....

docs/source/products/filerst_GEOMAG/external_flux_goes_timeseries.rst

+===============
+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

docs/source/products/filerst_GEOMAG/external_part_goes_timeseries.rst

+================
+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