timeseries.rst new file mode 100644 index 0000000..1fafe6c --- /dev/null +++ b/docs/source/products/filerst_GROUND/uniaq_mag_emma_timeseries.rst @@ -0,0 +1,127 @@ +=========================== +EMMA Geomagnetic field data +=========================== + +.. contents:: Table of contents + +1-minute averages of the magnetic field variations recorded at 27 ground stations located in Italy and Europe along a meridional chain covering a large range in geographical latitude (from 70 to 42 degrees). The data are automatically collected in near real-time and updated every 15 minutes. + +References +~~~~~~~~~~ + + + +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/filerst_IONO/inaf_cpcp_superdarn_datacube.rst b/docs/source/products/filerst_IONO/inaf_cpcp_superdarn_datacube.rst new file mode 100644 index 0000000..e6f1162 --- /dev/null +++ b/docs/source/products/filerst_IONO/inaf_cpcp_superdarn_datacube.rst @@ -0,0 +1,200 @@ +============================= +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/filerst_IONO/ingv_autoiono_bbla_timeseries.rst b/docs/source/products/filerst_IONO/ingv_autoiono_bbla_timeseries.rst new file mode 100644 index 0000000..ac14a8b --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_autoiono_bbla_timeseries.rst @@ -0,0 +1,117 @@ +====================================== +Autoscaled data Bahia Blanca Ionosonde +====================================== + +.. contents:: Table of contents + +Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Bahia Blanca + +References +~~~~~~~~~~ + +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/filerst_IONO/ingv_autoiono_gibi_timeseries.rst b/docs/source/products/filerst_IONO/ingv_autoiono_gibi_timeseries.rst new file mode 100644 index 0000000..a8a85d6 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_autoiono_gibi_timeseries.rst @@ -0,0 +1,117 @@ +==================================== +Autoscaled data Gibilmanna Ionosonde +==================================== + +.. contents:: Table of contents + +Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna + +References +~~~~~~~~~~ + +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/filerst_IONO/ingv_autoiono_rome_timeseries.rst b/docs/source/products/filerst_IONO/ingv_autoiono_rome_timeseries.rst new file mode 100644 index 0000000..287c30e --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_autoiono_rome_timeseries.rst @@ -0,0 +1,117 @@ +============================== +Autoscaled data Rome Ionosonde +============================== + +.. contents:: Table of contents + +Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Rome + +References +~~~~~~~~~~ + +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/filerst_IONO/ingv_autoiono_tucu_timeseries.rst b/docs/source/products/filerst_IONO/ingv_autoiono_tucu_timeseries.rst new file mode 100644 index 0000000..10e5a97 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_autoiono_tucu_timeseries.rst @@ -0,0 +1,117 @@ +================================= +Autoscaled data Tucuman Ionosonde +================================= + +.. contents:: Table of contents + +Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Tucuman + +References +~~~~~~~~~~ + +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/filerst_IONO/ingv_b_swarm_image.rst b/docs/source/products/filerst_IONO/ingv_b_swarm_image.rst new file mode 100644 index 0000000..e3a2275 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_b_swarm_image.rst @@ -0,0 +1,107 @@ +================================ +Swarm vector magnetic field maps +================================ + +.. contents:: Table of contents + +Vector magnetic field maps in quasi-dipole latitude vs magnetic local time coordinates derived from the Swarm constellation data acquired at 1 second cadence from 1 January 2014 to 31 December 2020. The output consists in nine .jpg or .png files mapping the three components of the vector magnetic field in polar and equatorial projections (3 images for the three components) for each of the 3 satellites of the Swarm constellation. Each map has a size of about 300 kB. + +References +~~~~~~~~~~ + + + +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:** + - IONO + * - **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/filerst_IONO/ingv_b_swarm_timeseries.rst b/docs/source/products/filerst_IONO/ingv_b_swarm_timeseries.rst new file mode 100644 index 0000000..4206a1a --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_b_swarm_timeseries.rst @@ -0,0 +1,147 @@ +======================================================================================= +1 Hz Swarm on track values of observed, external and projected vector geomagnetic field +======================================================================================= + +.. contents:: Table of contents + +In situ time series of vector geomagnetic field derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of one has a size of about 14.5 GB. The sample file attached is extracted from one month of data acquired by Swarm A + +References +~~~~~~~~~~ + + + +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:** + - IONO + * - **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/filerst_IONO/ingv_bvect_cses_tableset.rst b/docs/source/products/filerst_IONO/ingv_bvect_cses_tableset.rst new file mode 100644 index 0000000..789cab1 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_bvect_cses_tableset.rst @@ -0,0 +1,102 @@ +================================================ +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:** + - IONO + * - **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/filerst_IONO/ingv_evect_cses_tableset.rst b/docs/source/products/filerst_IONO/ingv_evect_cses_tableset.rst new file mode 100644 index 0000000..edb29a0 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_evect_cses_tableset.rst @@ -0,0 +1,102 @@ +================================================ +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:** + - IONO + * - **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/filerst_IONO/ingv_ltmuf_cagliari_tableset.rst b/docs/source/products/filerst_IONO/ingv_ltmuf_cagliari_tableset.rst new file mode 100644 index 0000000..227feeb --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_ltmuf_cagliari_tableset.rst @@ -0,0 +1,107 @@ +======================================= +Long Term MUF maps centered on Cagliari +======================================= + +.. contents:: Table of contents + +Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Cagliari over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. + +References +~~~~~~~~~~ + + + +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/filerst_IONO/ingv_ltmuf_catania_tableset.rst b/docs/source/products/filerst_IONO/ingv_ltmuf_catania_tableset.rst new file mode 100644 index 0000000..1fa87b3 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_ltmuf_catania_tableset.rst @@ -0,0 +1,107 @@ +====================================== +Long Term MUF maps centered on Catania +====================================== + +.. contents:: Table of contents + +Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. + +References +~~~~~~~~~~ + + + +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/filerst_IONO/ingv_ltmuf_milan_tableset.rst b/docs/source/products/filerst_IONO/ingv_ltmuf_milan_tableset.rst new file mode 100644 index 0000000..8e4b51e --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_ltmuf_milan_tableset.rst @@ -0,0 +1,107 @@ +===================================== +Long Term MUF maps centered on Milano +===================================== + +.. contents:: Table of contents + +Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. + +References +~~~~~~~~~~ + + + +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/filerst_IONO/ingv_ltmuf_rome_tableset.rst b/docs/source/products/filerst_IONO/ingv_ltmuf_rome_tableset.rst new file mode 100644 index 0000000..fdc73e1 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_ltmuf_rome_tableset.rst @@ -0,0 +1,107 @@ +=================================== +Long Term MUF maps centered on Roma +=================================== + +.. contents:: Table of contents + +Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. + +References +~~~~~~~~~~ + + + +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/filerst_IONO/ingv_ncmuf_cagliari_tableset.rst b/docs/source/products/filerst_IONO/ingv_ncmuf_cagliari_tableset.rst new file mode 100644 index 0000000..0e2a819 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_ncmuf_cagliari_tableset.rst @@ -0,0 +1,107 @@ +======================================= +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. + +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/filerst_IONO/ingv_ncmuf_catania_tableset.rst b/docs/source/products/filerst_IONO/ingv_ncmuf_catania_tableset.rst new file mode 100644 index 0000000..f720d9b --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_ncmuf_catania_tableset.rst @@ -0,0 +1,107 @@ +====================================== +Nowcasting MUF map centered on Catania +====================================== + +.. contents:: Table of contents + +Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. + +References +~~~~~~~~~~ + + + +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/filerst_IONO/ingv_ncmuf_milan_tableset.rst b/docs/source/products/filerst_IONO/ingv_ncmuf_milan_tableset.rst new file mode 100644 index 0000000..96508c1 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_ncmuf_milan_tableset.rst @@ -0,0 +1,107 @@ +===================================== +Nowcasting MUF map centered on Milano +===================================== + +.. contents:: Table of contents + +Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. + +References +~~~~~~~~~~ + + + +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/filerst_IONO/ingv_ncmuf_rome_tableset.rst b/docs/source/products/filerst_IONO/ingv_ncmuf_rome_tableset.rst new file mode 100644 index 0000000..7f3deb4 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_ncmuf_rome_tableset.rst @@ -0,0 +1,107 @@ +=================================== +Nowcasting MUF map centered on Roma +=================================== + +.. contents:: Table of contents + +Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. + +References +~~~~~~~~~~ + + + +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/filerst_IONO/ingv_valiiono_gibi_timeseries.rst b/docs/source/products/filerst_IONO/ingv_valiiono_gibi_timeseries.rst new file mode 100644 index 0000000..5090e8b --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_valiiono_gibi_timeseries.rst @@ -0,0 +1,147 @@ +=================================== +Validated data Gibilmanna Ionosonde +=================================== + +.. contents:: Table of contents + +Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna + +References +~~~~~~~~~~ + + + +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/filerst_IONO/ingv_valiiono_rome_timeseries.rst b/docs/source/products/filerst_IONO/ingv_valiiono_rome_timeseries.rst new file mode 100644 index 0000000..71ec384 --- /dev/null +++ b/docs/source/products/filerst_IONO/ingv_valiiono_rome_timeseries.rst @@ -0,0 +1,147 @@ +============================= +Validated data Rome Ionosonde +============================= + +.. contents:: Table of contents + +Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Rome + +References +~~~~~~~~~~ + + + +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/filerst_IONO/unitn_flux_cses_timeseries.rst b/docs/source/products/filerst_IONO/unitn_flux_cses_timeseries.rst new file mode 100644 index 0000000..d92ca63 --- /dev/null +++ b/docs/source/products/filerst_IONO/unitn_flux_cses_timeseries.rst @@ -0,0 +1,97 @@ +================================= +CSES satellite particle flux data +================================= + +.. contents:: Table of contents + +Particle flux in the Lshell – pitch reference frame. Lshell will be calculated using the IGRF model for the internal origin field and Tsyganenko model for the external origin field. + +References +~~~~~~~~~~ + + + +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/filerst_IP/inaf_data_solopas_timeseries.rst b/docs/source/products/filerst_IP/inaf_data_solopas_timeseries.rst new file mode 100644 index 0000000..b7d8d36 --- /dev/null +++ b/docs/source/products/filerst_IP/inaf_data_solopas_timeseries.rst @@ -0,0 +1,126 @@ +================================ +INAF-IAPS Solar Orbiter-PAS data +================================ + +.. contents:: Table of contents + +The product contains density N, speed vector V, pressure tensor P, temperature components (Tx, Ty, Tz), and the velocity of the satellite V_solo, computed using the data collected by the Proton-Alpha Sensor (PAS) onboard Solar Orbiter. +PAS measures the 3D distribution functions of the dominant ions of the solar wind, from 200 eV to 20 KeV, without mass and charge selection. In practice, this concerns mostly the proton and alfa populations (unseparated). At full resolution, PAS collects the 3D ion distribution function in about 1 second, even though the moments have a cadence of 4 seconds, while in “snapshot” mode the phase space sampling is reduced, allowing a greater cadence for the moments. + +Data is hosted on http://soar.esac.esa.int/soar/ + +References +~~~~~~~~~~ + +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) + +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/filerst_IP/inaf_gsmaps_datacube.rst b/docs/source/products/filerst_IP/inaf_gsmaps_datacube.rst new file mode 100644 index 0000000..1867a25 --- /dev/null +++ b/docs/source/products/filerst_IP/inaf_gsmaps_datacube.rst @@ -0,0 +1,92 @@ +===================================================== +IAPS Grad-Shafranov Reconstruction of Magnetic Clouds +===================================================== + +.. contents:: Table of contents + +Quasi 3-d magnetic field maps of magnetic field configuration within magnetic clouds for geoeffective target SWE events. Such maps will be estimated through the Grad-Shafranov reconstruction from single-spacecraft plasma and magnetic field data. + +References +~~~~~~~~~~ + + + +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/filerst_IP/inaf_tps_datacube.rst b/docs/source/products/filerst_IP/inaf_tps_datacube.rst new file mode 100644 index 0000000..35ccb1a --- /dev/null +++ b/docs/source/products/filerst_IP/inaf_tps_datacube.rst @@ -0,0 +1,92 @@ +================================================ +IAPS Test Particle Simulation on Magnetic Clouds +================================================ + +.. contents:: Table of contents + +Galactic cosmic ray intensity variations associated to the passage of magnetic clouds. The particle intensity variation is estimated through a dedicated full-orbit test-particle simulation. + +References +~~~~~~~~~~ + + + +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:** + - IP + * - **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/filerst_IP/unical_espseptransport_tableset.rst b/docs/source/products/filerst_IP/unical_espseptransport_tableset.rst new file mode 100644 index 0000000..eb692b8 --- /dev/null +++ b/docs/source/products/filerst_IP/unical_espseptransport_tableset.rst @@ -0,0 +1,117 @@ +=================================== +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/filerst_IP/unical_sep_psp_spectrum.rst b/docs/source/products/filerst_IP/unical_sep_psp_spectrum.rst new file mode 100644 index 0000000..db1f85a --- /dev/null +++ b/docs/source/products/filerst_IP/unical_sep_psp_spectrum.rst @@ -0,0 +1,107 @@ +========================================= +SEP Proton Spectra for the PSP spacecraft +========================================= + +.. contents:: Table of contents + +Proton spectra for widespread target SWE events from PSP spacecraft. + +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/filerst_IP/unical_sep_solo_spectrum.rst b/docs/source/products/filerst_IP/unical_sep_solo_spectrum.rst new file mode 100644 index 0000000..b3474e4 --- /dev/null +++ b/docs/source/products/filerst_IP/unical_sep_solo_spectrum.rst @@ -0,0 +1,107 @@ +========================================== +SEP Proton Spectra for the SolO spacecraft +========================================== + +.. contents:: Table of contents + +Proton spectra for widespread target SWE events from SolO spacecraft. + +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/filerst_IP/unical_sep_stra_spectrum.rst b/docs/source/products/filerst_IP/unical_sep_stra_spectrum.rst new file mode 100644 index 0000000..6fcd665 --- /dev/null +++ b/docs/source/products/filerst_IP/unical_sep_stra_spectrum.rst @@ -0,0 +1,107 @@ +============================================== +SEP Proton Spectra for the STEREO A spacecraft +============================================== + +.. contents:: Table of contents + +Proton spectra for widespread target SWE events from STEREO A spacecraft. + +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/filerst_IP/unical_shockpar_tableset.rst b/docs/source/products/filerst_IP/unical_shockpar_tableset.rst new file mode 100644 index 0000000..9e2c067 --- /dev/null +++ b/docs/source/products/filerst_IP/unical_shockpar_tableset.rst @@ -0,0 +1,217 @@ +=============================================== +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/filerst_IP/unitov_icme_tableset.rst b/docs/source/products/filerst_IP/unitov_icme_tableset.rst new file mode 100644 index 0000000..c8b0204 --- /dev/null +++ b/docs/source/products/filerst_IP/unitov_icme_tableset.rst @@ -0,0 +1,232 @@ +===================================== +UNITOV Catalogue of geoeffective CMEs +===================================== + +.. contents:: Table of contents + +A database associating L1 Time of Arrival and Speed of an interplanetary CME to the kinematic characteristics of the corresponding CME, covering the period 1996-2020. + +References +~~~~~~~~~~ + + + +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/filerst_L1/external_ace_swepam_timeseries.rst b/docs/source/products/filerst_L1/external_ace_swepam_timeseries.rst new file mode 100644 index 0000000..4be227e --- /dev/null +++ b/docs/source/products/filerst_L1/external_ace_swepam_timeseries.rst @@ -0,0 +1,92 @@ +==================== +ACE Solar Wind 1 min +==================== + +.. contents:: Table of contents + +qui dovra' esserci la descrizione del prodotto + +References +~~~~~~~~~~ + +qui invece la bibliografia + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC + * - 2 + - ProtonDensity + - p/cc + - double + - p/cm^3 + * - 3 + - BulkSpeed + - km/s + - double + - km/s + * - 4 + - IonTemperature + - K + - double + - K diff --git a/docs/source/products/filerst_L1/external_flux_goes_timeseries.rst b/docs/source/products/filerst_L1/external_flux_goes_timeseries.rst new file mode 100644 index 0000000..766cd96 --- /dev/null +++ b/docs/source/products/filerst_L1/external_flux_goes_timeseries.rst @@ -0,0 +1,87 @@ +=============== +GOES X-ray Flux +=============== + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC + * - 2 + - Short_Wave + - Watts/m^2 + - double + - W/m^2 + * - 3 + - Long_Wave + - Watts/m^2 + - double + - W/m^2 diff --git a/docs/source/products/filerst_L1/external_part_goes_timeseries.rst b/docs/source/products/filerst_L1/external_part_goes_timeseries.rst new file mode 100644 index 0000000..f179e8f --- /dev/null +++ b/docs/source/products/filerst_L1/external_part_goes_timeseries.rst @@ -0,0 +1,122 @@ +================ +GOES proton Flux +================ + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC + * - 2 + - P1 + - Protons/cm^2 - s^-1 - sr + - double + - >=1Mev integral proton flux 5min average + * - 3 + - P5 + - Protons/cm^2 - s^-1 - sr + - double + - >=5Mev integral proton flux 5min average + * - 4 + - P10 + - Protons/cm^2 - s^-1 - sr + - double + - >=10Mev integral proton flux 5min average + * - 5 + - P30 + - Protons/cm^2 - s^-1 - sr + - double + - >=30Mev integral proton flux 5min average + * - 6 + - P50 + - Protons/cm^2 - s^-1 - sr + - double + - >=50Mev integral proton flux 5min average + * - 7 + - P100 + - Protons/cm^2 - s^-1 - sr + - double + - >=100Mev integral proton flux 5min average + * - 8 + - E_8 + - Electrons/cm^2 - s^-1 - sr + - double + - >=0.8Mev integral electron flux 5min average + * - 9 + - E2_0 + - Electrons/cm^2 - s^-1 - sr + - double + - >=2Mev integral electron flux 5min average + * - 10 + - E4_0 + - Electrons/cm^2 - s^-1 - sr + - double + - >=4Mev integral electron flux 5min average diff --git a/docs/source/products/filerst_L1/inaf_vbcorr_wind_tableset.rst b/docs/source/products/filerst_L1/inaf_vbcorr_wind_tableset.rst new file mode 100644 index 0000000..46cb275 --- /dev/null +++ b/docs/source/products/filerst_L1/inaf_vbcorr_wind_tableset.rst @@ -0,0 +1,98 @@ +====================================================================================== +IAPS - Wind velocity-magnetic field correlation coefficient data of solar wind streams +====================================================================================== + +.. contents:: Table of contents + +The velocity - magnetic field (v-b) correlation coefficient unables to identify Alfvénic solar wind intervals (along with almost constant magnetic field magnitude and proton number density). It is derived as the ratio between the covariance of velocity and magnetic field (in Alfvén units) components and the product of their standard deviations, in a time window ranging between tens of minutes to hours. In principle, this formula should be applied to every component of the velocity (V_i) and magnetic fields (B_i) (with i = R, T, N in RTN coordinate system or i = X, Y, Z in GSE coordinate system). The total correlation coefficient is then derived as the average from the three components. However, for the sake of simplicity, we consider only the N component since more Alfvénic than the other two. + +References +~~~~~~~~~~ + +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/filerst_L1/unical_sep_ace_spectrum.rst b/docs/source/products/filerst_L1/unical_sep_ace_spectrum.rst new file mode 100644 index 0000000..e341290 --- /dev/null +++ b/docs/source/products/filerst_L1/unical_sep_ace_spectrum.rst @@ -0,0 +1,107 @@ +========================================= +SEP Proton Spectra for the ACE spacecraft +========================================= + +.. contents:: Table of contents + +Proton spectra for geoeffective target SWE events (at L1) from ACE spacecraft. + +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/filerst_L1/unical_sep_soho_spectrum.rst b/docs/source/products/filerst_L1/unical_sep_soho_spectrum.rst new file mode 100644 index 0000000..540262d --- /dev/null +++ b/docs/source/products/filerst_L1/unical_sep_soho_spectrum.rst @@ -0,0 +1,107 @@ +========================================== +SEP Proton Spectra for the SoHO spacecraft +========================================== + +.. contents:: Table of contents + +Proton spectra for: geoeffective target SWE events (at L1) from SoHO spacecraft. + +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/filerst_L1/unical_sep_wind_spectrum.rst b/docs/source/products/filerst_L1/unical_sep_wind_spectrum.rst new file mode 100644 index 0000000..104d36a --- /dev/null +++ b/docs/source/products/filerst_L1/unical_sep_wind_spectrum.rst @@ -0,0 +1,107 @@ +========================================== +SEP Proton Spectra for the WIND spacecraft +========================================== + +.. contents:: Table of contents + +Proton spectra for: geoeffective target SWE events (at L1) from Wind spacecraft. + +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/filerst_Mercury/inaf_na_mercexo_image.rst b/docs/source/products/filerst_Mercury/inaf_na_mercexo_image.rst new file mode 100644 index 0000000..c580787 --- /dev/null +++ b/docs/source/products/filerst_Mercury/inaf_na_mercexo_image.rst @@ -0,0 +1,157 @@ +=============================================== +INAF-bidimensional maps of Mercury Na exosphere +=============================================== + +.. 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/filerst_SUN/inaf_m2flare_tableset.rst b/docs/source/products/filerst_SUN/inaf_m2flare_tableset.rst new file mode 100644 index 0000000..b7baee1 --- /dev/null +++ b/docs/source/products/filerst_SUN/inaf_m2flare_tableset.rst @@ -0,0 +1,132 @@ +============================== +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/filerst_SUN/unict_facula_image.rst b/docs/source/products/filerst_SUN/unict_facula_image.rst new file mode 100644 index 0000000..7a7b2b9 --- /dev/null +++ b/docs/source/products/filerst_SUN/unict_facula_image.rst @@ -0,0 +1,127 @@ +=================================== +Faculae geometrical characteristics +=================================== + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 of the associated image + * - 2 + - Fac_index + - index + - int + - index of the facular feature + * - 3 + - Width of Contour + - arcsec + - float + - Width of contoured feature in arcseconds + * - 4 + - Height of Contour + - arcsec + - float + - Height of contoured feature in arcseconds + * - 5 + - HGS_Lon + - deg + - float + - Latitude of contoured Sunspot in Stonyhurst Heliographic Coordinates + * - 6 + - HGS_Lat + - deg + - float + - Longitude of contoured Sunspot in Stonyhurst Heliographic Coordinates + * - 7 + - Area of Contour + - arcsec**2 + - float + - Area of contoured feature in arcseconds squared + * - 8 + - Average Magnetic Field + - Gauss + - float + - Average Magnetic Field in Gauss + * - 9 + - data_name + - char + - string + - the name of the calibrated halpha image + * - 10 + - prew_name + - char + - string + - the name of the full preview file + * - 11 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/filerst_SUN/unict_filament_image.rst b/docs/source/products/filerst_SUN/unict_filament_image.rst new file mode 100644 index 0000000..d356947 --- /dev/null +++ b/docs/source/products/filerst_SUN/unict_filament_image.rst @@ -0,0 +1,122 @@ +================================================= +Filament position and geometrical characteristics +================================================= + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 of the associated image + * - 2 + - Fil_index + - index + - int + - index of the filament feature + * - 3 + - Width of Contour + - arcsec + - float + - Width of contoured feature in arcseconds + * - 4 + - Height of Contour + - arcsec + - float + - Height of contoured feature in arcseconds + * - 5 + - HGS_Lon + - deg + - float + - Latitude of contoured Sunspot in Stonyhurst Heliographic Coordinates + * - 6 + - HGS_Lat + - deg + - float + - Longitude of contoured Sunspot in Stonyhurst Heliographic Coordinates + * - 7 + - Area of Contour + - arcsec**2 + - float + - Area of contoured feature in arcseconds squared + * - 8 + - data_name + - char + - string + - the name of the calibrated halpha image + * - 9 + - prew_name + - char + - string + - the name of the full preview file + * - 10 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/filerst_SUN/unict_offlimb_image.rst b/docs/source/products/filerst_SUN/unict_offlimb_image.rst new file mode 100644 index 0000000..6298a66 --- /dev/null +++ b/docs/source/products/filerst_SUN/unict_offlimb_image.rst @@ -0,0 +1,122 @@ +====================================================== +Geometry and location of prominences on the solar limb +====================================================== + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 of the associated image + * - 2 + - feature_index + - index + - int + - index of the offlimb feature + * - 3 + - Width of Contour + - arcsec + - float + - Width of contoured feature in arcseconds + * - 4 + - Height of Contour + - arcsec + - float + - Height of contoured feature in arcseconds + * - 5 + - HGS_Lat + - arcsec + - float + - Latitude of contoured Sunspot in Stonyhurst Heliographic Coordinates + * - 6 + - HGS_Lon + - arcsec + - float + - Longitude of contoured Sunspot in Stonyhurst Heliographic Coordinates + * - 7 + - Area of Contour + - arcsec**2 + - float + - Area of contoured feature in arcseconds squared + * - 8 + - data_name + - char + - string + - the name of the calibrated halpha image + * - 9 + - prew_name + - char + - string + - the name of the full preview file + * - 10 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/filerst_SUN/unict_sunspot_image.rst b/docs/source/products/filerst_SUN/unict_sunspot_image.rst new file mode 100644 index 0000000..9a89ea7 --- /dev/null +++ b/docs/source/products/filerst_SUN/unict_sunspot_image.rst @@ -0,0 +1,197 @@ +================================== +Sunspots Zurich and McIntosh class +================================== + +.. contents:: Table of contents + +not available in DBF + +References +~~~~~~~~~~ + +not available in DBF + +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 +~~~~~~~~~~~~~~~~~~~~~ + +.. 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 of the associated image + * - 2 + - S_index + - index + - int + - index of the Sunspot + * - 3 + - Width of Contour + - arcsec + - float + - Width of contoured Sunspot in arcseconds + * - 4 + - Height of Contour + - arcsec + - float + - Height of contoured Sunspot in arcseconds + * - 5 + - HGS_Lon + - deg + - float + - Latitude of contoured Sunspot in Stonyhurst Heliographic Coordinates + * - 6 + - HGS_Lat + - deg + - float + - Longitude of contoured Sunspot in Stonyhurst Heliographic Coordinates + * - 7 + - Area of Contour + - arcsec**2 + - float + - Area of contoured Sunspot in arcseconds squared + * - 8 + - HMI_HGS_Lon + - deg + - float + - Latitude of contoured HMI magnetic field element in Stonyhurst Helio- graphic Coordinates + * - 9 + - HMI_HGS_Lat + - deg + - float + - Longitude of contoured HMI magnetic field element in Stonyhurst Helio- graphic Coordinates + * - 10 + - Average Magnetic Field + - Gauss + - float + - Average Magnetic Field in Gauss + * - 11 + - Lat_Distance_sunspot + - arcsec + - float + - Latitude difference between the contoured Sunspot and HMI magnetic field element + * - 12 + - Lon_Distance_sunspot + - arcsec + - float + - Longitude difference between the contoured Sunspot and HMI magnetic field element + * - 13 + - NOAA number + - index + - int + - NOAA number + * - 14 + - Center Latitude_hmi + - deg + - int + - Sunspot group latitude in heliographic degrees (mea- sured in degrees north or south) + * - 15 + - Center Longitude_hmi + - deg + - int + - Sunspot group longitude in heliographic degrees (mea- sured in degrees east or west). It provides the east-west position of the region on the Sun’s surface + * - 16 + - Area + - uSun + - int + - Total estimated area of the sunspot group in millionths of the solar hemisphere. This field quantifies the size or area covered by the entire sunspot group + * - 17 + - Z + - char + - string + - McIntosh classification of the sunspot group. The McIntosh classification is a system used to categorize sunspot groups based on their visual characteristics, including the arrangement and com- plexity of sunspots and magnetic fields. It provides informa + * - 18 + - LL + - deg + - int + - Longitudinal extent of the sunspot group in he- liographic degrees. This field indicates the east-west extent of the sunspot group on the solar surface + * - 19 + - NN + - index + - int + - Total number of individual sunspots visible in the sunspot group. This field specifies how many individual sunspots are part of the sunspot group + * - 20 + - Mag Type + - char + - string + - Modified Mount Wil- son classification of the sunspot group. The Mount Wilson classification is a system used to categorize sunspot groups based on their magnetic prop- erties. The ”Modified” classification may indicate a variation or adapta- tion of the + * - 21 + - Lon_Distance_hmi + - arcsec + - float + - Latitude difference between the HMI magnetic field element and Solar- monitor data + * - 22 + - Lat_Distance_hmi + - arcsec + - float + - Longitude difference between the HMI magnetic field element and Solar- monitor data + * - 23 + - data_name + - char + - string + - the name of the calibrated halpha image + * - 24 + - prew_name + - char + - string + - the name of the full preview file + * - 25 + - thumb_name + - char + - string + - the name of the thumbnail file diff --git a/docs/source/products/filerst_SUN/unitov_halpha_tsst_image.rst b/docs/source/products/filerst_SUN/unitov_halpha_tsst_image.rst new file mode 100644 index 0000000..da9827f --- /dev/null +++ b/docs/source/products/filerst_SUN/unitov_halpha_tsst_image.rst @@ -0,0 +1,137 @@ +============================= +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/filerst_SUN/unitov_mag_tsst_image.rst b/docs/source/products/filerst_SUN/unitov_mag_tsst_image.rst new file mode 100644 index 0000000..e409bc7 --- /dev/null +++ b/docs/source/products/filerst_SUN/unitov_mag_tsst_image.rst @@ -0,0 +1,137 @@ +================================ +TSST Full Disk LoS magnetic maps +================================ + +.. contents:: Table of contents + +The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. + +References +~~~~~~~~~~ + + + +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/filerst_SUN/unitov_rdparameter_tableset.rst b/docs/source/products/filerst_SUN/unitov_rdparameter_tableset.rst new file mode 100644 index 0000000..e35cf84 --- /dev/null +++ b/docs/source/products/filerst_SUN/unitov_rdparameter_tableset.rst @@ -0,0 +1,127 @@ +================================ +R and D Active Region parameters +================================ + +.. contents:: Table of contents + +Parameters for flare-forecasting applications, representing the complexity of a solar active region + +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/filerst_SUN/unitov_vel_tsst_image.rst b/docs/source/products/filerst_SUN/unitov_vel_tsst_image.rst new file mode 100644 index 0000000..fb7b190 --- /dev/null +++ b/docs/source/products/filerst_SUN/unitov_vel_tsst_image.rst @@ -0,0 +1,137 @@ +============================ +TSST Full Disk Velocity Maps +============================ + +.. contents:: Table of contents + +The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. + +References +~~~~~~~~~~ + + + +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 -- GitLab