diff --git a/docs/source/products/data/external_ace_swepam_timeseries.rst b/docs/source/products/data/external_ace_swepam_timeseries.rst index cd21da0ca29dd6d195572dec610b344fa8913201..4be227ea4bddcfbe8e01d48b11e1f47cb4571427 100644 --- a/docs/source/products/data/external_ace_swepam_timeseries.rst +++ b/docs/source/products/data/external_ace_swepam_timeseries.rst @@ -2,56 +2,60 @@ ACE Solar Wind 1 min ==================== -.. contents:: The tiny table of contents +.. contents:: Table of contents qui dovra' esserci la descrizione del prodotto -**References** +References +~~~~~~~~~~ qui invece la bibliografia -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** external_ace_swepam_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 101A - -**id_tmp:** 101 - -**short_name:** ace_1minute - -**identifier:** aspis:///external/ace_swepam_timeseries - -**dynamic:** Approx 2MB every week - -**size:** 100kB - -**format:** csv - -**type:** timeseries - -**records_number:** 21599 - -**time_start:** 2016-12-14 - -**time_stop:** 2020-12-31 - -**spatial:** L1 - -**messenger:** protons,electrons - -**spectral_min:** 0.26 - -**spectral_max:** 36 - -**spectral_units:** keV - -**observable:** CME,SW,SEP - -**latest update:** 2024-03-29 12:01:32 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - external_ace_swepam_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 101A + * - **id_tmp:** + - 101 + * - **short_name:** + - ace_1minute + * - **identifier:** + - aspis:///external/ace_swepam_timeseries + * - **dynamic:** + - Approx 2MB every week + * - **size:** + - 100kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 21599 + * - **time_start:** + - 2016-12-14 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - L1 + * - **messenger:** + - protons,electrons + * - **spectral_min:** + - 0.26 + * - **spectral_max:** + - 36 + * - **spectral_units:** + - keV + * - **observable:** + - CME,SW,SEP + * - **latest update:** + - 2024-03-29 12:01:32 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/external_flux_goes_timeseries.rst b/docs/source/products/data/external_flux_goes_timeseries.rst index 52fe3ff541bead24f9e0361d3330db2c52274a87..766cd96eba8891d7d67672139e6a63cb96bb27ec 100644 --- a/docs/source/products/data/external_flux_goes_timeseries.rst +++ b/docs/source/products/data/external_flux_goes_timeseries.rst @@ -2,56 +2,60 @@ GOES X-ray Flux =============== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** external_flux_goes_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 102A - -**id_tmp:** 102 - -**short_name:** goesx1min - -**identifier:** aspis:///external/flux_goes_timeseries - -**dynamic:** Approx 1MB every week - -**size:** 5MB - -**format:** csv - -**type:** timeseries - -**records_number:** 21599 - -**time_start:** 2016-12-14 - -**time_stop:** 2020-12-31 - -**spatial:** L1 - -**messenger:** photons - -**spectral_min:** 1 - -**spectral_max:** 8 - -**spectral_units:** Angstrom - -**observable:** flare - -**latest update:** 2024-03-28 05:08:04 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - external_flux_goes_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 102A + * - **id_tmp:** + - 102 + * - **short_name:** + - goesx1min + * - **identifier:** + - aspis:///external/flux_goes_timeseries + * - **dynamic:** + - Approx 1MB every week + * - **size:** + - 5MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 21599 + * - **time_start:** + - 2016-12-14 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - L1 + * - **messenger:** + - photons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 8 + * - **spectral_units:** + - Angstrom + * - **observable:** + - flare + * - **latest update:** + - 2024-03-28 05:08:04 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/external_part_goes_timeseries.rst b/docs/source/products/data/external_part_goes_timeseries.rst index ee4b7f357593e817fecb8834859aa7bdbf0dc64d..f179e8fb904b05ef6b65cbdb3aef81cd3ed50b33 100644 --- a/docs/source/products/data/external_part_goes_timeseries.rst +++ b/docs/source/products/data/external_part_goes_timeseries.rst @@ -2,56 +2,60 @@ GOES proton Flux ================ -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** external_part_goes_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 103A - -**id_tmp:** 103 - -**short_name:** GOES_particle1min - -**identifier:** aspis:///external/part_goes_timeseries - -**dynamic:** Approx 2MB every week - -**size:** 2MB - -**format:** csv - -**type:** timeseries - -**records_number:** 4319 - -**time_start:** 2016-12-14 - -**time_stop:** 2020-12-31 - -**spatial:** L1 - -**messenger:** protons,electrons - -**spectral_min:** 1 - -**spectral_max:** 100 - -**spectral_units:** MeV - -**observable:** flare,SEP,CME,ESP,SW - -**latest update:** 2024-03-28 05:08:04 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - external_part_goes_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 103A + * - **id_tmp:** + - 103 + * - **short_name:** + - GOES_particle1min + * - **identifier:** + - aspis:///external/part_goes_timeseries + * - **dynamic:** + - Approx 2MB every week + * - **size:** + - 2MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 4319 + * - **time_start:** + - 2016-12-14 + * - **time_stop:** + - 2020-12-31 + * - **spatial:** + - L1 + * - **messenger:** + - protons,electrons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - flare,SEP,CME,ESP,SW + * - **latest update:** + - 2024-03-28 05:08:04 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst b/docs/source/products/data/inaf_cpcp_superdarn_datacube.rst index 8e2d31c0fece1b2d5b50b65972aa82de6e4b27b2..e6f11622b2ea65f9527bc76920fd85724cca6933 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 cb30f8d2376d957673818e0a54a11d8ad5696fc1..b7d8d36e65884000536ec2a84acb48773eba8d0e 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 ece0c5690b10933382cfefaaf34372dda95a5dbf..3542b5cce86bf33329a9789a26015f8a93894bec 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 3248096c94619f4cd1af83261969929f982663f9..8e7960b4a4ca6168eef6d57cddf4918edec7ec5a 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 60bd736edde2a47c27aa9ab308a26cc10ddeb5a2..1867a25fbc0cb6c13ad51958e44d7bc50c5b89b7 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 55112868a8a9639da83a1fefbc8d4b741607f7ae..b7baee1975cd9338c0bfd2aa3fd80a483f0eac9b 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 3c2ad685e3b8bee0ed7c733642b36fd1ef1a48a6..c580787ea7e2696a7a0ef2aebf2643c5e5ce7209 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 1e164d2c12674f27ef95cf4ef82abfb956e8daa3..f60fb579494d9614b0a5e45a4c90d79274f77204 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 717b419d7ef19eb3ff0d45be48bbef5a12f6e391..0963e5ab3958144d73032121e120a6b42e9c64aa 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 8e6184bbb70f04c182eac1ea167a0599b54453cc..7777305761bda3574b940fc062193e693f907ec0 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 ad9a0c6e4a8b06d88fadb6006b6178e197f13bc0..46cb275230e05001532763fc09cf463e95980c3c 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 c52aa746445a6c3e7704849e4239b62cdff299f0..101557c299850c16766057dbdd2cd427af73f62f 100644 --- a/docs/source/products/data/infn_cses_hepd_spectrum.rst +++ b/docs/source/products/data/infn_cses_hepd_spectrum.rst @@ -2,56 +2,60 @@ HEPD-01 time-integrated proton spectrum during the Ground-Level Enhancement of October 28, 2021 =============================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Time-integrated spectrum of solar protons measured by the HEPD-01 detector from space during the Ground-Level Enhancement of October 28, 2021 -**References** +References +~~~~~~~~~~ https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2022SW003191 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_cses_hepd_spectrum - -**publisher:** not available in DBF - -**alphanumeric_code:** 44C - -**id_tmp:** 106 - -**short_name:** HEPD-proton - -**identifier:** aspis://infn/infn_cses_hepd_spectrum - -**dynamic:** - -**size:** 10kB - -**format:** csv - -**type:** spectrum - -**records_number:** 1 - -**time_start:** 2021-10-28 - -**time_stop:** 2021-11-03 - -**spatial:** GEOMAG - -**messenger:** protons - -**spectral_min:** 55 - -**spectral_max:** 250 - -**spectral_units:** MeV - -**observable:** GLE,flare,SEP,GCR,CME - -**latest update:** 2024-04-04 02:08:35 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_cses_hepd_spectrum + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 44C + * - **id_tmp:** + - 106 + * - **short_name:** + - HEPD-proton + * - **identifier:** + - aspis://infn/infn_cses_hepd_spectrum + * - **dynamic:** + - + * - **size:** + - 10kB + * - **format:** + - csv + * - **type:** + - spectrum + * - **records_number:** + - 1 + * - **time_start:** + - 2021-10-28 + * - **time_stop:** + - 2021-11-03 + * - **spatial:** + - GEOMAG + * - **messenger:** + - protons + * - **spectral_min:** + - 55 + * - **spectral_max:** + - 250 + * - **spectral_units:** + - MeV + * - **observable:** + - GLE,flare,SEP,GCR,CME + * - **latest update:** + - 2024-04-04 02:08:35 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_iss_ams_flux_timeseries.rst b/docs/source/products/data/infn_iss_ams_flux_timeseries.rst index fc1c94f081660fd35f5ee12e7944dcb305ee3833..9fc615e84ed6c9f28dc34fa6e5745b4204a12e92 100644 --- a/docs/source/products/data/infn_iss_ams_flux_timeseries.rst +++ b/docs/source/products/data/infn_iss_ams_flux_timeseries.rst @@ -2,56 +2,60 @@ INFN AMS daily proton time dependent fluxes =========================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Daily proton fluxes in cosmic rays were measured with the Alpha Magnetic Spectrometer aboard the International Space Station, from May 20, 2011 to October 29, 2019 (a total of 2824 days or 114 Bartels rotations) in the rigidity interval from 1 to 100 GV, based on 5.5×10^9 protons collected. Several Forbush decreases were also observed during the whole period, in connection with transient magnetic perturbations. The product provides these data as time-profiles from May 20, 2011 to October 29 2019 as a function of rigidity. In particular the daily proton fluxes are measured in 30 bins from 1.00 to 100 GV. The errors include statistics, time-dependent systematic errors and the total systematic error. -**References** +References +~~~~~~~~~~ https://doi.org/10.1103/PhysRevLett.127.271102 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_iss_ams_flux_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 50A - -**id_tmp:** 89 - -**short_name:** AMS_daily_H - -**identifier:** aspis:///infn/ams_protons - -**dynamic:** static - -**size:** 4.1MB - -**format:** csv - -**type:** timeseries - -**records_number:** 83757 - -**time_start:** 2011-05-20 - -**time_stop:** 2019-10-29 - -**spatial:** GEOMAG - -**messenger:** Protons - -**spectral_min:** 1 - -**spectral_max:** 100 - -**spectral_units:** GV - -**observable:** GCR - -**latest update:** 2024-04-04 02:10:23 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_iss_ams_flux_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 50A + * - **id_tmp:** + - 89 + * - **short_name:** + - AMS_daily_H + * - **identifier:** + - aspis:///infn/ams_protons + * - **dynamic:** + - static + * - **size:** + - 4.1MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 83757 + * - **time_start:** + - 2011-05-20 + * - **time_stop:** + - 2019-10-29 + * - **spatial:** + - GEOMAG + * - **messenger:** + - Protons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - GV + * - **observable:** + - GCR + * - **latest update:** + - 2024-04-04 02:10:23 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_pamela_flux_timeseries.rst b/docs/source/products/data/infn_pamela_flux_timeseries.rst index 6573397d674d84ddbc8fd45cb70407ed5b59d061..1d9f643431302241e82030de449dbfd522f22589 100644 --- a/docs/source/products/data/infn_pamela_flux_timeseries.rst +++ b/docs/source/products/data/infn_pamela_flux_timeseries.rst @@ -2,56 +2,60 @@ PAMELA time-profiles of protons during 4 Forbush Decreases ========================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents Time-profiles of galactic cosmic-ray protons measured by the PAMELA detector in space during 4 Forbush Decreases from March 2012 to June 2015 in various rigidity intervals. Each profile is scaled for a suitable period of quiet Sun, estimated about 10 days before each Forbush Decrease -**References** +References +~~~~~~~~~~ https://iopscience.iop.org/article/10.3847/1538-4357/aaa0c8 -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** infn_pamela_flux_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 50B - -**id_tmp:** 90 - -**short_name:** PAMELA-proton - -**identifier:** aspis://INFN-PAMELA/proton - -**dynamic:** Data collected starts on March 1, 2012 and is increasing with a daily resolution up until July 17, 2015 - -**size:** 200kB - -**format:** csv - -**type:** timeseries - -**records_number:** 2394 - -**time_start:** 2012-03-01 - -**time_stop:** 2015-07-17 - -**spatial:** GEOMAG - -**messenger:** protons - -**spectral_min:** 0.85 - -**spectral_max:** 8.68 - -**spectral_units:** GV - -**observable:** GCR - -**latest update:** 2024-04-04 02:12:29 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - infn_pamela_flux_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 50B + * - **id_tmp:** + - 90 + * - **short_name:** + - PAMELA-proton + * - **identifier:** + - aspis://INFN-PAMELA/proton + * - **dynamic:** + - Data collected starts on March 1, 2012 and is increasing with a daily resolution up until July 17, 2015 + * - **size:** + - 200kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 2394 + * - **time_start:** + - 2012-03-01 + * - **time_stop:** + - 2015-07-17 + * - **spatial:** + - GEOMAG + * - **messenger:** + - protons + * - **spectral_min:** + - 0.85 + * - **spectral_max:** + - 8.68 + * - **spectral_units:** + - GV + * - **observable:** + - GCR + * - **latest update:** + - 2024-04-04 02:12:29 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/infn_saandose_samadha_timeseries.rst b/docs/source/products/data/infn_saandose_samadha_timeseries.rst index b46635f717ddbfce58b1c9d778f58c6d7e8fb0b5..036958f43eed827a5cc00a41e2364e2cf94d1200 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 674c0e33ab311799517cab8d734440a518f2395c..e1a2431261658845ab4a16e89966adf91040310f 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 47abb7a41802206afb9caf9848ee37308ffb0b8a..03fd83b68173f900cee0ab437e7604e7d639ab31 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 9c7018ca5cf96f0f0d960d7585ad0e37baec7c03..fe23a673281bfb5e3f9557ee43a195b00898b670 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 76388d4970482475f5c5ca3b547cc43df6d8ab8a..3f667530123fb0edb31f4814e2a583c6eebb7f31 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 129b61e8812a85af0f6b78a14d6d18a61686d8ba..f3d991b67ad43ebd44a187ae51bfd1208a1898a0 100644 --- a/docs/source/products/data/ingv_alert_int_timeseries.rst +++ b/docs/source/products/data/ingv_alert_int_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: INTERMAGNET observatories ============================================================================ -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_int_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 48E - -**id_tmp:** 88 - -**short_name:** INGV_INT_alert - -**identifier:** aspis:///ingv/INGV_INT_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:07 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_int_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 48E + * - **id_tmp:** + - 88 + * - **short_name:** + - INGV_INT_alert + * - **identifier:** + - aspis:///ingv/INGV_INT_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:07 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_alert_lmp_timeseries.rst b/docs/source/products/data/ingv_alert_lmp_timeseries.rst index a13abd897efcc2cea4eb05d2691b1cd385c10836..c2feed37f52fa9df9d0385ed85f9ad61e33fad72 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 f6a5db5f711bd858e714e48715a9f006626ae179..1675fc8e4d8cff79f25c7ffc8d64424bb3eb7acb 100644 --- a/docs/source/products/data/ingv_alert_wdc_timeseries.rst +++ b/docs/source/products/data/ingv_alert_wdc_timeseries.rst @@ -2,56 +2,60 @@ Worldwide geomagnetic data, GIC indices and alert: World Data Center of Geomagnetism (WDC) observatories ======================================================================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** ingv_alert_wdc_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 48F - -**id_tmp:** 48 - -**short_name:** INGV_WDC_alert - -**identifier:** aspis:///ingv/INGV_WDC_alert - -**dynamic:** This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. - -**size:** 120MB - -**format:** csv - -**type:** timeseries - -**records_number:** 1274399 - -**time_start:** 2012-03-07 - -**time_stop:** 2017-09-15 - -**spatial:** GROUND - -**messenger:** - -**spectral_min:** 1 - -**spectral_max:** 1 - -**spectral_units:** 1/minute - -**observable:** GIC,GEOINDEX - -**latest update:** 2024-03-28 05:08:08 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - ingv_alert_wdc_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 48F + * - **id_tmp:** + - 48 + * - **short_name:** + - INGV_WDC_alert + * - **identifier:** + - aspis:///ingv/INGV_WDC_alert + * - **dynamic:** + - This peculialiar version is static being data related only to the 6 CAESAR target events, otherwise it is expected to grow. + * - **size:** + - 120MB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1274399 + * - **time_start:** + - 2012-03-07 + * - **time_stop:** + - 2017-09-15 + * - **spatial:** + - GROUND + * - **messenger:** + - + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 1 + * - **spectral_units:** + - 1/minute + * - **observable:** + - GIC,GEOINDEX + * - **latest update:** + - 2024-03-28 05:08:08 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst b/docs/source/products/data/ingv_autoiono_bbla_timeseries.rst index 80a2ba558a981cb6a5b2d7417ae451e531f7bea0..ac14a8b268e250b17b89151d3f621c6642abe9fd 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 59b191633508a1a5e49da7c2753d17cde015b45d..a8a85d6a4c81b75fd4bdd9c90328b9c5b5040fe2 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 e31ce5aff18128da8e0159efbebef304391f6e00..287c30e8277b743c59ee7a1179e366c6ec95bf66 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 bf95bc7c801951033d16ebb025c498fffab7819f..10e5a97b862e23bf44f3539c487b91a4ea8ef407 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 c01e835d7c4ff1eae16e44d465dd2c559f122062..3dbf61d258b3e75d97ff6497f8e29948cc9acb2d 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 a50603efdbadc2a9ec4b40a14467a914c9a1f8ad..4a8ca4566d72cd42f5aac67279558d910722022d 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 7bdb3353accfb5c352f0defcb97d3a22e4e81cea..f2f2a564ea8017ca3c14cf0b529341ff7bde1ae8 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 11760ed9ba95db454fc434c8c4ba9f974c9cbcc3..ed8d81ba3137c165ce9ddd586865ea1a04fa7609 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 96a9dfa7c2a5a8721d8f987f0b7074affd5cbc33..65ef3f8f903446d0f43c5313c2c2e3df8653337e 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 8c4523e5c6a1673fc2954e19eebc0743727a5d2d..ab407a60e4021de239839ce4a52897b1f9b18fa9 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 997436da361caeeb49d87e469395aa60806a20f8..d1025184ac4e44f0dda1ea1f5f6e9433b306f758 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 c12f5a3fb91d4c95ef29261e6e39ff30366c684f..47efee6190e55abc61f013edfd2d4742b2e6cf5a 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 3e501e2b9b3df0c2d07f787d2fdc489042f2c62d..e7cbb63b23d68662b595e490bf915e7a40e3921a 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 d86724cc55a9ffa719285c665253a02725a66463..a150198ca0bb3599e3b5bd983a3048351af33263 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 c5d0e4ac1303070a837531080845672927ba580c..227feeb0a77148e72d227039f7c854c6f1d59345 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 e65976eccb5d413997b61a8805a39569efa21a0e..1fa87b3ef73db3047633ccaec999506d80e8a898 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 325f46323e096fac9a7588adc98ae0d8294976d2..8e4b51e486eee85f6e03cd3d51b0c3fc1fb41ee0 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 061f2e18a89b030163e320903d7f08cd3c957624..fdc73e1052b0512259360fa2511a83332fffa560 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 7032fc4c7b2367710a6f300bc965a0a383bbb6c2..a47bd7eadf4a94e85ff9d99364e0b76d02c81f80 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 db535593efbfcc07bd079f7cb81f7ae62986468b..a544bfc382bb9929849c38b32718f36e0802e531 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 a810c5bbaa008a322c5c52a67d6ab5755784e6dd..84229117b4afcb3b5c95618eb90f1d189ecade12 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 f598575eed58c41e1452007e04b3e0f41c3e6401..c4c3054c5b54869755c59d82b33791d1f5b684a3 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 84e5be3569c81dda63845df75b7f27aef976b6ab..06f912f8ada46d7b68f4a76188707f5384e65cfa 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 cdf193bb480fc155a4ba8f455a37b58ca8e2a07e..afb19d813ec23d44357542154418a251923d15e2 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 97a05bbf77ff2fb8bec561402b7256499f516edc..2988f79e6ee991aeba674cb6e57af2e3a67da8a4 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 fa9c8ab2cb5175a10001b9ea0cc0cc9938360fe9..fc9c041bc7890c1e4e435ac741d03041e15a980b 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 187adac60b88c74123666150f854e85eb4674a0c..3ab56612f174a35ebf070167ddf8615d38a54aa4 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 40d43f60f5aeeb3bd88b458d03d354628662f3bb..9d8e7e3ff95e8732b77ed33f9180786e0cb22b27 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 053d383b40d1ab64c6ef6c425d9bd805631c1caa..0e2a819f3b2c623d5348cd68f620b1a7c42c95d4 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 e257ba3a76b18cd4b266bcb65c0ddee74202e24c..f720d9b5965c2f9a23d412f088913ebd64dabafc 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 6a29c09e457e20b4258c2c409d9edd33f8f96315..96508c160f6427bafc5c6cf3876a24116913ab00 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 acf8ec2397a6ee097c79f7a65626a6a5546916f0..7f3deb453863da606524dae06b270e4fc0836b4b 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 ed243ccc9054eed98c3e06667837d1d730adca3d..5090e8b7a9a68c3c03993e45de29e811211da442 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 2b464961c0810c084d0a400ebccf2a1763b8b925..71ec3843a88113dd6658d48e8d04e5dbf3a3a412 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 3fe7a42b78092bb8eda9c56acd87f57cbe3fabfa..9933cf02210db52457c2ec1048c7423c9156e561 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 72509e5a249cd1ee61fe7568f6a03b0334c1679c..5e1c4e8231128acdc1f822e9813741d447cb1cff 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 0838e283596ef3edc4f72015d5ac6f4195f4b553..99dc51e6d035a6fc2cdaf731e3eba6c13fb6ca70 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 3fbc6332aeea77e1244ade247db71e1160578285..1fafe6cadeb890c591d14ab66844224dc15891ac 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 fdf662baa4e9b66be9c7acb867265264062815d2..eb692b89f71f87f49c4450da4291cc2c9f6da438 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 89b5ab3cf49656886fce069d2e9c946a95cc5298..e341290f364c50cec2f9da79ef32f861cf7e1052 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 cf69c7e997b4143c337a34839dcde553e15bb4aa..db1f85a9014daa2ba9dc900ee288774d74bd2677 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 901d35c19ae1cdec835771a814effb663cc59686..540262dd0667a5d13801c5711d2fdf3eb8f4f2c4 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 799fa6652e6f9f5f347188693bb87cfc0016abd1..b3474e49fdcb40f2ba16ab862396d672bb551e19 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 d9716a20aae8c1fa9887a3edab745af0fa4c4434..6fcd665648dd0bd9cabbdee680b615432088e7b3 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 ad4bfb6b5b40b67cb7c5e60391f406b127161d7e..104d36ada67638b3f88970c1b1c490ec4e1f8f62 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 c7ee3f039e41cd13609d58764d9d0ed0cda1c0f9..9e2c06776466958b8403f1555d9bb8f0b42377a7 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 15404278bdd2bf5c4ddb846ab519beea03944200..7a7b2b9027e1fb35e8122f1db9955549af3c0581 100644 --- a/docs/source/products/data/unict_facula_image.rst +++ b/docs/source/products/data/unict_facula_image.rst @@ -2,56 +2,60 @@ Faculae geometrical characteristics =================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_facula_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 5B - -**id_tmp:** 91 - -**short_name:** Facular area - -**identifier:** aspis:///unict/unict_facula_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-10-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_facula_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 5B + * - **id_tmp:** + - 91 + * - **short_name:** + - Facular area + * - **identifier:** + - aspis:///unict/unict_facula_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-10-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_filament_image.rst b/docs/source/products/data/unict_filament_image.rst index 492e8175fb28e4c0057d8dbadfabb39e97e5d8fc..d35694794c328831fdd80dc837d6bf19ad5aac1a 100644 --- a/docs/source/products/data/unict_filament_image.rst +++ b/docs/source/products/data/unict_filament_image.rst @@ -2,56 +2,60 @@ Filament position and geometrical characteristics ================================================= -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_filament_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 5C - -**id_tmp:** 92 - -**short_name:** Solar Filaments - -**identifier:** aspis:///unict/unict_filament_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 36 - -**time_start:** 2022-09-01 - -**time_stop:** 2023-10-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_filament_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 5C + * - **id_tmp:** + - 92 + * - **short_name:** + - Solar Filaments + * - **identifier:** + - aspis:///unict/unict_filament_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 36 + * - **time_start:** + - 2022-09-01 + * - **time_stop:** + - 2023-10-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_offlimb_image.rst b/docs/source/products/data/unict_offlimb_image.rst index ddf5412cdf7db39641bf84205ae7c52f96f0c136..6298a66491117ca500bab5bf361e6a53cbe5f83c 100644 --- a/docs/source/products/data/unict_offlimb_image.rst +++ b/docs/source/products/data/unict_offlimb_image.rst @@ -2,56 +2,60 @@ Geometry and location of prominences on the solar limb ====================================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_offlimb_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 6B - -**id_tmp:** 93 - -**short_name:** Prominences location and geometry - -**identifier:** aspis:///unict/unict_offlimb_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 3 - -**time_start:** 2022-12-15 - -**time_stop:** 2023-10-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:16 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_offlimb_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 6B + * - **id_tmp:** + - 93 + * - **short_name:** + - Prominences location and geometry + * - **identifier:** + - aspis:///unict/unict_offlimb_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 3 + * - **time_start:** + - 2022-12-15 + * - **time_stop:** + - 2023-10-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:16 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unict_sunspot_image.rst b/docs/source/products/data/unict_sunspot_image.rst index c1a96b03dc57bf917f5443130b8b9af48a609336..9a89ea74478306926483b48b4d1f08929e0309ae 100644 --- a/docs/source/products/data/unict_sunspot_image.rst +++ b/docs/source/products/data/unict_sunspot_image.rst @@ -2,56 +2,60 @@ Sunspots Zurich and McIntosh class ================================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unict_sunspot_image - -**publisher:** not available in DBF - -**alphanumeric_code:** 4B - -**id_tmp:** 94 - -**short_name:** Sunspots class - -**identifier:** aspis:///unict/unict_sunspot_image - -**dynamic:** Grows in time 16 MB/day - -**size:** 16MB - -**format:** fits - -**type:** image - -**records_number:** 10 - -**time_start:** 2022-12-15 - -**time_stop:** 2023-02-23 - -**spatial:** SUN - -**messenger:** Photons - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** AR - -**latest update:** 2024-03-28 05:08:17 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unict_sunspot_image + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 4B + * - **id_tmp:** + - 94 + * - **short_name:** + - Sunspots class + * - **identifier:** + - aspis:///unict/unict_sunspot_image + * - **dynamic:** + - Grows in time 16 MB/day + * - **size:** + - 16MB + * - **format:** + - fits + * - **type:** + - image + * - **records_number:** + - 10 + * - **time_start:** + - 2022-12-15 + * - **time_stop:** + - 2023-02-23 + * - **spatial:** + - SUN + * - **messenger:** + - Photons + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - AR + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitn_flux_cses_timeseries.rst b/docs/source/products/data/unitn_flux_cses_timeseries.rst index f1172c7430f9e26384aab6573b7c8f7da07181ff..d92ca63f8134e5b5d28e22884e7090ae7144177c 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 52acbd5a08ae3973a5a2c11256b1e486d7ccf778..da9827f855b089bcc924086e90fa6caa98410f0d 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 0697ea99792b2c18bfad5062476b6519f81dd323..c8b0204eab7cf0c34ea1c9204dfdbb5aea87147a 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 1b70ce921d0b6899ee07bfa9ea5e2135ea7cb9e9..9ee9f05d6888eb4b92b31849dd4d43904782f6db 100644 --- a/docs/source/products/data/unitov_iss_lidal_timeseries.rst +++ b/docs/source/products/data/unitov_iss_lidal_timeseries.rst @@ -2,56 +2,60 @@ LIDAL Flux and Dose timeseries ============================== -.. contents:: The tiny table of contents +.. contents:: Table of contents not available in DBF -**References** +References +~~~~~~~~~~ not available in DBF -Data description -~~~~~~~~~~~~~~~~ - -**internal_name:** unitov_iss_lidal_timeseries - -**publisher:** not available in DBF - -**alphanumeric_code:** 64A - -**id_tmp:** 50 - -**short_name:** LIDAL_values - -**identifier:** aspis:///unitov/lidal - -**dynamic:** LIDAL is foreseen to be acquiring data utnil 2028. Estimation is 1 MB per year - -**size:** 60kB - -**format:** csv - -**type:** timeseries - -**records_number:** 1096 - -**time_start:** 2020-01-19 - -**time_stop:** 2022-12-31 - -**spatial:** GEOMAG - -**messenger:** charged nuclei - -**spectral_min:** - -**spectral_max:** - -**spectral_units:** - -**observable:** SEP,ESP,GCR - -**latest update:** 2024-03-28 05:08:17 +Dataset summary +~~~~~~~~~~~~~~~ + +.. list-table:: + + * - **internal_name:** + - unitov_iss_lidal_timeseries + * - **publisher:** + - not available in DBF + * - **alph_code:** + - 64A + * - **id_tmp:** + - 50 + * - **short_name:** + - LIDAL_values + * - **identifier:** + - aspis:///unitov/lidal + * - **dynamic:** + - LIDAL is foreseen to be acquiring data utnil 2028. Estimation is 1 MB per year + * - **size:** + - 60kB + * - **format:** + - csv + * - **type:** + - timeseries + * - **records_number:** + - 1096 + * - **time_start:** + - 2020-01-19 + * - **time_stop:** + - 2022-12-31 + * - **spatial:** + - GEOMAG + * - **messenger:** + - charged nuclei + * - **spectral_min:** + - + * - **spectral_max:** + - + * - **spectral_units:** + - + * - **observable:** + - SEP,ESP,GCR + * - **latest update:** + - 2024-03-28 05:08:17 Columns specification ~~~~~~~~~~~~~~~~~~~~~ diff --git a/docs/source/products/data/unitov_mag_tsst_image.rst b/docs/source/products/data/unitov_mag_tsst_image.rst index 4e8cddb8f978422e38fc834793856e36f9df8b24..e409bc7e70b74f2786d44d3421a65559ea74a605 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 ccdb3bbd0eafb4cacd71b8cc3f78b8fa03cacdf8..e35cf84311cec65a377c8b894656803d744be570 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 e53452969c37e4428f43392c470982c5f615a6f7..fb7b19000c7a2220258da2d60ef9d842a2c5e5d3 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 ~~~~~~~~~~~~~~~~~~~~~