From 3068206d211f6f92940576e1b93b9bfae8e0e820 Mon Sep 17 00:00:00 2001 From: stefano scardigli <stefano.scardigli@roma2.infn.it> Date: Wed, 10 Apr 2024 12:54:24 +0200 Subject: [PATCH] yes yes yes... --- .../data/external_ace_swepam_timeseries.rst | 92 ++++++++--------- .../data/external_flux_goes_timeseries.rst | 92 ++++++++--------- .../data/external_part_goes_timeseries.rst | 92 ++++++++--------- .../data/inaf_cpcp_superdarn_datacube.rst | 92 ++++++++--------- .../data/inaf_data_solopas_timeseries.rst | 92 ++++++++--------- .../data/inaf_flux1h_svirco_timeseries.rst | 98 ++++++++++--------- .../data/inaf_flux5m_svirco_timeseries.rst | 98 ++++++++++--------- .../products/data/inaf_gsmaps_datacube.rst | 98 ++++++++++--------- .../products/data/inaf_m2flare_tableset.rst | 98 ++++++++++--------- .../products/data/inaf_na_mercexo_image.rst | 92 ++++++++--------- .../products/data/inaf_s1sep_tableset.rst | 98 ++++++++++--------- .../products/data/inaf_s2sep_tableset.rst | 98 ++++++++++--------- .../products/data/inaf_tps_datacube.rst | 98 ++++++++++--------- .../data/inaf_vbcorr_wind_tableset.rst | 92 ++++++++--------- .../products/data/infn_cses_hepd_spectrum.rst | 92 ++++++++--------- .../data/infn_iss_ams_flux_timeseries.rst | 92 ++++++++--------- .../data/infn_pamela_flux_timeseries.rst | 92 ++++++++--------- .../data/infn_saandose_samadha_timeseries.rst | 92 ++++++++--------- .../data/infn_tgndose_samadha_timeseries.rst | 92 ++++++++--------- .../data/ingv_alert_aqu_timeseries.rst | 98 ++++++++++--------- .../data/ingv_alert_cts_timeseries.rst | 98 ++++++++++--------- .../data/ingv_alert_dur_timeseries.rst | 98 ++++++++++--------- .../data/ingv_alert_int_timeseries.rst | 92 ++++++++--------- .../data/ingv_alert_lmp_timeseries.rst | 98 ++++++++++--------- .../data/ingv_alert_wdc_timeseries.rst | 92 ++++++++--------- .../data/ingv_autoiono_bbla_timeseries.rst | 92 ++++++++--------- .../data/ingv_autoiono_gibi_timeseries.rst | 92 ++++++++--------- .../data/ingv_autoiono_rome_timeseries.rst | 92 ++++++++--------- .../data/ingv_autoiono_tucu_timeseries.rst | 92 ++++++++--------- .../products/data/ingv_b_swarm_image.rst | 98 ++++++++++--------- .../products/data/ingv_b_swarm_timeseries.rst | 98 ++++++++++--------- .../data/ingv_bvect_cses_tableset.rst | 98 ++++++++++--------- .../data/ingv_evect_cses_tableset.rst | 98 ++++++++++--------- .../products/data/ingv_gic_aqu_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_cts_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_dur_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_int_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_lmp_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_gic_wdc_timeseries.rst | 98 ++++++++++--------- .../data/ingv_ltmuf_cagliari_tableset.rst | 98 ++++++++++--------- .../data/ingv_ltmuf_catania_tableset.rst | 98 ++++++++++--------- .../data/ingv_ltmuf_milan_tableset.rst | 98 ++++++++++--------- .../data/ingv_ltmuf_rome_tableset.rst | 98 ++++++++++--------- .../products/data/ingv_mag_aqu_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_cts_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_dmc_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_dur_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_int_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_lmp_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_tnb_timeseries.rst | 98 ++++++++++--------- .../products/data/ingv_mag_wdc_timeseries.rst | 98 ++++++++++--------- .../data/ingv_magdef_cts_timeseries.rst | 98 ++++++++++--------- .../data/ingv_magdef_dur_timeseries.rst | 98 ++++++++++--------- .../data/ingv_ncmuf_cagliari_tableset.rst | 98 ++++++++++--------- .../data/ingv_ncmuf_catania_tableset.rst | 98 ++++++++++--------- .../data/ingv_ncmuf_milan_tableset.rst | 98 ++++++++++--------- .../data/ingv_ncmuf_rome_tableset.rst | 98 ++++++++++--------- .../data/ingv_valiiono_gibi_timeseries.rst | 98 ++++++++++--------- .../data/ingv_valiiono_rome_timeseries.rst | 98 ++++++++++--------- .../data/uniaq_curr_maigic_tableset.rst | 98 ++++++++++--------- .../data/uniaq_epmde_emma_timeseries.rst | 98 ++++++++++--------- .../data/uniaq_field_maigic_tableset.rst | 98 ++++++++++--------- .../data/uniaq_mag_emma_timeseries.rst | 98 ++++++++++--------- .../data/unical_espseptransport_tableset.rst | 92 ++++++++--------- .../products/data/unical_sep_ace_spectrum.rst | 98 ++++++++++--------- .../products/data/unical_sep_psp_spectrum.rst | 98 ++++++++++--------- .../data/unical_sep_soho_spectrum.rst | 98 ++++++++++--------- .../data/unical_sep_solo_spectrum.rst | 98 ++++++++++--------- .../data/unical_sep_stra_spectrum.rst | 98 ++++++++++--------- .../data/unical_sep_wind_spectrum.rst | 98 ++++++++++--------- .../data/unical_shockpar_tableset.rst | 92 ++++++++--------- .../products/data/unict_facula_image.rst | 92 ++++++++--------- .../products/data/unict_filament_image.rst | 92 ++++++++--------- .../products/data/unict_offlimb_image.rst | 92 ++++++++--------- .../products/data/unict_sunspot_image.rst | 92 ++++++++--------- .../data/unitn_flux_cses_timeseries.rst | 98 ++++++++++--------- .../data/unitov_halpha_tsst_image.rst | 98 ++++++++++--------- .../products/data/unitov_icme_tableset.rst | 98 ++++++++++--------- .../data/unitov_iss_lidal_timeseries.rst | 92 ++++++++--------- .../products/data/unitov_mag_tsst_image.rst | 98 ++++++++++--------- .../data/unitov_rdparameter_tableset.rst | 98 ++++++++++--------- .../products/data/unitov_vel_tsst_image.rst | 98 ++++++++++--------- 82 files changed, 4107 insertions(+), 3779 deletions(-) diff --git a/docs/source/products/data/external_ace_swepam_timeseries.rst b/docs/source/products/data/external_ace_swepam_timeseries.rst index cd21da0..4be227e 100644 --- a/docs/source/products/data/external_ace_swepam_timeseries.rst +++ b/docs/source/products/data/external_ace_swepam_timeseries.rst @@ -2,56 +2,60 @@ ACE Solar Wind 1 min ==================== -.. contents:: The tiny table of contents +.. contents:: Table of contents qui dovra' esserci la descrizione del prodotto -**References** +References +~~~~~~~~~~ qui invece la bibliografia -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** external_ace_swepam_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 101A - -**id_tmp:** 101 - -**short_name:** ace_1minute - -**identifier:** aspis:///external/ace_swepam_timeseries - -**dynamic:** Approx 2MB every week - -**size:** 100kB - -**format:** csv - -**type:** timeseries - -**records_number:** 21599 - -**time_start:** 2016-12-14 - -**time_stop:** 2020-12-31 - -**spatial:** L1 - -**messenger:** protons,electrons - -**spectral_min:** 0.26 - -**spectral_max:** 36 - -**spectral_units:** keV - -**observable:** CME,SW,SEP - -**latest update:** 2024-03-29 12:01:32 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - external_ace_swepam_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 101A + * - **id_tmp:** + - 101 + * - **short_name:** + - ace_1minute + * - **identifier:** + - aspis:///external/ace_swepam_timeseries + * - **dynamic:** + - Approx 2MB every week + * - **size:** + - 100kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 21599 + * - **time_start:** + - 2016-12-14 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - L1 + * - **messenger:** + - protons,electrons + * - **spectral_min:** + - 0.26 + * - **spectral_max:** + - 36 + * - **spectral_units:** + - keV + * - **observable:** + - CME,SW,SEP + * - **latest update:** + - 2024-03-29 12:01:32 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/external_flux_goes_timeseries.rst b/docs/source/products/data/external_flux_goes_timeseries.rst index 52fe3ff..766cd96 100644 --- a/docs/source/products/data/external_flux_goes_timeseries.rst +++ b/docs/source/products/data/external_flux_goes_timeseries.rst @@ -2,56 +2,60 @@ GOES X-ray Flux =============== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** external_flux_goes_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 102A - -**id_tmp:** 102 - -**short_name:** goesx1min - -**identifier:** aspis:///external/flux_goes_timeseries - -**dynamic:** Approx 1MB every week - -**size:** 5MB - -**format:** csv - -**type:** timeseries - -**records_number:** 21599 - -**time_start:** 2016-12-14 - -**time_stop:** 2020-12-31 - -**spatial:** L1 - -**messenger:** photons - -**spectral_min:** 1 - -**spectral_max:** 8 - -**spectral_units:** Angstrom - -**observable:** flare - -**latest update:** 2024-03-28 05:08:04 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - external_flux_goes_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 102A + * - **id_tmp:** + - 102 + * - **short_name:** + - goesx1min + * - **identifier:** + - aspis:///external/flux_goes_timeseries + * - **dynamic:** + - Approx 1MB every week + * - **size:** + - 5MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 21599 + * - **time_start:** + - 2016-12-14 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - L1 + * - **messenger:** + - photons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 8 + * - **spectral_units:** + - Angstrom + * - **observable:** + - flare + * - **latest update:** + - 2024-03-28 05:08:04 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/external_part_goes_timeseries.rst b/docs/source/products/data/external_part_goes_timeseries.rst index ee4b7f3..f179e8f 100644 --- a/docs/source/products/data/external_part_goes_timeseries.rst +++ b/docs/source/products/data/external_part_goes_timeseries.rst @@ -2,56 +2,60 @@ GOES proton Flux ================ -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** external_part_goes_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 103A - -**id_tmp:** 103 - -**short_name:** GOES_particle1min - -**identifier:** aspis:///external/part_goes_timeseries - -**dynamic:** Approx 2MB every week - -**size:** 2MB - -**format:** csv - -**type:** timeseries - -**records_number:** 4319 - -**time_start:** 2016-12-14 - -**time_stop:** 2020-12-31 - -**spatial:** L1 - -**messenger:** protons,electrons - -**spectral_min:** 1 - -**spectral_max:** 100 - -**spectral_units:** MeV - -**observable:** flare,SEP,CME,ESP,SW - -**latest update:** 2024-03-28 05:08:04 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - external_part_goes_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 103A + * - **id_tmp:** + - 103 + * - **short_name:** + - GOES_particle1min + * - **identifier:** + - aspis:///external/part_goes_timeseries + * - **dynamic:** + - Approx 2MB every week + * - **size:** + - 2MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 4319 + * - **time_start:** + - 2016-12-14 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - L1 + * - **messenger:** + - protons,electrons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - flare,SEP,CME,ESP,SW + * - **latest update:** + - 2024-03-28 05:08:04 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst b/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst index 8e2d31c..e6f1162 100644 --- a/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst +++ b/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst @@ -2,7 +2,7 @@ SuperDARN Polar Cap Potential ============================= -.. contents:: The tiny table of contents +.. contents:: Table of contents The Super Dual Auroral Radar Network (SuperDARN) is an international network of High Frequency coherent scatter radars. A map of the fields of view of the radars @@ -22,7 +22,8 @@ As ionospheric irregularities are dragged in the large scale convection at high allows to infer the velocity of the ambient plasma with respect to the sounded direction and gate. -**References** +References +~~~~~~~~~~ https://www.sciencedirect.com/science/article/abs/pii/S136468260600263X @@ -48,48 +49,51 @@ https://doi.org/10.1002/2018JA025280 and Functional Approximations, J. Geophys. Res., Space Physics, 119(9), 7501-7521 (2014). https://doi.org/10.1002/2014JA020264 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_cpcp_superdarn_datacube - -**publisher:** INAF - -**alphanumeric_code:** 31 - -**id_tmp:** 71 - -**short_name:** SuperDARN CPCP - -**identifier:** aspis://inaf/cpcp_superdarn_datacube - -**dynamic:** static - -**size:** 200MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1515672 - -**time_start:** 2015-06-21 - -**time_stop:** 2017-09-11 - -**spatial:** IONO - -**messenger:** electrons, - -**spectral_min:** 0 - -**spectral_max:** 1 - -**spectral_units:** dimensionless - -**observable:** IMF,GEOINDEX - -**latest update:** 2024-04-04 01:53:25 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_cpcp_superdarn_datacube + * - **publisher:** + - INAF + * - **alph_code:** + - 31 + * - **id_tmp:** + - 71 + * - **short_name:** + - SuperDARN CPCP + * - **identifier:** + - aspis://inaf/cpcp_superdarn_datacube + * - **dynamic:** + - static + * - **size:** + - 200MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1515672 + * - **time_start:** + - 2015-06-21 + * - **time_stop:** + - 2017-09-11 + * - **spatial:** + - IONO + * - **messenger:** + - electrons, + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - dimensionless + * - **observable:** + - IMF,GEOINDEX + * - **latest update:** + - 2024-04-04 01:53:25 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_data_solopas_timeseries.rst b/docs/source/products/data/inaf_data_solopas_timeseries.rst index cb30f8d..b7d8d36 100644 --- a/docs/source/products/data/inaf_data_solopas_timeseries.rst +++ b/docs/source/products/data/inaf_data_solopas_timeseries.rst @@ -2,14 +2,15 @@ INAF-IAPS Solar Orbiter-PAS data ================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The product contains density N, speed vector V, pressure tensor P, temperature components (Tx, Ty, Tz), and the velocity of the satellite V_solo, computed using the data collected by the Proton-Alpha Sensor (PAS) onboard Solar Orbiter. PAS measures the 3D distribution functions of the dominant ions of the solar wind, from 200 eV to 20 KeV, without mass and charge selection. In practice, this concerns mostly the proton and alfa populations (unseparated). At full resolution, PAS collects the 3D ion distribution function in about 1 second, even though the moments have a cadence of 4 seconds, while in “snapshot” mode the phase space sampling is reduced, allowing a greater cadence for the moments. Data is hosted on http://soar.esac.esa.int/soar/ -**References** +References +~~~~~~~~~~ R. D’Amicis et al, Astronomy &Astrophysics 656, A21 (2021) @@ -19,48 +20,51 @@ D. Perrone et al, Astronomy &Astrophysics 668, A189 (2022) R. De Marco et al, Astronomy &Astrophysics, 669, A108 (2023) -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_data_solopas_timeseries - -**publisher:** INAF-IAPS, Plasma & Space Weather Group - -**alphanumeric_code:** 14 - -**id_tmp:** 72 - -**short_name:** SolO-PAS_data - -**identifier:** aspis://inaf/data_solopas_timeseries - -**dynamic:** a file each day (file size between 3 and 4 Mb). As a general rule, one month of data is uploaded each month, generally relating to 3 months before the upload date - -**size:** 2GB - -**format:** dsv - -**type:** timeseries - -**records_number:** 38653 - -**time_start:** 2020-07-06 - -**time_stop:** 2022-01-31 - -**spatial:** IP - -**messenger:** Protons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** SW,SEP - -**latest update:** 2024-04-04 01:54:59 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_data_solopas_timeseries + * - **publisher:** + - INAF-IAPS, Plasma & Space Weather Group + * - **alph_code:** + - 14 + * - **id_tmp:** + - 72 + * - **short_name:** + - SolO-PAS_data + * - **identifier:** + - aspis://inaf/data_solopas_timeseries + * - **dynamic:** + - a file each day (file size between 3 and 4 Mb). As a general rule, one month of data is uploaded each month, generally relating to 3 months before the upload date + * - **size:** + - 2GB + * - **format:** + - dsv + * - **type:** + - timeseries + * - **records_number:** + - 38653 + * - **time_start:** + - 2020-07-06 + * - **time_stop:** + - 2022-01-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - SW,SEP + * - **latest update:** + - 2024-04-04 01:54:59 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst b/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst index ece0c56..3542b5c 100644 --- a/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst +++ b/docs/source/products/data/inaf_flux1h_svirco_timeseries.rst @@ -2,56 +2,60 @@ SVIRCO Observatory - the Rome neutron monitor ============================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 1h. Average intensity of January-February 1997 = 100% -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_flux1h_svirco_timeseries - -**publisher:** INAF - -**alphanumeric_code:** 42C - -**id_tmp:** 73 - -**short_name:** flux1h_SVIRCO - -**identifier:** inaf_flux1h_svirco_timeseries - -**dynamic:** Data collection grows in time. - -**size:** 13MB - -**format:** CSV - -**type:** timeseries - -**records_number:** 479976 - -**time_start:** 1966-04-01 - -**time_stop:** 2020-12-31 - -**spatial:** GROUND - -**messenger:** Nucleons - -**spectral_min:** 6.3 - -**spectral_max:** 9999 - -**spectral_units:** GeV - -**observable:** GLE,GCR - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_flux1h_svirco_timeseries + * - **publisher:** + - INAF + * - **alph_code:** + - 42C + * - **id_tmp:** + - 73 + * - **short_name:** + - flux1h_SVIRCO + * - **identifier:** + - inaf_flux1h_svirco_timeseries + * - **dynamic:** + - Data collection grows in time. + * - **size:** + - 13MB + * - **format:** + - CSV + * - **type:** + - timeseries + * - **records_number:** + - 479976 + * - **time_start:** + - 1966-04-01 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - GROUND + * - **messenger:** + - Nucleons + * - **spectral_min:** + - 6.3 + * - **spectral_max:** + - 9999 + * - **spectral_units:** + - GeV + * - **observable:** + - GLE,GCR + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst b/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst index 3248096..8e7960b 100644 --- a/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst +++ b/docs/source/products/data/inaf_flux5m_svirco_timeseries.rst @@ -2,56 +2,60 @@ SVIRCO Obser vatory - the Rome neutron monitor ============================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Intensity in percent of cosmic ray secondary nucleonic component of Rome neutron monitor. Data corrected for pressure with barometric coefficient variable with solar cycle and corrected for efficiency changes. Resolution: 5min Average intensity of January-February 1997 = 100% -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_flux5m_svirco_timeseries - -**publisher:** INAF - -**alphanumeric_code:** 42B - -**id_tmp:** 74 - -**short_name:** flux5m_SVIRCO - -**identifier:** inaf_flux5m_svirco_timeseries - -**dynamic:** Data collection grows in time. - -**size:** 80MB - -**format:** CSV - -**type:** timeseries - -**records_number:** 2007072 - -**time_start:** 1997-05-21 - -**time_stop:** 2017-01-01 - -**spatial:** GROUND - -**messenger:** Neutrons - -**spectral_min:** 6.3 - -**spectral_max:** 9999 - -**spectral_units:** GeV - -**observable:** GLE,GCR - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_flux5m_svirco_timeseries + * - **publisher:** + - INAF + * - **alph_code:** + - 42B + * - **id_tmp:** + - 74 + * - **short_name:** + - flux5m_SVIRCO + * - **identifier:** + - inaf_flux5m_svirco_timeseries + * - **dynamic:** + - Data collection grows in time. + * - **size:** + - 80MB + * - **format:** + - CSV + * - **type:** + - timeseries + * - **records_number:** + - 2007072 + * - **time_start:** + - 1997-05-21 + * - **time_stop:** + - 2017-01-01 + * - **spatial:** + - GROUND + * - **messenger:** + - Neutrons + * - **spectral_min:** + - 6.3 + * - **spectral_max:** + - 9999 + * - **spectral_units:** + - GeV + * - **observable:** + - GLE,GCR + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_gsmaps_datacube.rst b/docs/source/products/data/inaf_gsmaps_datacube.rst index 60bd736..1867a25 100644 --- a/docs/source/products/data/inaf_gsmaps_datacube.rst +++ b/docs/source/products/data/inaf_gsmaps_datacube.rst @@ -2,56 +2,60 @@ IAPS Grad-Shafranov Reconstruction of Magnetic Clouds ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Quasi 3-d magnetic field maps of magnetic field configuration within magnetic clouds for geoeffective target SWE events. Such maps will be estimated through the Grad-Shafranov reconstruction from single-spacecraft plasma and magnetic field data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_gsmaps_datacube - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 25 - -**id_tmp:** 96 - -**short_name:** gsmaps-cubes - -**identifier:** aspis://inaf/gsmaps_datacube - -**dynamic:** static - -**size:** 300kB - -**format:** nc - -**type:** spectrum - -**records_number:** 3 - -**time_start:** 1997-01-01 - -**time_stop:** 2022-01-01 - -**spatial:** IP - -**messenger:** Magnetic field,Magnetic vector potential,Flux rope coordinates - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** phys.magField,phys.potential,phys.size - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_gsmaps_datacube + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 25 + * - **id_tmp:** + - 96 + * - **short_name:** + - gsmaps-cubes + * - **identifier:** + - aspis://inaf/gsmaps_datacube + * - **dynamic:** + - static + * - **size:** + - 300kB + * - **format:** + - nc + * - **type:** + - spectrum + * - **records_number:** + - 3 + * - **time_start:** + - 1997-01-01 + * - **time_stop:** + - 2022-01-01 + * - **spatial:** + - IP + * - **messenger:** + - Magnetic field,Magnetic vector potential,Flux rope coordinates + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - phys.magField,phys.potential,phys.size + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_m2flare_tableset.rst b/docs/source/products/data/inaf_m2flare_tableset.rst index 5511286..b7baee1 100644 --- a/docs/source/products/data/inaf_m2flare_tableset.rst +++ b/docs/source/products/data/inaf_m2flare_tableset.rst @@ -2,56 +2,60 @@ IAPS ≥M2 SXR Flare Catalogue ============================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The catalogue will contain the > M2 Soft X- Ray (SXR) flares from 1995 to 2017. The columns in the table are defined as follows: (1) event number (2) date of the SXR flare (3) peak time of SXR flare (4) peak SXR classification (saturated events flagged with an S in which case (3) refers to the onset of saturation), (5) flare location, (6) time-integrated SXR intensity (nominally between the 1/3 power points on rise and fall), (7) time-integrated 1 MHz Wind/WAVES intensity from 10 minutes before the onset of integration for the SXR burst to 10 minutes after the SXR burst peak, (8) Waves frequency used. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_m2flare_tableset - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 7 - -**id_tmp:** 75 - -**short_name:** IAPS-M2SXR - -**identifier:** aspis://inaf/m2flare_tableset - -**dynamic:** static - -**size:** 100kB - -**format:** xlsx - -**type:** tableset - -**records_number:** 1040 - -**time_start:** 1995-01-01 - -**time_stop:** 2017-05-03 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** phys.flux - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_m2flare_tableset + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 7 + * - **id_tmp:** + - 75 + * - **short_name:** + - IAPS-M2SXR + * - **identifier:** + - aspis://inaf/m2flare_tableset + * - **dynamic:** + - static + * - **size:** + - 100kB + * - **format:** + - xlsx + * - **type:** + - tableset + * - **records_number:** + - 1040 + * - **time_start:** + - 1995-01-01 + * - **time_stop:** + - 2017-05-03 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - phys.flux + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_na_mercexo_image.rst b/docs/source/products/data/inaf_na_mercexo_image.rst index 3c2ad68..c580787 100644 --- a/docs/source/products/data/inaf_na_mercexo_image.rst +++ b/docs/source/products/data/inaf_na_mercexo_image.rst @@ -2,11 +2,12 @@ INAF-bidimensional maps of Mercury Na exosphere =============================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Dataset of observations of Mercury's exosphere in the sodium D lines. Data are taken from the ground-based solar telescope THEMIS (years 2009-2013). They have been produced in both D1 and D2 lines (when both available) and converted into bi-dimensional maps of Rayleigh emission. Estimation of the “seeing” parameter is included in the jpeg files. Here the original fits files are given too for the whole data base (2007-2014), and it may be expanded to the most recent data from 2021 and 2022 (TBC). Data can be provided both uncalibrated and/or calibrated (TBD). -**References** +References +~~~~~~~~~~ Leblanc, F., Doressoundiram, A., Schneider, N., Mangano, V., López Ariste, A., Lemen, C., Gelly, B., Barbieri, C. and Cremonese, G., 2008. High latitude peaks in Mercury's sodium exosphere: Spectral signature using THEMIS solar telescope. Geophysical Research Letters, 35(18). @@ -20,48 +21,51 @@ Massetti, S., Mangano, V., Milillo, A., Mura, A., Orsini, S. and Plainaki, C., 2 Orsini, S., Mangano, V., Milillo, A., Plainaki, C., Mura, A., Raines, J.M., De Angelis, E., Rispoli, R., Lazzarotto, F. and Aronica, A., 2018. Mercury sodium exospheric emission as a proxy for solar perturbations transit. Scientific reports, 8(1), p.928. -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_na_mercexo_image - -**publisher:** Valeria Mangano, INAF-IAPS - -**alphanumeric_code:** 57 - -**id_tmp:** 76 - -**short_name:** Merc_exos_Na_fts - -**identifier:** aspis://inaf/na_mercexo_image - -**dynamic:** period 2009-2013 is static, but if we decide to include also most recent data, it will grow in time. - -**size:** 1GB - -**format:** fits - -**type:** image - -**records_number:** 7 - -**time_start:** 2009-04-17 - -**time_stop:** 2013-05-25 - -**spatial:** Mercury - -**messenger:** photons - -**spectral_min:** 5890 - -**spectral_max:** 5896 - -**spectral_units:** Angstrom - -**observable:** IMF,SW,CME - -**latest update:** 2024-04-04 01:59:34 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_na_mercexo_image + * - **publisher:** + - Valeria Mangano, INAF-IAPS + * - **alph_code:** + - 57 + * - **id_tmp:** + - 76 + * - **short_name:** + - Merc_exos_Na_fts + * - **identifier:** + - aspis://inaf/na_mercexo_image + * - **dynamic:** + - period 2009-2013 is static, but if we decide to include also most recent data, it will grow in time. + * - **size:** + - 1GB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 7 + * - **time_start:** + - 2009-04-17 + * - **time_stop:** + - 2013-05-25 + * - **spatial:** + - Mercury + * - **messenger:** + - photons + * - **spectral_min:** + - 5890 + * - **spectral_max:** + - 5896 + * - **spectral_units:** + - Angstrom + * - **observable:** + - IMF,SW,CME + * - **latest update:** + - 2024-04-04 01:59:34 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_s1sep_tableset.rst b/docs/source/products/data/inaf_s1sep_tableset.rst index 1e164d2..f60fb57 100644 --- a/docs/source/products/data/inaf_s1sep_tableset.rst +++ b/docs/source/products/data/inaf_s1sep_tableset.rst @@ -2,56 +2,60 @@ IAPS S1 SEP events Catalogue ============================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The catalogue contains SEP events observed at the Earth of class S1, i.e. with flux in the range [10, 100) pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux >= 100 pfu at > 10 MeV are listed in the companion table S2 SEP Catalogue. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_s1sep_tableset - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 16A - -**id_tmp:** 77 - -**short_name:** IAPS-S1 SEP events - -**identifier:** aspis://inaf/s1sep_tableset - -**dynamic:** static - -**size:** 100kB - -**format:** csv - -**type:** tableset - -**records_number:** 68 - -**time_start:** 1995-01-01 - -**time_stop:** 2014-09-10 - -**spatial:** Earth - -**messenger:** Protons,Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** flare,CME,SEP - -**latest update:** 2024-03-28 05:08:05 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_s1sep_tableset + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 16A + * - **id_tmp:** + - 77 + * - **short_name:** + - IAPS-S1 SEP events + * - **identifier:** + - aspis://inaf/s1sep_tableset + * - **dynamic:** + - static + * - **size:** + - 100kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 68 + * - **time_start:** + - 1995-01-01 + * - **time_stop:** + - 2014-09-10 + * - **spatial:** + - Earth + * - **messenger:** + - Protons,Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - flare,CME,SEP + * - **latest update:** + - 2024-03-28 05:08:05 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_s2sep_tableset.rst b/docs/source/products/data/inaf_s2sep_tableset.rst index 717b419..0963e5a 100644 --- a/docs/source/products/data/inaf_s2sep_tableset.rst +++ b/docs/source/products/data/inaf_s2sep_tableset.rst @@ -2,56 +2,60 @@ IAPS S2 SEP events Catalogue ============================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The catalogue contains SEP events observed at the Earth of class S2, i.e. with flux >100 pfu, at >10 MeV from 1995 and their properties (onset, peak flux, fluence) as well as features of the associated flare (peak time, class, location), CME (lift off, position, angle width, speed) and radio burst (occurrence of type II or IV). The SEP events having flux in the interval [10, 100) pfu at > 10 MeV are listed in the companion table S1 SEP Catalogue. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_s2sep_tableset - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 16B - -**id_tmp:** 78 - -**short_name:** IAPS-S2 SEP events - -**identifier:** aspis://inaf/s1sep_tableset - -**dynamic:** static - -**size:** 100kB - -**format:** csv - -**type:** tableset - -**records_number:** 60 - -**time_start:** 1995-01-01 - -**time_stop:** 2014-09-10 - -**spatial:** Earth - -**messenger:** Protons,Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** flare,CME,SEP - -**latest update:** 2024-03-28 05:08:06 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_s2sep_tableset + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 16B + * - **id_tmp:** + - 78 + * - **short_name:** + - IAPS-S2 SEP events + * - **identifier:** + - aspis://inaf/s1sep_tableset + * - **dynamic:** + - static + * - **size:** + - 100kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 60 + * - **time_start:** + - 1995-01-01 + * - **time_stop:** + - 2014-09-10 + * - **spatial:** + - Earth + * - **messenger:** + - Protons,Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - flare,CME,SEP + * - **latest update:** + - 2024-03-28 05:08:06 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_tps_datacube.rst b/docs/source/products/data/inaf_tps_datacube.rst index 8e6184b..7777305 100644 --- a/docs/source/products/data/inaf_tps_datacube.rst +++ b/docs/source/products/data/inaf_tps_datacube.rst @@ -2,56 +2,60 @@ IAPS Test Particle Simulation on Magnetic Clouds ================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents Galactic cosmic ray intensity variations associated to the passage of magnetic clouds. The particle intensity variation is estimated through a dedicated full-orbit test-particle simulation. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_tps_datacube - -**publisher:** INAF - Istituto di Astrofisica e Planetologia Spaziali - -**alphanumeric_code:** 51 - -**id_tmp:** 97 - -**short_name:** IAPS-TPS - -**identifier:** aspis://inaf/tps_datacube - -**dynamic:** static - -**size:** 300kB - -**format:** nc - -**type:** spectrum - -**records_number:** 3 - -**time_start:** 1997-01-01 - -**time_stop:** 2022-01-01 - -**spatial:** Interplanetary Space (not L1 and Planets),Sun-Earth L1 - -**messenger:** Particle intensity variation - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** phys.flux,phys.particle.proton - -**latest update:** 2024-03-28 05:08:06 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_tps_datacube + * - **publisher:** + - INAF - Istituto di Astrofisica e Planetologia Spaziali + * - **alph_code:** + - 51 + * - **id_tmp:** + - 97 + * - **short_name:** + - IAPS-TPS + * - **identifier:** + - aspis://inaf/tps_datacube + * - **dynamic:** + - static + * - **size:** + - 300kB + * - **format:** + - nc + * - **type:** + - spectrum + * - **records_number:** + - 3 + * - **time_start:** + - 1997-01-01 + * - **time_stop:** + - 2022-01-01 + * - **spatial:** + - Interplanetary Space (not L1 and Planets),Sun-Earth L1 + * - **messenger:** + - Particle intensity variation + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - phys.flux,phys.particle.proton + * - **latest update:** + - 2024-03-28 05:08:06 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_vbcorr_wind_tableset.rst b/docs/source/products/data/inaf_vbcorr_wind_tableset.rst index ad9a0c6..46cb275 100644 --- a/docs/source/products/data/inaf_vbcorr_wind_tableset.rst +++ b/docs/source/products/data/inaf_vbcorr_wind_tableset.rst @@ -2,11 +2,12 @@ IAPS - Wind velocity-magnetic field correlation coefficient data of solar wind streams ====================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The velocity - magnetic field (v-b) correlation coefficient unables to identify Alfvénic solar wind intervals (along with almost constant magnetic field magnitude and proton number density). It is derived as the ratio between the covariance of velocity and magnetic field (in Alfvén units) components and the product of their standard deviations, in a time window ranging between tens of minutes to hours. In principle, this formula should be applied to every component of the velocity (V_i) and magnetic fields (B_i) (with i = R, T, N in RTN coordinate system or i = X, Y, Z in GSE coordinate system). The total correlation coefficient is then derived as the average from the three components. However, for the sake of simplicity, we consider only the N component since more Alfvénic than the other two. -**References** +References +~~~~~~~~~~ D’Amicis et al, GRL, 34, L05108, 2007; Frontiers in Physics, 8, 541, 2020 @@ -16,48 +17,51 @@ D’Amicis et al, A&A, 656, A21, 2021 Tu et al., JGR, 94, 11739, 1989 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** inaf_vbcorr_wind_tableset - -**publisher:** INAF-IAPS, Fisica dei Plasmi Spaziali e Space Weather - -**alphanumeric_code:** 24C - -**id_tmp:** 98 - -**short_name:** wind_v-b_corr - -**identifier:** aspis://inaf/vbcorr_wind_tableset - -**dynamic:** static - -**size:** 35MB - -**format:** csv - -**type:** tableset - -**records_number:** 538 - -**time_start:** 1998-10-01 - -**time_stop:** 2022-05-06 - -**spatial:** L1 - -**messenger:** protons - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - - -**observable:** SW - -**latest update:** 2024-04-04 02:05:02 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - inaf_vbcorr_wind_tableset + * - **publisher:** + - INAF-IAPS, Fisica dei Plasmi Spaziali e Space Weather + * - **alph_code:** + - 24C + * - **id_tmp:** + - 98 + * - **short_name:** + - wind_v-b_corr + * - **identifier:** + - aspis://inaf/vbcorr_wind_tableset + * - **dynamic:** + - static + * - **size:** + - 35MB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 538 + * - **time_start:** + - 1998-10-01 + * - **time_stop:** + - 2022-05-06 + * - **spatial:** + - L1 + * - **messenger:** + - protons + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - - + * - **observable:** + - SW + * - **latest update:** + - 2024-04-04 02:05:02 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_cses_hepd_spectrum.rst b/docs/source/products/data/infn_cses_hepd_spectrum.rst index c52aa74..101557c 100644 --- a/docs/source/products/data/infn_cses_hepd_spectrum.rst +++ b/docs/source/products/data/infn_cses_hepd_spectrum.rst @@ -2,56 +2,60 @@ HEPD-01 time-integrated proton spectrum during the Ground-Level Enhancement of October 28, 2021 =============================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Time-integrated spectrum of solar protons measured by the HEPD-01 detector from space during the Ground-Level Enhancement of October 28, 2021 -**References** +References +~~~~~~~~~~ https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2022SW003191 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_cses_hepd_spectrum - -**publisher:** not available in DBF - -**alphanumeric_code:** 44C - -**id_tmp:** 106 - -**short_name:** HEPD-proton - -**identifier:** aspis://infn/infn_cses_hepd_spectrum - -**dynamic:** - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 1 - -**time_start:** 2021-10-28 - -**time_stop:** 2021-11-03 - -**spatial:** GEOMAG - -**messenger:** protons - -**spectral_min:** 55 - -**spectral_max:** 250 - -**spectral_units:** MeV - -**observable:** GLE,flare,SEP,GCR,CME - -**latest update:** 2024-04-04 02:08:35 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_cses_hepd_spectrum + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 44C + * - **id_tmp:** + - 106 + * - **short_name:** + - HEPD-proton + * - **identifier:** + - aspis://infn/infn_cses_hepd_spectrum + * - **dynamic:** + - + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 1 + * - **time_start:** + - 2021-10-28 + * - **time_stop:** + - 2021-11-03 + * - **spatial:** + - GEOMAG + * - **messenger:** + - protons + * - **spectral_min:** + - 55 + * - **spectral_max:** + - 250 + * - **spectral_units:** + - MeV + * - **observable:** + - GLE,flare,SEP,GCR,CME + * - **latest update:** + - 2024-04-04 02:08:35 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_iss_ams_flux_timeseries.rst b/docs/source/products/data/infn_iss_ams_flux_timeseries.rst index fc1c94f..9fc615e 100644 --- a/docs/source/products/data/infn_iss_ams_flux_timeseries.rst +++ b/docs/source/products/data/infn_iss_ams_flux_timeseries.rst @@ -2,56 +2,60 @@ INFN AMS daily proton time dependent fluxes =========================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Daily proton fluxes in cosmic rays were measured with the Alpha Magnetic Spectrometer aboard the International Space Station, from May 20, 2011 to October 29, 2019 (a total of 2824 days or 114 Bartels rotations) in the rigidity interval from 1 to 100 GV, based on 5.5×10^9 protons collected. Several Forbush decreases were also observed during the whole period, in connection with transient magnetic perturbations. The product provides these data as time-profiles from May 20, 2011 to October 29 2019 as a function of rigidity. In particular the daily proton fluxes are measured in 30 bins from 1.00 to 100 GV. The errors include statistics, time-dependent systematic errors and the total systematic error. -**References** +References +~~~~~~~~~~ https://doi.org/10.1103/PhysRevLett.127.271102 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_iss_ams_flux_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 50A - -**id_tmp:** 89 - -**short_name:** AMS_daily_H - -**identifier:** aspis:///infn/ams_protons - -**dynamic:** static - -**size:** 4.1MB - -**format:** csv - -**type:** timeseries - -**records_number:** 83757 - -**time_start:** 2011-05-20 - -**time_stop:** 2019-10-29 - -**spatial:** GEOMAG - -**messenger:** Protons - -**spectral_min:** 1 - -**spectral_max:** 100 - -**spectral_units:** GV - -**observable:** GCR - -**latest update:** 2024-04-04 02:10:23 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_iss_ams_flux_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 50A + * - **id_tmp:** + - 89 + * - **short_name:** + - AMS_daily_H + * - **identifier:** + - aspis:///infn/ams_protons + * - **dynamic:** + - static + * - **size:** + - 4.1MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 83757 + * - **time_start:** + - 2011-05-20 + * - **time_stop:** + - 2019-10-29 + * - **spatial:** + - GEOMAG + * - **messenger:** + - Protons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - GV + * - **observable:** + - GCR + * - **latest update:** + - 2024-04-04 02:10:23 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_pamela_flux_timeseries.rst b/docs/source/products/data/infn_pamela_flux_timeseries.rst index 6573397..1d9f643 100644 --- a/docs/source/products/data/infn_pamela_flux_timeseries.rst +++ b/docs/source/products/data/infn_pamela_flux_timeseries.rst @@ -2,56 +2,60 @@ PAMELA time-profiles of protons during 4 Forbush Decreases ========================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Time-profiles of galactic cosmic-ray protons measured by the PAMELA detector in space during 4 Forbush Decreases from March 2012 to June 2015 in various rigidity intervals. Each profile is scaled for a suitable period of quiet Sun, estimated about 10 days before each Forbush Decrease -**References** +References +~~~~~~~~~~ https://iopscience.iop.org/article/10.3847/1538-4357/aaa0c8 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_pamela_flux_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 50B - -**id_tmp:** 90 - -**short_name:** PAMELA-proton - -**identifier:** aspis://INFN-PAMELA/proton - -**dynamic:** Data collected starts on March 1, 2012 and is increasing with a daily resolution up until July 17, 2015 - -**size:** 200kB - -**format:** csv - -**type:** timeseries - -**records_number:** 2394 - -**time_start:** 2012-03-01 - -**time_stop:** 2015-07-17 - -**spatial:** GEOMAG - -**messenger:** protons - -**spectral_min:** 0.85 - -**spectral_max:** 8.68 - -**spectral_units:** GV - -**observable:** GCR - -**latest update:** 2024-04-04 02:12:29 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_pamela_flux_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 50B + * - **id_tmp:** + - 90 + * - **short_name:** + - PAMELA-proton + * - **identifier:** + - aspis://INFN-PAMELA/proton + * - **dynamic:** + - Data collected starts on March 1, 2012 and is increasing with a daily resolution up until July 17, 2015 + * - **size:** + - 200kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 2394 + * - **time_start:** + - 2012-03-01 + * - **time_stop:** + - 2015-07-17 + * - **spatial:** + - GEOMAG + * - **messenger:** + - protons + * - **spectral_min:** + - 0.85 + * - **spectral_max:** + - 8.68 + * - **spectral_units:** + - GV + * - **observable:** + - GCR + * - **latest update:** + - 2024-04-04 02:12:29 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_saandose_samadha_timeseries.rst b/docs/source/products/data/infn_saandose_samadha_timeseries.rst index b46635f..036958f 100644 --- a/docs/source/products/data/infn_saandose_samadha_timeseries.rst +++ b/docs/source/products/data/infn_saandose_samadha_timeseries.rst @@ -2,56 +2,60 @@ SAMADHA neutron dose rate at Mount Chacaltaya ============================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) is an INFN project aimed to monitor the neutron dose rate due to cosmic rays at the Chacaltaya Station (Bolivia, 5200 m) inside the South Atlantic Anomaly region, to study possible correlation between space weather events and dose rate at the ground, considering the proximity of the Van Allen Belts to the Earth's surface in the SAA region. -**References** +References +~~~~~~~~~~ http://samadha.to.infn.it -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_saandose_samadha_timeseries - -**publisher:** SAMADHA - -**alphanumeric_code:** 75A - -**id_tmp:** 99 - -**short_name:** SAA_Ndose - -**identifier:** aspis://infn/saandose_samadha_timeseries - -**dynamic:** one dataset per day (50 kB/day) - -**size:** 50kB - -**format:** text - -**type:** tableset - -**records_number:** 2358 - -**time_start:** 2022-10-01 - -**time_stop:** 2023-12-31 - -**spatial:** Earth's Ground - -**messenger:** neutrons - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** - -**latest update:** 2024-04-04 02:14:12 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_saandose_samadha_timeseries + * - **publisher:** + - SAMADHA + * - **alph_code:** + - 75A + * - **id_tmp:** + - 99 + * - **short_name:** + - SAA_Ndose + * - **identifier:** + - aspis://infn/saandose_samadha_timeseries + * - **dynamic:** + - one dataset per day (50 kB/day) + * - **size:** + - 50kB + * - **format:** + - text + * - **type:** + - tableset + * - **records_number:** + - 2358 + * - **time_start:** + - 2022-10-01 + * - **time_stop:** + - 2023-12-31 + * - **spatial:** + - Earth's Ground + * - **messenger:** + - neutrons + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - + * - **latest update:** + - 2024-04-04 02:14:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_tgndose_samadha_timeseries.rst b/docs/source/products/data/infn_tgndose_samadha_timeseries.rst index 674c0e3..e1a2431 100644 --- a/docs/source/products/data/infn_tgndose_samadha_timeseries.rst +++ b/docs/source/products/data/infn_tgndose_samadha_timeseries.rst @@ -2,56 +2,60 @@ SAMADHA neutron dose rate at Testa Grigia ========================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Monitoring of the neutron dose rate due to cosmic rays at the Testa Grigia Station (3480 m, Cervinia, Italy), to study possible correlation between space weather events and dose rate at the ground. This measurement is part of the INFN project SAMADHA (South Atlantic Magnetic Anomaly Dosimetry at High Altitude) aimed to monitor the neutron dose inside the South Atlantic Anomaly (SAA) region in Bolivia. The data taken at Testa Grigia are a term of comparison for those collected in the SAA region. -**References** +References +~~~~~~~~~~ http://samadha.to.infn.it -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_tgndose_samadha_timeseries - -**publisher:** samadha - -**alphanumeric_code:** 75B - -**id_tmp:** 79 - -**short_name:** TG_Ndose - -**identifier:** aspis://infn/tgndose_samadha_timeseries - -**dynamic:** one dataset per day (50 kB/day) - -**size:** 50kB - -**format:** text - -**type:** timeseries - -**records_number:** 2835 - -**time_start:** 2021-09-01 - -**time_stop:** 2023-12-31 - -**spatial:** Earth's Ground - -**messenger:** neutrons - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** - -**latest update:** 2024-04-04 02:15:39 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_tgndose_samadha_timeseries + * - **publisher:** + - samadha + * - **alph_code:** + - 75B + * - **id_tmp:** + - 79 + * - **short_name:** + - TG_Ndose + * - **identifier:** + - aspis://infn/tgndose_samadha_timeseries + * - **dynamic:** + - one dataset per day (50 kB/day) + * - **size:** + - 50kB + * - **format:** + - text + * - **type:** + - timeseries + * - **records_number:** + - 2835 + * - **time_start:** + - 2021-09-01 + * - **time_stop:** + - 2023-12-31 + * - **spatial:** + - Earth's Ground + * - **messenger:** + - neutrons + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - + * - **latest update:** + - 2024-04-04 02:15:39 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_aqu_timeseries.rst b/docs/source/products/data/ingv_alert_aqu_timeseries.rst index 47abb7a..03fd83b 100644 --- a/docs/source/products/data/ingv_alert_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_alert_aqu_timeseries.rst @@ -2,59 +2,63 @@ INGV geomagnetic data, GIC indices and alert: L'Aquila ====================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents From both components of GIC index for L'Aquila observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) This tableset contains a set of data corresponding to products with ids 8, 47 and 48. In detail it contains the definitive values of the X,Y and Z components (in NEC coordinates) and of total intensity F of the geomagnetic field recorded at ground magnetic observatories managed by INGV. Besides, it contains the values of the GicX and GicY indices calculated from the Y and X components, respectively. To finish it contains values of the risk (i.e. alertX and alertY) , corresponding to the estimated values of the GicX and GicY indices. Data sampling is of 1-minute. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_aqu_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 48A - -**id_tmp:** 80 - -**short_name:** INGV_AQU_alert - -**identifier:** aspis:///ingv/INGV_AQU_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-04-04 02:27:54 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_aqu_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 48A + * - **id_tmp:** + - 80 + * - **short_name:** + - INGV_AQU_alert + * - **identifier:** + - aspis:///ingv/INGV_AQU_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-04-04 02:27:54 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_cts_timeseries.rst b/docs/source/products/data/ingv_alert_cts_timeseries.rst index 9c7018c..fe23a67 100644 --- a/docs/source/products/data/ingv_alert_cts_timeseries.rst +++ b/docs/source/products/data/ingv_alert_cts_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Castello Tesino ============================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents From both components of GIC index for Castello Tesino observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_cts_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 48B - -**id_tmp:** 81 - -**short_name:** INGV_CTS_alert - -**identifier:** aspis:///ingv/INGV_CTS_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:07 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_cts_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 48B + * - **id_tmp:** + - 81 + * - **short_name:** + - INGV_CTS_alert + * - **identifier:** + - aspis:///ingv/INGV_CTS_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:07 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_dur_timeseries.rst b/docs/source/products/data/ingv_alert_dur_timeseries.rst index 76388d4..3f66753 100644 --- a/docs/source/products/data/ingv_alert_dur_timeseries.rst +++ b/docs/source/products/data/ingv_alert_dur_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Duronia ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents From both components of GIC index for Duronia observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_dur_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 48C - -**id_tmp:** 82 - -**short_name:** INGV_DUR_alert - -**identifier:** aspis:///ingv/INGV_DUR_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:07 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_dur_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 48C + * - **id_tmp:** + - 82 + * - **short_name:** + - INGV_DUR_alert + * - **identifier:** + - aspis:///ingv/INGV_DUR_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:07 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_int_timeseries.rst b/docs/source/products/data/ingv_alert_int_timeseries.rst index 129b61e..f3d991b 100644 --- a/docs/source/products/data/ingv_alert_int_timeseries.rst +++ b/docs/source/products/data/ingv_alert_int_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories ============================================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_int_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 48E - -**id_tmp:** 88 - -**short_name:** INGV_INT_alert - -**identifier:** aspis:///ingv/INGV_INT_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:07 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_int_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 48E + * - **id_tmp:** + - 88 + * - **short_name:** + - INGV_INT_alert + * - **identifier:** + - aspis:///ingv/INGV_INT_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:07 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_lmp_timeseries.rst b/docs/source/products/data/ingv_alert_lmp_timeseries.rst index a13abd8..c2feed3 100644 --- a/docs/source/products/data/ingv_alert_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_alert_lmp_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Lampedusa ======================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents From both components of GIC index for Lampedusa observatory it is possible to calculate an alert based on a risk scale that associates GIC index to the probability to observe damages to the power network. At present sample files are not available since so far this kind of computation has been performed all within a peculiar software environment (IgorPro), anyway if data were stored in txt files they would be arranged in 3-columns (1-minute data) -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_lmp_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 48D - -**id_tmp:** 83 - -**short_name:** INGV_LMP_alert - -**identifier:** aspis:///ingv/INGV_LMP_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:08 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_lmp_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 48D + * - **id_tmp:** + - 83 + * - **short_name:** + - INGV_LMP_alert + * - **identifier:** + - aspis:///ingv/INGV_LMP_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:08 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_wdc_timeseries.rst b/docs/source/products/data/ingv_alert_wdc_timeseries.rst index f6a5db5..1675fc8 100644 --- a/docs/source/products/data/ingv_alert_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_alert_wdc_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories ======================================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_wdc_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 48F - -**id_tmp:** 48 - -**short_name:** INGV_WDC_alert - -**identifier:** aspis:///ingv/INGV_WDC_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:08 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_wdc_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 48F + * - **id_tmp:** + - 48 + * - **short_name:** + - INGV_WDC_alert + * - **identifier:** + - aspis:///ingv/INGV_WDC_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:08 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst b/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst index 80a2ba5..ac14a8b 100644 --- a/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst @@ -2,56 +2,60 @@ Autoscaled data Bahia Blanca Ionosonde ====================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Bahia Blanca -**References** +References +~~~~~~~~~~ http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_autoiono_bbla_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 12A - -**id_tmp:** 1 - -**short_name:** AutoIonoBBla - -**identifier:** aspis://ingv/autoiono_bbla_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Bahia Blanca AIS-INGV ionosonde started sounding in September 2016, this is why in the Number of datasets field you will find the number 7 (years 2016-2022). This collection grows in real time, because th - -**size:** 15MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1558 - -**time_start:** 2016-09-26 - -**time_stop:** 2022-04-14 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-04-04 05:53:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_autoiono_bbla_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 12A + * - **id_tmp:** + - 1 + * - **short_name:** + - AutoIonoBBla + * - **identifier:** + - aspis://ingv/autoiono_bbla_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Bahia Blanca AIS-INGV ionosonde started sounding in September 2016, this is why in the Number of datasets field you will find the number 7 (years 2016-2022). This collection grows in real time, because th + * - **size:** + - 15MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1558 + * - **time_start:** + - 2016-09-26 + * - **time_stop:** + - 2022-04-14 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-04-04 05:53:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst b/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst index 59b1916..a8a85d6 100644 --- a/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_gibi_timeseries.rst @@ -2,56 +2,60 @@ Autoscaled data Gibilmanna Ionosonde ==================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna -**References** +References +~~~~~~~~~~ http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_autoiono_gibi_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 12B - -**id_tmp:** 2 - -**short_name:** AutoIonoGibi - -**identifier:** aspis://ingv/autoiono_gibi_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Gibilmanna AIS-INGV ionosonde started sounding in November 2002, this is why in the Number of datasets field you will find the number 21 (years 2002-2022). This collection grows in real time, because the - -**size:** 15MB - -**format:** csv - -**type:** timeseries - -**records_number:** 5793 - -**time_start:** 2002-11-26 - -**time_stop:** 2022-04-14 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-04-04 05:55:21 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_autoiono_gibi_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 12B + * - **id_tmp:** + - 2 + * - **short_name:** + - AutoIonoGibi + * - **identifier:** + - aspis://ingv/autoiono_gibi_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Gibilmanna AIS-INGV ionosonde started sounding in November 2002, this is why in the Number of datasets field you will find the number 21 (years 2002-2022). This collection grows in real time, because the + * - **size:** + - 15MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 5793 + * - **time_start:** + - 2002-11-26 + * - **time_stop:** + - 2022-04-14 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-04-04 05:55:21 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_autoiono_rome_timeseries.rst b/docs/source/products/data/ingv_autoiono_rome_timeseries.rst index e31ce5a..287c30e 100644 --- a/docs/source/products/data/ingv_autoiono_rome_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_rome_timeseries.rst @@ -2,56 +2,60 @@ Autoscaled data Rome Ionosonde ============================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Ionospheric parameters (foF2, foF1, foE, ftEs, hmF2, hmE, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Rome -**References** +References +~~~~~~~~~~ http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_autoiono_rome_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 12C - -**id_tmp:** 3 - -**short_name:** AutoIonoRome - -**identifier:** aspis://ingv/autoiono_rome_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Rome AIS-INGV ionosonde started sounding in November 2004, this is why in the Number of datasets field you will find the number 19 (years 2004-2022). This collection grows in real time, because the ionoso - -**size:** 15MB - -**format:** csv - -**type:** timeseries - -**records_number:** 7303 - -**time_start:** 2004-11-25 - -**time_stop:** 2022-04-14 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-04-04 05:56:30 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_autoiono_rome_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 12C + * - **id_tmp:** + - 3 + * - **short_name:** + - AutoIonoRome + * - **identifier:** + - aspis://ingv/autoiono_rome_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Rome AIS-INGV ionosonde started sounding in November 2004, this is why in the Number of datasets field you will find the number 19 (years 2004-2022). This collection grows in real time, because the ionoso + * - **size:** + - 15MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 7303 + * - **time_start:** + - 2004-11-25 + * - **time_stop:** + - 2022-04-14 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-04-04 05:56:30 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst b/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst index bf95bc7..10e5a97 100644 --- a/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst +++ b/docs/source/products/data/ingv_autoiono_tucu_timeseries.rst @@ -2,56 +2,60 @@ Autoscaled data Tucuman Ionosonde ================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Ionospheric parameters (foF2, foF1, ftEs, h'Es, MUF(3000)F2, M(3000)F2) as automatically measured by the AIS-INGV ionosonde installed at the ionospheric station of Tucuman -**References** +References +~~~~~~~~~~ http://eswua.ingv.it/index.php/hf-systems/real-time-vertical-soundings -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_autoiono_tucu_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 12D - -**id_tmp:** 4 - -**short_name:** AutoIonoTucu - -**identifier:** aspis://ingv/autoiono_tucu_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Tucuman AIS-INGV ionosonde started sounding in August 2007, this is why in the Number of datasets field you will find the number 16 (years 2007-2022). This collection grows in real time, because the ionos - -**size:** 15MB - -**format:** csv - -**type:** timeseries - -**records_number:** 6283 - -**time_start:** 2007-08-04 - -**time_stop:** 2022-04-14 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-04-04 05:57:34 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_autoiono_tucu_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 12D + * - **id_tmp:** + - 4 + * - **short_name:** + - AutoIonoTucu + * - **identifier:** + - aspis://ingv/autoiono_tucu_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Tucuman AIS-INGV ionosonde started sounding in August 2007, this is why in the Number of datasets field you will find the number 16 (years 2007-2022). This collection grows in real time, because the ionos + * - **size:** + - 15MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 6283 + * - **time_start:** + - 2007-08-04 + * - **time_stop:** + - 2022-04-14 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-04-04 05:57:34 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_b_swarm_image.rst b/docs/source/products/data/ingv_b_swarm_image.rst index c01e835..3dbf61d 100644 --- a/docs/source/products/data/ingv_b_swarm_image.rst +++ b/docs/source/products/data/ingv_b_swarm_image.rst @@ -2,56 +2,60 @@ Swarm vector magnetic field maps ================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents Vector magnetic field maps in quasi-dipole latitude vs magnetic local time coordinates derived from the Swarm constellation data acquired at 1 second cadence from 1 January 2014 to 31 December 2020. The output consists in nine .jpg or .png files mapping the three components of the vector magnetic field in polar and equatorial projections (3 images for the three components) for each of the 3 satellites of the Swarm constellation. Each map has a size of about 300 kB. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_b_swarm_image - -**publisher:** INGV group - -**alphanumeric_code:** 35B - -**id_tmp:** 62 - -**short_name:** Swarm_B_maps - -**identifier:** aspis://ingv/b_swarm_image - -**dynamic:** static - -**size:** 300kB - -**format:** FITS - -**type:** image - -**records_number:** 24 - -**time_start:** 2014-01-01 - -**time_stop:** 2020-12-31 - -**spatial:** Earth's Ionosphere - -**messenger:** - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** phys.magField - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_b_swarm_image + * - **publisher:** + - INGV group + * - **alph_code:** + - 35B + * - **id_tmp:** + - 62 + * - **short_name:** + - Swarm_B_maps + * - **identifier:** + - aspis://ingv/b_swarm_image + * - **dynamic:** + - static + * - **size:** + - 300kB + * - **format:** + - FITS + * - **type:** + - image + * - **records_number:** + - 24 + * - **time_start:** + - 2014-01-01 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - Earth's Ionosphere + * - **messenger:** + - + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - phys.magField + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_b_swarm_timeseries.rst b/docs/source/products/data/ingv_b_swarm_timeseries.rst index a50603e..4a8ca45 100644 --- a/docs/source/products/data/ingv_b_swarm_timeseries.rst +++ b/docs/source/products/data/ingv_b_swarm_timeseries.rst @@ -2,56 +2,60 @@ 1 Hz Swarm on track values of observed, external and projected vector geomagnetic field ======================================================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents In situ time series of vector geomagnetic field derived from the Swarm constellation at 1 second cadence from 1 January 2014 to 31 December 2020. The output is a single .txt formatted file for each of the 3 satellites of the Swarm constellation, each of one has a size of about 14.5 GB. The sample file attached is extracted from one month of data acquired by Swarm A -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_b_swarm_timeseries - -**publisher:** INGV group - -**alphanumeric_code:** 35A - -**id_tmp:** 52 - -**short_name:** Swarm_B_tseries - -**identifier:** aspis://ingv/b_swarm_timeseries - -**dynamic:** static - -**size:** 20GB - -**format:** text file - -**type:** tableset - -**records_number:** 2634060 - -**time_start:** 2014-01-01 - -**time_stop:** 2022-12-31 - -**spatial:** Earth's Ionosphere - -**messenger:** - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** phys.magField - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_b_swarm_timeseries + * - **publisher:** + - INGV group + * - **alph_code:** + - 35A + * - **id_tmp:** + - 52 + * - **short_name:** + - Swarm_B_tseries + * - **identifier:** + - aspis://ingv/b_swarm_timeseries + * - **dynamic:** + - static + * - **size:** + - 20GB + * - **format:** + - text file + * - **type:** + - tableset + * - **records_number:** + - 2634060 + * - **time_start:** + - 2014-01-01 + * - **time_stop:** + - 2022-12-31 + * - **spatial:** + - Earth's Ionosphere + * - **messenger:** + - + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - phys.magField + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_bvect_cses_tableset.rst b/docs/source/products/data/ingv_bvect_cses_tableset.rst index 7bdb335..f2f2a56 100644 --- a/docs/source/products/data/ingv_bvect_cses_tableset.rst +++ b/docs/source/products/data/ingv_bvect_cses_tableset.rst @@ -2,56 +2,60 @@ CSES-01 on track values of vector magnetic field ================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents In situ time series of vector magnetic field derived from the CSES-01 satellite from 1 January 2019 to 30 September 2021. The output is a single .txt formatted file for both diurnal and nocturnal orbits, each of which has a size of about 3 GB. The sample file attached is extracted from one minute acquired by CSES-01 -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_bvect_cses_tableset - -**publisher:** INGV group - -**alphanumeric_code:** 46B - -**id_tmp:** 84 - -**short_name:** CSES_Bvect_ts - -**identifier:** aspis://ingv/bvect_cses_tableset - -**dynamic:** static - -**size:** 3GB - -**format:** csv - -**type:** timeseries - -**records_number:** 10356758 - -**time_start:** 2019-01-01 - -**time_stop:** 2021-09-30 - -**spatial:** Earth's Ionosphere - -**messenger:** - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** phys.density,phys.electron - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_bvect_cses_tableset + * - **publisher:** + - INGV group + * - **alph_code:** + - 46B + * - **id_tmp:** + - 84 + * - **short_name:** + - CSES_Bvect_ts + * - **identifier:** + - aspis://ingv/bvect_cses_tableset + * - **dynamic:** + - static + * - **size:** + - 3GB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 10356758 + * - **time_start:** + - 2019-01-01 + * - **time_stop:** + - 2021-09-30 + * - **spatial:** + - Earth's Ionosphere + * - **messenger:** + - + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - phys.density,phys.electron + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_evect_cses_tableset.rst b/docs/source/products/data/ingv_evect_cses_tableset.rst index 11760ed..ed8d81b 100644 --- a/docs/source/products/data/ingv_evect_cses_tableset.rst +++ b/docs/source/products/data/ingv_evect_cses_tableset.rst @@ -2,56 +2,60 @@ CSES-01 on track values of vector electric field ================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents In situ time series of vector electric field derived from the CSES-01 satellite from 1 January 2019 to 30 September 2021. The output is a single .txt formatted file for both diurnal and nocturnal orbits, each of which has a size of about 3 GB. The sample file attached is extracted from about ten minutes acquired by CSES-01 -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_evect_cses_tableset - -**publisher:** INGV group - -**alphanumeric_code:** 46A - -**id_tmp:** 85 - -**short_name:** CSES_Evec_ts - -**identifier:** aspis://ingv/evect_cses_tableset - -**dynamic:** static - -**size:** 3GB - -**format:** csv - -**type:** tableset - -**records_number:** 9769594 - -**time_start:** 2019-01-01 - -**time_stop:** 2021-09-30 - -**spatial:** Earth's Ionosphere - -**messenger:** - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** phys.density,phys.electron - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_evect_cses_tableset + * - **publisher:** + - INGV group + * - **alph_code:** + - 46A + * - **id_tmp:** + - 85 + * - **short_name:** + - CSES_Evec_ts + * - **identifier:** + - aspis://ingv/evect_cses_tableset + * - **dynamic:** + - static + * - **size:** + - 3GB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 9769594 + * - **time_start:** + - 2019-01-01 + * - **time_stop:** + - 2021-09-30 + * - **spatial:** + - Earth's Ionosphere + * - **messenger:** + - + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - phys.density,phys.electron + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_aqu_timeseries.rst b/docs/source/products/data/ingv_gic_aqu_timeseries.rst index 96a9dfa..65ef3f8 100644 --- a/docs/source/products/data/ingv_gic_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_gic_aqu_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: L'Aquila ====================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents GIC index for L'Aquila observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. Since for L'Aquila observatory only preliminary data are available, before obtaining GICxy index it will be necessary to estimate X and Y from H and D preliminary data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_aqu_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47A - -**id_tmp:** 7 - -**short_name:** INGV_AQU_gic - -**identifier:** aspis:///ingv/INGV_AQU_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_aqu_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47A + * - **id_tmp:** + - 7 + * - **short_name:** + - INGV_AQU_gic + * - **identifier:** + - aspis:///ingv/INGV_AQU_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_cts_timeseries.rst b/docs/source/products/data/ingv_gic_cts_timeseries.rst index 8c4523e..ab407a6 100644 --- a/docs/source/products/data/ingv_gic_cts_timeseries.rst +++ b/docs/source/products/data/ingv_gic_cts_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Castello Tesino ============================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents GIC index for Castello Tesino observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. If definitive values for Castello Tesino are available GICxy indices will calculates directly from X and Y 1-minute data, otherwise an estimate of X and Y will be first obtained from H and D preliminary data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_cts_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47B - -**id_tmp:** 8 - -**short_name:** INGV_CTS_gic - -**identifier:** aspis:///ingv/INGV_CTS_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:09 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_cts_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47B + * - **id_tmp:** + - 8 + * - **short_name:** + - INGV_CTS_gic + * - **identifier:** + - aspis:///ingv/INGV_CTS_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:09 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_dur_timeseries.rst b/docs/source/products/data/ingv_gic_dur_timeseries.rst index 997436d..d102518 100644 --- a/docs/source/products/data/ingv_gic_dur_timeseries.rst +++ b/docs/source/products/data/ingv_gic_dur_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Duronia ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents GIC index for Duronia observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. If definitive values for Duronia are available GICxy indices will calculates directly from X and Y 1-minute data, otherwise an estimate of X and Y will be first obtained from H and D preliminary data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_dur_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47C - -**id_tmp:** 9 - -**short_name:** INGV_DUR_gic - -**identifier:** aspis:///ingv/INGV_DUR_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_dur_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47C + * - **id_tmp:** + - 9 + * - **short_name:** + - INGV_DUR_gic + * - **identifier:** + - aspis:///ingv/INGV_DUR_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_int_timeseries.rst b/docs/source/products/data/ingv_gic_int_timeseries.rst index c12f5a3..47efee6 100644 --- a/docs/source/products/data/ingv_gic_int_timeseries.rst +++ b/docs/source/products/data/ingv_gic_int_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories ============================================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents As specified for product INTmag, data from INTERMAGNET observatories will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. For the selected observatories GIC index (specifically GICx and GICy) will be calculated. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_int_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47E - -**id_tmp:** 10 - -**short_name:** INGV_INT_gic - -**identifier:** aspis:///ingv/INGV_INT_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_int_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47E + * - **id_tmp:** + - 10 + * - **short_name:** + - INGV_INT_gic + * - **identifier:** + - aspis:///ingv/INGV_INT_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_lmp_timeseries.rst b/docs/source/products/data/ingv_gic_lmp_timeseries.rst index 3e501e2..e7cbb63 100644 --- a/docs/source/products/data/ingv_gic_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_gic_lmp_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Lampedusa ======================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents GIC index for Lampedusa observatory that consists of two components (i.e. GICx and GICy) calculated from magnetic measurements. Since for Lampedusa observatory only preliminary data are available, before obtaining GICxy index it will be necessary to estimate X and Y from H and D preliminary data. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_lmp_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47D - -**id_tmp:** 11 - -**short_name:** INGV_LMP_gic - -**identifier:** aspis:///ingv/INGV_LMP_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_lmp_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47D + * - **id_tmp:** + - 11 + * - **short_name:** + - INGV_LMP_gic + * - **identifier:** + - aspis:///ingv/INGV_LMP_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_gic_wdc_timeseries.rst b/docs/source/products/data/ingv_gic_wdc_timeseries.rst index d86724c..a150198 100644 --- a/docs/source/products/data/ingv_gic_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_gic_wdc_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories ======================================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents As specified for product WDCmag, data from World Data Center of Geomagnetism observatories will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. For the selected observatories GIC index (specifically GICx and GICy) will be calculated. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_gic_wdc_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 47F - -**id_tmp:** 12 - -**short_name:** INGV_WDC_gic - -**identifier:** aspis:///ingv/INGV_WDC_gic - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_gic_wdc_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 47F + * - **id_tmp:** + - 12 + * - **short_name:** + - INGV_WDC_gic + * - **identifier:** + - aspis:///ingv/INGV_WDC_gic + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst b/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst index c5d0e4a..227feeb 100644 --- a/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_cagliari_tableset.rst @@ -2,56 +2,60 @@ Long Term MUF maps centered on Cagliari ======================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Cagliari over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ltmuf_cagliari_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28A - -**id_tmp:** 63 - -**short_name:** LTMUFCagliari - -**identifier:** aspis://ingv/ltmuf_cagliari_tableset - -**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. - -**size:** 1MB - -**format:** dat,png - -**type:** tableset - -**records_number:** 48 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ltmuf_cagliari_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28A + * - **id_tmp:** + - 63 + * - **short_name:** + - LTMUFCagliari + * - **identifier:** + - aspis://ingv/ltmuf_cagliari_tableset + * - **dynamic:** + - The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + * - **size:** + - 1MB + * - **format:** + - dat,png + * - **type:** + - tableset + * - **records_number:** + - 48 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ltmuf_catania_tableset.rst b/docs/source/products/data/ingv_ltmuf_catania_tableset.rst index e65976e..1fa87b3 100644 --- a/docs/source/products/data/ingv_ltmuf_catania_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_catania_tableset.rst @@ -2,56 +2,60 @@ Long Term MUF maps centered on Catania ====================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ltmuf_catania_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28B - -**id_tmp:** 70 - -**short_name:** LTMUFCatania - -**identifier:** aspis://ingv/ltmuf_catania_tableset - -**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. - -**size:** 1MB - -**format:** dat,png - -**type:** tableset - -**records_number:** 48 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:10 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ltmuf_catania_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28B + * - **id_tmp:** + - 70 + * - **short_name:** + - LTMUFCatania + * - **identifier:** + - aspis://ingv/ltmuf_catania_tableset + * - **dynamic:** + - The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + * - **size:** + - 1MB + * - **format:** + - dat,png + * - **type:** + - tableset + * - **records_number:** + - 48 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:10 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ltmuf_milan_tableset.rst b/docs/source/products/data/ingv_ltmuf_milan_tableset.rst index 325f463..8e4b51e 100644 --- a/docs/source/products/data/ingv_ltmuf_milan_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_milan_tableset.rst @@ -2,56 +2,60 @@ Long Term MUF maps centered on Milano ===================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ltmuf_milan_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28C - -**id_tmp:** 68 - -**short_name:** LTMUFMilano - -**identifier:** aspis://ingv/ltmuf_milano_tableset - -**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. - -**size:** 1MB - -**format:** dat,png - -**type:** tableset - -**records_number:** 48 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ltmuf_milan_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28C + * - **id_tmp:** + - 68 + * - **short_name:** + - LTMUFMilano + * - **identifier:** + - aspis://ingv/ltmuf_milano_tableset + * - **dynamic:** + - The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + * - **size:** + - 1MB + * - **format:** + - dat,png + * - **type:** + - tableset + * - **records_number:** + - 48 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ltmuf_rome_tableset.rst b/docs/source/products/data/ingv_ltmuf_rome_tableset.rst index 061f2e1..fdc73e1 100644 --- a/docs/source/products/data/ingv_ltmuf_rome_tableset.rst +++ b/docs/source/products/data/ingv_ltmuf_rome_tableset.rst @@ -2,56 +2,60 @@ Long Term MUF maps centered on Roma =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Long Term maps of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Long term maps are 24, one for each hour of the month, valid for the whole month, and are calculated on the basis of the predicted 12-months smoothed sunspots number. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ltmuf_rome_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28D - -**id_tmp:** 69 - -**short_name:** LTMUFRoma - -**identifier:** aspis://ingv/ltmuf_roma_tableset - -**dynamic:** The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. - -**size:** 1MB - -**format:** dat,png - -**type:** tableset - -**records_number:** 48 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ltmuf_rome_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28D + * - **id_tmp:** + - 69 + * - **short_name:** + - LTMUFRoma + * - **identifier:** + - aspis://ingv/ltmuf_roma_tableset + * - **dynamic:** + - The Data bulk size refers to the size of one map. The number of maps will be 24, one for each hour of the day, valid for the whole month. The first day of a new month a new collection of 24 maps will be calculated. + * - **size:** + - 1MB + * - **format:** + - dat,png + * - **type:** + - tableset + * - **records_number:** + - 48 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_aqu_timeseries.rst b/docs/source/products/data/ingv_mag_aqu_timeseries.rst index 7032fc4..a47bd7e 100644 --- a/docs/source/products/data/ingv_mag_aqu_timeseries.rst +++ b/docs/source/products/data/ingv_mag_aqu_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: L'Aquila ====================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at L'Aquila magnetic observatory (IAGA code: AQU Latitude: 42.383000° Longitude: 13.316000° Altitude: 682.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_aqu_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8A - -**id_tmp:** 17 - -**short_name:** INGV_AQU_mag - -**identifier:** aspis:///ingv/INGV_AQU_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_aqu_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8A + * - **id_tmp:** + - 17 + * - **short_name:** + - INGV_AQU_mag + * - **identifier:** + - aspis:///ingv/INGV_AQU_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_cts_timeseries.rst b/docs/source/products/data/ingv_mag_cts_timeseries.rst index db53559..a544bfc 100644 --- a/docs/source/products/data/ingv_mag_cts_timeseries.rst +++ b/docs/source/products/data/ingv_mag_cts_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Castello Tesino ============================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino (TN) magnetic observatory (IAGA code: CTS Latitude: 46.047000° Longitude: 11.649000° Altitude : 1175.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. For this observatory also definitive data are available. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_cts_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8B - -**id_tmp:** 18 - -**short_name:** INGV_CTS_mag - -**identifier:** aspis:///ingv/INGV_CTS_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_cts_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8B + * - **id_tmp:** + - 18 + * - **short_name:** + - INGV_CTS_mag + * - **identifier:** + - aspis:///ingv/INGV_CTS_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_dmc_timeseries.rst b/docs/source/products/data/ingv_mag_dmc_timeseries.rst index a810c5b..8422911 100644 --- a/docs/source/products/data/ingv_mag_dmc_timeseries.rst +++ b/docs/source/products/data/ingv_mag_dmc_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Dome C ==================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Dome C magnetic observatory(AGA code: DMC Latitude: -75.250000° Longitude: 124.167000° Altitude: 3250.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_dmc_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8D - -**id_tmp:** 19 - -**short_name:** INGV_DMC_mag - -**identifier:** aspis:///ingv/INGV_DMC_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_dmc_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8D + * - **id_tmp:** + - 19 + * - **short_name:** + - INGV_DMC_mag + * - **identifier:** + - aspis:///ingv/INGV_DMC_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_dur_timeseries.rst b/docs/source/products/data/ingv_mag_dur_timeseries.rst index f598575..c4c3054 100644 --- a/docs/source/products/data/ingv_mag_dur_timeseries.rst +++ b/docs/source/products/data/ingv_mag_dur_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Duronia ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Duronia magnetic observatory (IAGA code: DUR Latitude: 41.650000° Longitude: 14.466000° Altitude: 895.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. For this observatory also definitive data are available. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_dur_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8E - -**id_tmp:** 20 - -**short_name:** INGV_DUR_mag - -**identifier:** aspis:///ingv/INGV_DUR_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_dur_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8E + * - **id_tmp:** + - 20 + * - **short_name:** + - INGV_DUR_mag + * - **identifier:** + - aspis:///ingv/INGV_DUR_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_int_timeseries.rst b/docs/source/products/data/ingv_mag_int_timeseries.rst index 84e5be3..06f912f 100644 --- a/docs/source/products/data/ingv_mag_int_timeseries.rst +++ b/docs/source/products/data/ingv_mag_int_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories ============================================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The INTERMAGNET programme exists to establish a global network of cooperating digital magnetic observatories, adopting modern standard specifications for measuring and recording equipment, in order to facilitate data exchanges and the production of geomagnetic products in close to real time. From the INTERMAGNET website it is possible to download 1-minute averages (in daily files) of vector components in either (H, D, Z) or (X, Y, Z) reference frame from world wide magnetic observatories. For this reason, it is not possible to exhaustively fill this form. For instance, the time window of data availability changes from observatory to observatory as well as the tern provided (either (H, D, Z) or (X, Y, Z)) . Data from INTERMAGNET will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. Data can be downloaded as .gz files from an ftp (ftp://ftp.seismo.nrcan.gc.ca/intermagnet/). Each file contains 1 day of 1-minute magnetic data for a single INTERMAGNET observatory -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_int_timeseries - -**publisher:** INTERMAGNET - -**alphanumeric_code:** 9A - -**id_tmp:** 21 - -**short_name:** INGV_INT_mag - -**identifier:** aspis:///ingv/INGV_INT_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_int_timeseries + * - **publisher:** + - INTERMAGNET + * - **alph_code:** + - 9A + * - **id_tmp:** + - 21 + * - **short_name:** + - INGV_INT_mag + * - **identifier:** + - aspis:///ingv/INGV_INT_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_lmp_timeseries.rst b/docs/source/products/data/ingv_mag_lmp_timeseries.rst index cdf193b..afb19d8 100644 --- a/docs/source/products/data/ingv_mag_lmp_timeseries.rst +++ b/docs/source/products/data/ingv_mag_lmp_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Lampedusa ======================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Lampedusa magnetic observatory (IAGA code: LMP Latitude: 35.517000° Longitude: 12.545000° Altitude: 93.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_lmp_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8G - -**id_tmp:** 22 - -**short_name:** INGV_LMP_mag - -**identifier:** aspis:///ingv/INGV_LMP_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_lmp_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8G + * - **id_tmp:** + - 22 + * - **short_name:** + - INGV_LMP_mag + * - **identifier:** + - aspis:///ingv/INGV_LMP_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_tnb_timeseries.rst b/docs/source/products/data/ingv_mag_tnb_timeseries.rst index 97a05bb..2988f79 100644 --- a/docs/source/products/data/ingv_mag_tnb_timeseries.rst +++ b/docs/source/products/data/ingv_mag_tnb_timeseries.rst @@ -2,56 +2,60 @@ INGV geomagnetic data, GIC indices and alert: Terra Nova Bay ============================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of vector the variations of the components (H, D, Z) and of total intensity (F) of the Earth's geomagnetic field measured at Terra Nova Bay magnetic observatory (IAGA code: TNB Latitude: -74.693000° Longitude: 164.099000° Altitude: 59.000 m). In detail, preliminary pseudo H and D values (that are expressed in the instrument frame) will be used to estimate of the horizontal components (i.e. X and Y) in the NEC (North-East-Center) frame. X and Y so estimated will be then used to estimate GICx and GICy indices. These data are updated in real-time and can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_tnb_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8H - -**id_tmp:** 23 - -**short_name:** INGV_TNB_mag - -**identifier:** aspis:///ingv/INGV_TNB_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_tnb_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8H + * - **id_tmp:** + - 23 + * - **short_name:** + - INGV_TNB_mag + * - **identifier:** + - aspis:///ingv/INGV_TNB_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_mag_wdc_timeseries.rst b/docs/source/products/data/ingv_mag_wdc_timeseries.rst index fa9c8ab..fc9c041 100644 --- a/docs/source/products/data/ingv_mag_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_mag_wdc_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories ======================================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The mission of the World Data Center for Geomagnetism is to provide geomagnetic field data supplied from a worldwide network of magnetic observatories, as well as geomagnetic indices (AE index, ASY/SYM index, and Dst index) derived in this data center to researchers specializing mostly in solar terrestrial physics, and geomagnetism in order to facilitate the global exchange of the geomagnetic field data including the geomagnetic indices. From the WDC websites it is possible to download 1-minute averages (in daily files) of vector components in either (H, D, Z) or (X, Y, Z) reference frame from world wide magnetic observatories. For this reason, it is not possible to exhaustively fill this form. For instance, the time window of data availability changes from observatory to observatory as well as the tern provided (either (H, D, Z) or (X, Y, Z)) . Data from WDC will be used only for the limited number of events that will be selected, so that a manual selection of the observatories and of the time period will be made. The set of WDC observatories well overlap to the set of INTERMAGNET observatories. WDC data can be retrieved through queries to a web service (http://www.wdc.bgs.ac.uk/dataportal/webservice_doc.html). At the present moment, however, the service and the website are not working properly and it is not possible to download a sample file. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_mag_wdc_timeseries - -**publisher:** World Data Center for Geomagnetism - -**alphanumeric_code:** 9B - -**id_tmp:** 24 - -**short_name:** INGV_WDC_mag - -**identifier:** aspis:///ingv/INGV_WDC_mag - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:12 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_mag_wdc_timeseries + * - **publisher:** + - World Data Center for Geomagnetism + * - **alph_code:** + - 9B + * - **id_tmp:** + - 24 + * - **short_name:** + - INGV_WDC_mag + * - **identifier:** + - aspis:///ingv/INGV_WDC_mag + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:12 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_magdef_cts_timeseries.rst b/docs/source/products/data/ingv_magdef_cts_timeseries.rst index 187adac..3ab5661 100644 --- a/docs/source/products/data/ingv_magdef_cts_timeseries.rst +++ b/docs/source/products/data/ingv_magdef_cts_timeseries.rst @@ -2,57 +2,61 @@ INGV geomagnetic data, GIC indices and alert: Castello Tesino ============================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of the components (X, Y, Z in the NEC, i.e. North-East-Center frame) and of total intensity (F) of the Earth's geomagnetic field measured at Castello Tesino magnetic observatory (IAGA code: CTS Latitude: 46.047000° Longitude: 11.649000° Altitude: 1175.000 m). These are the definitive values that will be used to calculate GICx and GICy indices. These data are definitive, new definitive data are added yearly. They can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_magdef_cts_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8C - -**id_tmp:** 25 - -**short_name:** INGV_CTS_magdef - -**identifier:** aspis:///ingv/INGV_CTS_magdef - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_magdef_cts_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8C + * - **id_tmp:** + - 25 + * - **short_name:** + - INGV_CTS_magdef + * - **identifier:** + - aspis:///ingv/INGV_CTS_magdef + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_magdef_dur_timeseries.rst b/docs/source/products/data/ingv_magdef_dur_timeseries.rst index 40d43f6..9d8e7e3 100644 --- a/docs/source/products/data/ingv_magdef_dur_timeseries.rst +++ b/docs/source/products/data/ingv_magdef_dur_timeseries.rst @@ -2,57 +2,61 @@ INGV geomagnetic data, GIC indices and alert: Duronia ===================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of the components (X, Y, Z in the NEC, i.e. North-East-Center frame) and of total intensity (F) of the Earth's geomagnetic field measured at Duronia magnetic observatory (IAGA code: DUR Latitude: 41.650000° Longitude: 14.466000° Altitude: 895.000 m). These are the definitive values that will be used to calculate GICx and GICy indices. These data are definitive, new definitive data are added yearly. They can be retrieved from in json format from a web service so that the size of the file (estimated in the DATA DESCRIPTION TAB) actually depends on the query. Queries for a few-days data obtain a rapid reply while for longer queries (say from 1-month upward) obtain slow replies. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_magdef_dur_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 8F - -**id_tmp:** 26 - -**short_name:** INGV_DUR_magdef - -**identifier:** aspis:///ingv/INGV_DUR_magdef - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 84960 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:11 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_magdef_dur_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 8F + * - **id_tmp:** + - 26 + * - **short_name:** + - INGV_DUR_magdef + * - **identifier:** + - aspis:///ingv/INGV_DUR_magdef + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 84960 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:11 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst b/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst index 053d383..0e2a819 100644 --- a/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_cagliari_tableset.rst @@ -2,56 +2,60 @@ Nowcasting MUF map centered on Cagliari ======================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Cagliari over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ncmuf_cagliari_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28E - -**id_tmp:** 27 - -**short_name:** NCMUFCagliari - -**identifier:** aspis://ingv/ncmuf_cagliari_tableset - -**dynamic:** The map is a nowcasting map, generated every 15 minutes. - -**size:** 1MB - -**format:** png,dat - -**type:** tableset - -**records_number:** 192 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:13 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ncmuf_cagliari_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28E + * - **id_tmp:** + - 27 + * - **short_name:** + - NCMUFCagliari + * - **identifier:** + - aspis://ingv/ncmuf_cagliari_tableset + * - **dynamic:** + - The map is a nowcasting map, generated every 15 minutes. + * - **size:** + - 1MB + * - **format:** + - png,dat + * - **type:** + - tableset + * - **records_number:** + - 192 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:13 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ncmuf_catania_tableset.rst b/docs/source/products/data/ingv_ncmuf_catania_tableset.rst index e257ba3..f720d9b 100644 --- a/docs/source/products/data/ingv_ncmuf_catania_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_catania_tableset.rst @@ -2,56 +2,60 @@ Nowcasting MUF map centered on Catania ====================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Catania over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ncmuf_catania_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28F - -**id_tmp:** 28 - -**short_name:** NCMUFCatania - -**identifier:** aspis://ingv/ncmuf_catania_tableset - -**dynamic:** The map is a nowcasting map, generated every 15 minutes. - -**size:** 1MB - -**format:** png,dat - -**type:** tableset - -**records_number:** 192 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:13 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ncmuf_catania_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28F + * - **id_tmp:** + - 28 + * - **short_name:** + - NCMUFCatania + * - **identifier:** + - aspis://ingv/ncmuf_catania_tableset + * - **dynamic:** + - The map is a nowcasting map, generated every 15 minutes. + * - **size:** + - 1MB + * - **format:** + - png,dat + * - **type:** + - tableset + * - **records_number:** + - 192 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:13 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ncmuf_milan_tableset.rst b/docs/source/products/data/ingv_ncmuf_milan_tableset.rst index 6a29c09..96508c1 100644 --- a/docs/source/products/data/ingv_ncmuf_milan_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_milan_tableset.rst @@ -2,56 +2,60 @@ Nowcasting MUF map centered on Milano ===================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Milan over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ncmuf_milan_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28G - -**id_tmp:** 29 - -**short_name:** NCMUFMilano - -**identifier:** aspis://ingv/ncmuf_milano_tableset - -**dynamic:** The map is a nowcasting map, generated every 15 minutes. - -**size:** 1MB - -**format:** png,dat - -**type:** tableset - -**records_number:** 192 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:13 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ncmuf_milan_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28G + * - **id_tmp:** + - 29 + * - **short_name:** + - NCMUFMilano + * - **identifier:** + - aspis://ingv/ncmuf_milano_tableset + * - **dynamic:** + - The map is a nowcasting map, generated every 15 minutes. + * - **size:** + - 1MB + * - **format:** + - png,dat + * - **type:** + - tableset + * - **records_number:** + - 192 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:13 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_ncmuf_rome_tableset.rst b/docs/source/products/data/ingv_ncmuf_rome_tableset.rst index acf8ec2..7f3deb4 100644 --- a/docs/source/products/data/ingv_ncmuf_rome_tableset.rst +++ b/docs/source/products/data/ingv_ncmuf_rome_tableset.rst @@ -2,56 +2,60 @@ Nowcasting MUF map centered on Roma =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Nowcasting map of Maximum Usable Frequency (MUF) and skip distance centered on Rome over an area extending in latitude from 34° N to 48° N and in longitude from 5° W to 20° E, which includes the whole Italian territory. Nowcasting map is generated every 15 minutes exploiting foF2 and M(3000)F2 data autoscaled at the ionospheric stations of Rome (41.8°N, 12.5°E) and Gibilmanna (37.6°N, 14.0°E). Nowcasting maps constitute a powerful tool because they let High Frequency (HF) users know in near real-time the radio propagation conditions. This turns out to be very valuable in terms of reliable radio links, especially in case of adverse space weather events. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_ncmuf_rome_tableset - -**publisher:** INGV - -**alphanumeric_code:** 28H - -**id_tmp:** 30 - -**short_name:** NCMUFCatania - -**identifier:** aspis://ingv/ncmuf_roma_tableset - -**dynamic:** The map is a nowcasting map, generated every 15 minutes. - -**size:** 1MB - -**format:** png,dat - -**type:** tableset - -**records_number:** 192 - -**time_start:** 2017-09-07 - -**time_stop:** 2017-09-08 - -**spatial:** IONO - -**messenger:** electrons - the maps are strictly connected with the electron density of the ionosphere - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_ncmuf_rome_tableset + * - **publisher:** + - INGV + * - **alph_code:** + - 28H + * - **id_tmp:** + - 30 + * - **short_name:** + - NCMUFCatania + * - **identifier:** + - aspis://ingv/ncmuf_roma_tableset + * - **dynamic:** + - The map is a nowcasting map, generated every 15 minutes. + * - **size:** + - 1MB + * - **format:** + - png,dat + * - **type:** + - tableset + * - **records_number:** + - 192 + * - **time_start:** + - 2017-09-07 + * - **time_stop:** + - 2017-09-08 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the maps are strictly connected with the electron density of the ionosphere + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst b/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst index ed243cc..5090e8b 100644 --- a/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst +++ b/docs/source/products/data/ingv_valiiono_gibi_timeseries.rst @@ -2,56 +2,60 @@ Validated data Gibilmanna Ionosonde =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Gibilmanna -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_valiiono_gibi_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 13A - -**id_tmp:** 31 - -**short_name:** ValiIonoGibi - -**identifier:** aspis://ingv/valiiono_gibi_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1463 - -**time_start:** 2012-03-07 - -**time_stop:** 2015-06-30 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_valiiono_gibi_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 13A + * - **id_tmp:** + - 31 + * - **short_name:** + - ValiIonoGibi + * - **identifier:** + - aspis://ingv/valiiono_gibi_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1463 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2015-06-30 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_valiiono_rome_timeseries.rst b/docs/source/products/data/ingv_valiiono_rome_timeseries.rst index 2b46496..71ec384 100644 --- a/docs/source/products/data/ingv_valiiono_rome_timeseries.rst +++ b/docs/source/products/data/ingv_valiiono_rome_timeseries.rst @@ -2,56 +2,60 @@ Validated data Rome Ionosonde ============================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Hourly ionospheric parameters (foF2, foF1, foE, foEs, fbEs, fmin, h'F2, h'F, h'E, h'Es, MUF(3000)F2, M(3000)F2) as validated by an operator from the ionograms obtained by the AIS-INGV ionosonde installed at the ionospheric station of Rome -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_valiiono_rome_timeseries - -**publisher:** INGV - -**alphanumeric_code:** 13B - -**id_tmp:** 32 - -**short_name:** ValiIonoRome - -**identifier:** aspis://ingv/valiiono_rome_timeseries - -**dynamic:** The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated - -**size:** 10MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1727 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** IONO - -**messenger:** electrons - the parameters are linked to the ionospheric vertical electron density profile - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_valiiono_rome_timeseries + * - **publisher:** + - INGV + * - **alph_code:** + - 13B + * - **id_tmp:** + - 32 + * - **short_name:** + - ValiIonoRome + * - **identifier:** + - aspis://ingv/valiiono_rome_timeseries + * - **dynamic:** + - The Data bulk size refers to one year of data. The Rome ionosonde data started being validated in January 1976, this is why in the Number of datasets field you will find the number 47 (years 1976-2022). This collection grows in time. Usually it is updated + * - **size:** + - 10MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1727 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - IONO + * - **messenger:** + - electrons - the parameters are linked to the ionospheric vertical electron density profile + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/uniaq_curr_maigic_tableset.rst b/docs/source/products/data/uniaq_curr_maigic_tableset.rst index 3fe7a42..9933cf0 100644 --- a/docs/source/products/data/uniaq_curr_maigic_tableset.rst +++ b/docs/source/products/data/uniaq_curr_maigic_tableset.rst @@ -2,56 +2,60 @@ Magnetospheric-Ionospheric-Ground Induced Current model - currents ================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** uniaq_curr_maigic_tableset - -**publisher:** Mirko Piersanti - -**alphanumeric_code:** 40B - -**id_tmp:** 86 - -**short_name:** MA.I.GIC. current - -**identifier:** aspis://uniaq//curr_maigic_tableset - -**dynamic:** Static and depending on the length of the input data - -**size:** 5MB - -**format:** .mat - -**type:** tableset - -**records_number:** 8641 - -**time_start:** 2021-04-12 - -**time_stop:** 2021-04-13 - -**spatial:** GEOMAG - -**messenger:** magnetic field - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - uniaq_curr_maigic_tableset + * - **publisher:** + - Mirko Piersanti + * - **alph_code:** + - 40B + * - **id_tmp:** + - 86 + * - **short_name:** + - MA.I.GIC. current + * - **identifier:** + - aspis://uniaq//curr_maigic_tableset + * - **dynamic:** + - Static and depending on the length of the input data + * - **size:** + - 5MB + * - **format:** + - .mat + * - **type:** + - tableset + * - **records_number:** + - 8641 + * - **time_start:** + - 2021-04-12 + * - **time_stop:** + - 2021-04-13 + * - **spatial:** + - GEOMAG + * - **messenger:** + - magnetic field + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/uniaq_epmde_emma_timeseries.rst b/docs/source/products/data/uniaq_epmde_emma_timeseries.rst index 72509e5..5e1c4e8 100644 --- a/docs/source/products/data/uniaq_epmde_emma_timeseries.rst +++ b/docs/source/products/data/uniaq_epmde_emma_timeseries.rst @@ -2,56 +2,60 @@ Equatorial Plasma Mass Density estimates in Plasmasphere ======================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Equatorial plasma mass density estimates in plasmasphere (2 < L < 6) are derived from the the EMMA magnetometers network, updated every 15 minutes. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** uniaq_epmde_emma_timeseries - -**publisher:** University of L'Aquila Dept. of Physical and Chemical Sciences - -**alphanumeric_code:** 29 - -**id_tmp:** 33 - -**short_name:** EPMDP-Estimates - -**identifier:** aspis:///uniaq/epmdp - -**dynamic:** Static - -**size:** 200kB - -**format:** csv - -**type:** timeseries - -**records_number:** 1951 - -**time_start:** 2022-01-01 - -**time_stop:** 2023-12-21 - -**spatial:** GEOMAG - -**messenger:** MHD waves - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** ESP - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - uniaq_epmde_emma_timeseries + * - **publisher:** + - University of L'Aquila Dept. of Physical and Chemical Sciences + * - **alph_code:** + - 29 + * - **id_tmp:** + - 33 + * - **short_name:** + - EPMDP-Estimates + * - **identifier:** + - aspis:///uniaq/epmdp + * - **dynamic:** + - Static + * - **size:** + - 200kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1951 + * - **time_start:** + - 2022-01-01 + * - **time_stop:** + - 2023-12-21 + * - **spatial:** + - GEOMAG + * - **messenger:** + - MHD waves + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - ESP + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/uniaq_field_maigic_tableset.rst b/docs/source/products/data/uniaq_field_maigic_tableset.rst index 0838e28..99dc51e 100644 --- a/docs/source/products/data/uniaq_field_maigic_tableset.rst +++ b/docs/source/products/data/uniaq_field_maigic_tableset.rst @@ -2,56 +2,60 @@ Magnetospheric-Ionospheric-Gound Induced Current model - Geoelectric Field ========================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents The MA.I.GIC. model is based on the equation which describes a possible disturbance in the magnetospheric-ionospheric system propagating vertically downward from the ionosphere as plane waves. In this scenario, the Earth is assumed as uniform (or a layered) half-space conductor with conductivity in which the magnetic field (B) is obtained from ground magnetometer observatories and the impedance Z is obtained considering the corresponding local conductivity. To evaluate the conductivity, the global model by Alekseev et al. (2015), which provides the Earth's conductivity on a series of 0.25 × 0.25 degrees grid spherical layers covering a depth range of 0–100 km, is considered. So the geoelectric field (E) is evaluated. To discriminate between ionospheric and magnetospheric origin contribution, the ground geomagnetic field observations are first decomposed into several Intrinsic Mode Components (IMCs), which are oscillating functions modulated in both amplitude and frequency, using Fast Iterative Filtering . Then, in order to analyze the physical meaning of each IMC and connect them to the timescales involved in the magnetospheric and ionospheric origin fields, we used a statistical test, which allows to evaluate clear timescale separation in a certain data set. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** uniaq_field_maigic_tableset - -**publisher:** Mirko Piersanti - -**alphanumeric_code:** 41B - -**id_tmp:** 87 - -**short_name:** MA.I.GIC. Geoelectric Field - -**identifier:** aspis:///univaq/field_maigic_tableset - -**dynamic:** Static and depending on the length of the input data - -**size:** 5MB - -**format:** .mat - -**type:** tableset - -**records_number:** 8641 - -**time_start:** 2021-04-12 - -**time_stop:** 2021-04-13 - -**spatial:** GEOMAG - -**messenger:** Electric Field - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:14 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - uniaq_field_maigic_tableset + * - **publisher:** + - Mirko Piersanti + * - **alph_code:** + - 41B + * - **id_tmp:** + - 87 + * - **short_name:** + - MA.I.GIC. Geoelectric Field + * - **identifier:** + - aspis:///univaq/field_maigic_tableset + * - **dynamic:** + - Static and depending on the length of the input data + * - **size:** + - 5MB + * - **format:** + - .mat + * - **type:** + - tableset + * - **records_number:** + - 8641 + * - **time_start:** + - 2021-04-12 + * - **time_stop:** + - 2021-04-13 + * - **spatial:** + - GEOMAG + * - **messenger:** + - Electric Field + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:14 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/uniaq_mag_emma_timeseries.rst b/docs/source/products/data/uniaq_mag_emma_timeseries.rst index 3fbc633..1fafe6c 100644 --- a/docs/source/products/data/uniaq_mag_emma_timeseries.rst +++ b/docs/source/products/data/uniaq_mag_emma_timeseries.rst @@ -2,56 +2,60 @@ EMMA Geomagnetic field data =========================== -.. contents:: The tiny table of contents +.. contents:: Table of contents 1-minute averages of the magnetic field variations recorded at 27 ground stations located in Italy and Europe along a meridional chain covering a large range in geographical latitude (from 70 to 42 degrees). The data are automatically collected in near real-time and updated every 15 minutes. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** uniaq_mag_emma_timeseries - -**publisher:** University of L'Aquila Dept. of Physical and Chemical Sciences - -**alphanumeric_code:** 10 - -**id_tmp:** 34 - -**short_name:** EMMA-data - -**identifier:** aspis://uniaq/emma - -**dynamic:** For each day, there is one master dataset containing the general information of each station and related dataset and n (maximum value 27) datasets containing the 1-minute averages of the individual stations. - -**size:** 2MB - -**format:** csv - -**type:** tableset - -**records_number:** 277 - -**time_start:** 2022-01-01 - -**time_stop:** 2023-12-21 - -**spatial:** GROUND - -**messenger:** MHD waves - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** GLE - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - uniaq_mag_emma_timeseries + * - **publisher:** + - University of L'Aquila Dept. of Physical and Chemical Sciences + * - **alph_code:** + - 10 + * - **id_tmp:** + - 34 + * - **short_name:** + - EMMA-data + * - **identifier:** + - aspis://uniaq/emma + * - **dynamic:** + - For each day, there is one master dataset containing the general information of each station and related dataset and n (maximum value 27) datasets containing the 1-minute averages of the individual stations. + * - **size:** + - 2MB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 277 + * - **time_start:** + - 2022-01-01 + * - **time_stop:** + - 2023-12-21 + * - **spatial:** + - GROUND + * - **messenger:** + - MHD waves + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - GLE + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_espseptransport_tableset.rst b/docs/source/products/data/unical_espseptransport_tableset.rst index fdf662b..eb692b8 100644 --- a/docs/source/products/data/unical_espseptransport_tableset.rst +++ b/docs/source/products/data/unical_espseptransport_tableset.rst @@ -2,56 +2,60 @@ Energetic particle spectral indices =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_espseptransport_tableset - -**publisher:** not available in DBF - -**alphanumeric_code:** 20B - -**id_tmp:** 57 - -**short_name:** SEP+ESP-spectral - -**identifier:** aspis:///unical/espseptransport_tableset_old - -**dynamic:** Static collection - -**size:** 1kB - -**format:** csv - -**type:** tableset - -**records_number:** 59 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** protons - -**spectral_min:** 0.01 - -**spectral_max:** 100 - -**spectral_units:** MeV - -**observable:** SEP,ESP,IPS,CME - -**latest update:** 2024-03-28 05:08:15 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_espseptransport_tableset + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 20B + * - **id_tmp:** + - 57 + * - **short_name:** + - SEP+ESP-spectral + * - **identifier:** + - aspis:///unical/espseptransport_tableset_old + * - **dynamic:** + - Static collection + * - **size:** + - 1kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 59 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - protons + * - **spectral_min:** + - 0.01 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,ESP,IPS,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_ace_spectrum.rst b/docs/source/products/data/unical_sep_ace_spectrum.rst index 89b5ab3..e341290 100644 --- a/docs/source/products/data/unical_sep_ace_spectrum.rst +++ b/docs/source/products/data/unical_sep_ace_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the ACE spacecraft ========================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for geoeffective target SWE events (at L1) from ACE spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_ace_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20C - -**id_tmp:** 36 - -**short_name:** SEP-spectrum-Ace - -**identifier:** aspis://unical/unical_sep_ace_spectrum - -**dynamic:** +1 kb updated every SEP event - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 8 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** L1 - -**messenger:** Protons - -**spectral_min:** 0.04 - -**spectral_max:** 5 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_ace_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20C + * - **id_tmp:** + - 36 + * - **short_name:** + - SEP-spectrum-Ace + * - **identifier:** + - aspis://unical/unical_sep_ace_spectrum + * - **dynamic:** + - +1 kb updated every SEP event + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 8 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - L1 + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.04 + * - **spectral_max:** + - 5 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_psp_spectrum.rst b/docs/source/products/data/unical_sep_psp_spectrum.rst index cf69c7e..db1f85a 100644 --- a/docs/source/products/data/unical_sep_psp_spectrum.rst +++ b/docs/source/products/data/unical_sep_psp_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the PSP spacecraft ========================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for widespread target SWE events from PSP spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_psp_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20E - -**id_tmp:** 37 - -**short_name:** SEP-spectrum-PSP - -**identifier:** aspis://unical/unical_sep_psp_spectrum - -**dynamic:** +5 kb updated every SEP event - -**size:** 5kB - -**format:** csv - -**type:** spectrum - -**records_number:** 1 - -**time_start:** 2020-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** Protons - -**spectral_min:** 0.6 - -**spectral_max:** 95 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_psp_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20E + * - **id_tmp:** + - 37 + * - **short_name:** + - SEP-spectrum-PSP + * - **identifier:** + - aspis://unical/unical_sep_psp_spectrum + * - **dynamic:** + - +5 kb updated every SEP event + * - **size:** + - 5kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 1 + * - **time_start:** + - 2020-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.6 + * - **spectral_max:** + - 95 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_soho_spectrum.rst b/docs/source/products/data/unical_sep_soho_spectrum.rst index 901d35c..540262d 100644 --- a/docs/source/products/data/unical_sep_soho_spectrum.rst +++ b/docs/source/products/data/unical_sep_soho_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the SoHO spacecraft ========================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for: geoeffective target SWE events (at L1) from SoHO spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_soho_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20F - -**id_tmp:** 58 - -**short_name:** SEP-spectrum-Soho - -**identifier:** aspis://unical/unical_sep_soho_spectrum - -**dynamic:** +1 kb updated every SEP event - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 7 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** L1 - -**messenger:** Protons - -**spectral_min:** 1.3 - -**spectral_max:** 130 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_soho_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20F + * - **id_tmp:** + - 58 + * - **short_name:** + - SEP-spectrum-Soho + * - **identifier:** + - aspis://unical/unical_sep_soho_spectrum + * - **dynamic:** + - +1 kb updated every SEP event + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 7 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - L1 + * - **messenger:** + - Protons + * - **spectral_min:** + - 1.3 + * - **spectral_max:** + - 130 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_solo_spectrum.rst b/docs/source/products/data/unical_sep_solo_spectrum.rst index 799fa66..b3474e4 100644 --- a/docs/source/products/data/unical_sep_solo_spectrum.rst +++ b/docs/source/products/data/unical_sep_solo_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the SolO spacecraft ========================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for widespread target SWE events from SolO spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_solo_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20G - -**id_tmp:** 39 - -**short_name:** SEP-spectrum-SolO - -**identifier:** aspis://unical/unical_sep_solo_spectrum - -**dynamic:** +2 kb updated every SEP event - -**size:** 5kB - -**format:** csv - -**type:** spectrum - -**records_number:** 2 - -**time_start:** 2020-03-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** Protons - -**spectral_min:** 0.03 - -**spectral_max:** 90 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:15 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_solo_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20G + * - **id_tmp:** + - 39 + * - **short_name:** + - SEP-spectrum-SolO + * - **identifier:** + - aspis://unical/unical_sep_solo_spectrum + * - **dynamic:** + - +2 kb updated every SEP event + * - **size:** + - 5kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 2 + * - **time_start:** + - 2020-03-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.03 + * - **spectral_max:** + - 90 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:15 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_stra_spectrum.rst b/docs/source/products/data/unical_sep_stra_spectrum.rst index d9716a2..6fcd665 100644 --- a/docs/source/products/data/unical_sep_stra_spectrum.rst +++ b/docs/source/products/data/unical_sep_stra_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the STEREO A spacecraft ============================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for widespread target SWE events from STEREO A spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_stra_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20H - -**id_tmp:** 40 - -**short_name:** SEP-spectrum-StereoA - -**identifier:** aspis://unical/unical_sep_stra_spectrum - -**dynamic:** +1 kb updated every SEP event - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 2 - -**time_start:** 2020-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** Protons - -**spectral_min:** 0.08 - -**spectral_max:** 100 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:16 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_stra_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20H + * - **id_tmp:** + - 40 + * - **short_name:** + - SEP-spectrum-StereoA + * - **identifier:** + - aspis://unical/unical_sep_stra_spectrum + * - **dynamic:** + - +1 kb updated every SEP event + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 2 + * - **time_start:** + - 2020-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.08 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_sep_wind_spectrum.rst b/docs/source/products/data/unical_sep_wind_spectrum.rst index ad4bfb6..104d36a 100644 --- a/docs/source/products/data/unical_sep_wind_spectrum.rst +++ b/docs/source/products/data/unical_sep_wind_spectrum.rst @@ -2,56 +2,60 @@ SEP Proton Spectra for the WIND spacecraft ========================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Proton spectra for: geoeffective target SWE events (at L1) from Wind spacecraft. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_sep_wind_spectrum - -**publisher:** University of Calabria Dept. of Physics - -**alphanumeric_code:** 20I - -**id_tmp:** 41 - -**short_name:** SEP-spectrum-Wind - -**identifier:** aspis://unical/unical_sep_wind_spectrum - -**dynamic:** +1 kb updated every SEP event - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 8 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** L1 - -**messenger:** Protons - -**spectral_min:** 0.07 - -**spectral_max:** 80 - -**spectral_units:** MeV - -**observable:** SEP,CME - -**latest update:** 2024-03-28 05:08:16 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_sep_wind_spectrum + * - **publisher:** + - University of Calabria Dept. of Physics + * - **alph_code:** + - 20I + * - **id_tmp:** + - 41 + * - **short_name:** + - SEP-spectrum-Wind + * - **identifier:** + - aspis://unical/unical_sep_wind_spectrum + * - **dynamic:** + - +1 kb updated every SEP event + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 8 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - L1 + * - **messenger:** + - Protons + * - **spectral_min:** + - 0.07 + * - **spectral_max:** + - 80 + * - **spectral_units:** + - MeV + * - **observable:** + - SEP,CME + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unical_shockpar_tableset.rst b/docs/source/products/data/unical_shockpar_tableset.rst index c7ee3f0..9e2c067 100644 --- a/docs/source/products/data/unical_shockpar_tableset.rst +++ b/docs/source/products/data/unical_shockpar_tableset.rst @@ -2,56 +2,60 @@ Parameters of shocks associated with ESP events =============================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unical_shockpar_tableset - -**publisher:** not available in DBF - -**alphanumeric_code:** 22A - -**id_tmp:** 49 - -**short_name:** Shocks-parameters - -**identifier:** aspis://unical/unical_shockpar_tableset - -**dynamic:** +300 byte updated every event - -**size:** 20kB - -**format:** csv - -**type:** tableset - -**records_number:** 65 - -**time_start:** 2009-01-01 - -**time_stop:** 2022-03-31 - -**spatial:** IP - -**messenger:** Protons,Magnetic field - -**spectral_min:** 0.01 - -**spectral_max:** 100 - -**spectral_units:** MeV - -**observable:** IPS,SW,SEP,ESP,IMF - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unical_shockpar_tableset + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 22A + * - **id_tmp:** + - 49 + * - **short_name:** + - Shocks-parameters + * - **identifier:** + - aspis://unical/unical_shockpar_tableset + * - **dynamic:** + - +300 byte updated every event + * - **size:** + - 20kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 65 + * - **time_start:** + - 2009-01-01 + * - **time_stop:** + - 2022-03-31 + * - **spatial:** + - IP + * - **messenger:** + - Protons,Magnetic field + * - **spectral_min:** + - 0.01 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - IPS,SW,SEP,ESP,IMF + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_facula_image.rst b/docs/source/products/data/unict_facula_image.rst index 1540427..7a7b2b9 100644 --- a/docs/source/products/data/unict_facula_image.rst +++ b/docs/source/products/data/unict_facula_image.rst @@ -2,56 +2,60 @@ Faculae geometrical characteristics =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_facula_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 5B - -**id_tmp:** 91 - -**short_name:** Facular area - -**identifier:** aspis:///unict/unict_facula_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-10-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_facula_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 5B + * - **id_tmp:** + - 91 + * - **short_name:** + - Facular area + * - **identifier:** + - aspis:///unict/unict_facula_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-10-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_filament_image.rst b/docs/source/products/data/unict_filament_image.rst index 492e817..d356947 100644 --- a/docs/source/products/data/unict_filament_image.rst +++ b/docs/source/products/data/unict_filament_image.rst @@ -2,56 +2,60 @@ Filament position and geometrical characteristics ================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_filament_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 5C - -**id_tmp:** 92 - -**short_name:** Solar Filaments - -**identifier:** aspis:///unict/unict_filament_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 36 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-10-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_filament_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 5C + * - **id_tmp:** + - 92 + * - **short_name:** + - Solar Filaments + * - **identifier:** + - aspis:///unict/unict_filament_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 36 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-10-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_offlimb_image.rst b/docs/source/products/data/unict_offlimb_image.rst index ddf5412..6298a66 100644 --- a/docs/source/products/data/unict_offlimb_image.rst +++ b/docs/source/products/data/unict_offlimb_image.rst @@ -2,56 +2,60 @@ Geometry and location of prominences on the solar limb ====================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_offlimb_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 6B - -**id_tmp:** 93 - -**short_name:** Prominences location and geometry - -**identifier:** aspis:///unict/unict_offlimb_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 3 - -**time_start:** 2022-12-15 - -**time_stop:** 2023-10-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_offlimb_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 6B + * - **id_tmp:** + - 93 + * - **short_name:** + - Prominences location and geometry + * - **identifier:** + - aspis:///unict/unict_offlimb_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 3 + * - **time_start:** + - 2022-12-15 + * - **time_stop:** + - 2023-10-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_sunspot_image.rst b/docs/source/products/data/unict_sunspot_image.rst index c1a96b0..9a89ea7 100644 --- a/docs/source/products/data/unict_sunspot_image.rst +++ b/docs/source/products/data/unict_sunspot_image.rst @@ -2,56 +2,60 @@ Sunspots Zurich and McIntosh class ================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_sunspot_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 4B - -**id_tmp:** 94 - -**short_name:** Sunspots class - -**identifier:** aspis:///unict/unict_sunspot_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-12-15 - -**time_stop:** 2023-02-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:17 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_sunspot_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 4B + * - **id_tmp:** + - 94 + * - **short_name:** + - Sunspots class + * - **identifier:** + - aspis:///unict/unict_sunspot_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-12-15 + * - **time_stop:** + - 2023-02-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitn_flux_cses_timeseries.rst b/docs/source/products/data/unitn_flux_cses_timeseries.rst index f1172c7..d92ca63 100644 --- a/docs/source/products/data/unitn_flux_cses_timeseries.rst +++ b/docs/source/products/data/unitn_flux_cses_timeseries.rst @@ -2,56 +2,60 @@ CSES satellite particle flux data ================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents Particle flux in the Lshell – pitch reference frame. Lshell will be calculated using the IGRF model for the internal origin field and Tsyganenko model for the external origin field. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitn_flux_cses_timeseries - -**publisher:** Roberto Battiston - -**alphanumeric_code:** 44 - -**id_tmp:** 42 - -**short_name:** CSES Flux - -**identifier:** aspis://unitn/flux_cses_timeseries - -**dynamic:** Static and depending on the length of the input data - -**size:** 5MB - -**format:** .mat - -**type:** timeseries - -**records_number:** 18129 - -**time_start:** 2021-04-12 - -**time_stop:** 2021-04-13 - -**spatial:** IONO - -**messenger:** phys.flux - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** 0 - -**observable:** GCR,ESP,SEP - -**latest update:** 2024-03-28 05:08:17 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitn_flux_cses_timeseries + * - **publisher:** + - Roberto Battiston + * - **alph_code:** + - 44 + * - **id_tmp:** + - 42 + * - **short_name:** + - CSES Flux + * - **identifier:** + - aspis://unitn/flux_cses_timeseries + * - **dynamic:** + - Static and depending on the length of the input data + * - **size:** + - 5MB + * - **format:** + - .mat + * - **type:** + - timeseries + * - **records_number:** + - 18129 + * - **time_start:** + - 2021-04-12 + * - **time_stop:** + - 2021-04-13 + * - **spatial:** + - IONO + * - **messenger:** + - phys.flux + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - 0 + * - **observable:** + - GCR,ESP,SEP + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_halpha_tsst_image.rst b/docs/source/products/data/unitov_halpha_tsst_image.rst index 52acbd5..da9827f 100644 --- a/docs/source/products/data/unitov_halpha_tsst_image.rst +++ b/docs/source/products/data/unitov_halpha_tsst_image.rst @@ -2,56 +2,60 @@ TSST H-alpha Full Disk Images ============================= -.. contents:: The tiny table of contents +.. contents:: Table of contents The Hα channel of the TSST is a Daystar SR-127 QT, an achromatic refractor with 127 mm aperture and a focal length of 2667 mm. The telescope features a narrow band filter with a passband of 0.04 nm centered at the Hα line. The filter is a temperature stabilized etalon in collimated configuration, and it is the same filter used in the GONG network for the Hα channel to monitor the chromospheric transients (Giersch, 2013). The Hα channel is equipped with a focal reducer, acting also as a field curvature corrector, to match the Dalsa Pantera 1M60 pixel scale of the MOF channel (2.6 arcsec/pixel). The main goal of this TSST channel is the real time detection of flaring region (Piazzesi et al., 2012, Pötzi et al., 2015, 2018) during the impulsive and flash phases when the intensity reaches its maximum (Benz, 2017). Hα images are extremely important for ground based SWe monitoring (see, e.g. Veronig & Potzi, 2016) and to automatically detect and track structures in the solar chromosphere, as filaments (Bernasconi et al., 2005, Fuller et al., 2005, Bonnin et al., 2013) and prominences (Wang et al., 2010), that can be associated with flare and coronal mass ejections. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_halpha_tsst_image - -**publisher:** University of Rome Tor Vergata - -**alphanumeric_code:** 2 - -**id_tmp:** 59 - -**short_name:** TSST-halpha - -**identifier:** aspis:///unitov/halpha_tsst_image - -**dynamic:** data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares - -**size:** 20GB - -**format:** .fits - -**type:** image - -**records_number:** 9 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-05-01 - -**spatial:** SUN - -**messenger:** photons - -**spectral_min:** 656.26 - -**spectral_max:** 656.34 - -**spectral_units:** nm - -**observable:** spect.line.intensity,AR,flare - -**latest update:** 2024-03-28 05:08:17 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_halpha_tsst_image + * - **publisher:** + - University of Rome Tor Vergata + * - **alph_code:** + - 2 + * - **id_tmp:** + - 59 + * - **short_name:** + - TSST-halpha + * - **identifier:** + - aspis:///unitov/halpha_tsst_image + * - **dynamic:** + - data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares + * - **size:** + - 20GB + * - **format:** + - .fits + * - **type:** + - image + * - **records_number:** + - 9 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-05-01 + * - **spatial:** + - SUN + * - **messenger:** + - photons + * - **spectral_min:** + - 656.26 + * - **spectral_max:** + - 656.34 + * - **spectral_units:** + - nm + * - **observable:** + - spect.line.intensity,AR,flare + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_icme_tableset.rst b/docs/source/products/data/unitov_icme_tableset.rst index 0697ea9..c8b0204 100644 --- a/docs/source/products/data/unitov_icme_tableset.rst +++ b/docs/source/products/data/unitov_icme_tableset.rst @@ -2,56 +2,60 @@ UNITOV Catalogue of geoeffective CMEs ===================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents A database associating L1 Time of Arrival and Speed of an interplanetary CME to the kinematic characteristics of the corresponding CME, covering the period 1996-2020. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_icme_tableset - -**publisher:** University of Rome Tor Vergata Dept. of Physics - -**alphanumeric_code:** 15 - -**id_tmp:** 44 - -**short_name:** UNITOV-ICME - -**identifier:** aspis:/unitov/icme_tableset - -**dynamic:** +10kB updated every year - -**size:** 100kB - -**format:** csv - -**type:** tableset - -**records_number:** 213 - -**time_start:** 1997-01-01 - -**time_stop:** 2019-12-31 - -**spatial:** IP - -**messenger:** Photons,Protons - -**spectral_min:** 0 - -**spectral_max:** 0 - -**spectral_units:** - -**observable:** - -**latest update:** 2024-03-28 05:08:17 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_icme_tableset + * - **publisher:** + - University of Rome Tor Vergata Dept. of Physics + * - **alph_code:** + - 15 + * - **id_tmp:** + - 44 + * - **short_name:** + - UNITOV-ICME + * - **identifier:** + - aspis:/unitov/icme_tableset + * - **dynamic:** + - +10kB updated every year + * - **size:** + - 100kB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 213 + * - **time_start:** + - 1997-01-01 + * - **time_stop:** + - 2019-12-31 + * - **spatial:** + - IP + * - **messenger:** + - Photons,Protons + * - **spectral_min:** + - 0 + * - **spectral_max:** + - 0 + * - **spectral_units:** + - + * - **observable:** + - + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_iss_lidal_timeseries.rst b/docs/source/products/data/unitov_iss_lidal_timeseries.rst index 1b70ce9..9ee9f05 100644 --- a/docs/source/products/data/unitov_iss_lidal_timeseries.rst +++ b/docs/source/products/data/unitov_iss_lidal_timeseries.rst @@ -2,56 +2,60 @@ LIDAL Flux and Dose timeseries ============================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_iss_lidal_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 64A - -**id_tmp:** 50 - -**short_name:** LIDAL_values - -**identifier:** aspis:///unitov/lidal - -**dynamic:** LIDAL is foreseen to be acquiring data utnil 2028. Estimation is 1 MB per year - -**size:** 60kB - -**format:** csv - -**type:** timeseries - -**records_number:** 1096 - -**time_start:** 2020-01-19 - -**time_stop:** 2022-12-31 - -**spatial:** GEOMAG - -**messenger:** charged nuclei - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** SEP,ESP,GCR - -**latest update:** 2024-03-28 05:08:17 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_iss_lidal_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 64A + * - **id_tmp:** + - 50 + * - **short_name:** + - LIDAL_values + * - **identifier:** + - aspis:///unitov/lidal + * - **dynamic:** + - LIDAL is foreseen to be acquiring data utnil 2028. Estimation is 1 MB per year + * - **size:** + - 60kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1096 + * - **time_start:** + - 2020-01-19 + * - **time_stop:** + - 2022-12-31 + * - **spatial:** + - GEOMAG + * - **messenger:** + - charged nuclei + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - SEP,ESP,GCR + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_mag_tsst_image.rst b/docs/source/products/data/unitov_mag_tsst_image.rst index 4e8cddb..e409bc7 100644 --- a/docs/source/products/data/unitov_mag_tsst_image.rst +++ b/docs/source/products/data/unitov_mag_tsst_image.rst @@ -2,56 +2,60 @@ TSST Full Disk LoS magnetic maps ================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_mag_tsst_image - -**publisher:** University of Rome Tor Vergata - -**alphanumeric_code:** 1A - -**id_tmp:** 60 - -**short_name:** TSST-mag - -**identifier:** aspis:///unitov/mag_tsst_image - -**dynamic:** data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares - -**size:** 300GB - -**format:** .fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-05-01 - -**spatial:** SUN - -**messenger:** photons - -**spectral_min:** 769.88 - -**spectral_max:** 769.92 - -**spectral_units:** nm - -**observable:** phys.magField,AR - -**latest update:** 2024-03-28 05:08:17 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_mag_tsst_image + * - **publisher:** + - University of Rome Tor Vergata + * - **alph_code:** + - 1A + * - **id_tmp:** + - 60 + * - **short_name:** + - TSST-mag + * - **identifier:** + - aspis:///unitov/mag_tsst_image + * - **dynamic:** + - data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares + * - **size:** + - 300GB + * - **format:** + - .fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-05-01 + * - **spatial:** + - SUN + * - **messenger:** + - photons + * - **spectral_min:** + - 769.88 + * - **spectral_max:** + - 769.92 + * - **spectral_units:** + - nm + * - **observable:** + - phys.magField,AR + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_rdparameter_tableset.rst b/docs/source/products/data/unitov_rdparameter_tableset.rst index ccdb3bb..e35cf84 100644 --- a/docs/source/products/data/unitov_rdparameter_tableset.rst +++ b/docs/source/products/data/unitov_rdparameter_tableset.rst @@ -2,56 +2,60 @@ R and D Active Region parameters ================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents Parameters for flare-forecasting applications, representing the complexity of a solar active region -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_rdparameter_tableset - -**publisher:** University of Rome Tor Vergata Dept. of Physics - -**alphanumeric_code:** 3 - -**id_tmp:** 46 - -**short_name:** AR-parameters - -**identifier:** aspis:///unitov/rdparameter_tableset - -**dynamic:** +1MB updated every month - -**size:** 20MB - -**format:** csv - -**type:** tableset - -**records_number:** 35998 - -**time_start:** 2012-09-14 - -**time_stop:** 2016-04-13 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR,flare - -**latest update:** 2024-03-28 05:08:18 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_rdparameter_tableset + * - **publisher:** + - University of Rome Tor Vergata Dept. of Physics + * - **alph_code:** + - 3 + * - **id_tmp:** + - 46 + * - **short_name:** + - AR-parameters + * - **identifier:** + - aspis:///unitov/rdparameter_tableset + * - **dynamic:** + - +1MB updated every month + * - **size:** + - 20MB + * - **format:** + - csv + * - **type:** + - tableset + * - **records_number:** + - 35998 + * - **time_start:** + - 2012-09-14 + * - **time_stop:** + - 2016-04-13 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR,flare + * - **latest update:** + - 2024-03-28 05:08:18 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_vel_tsst_image.rst b/docs/source/products/data/unitov_vel_tsst_image.rst index e534529..fb7b190 100644 --- a/docs/source/products/data/unitov_vel_tsst_image.rst +++ b/docs/source/products/data/unitov_vel_tsst_image.rst @@ -2,56 +2,60 @@ TSST Full Disk Velocity Maps ============================ -.. contents:: The tiny table of contents +.. contents:: Table of contents The TSST potassium MOF-based channel operate at 769.9 nm, sounding an atmospheric layer about 300–400 km over the solar photosphere. The TSST acquires simultaneously photospheric LoS velocity and magnetic maps with a maximum cadence of 15 s. -**References** - - - -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_vel_tsst_image - -**publisher:** University of Rome Tor Vergata - -**alphanumeric_code:** 1B - -**id_tmp:** 61 - -**short_name:** TSST-vel - -**identifier:** aspis:///unitov/vel_tsst_image - -**dynamic:** data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares - -**size:** 300GB - -**format:** .fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-05-01 - -**spatial:** SUN - -**messenger:** photons - -**spectral_min:** 769.88 - -**spectral_max:** 769.92 - -**spectral_units:** nm - -**observable:** phys.veloc,AR - -**latest update:** 2024-03-28 05:08:18 +References +~~~~~~~~~~ + + + +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_vel_tsst_image + * - **publisher:** + - University of Rome Tor Vergata + * - **alph_code:** + - 1B + * - **id_tmp:** + - 61 + * - **short_name:** + - TSST-vel + * - **identifier:** + - aspis:///unitov/vel_tsst_image + * - **dynamic:** + - data collection grows in time. Bulk size estimated on 1 yr. Cadence: at least one image per day in clear weather conditions (up to 5/8 per day) one image every 5 s for some minutes (<60 minutes) during flares + * - **size:** + - 300GB + * - **format:** + - .fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-05-01 + * - **spatial:** + - SUN + * - **messenger:** + - photons + * - **spectral_min:** + - 769.88 + * - **spectral_max:** + - 769.92 + * - **spectral_units:** + - nm + * - **observable:** + - phys.veloc,AR + * - **latest update:** + - 2024-03-28 05:08:18 Columns specification ~~~~~~~~~~~~~~~~~~~~~ -- GitLab