From caa676f4f6958f65696bae4ceb4bb0213aab64fa Mon Sep 17 00:00:00 2001 From: stefano scardigli <stefano.scardigli@roma2.infn.it> Date: Mon, 15 Apr 2024 14:42:20 +0200 Subject: [PATCH] .... --- .../external_flux_goes_timeseries.rst | 87 +++++++++++++ .../external_part_goes_timeseries.rst | 122 ++++++++++++++++++ 2 files changed, 209 insertions(+) create mode 100644 docs/source/products/filerst_GEOMAG/external_flux_goes_timeseries.rst create mode 100644 docs/source/products/filerst_GEOMAG/external_part_goes_timeseries.rst diff --git a/docs/source/products/filerst_GEOMAG/external_flux_goes_timeseries.rst b/docs/source/products/filerst_GEOMAG/external_flux_goes_timeseries.rst new file mode 100644 index 0000000..0e39b84 --- /dev/null +++ b/docs/source/products/filerst_GEOMAG/external_flux_goes_timeseries.rst @@ -0,0 +1,87 @@ +=============== +GOES X-ray Flux +=============== + +.. contents:: Table of contents + +The GOES X-ray flux contain 1-minute averages of solar X-rays in the 1-8 Angstrom (0.1-0.8 nm) and 0.5-4.0 Angstrom (0.05-0.4 nm) passbands. + +References +~~~~~~~~~~ + +https://www.swpc.noaa.gov/products/goes-x-ray-flux + +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:** + - GEOMAG + * - **messenger:** + - photons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 8 + * - **spectral_units:** + - Angstrom + * - **observable:** + - flare + * - **latest update:** + - 2024-04-15 05:29:01 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC + * - 2 + - Short_Wave + - Watts/m^2 + - double + - W/m^2 + * - 3 + - Long_Wave + - Watts/m^2 + - double + - W/m^2 diff --git a/docs/source/products/filerst_GEOMAG/external_part_goes_timeseries.rst b/docs/source/products/filerst_GEOMAG/external_part_goes_timeseries.rst new file mode 100644 index 0000000..3728089 --- /dev/null +++ b/docs/source/products/filerst_GEOMAG/external_part_goes_timeseries.rst @@ -0,0 +1,122 @@ +================ +GOES proton Flux +================ + +.. contents:: Table of contents + +SWPC has high-energy proton detectors on the GOES geostationary and NOAA polar-orbiting satellites. GOES 5-minute averaged integral proton flux (protons/cm2-s-sr), as measured by the SWPC primary GOES satellite for energy thresholds of >=10, >=50, and >=100 MeV, are provided. SWPC's proton event threshold is 10 protons/cm2-s-sr at >=10 MeV. GOES 5-minute averaged integral electron flux (electrons/cm2-s-sr). Measurements are made in three integral flux channels, one channel measuring all electrons with energies greater than 0.8 million electron Volts (MeV), one channel measuring all electrons with energies greater than 2 MeV, and one channel measuring all electrons with energies greater than 4 MeV. High-energy particles can reach Earth anywhere from 20 minutes to many hours following the initiating solar event. The particle energy spectrum and arrival time seen by satellites vary with the location and nature of the event on the solar disk. + +References +~~~~~~~~~~ + +https://www.swpc.noaa.gov/products/goes-proton-flux + +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:** + - GEOMAG + * - **messenger:** + - protons,electrons + * - **spectral_min:** + - 1 + * - **spectral_max:** + - 100 + * - **spectral_units:** + - MeV + * - **observable:** + - flare,SEP,CME,ESP,SW + * - **latest update:** + - 2024-04-15 03:37:42 + +Columns specification +~~~~~~~~~~~~~~~~~~~~~ + +.. list-table:: + :widths: 7 20 15 10 48 + :align: right + :header-rows: 1 + + * - progr + - column + - units + - type + - description + * - 1 + - time + - UTC + - datetime + - UTC + * - 2 + - P1 + - Protons/cm^2 - s^-1 - sr + - double + - >=1Mev integral proton flux 5min average + * - 3 + - P5 + - Protons/cm^2 - s^-1 - sr + - double + - >=5Mev integral proton flux 5min average + * - 4 + - P10 + - Protons/cm^2 - s^-1 - sr + - double + - >=10Mev integral proton flux 5min average + * - 5 + - P30 + - Protons/cm^2 - s^-1 - sr + - double + - >=30Mev integral proton flux 5min average + * - 6 + - P50 + - Protons/cm^2 - s^-1 - sr + - double + - >=50Mev integral proton flux 5min average + * - 7 + - P100 + - Protons/cm^2 - s^-1 - sr + - double + - >=100Mev integral proton flux 5min average + * - 8 + - E_8 + - Electrons/cm^2 - s^-1 - sr + - double + - >=0.8Mev integral electron flux 5min average + * - 9 + - E2_0 + - Electrons/cm^2 - s^-1 - sr + - double + - >=2Mev integral electron flux 5min average + * - 10 + - E4_0 + - Electrons/cm^2 - s^-1 - sr + - double + - >=4Mev integral electron flux 5min average -- GitLab