diff --git a/docs/source/products/filerst_L1/external_flux_goes_timeseries.rst b/docs/source/products/filerst_GEOMAG/external_flux_goes_timeseries.rst
similarity index 84%
rename from docs/source/products/filerst_L1/external_flux_goes_timeseries.rst
rename to docs/source/products/filerst_GEOMAG/external_flux_goes_timeseries.rst
index 766cd96eba8891d7d67672139e6a63cb96bb27ec..0e39b849ffd68c206ea16cb5dd2b610a757b7a8e 100644
--- a/docs/source/products/filerst_L1/external_flux_goes_timeseries.rst
+++ b/docs/source/products/filerst_GEOMAG/external_flux_goes_timeseries.rst
@@ -4,12 +4,12 @@ GOES X-ray Flux
 
 .. contents:: Table of contents
 
-not available in DBF
+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
 ~~~~~~~~~~
 
-not available in DBF
+https://www.swpc.noaa.gov/products/goes-x-ray-flux
 
 Dataset summary
 ~~~~~~~~~~~~~~~
@@ -43,7 +43,7 @@ Dataset summary
   * - **time_stop:**
     - 2020-12-31
   * - **spatial:**
-    - L1
+    - GEOMAG
   * - **messenger:**
     - photons
   * - **spectral_min:**
@@ -55,7 +55,7 @@ Dataset summary
   * - **observable:**
     - flare
   * - **latest update:**
-    - 2024-03-28 05:08:04
+    - 2024-04-15 05:29:01
 
 Columns specification
 ~~~~~~~~~~~~~~~~~~~~~
diff --git a/docs/source/products/filerst_L1/external_part_goes_timeseries.rst b/docs/source/products/filerst_GEOMAG/external_part_goes_timeseries.rst
similarity index 68%
rename from docs/source/products/filerst_L1/external_part_goes_timeseries.rst
rename to docs/source/products/filerst_GEOMAG/external_part_goes_timeseries.rst
index f179e8fb904b05ef6b65cbdb3aef81cd3ed50b33..3728089bf234784c5a55ca0ea6597b7367218fa7 100644
--- a/docs/source/products/filerst_L1/external_part_goes_timeseries.rst
+++ b/docs/source/products/filerst_GEOMAG/external_part_goes_timeseries.rst
@@ -4,12 +4,12 @@ GOES proton Flux
 
 .. contents:: Table of contents
 
-not available in DBF
+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
 ~~~~~~~~~~
 
-not available in DBF
+https://www.swpc.noaa.gov/products/goes-proton-flux
 
 Dataset summary
 ~~~~~~~~~~~~~~~
@@ -43,7 +43,7 @@ Dataset summary
   * - **time_stop:**
     - 2020-12-31
   * - **spatial:**
-    - L1
+    - GEOMAG
   * - **messenger:**
     - protons,electrons
   * - **spectral_min:**
@@ -55,7 +55,7 @@ Dataset summary
   * - **observable:**
     - flare,SEP,CME,ESP,SW
   * - **latest update:**
-    - 2024-03-28 05:08:04
+    - 2024-04-15 03:37:42
 
 Columns specification
 ~~~~~~~~~~~~~~~~~~~~~
diff --git a/docs/source/products/filerst_L1/external_ace_swepam_timeseries.rst b/docs/source/products/filerst_L1/external_ace_swepam_timeseries.rst
index 4be227ea4bddcfbe8e01d48b11e1f47cb4571427..d24a6b81c9d3dc276f0549deb2660552010df3a0 100644
--- a/docs/source/products/filerst_L1/external_ace_swepam_timeseries.rst
+++ b/docs/source/products/filerst_L1/external_ace_swepam_timeseries.rst
@@ -4,12 +4,12 @@ ACE Solar Wind 1 min
 
 .. contents:: Table of contents
 
-qui dovra' esserci la descrizione del prodotto
+The location of the NASA Advanced Composition Explorer (ACE) satellite at the L1 libration point between the Earth and the Sun, about 1,500,000 km forward of Earth, enables ACE to give up to one-hour advance warning of the arrival of damaging space weather events at Earth. The Solar Wind Electron Proton Alpha Monitor (SWEPAM) experiment provides the bulk solar wind observations for ACE.
 
 References
 ~~~~~~~~~~
 
-qui invece la bibliografia
+https://www.swpc.noaa.gov/products/ace-real-time-solar-wind
 
 Dataset summary
 ~~~~~~~~~~~~~~~
@@ -55,7 +55,7 @@ Dataset summary
   * - **observable:**
     - CME,SW,SEP
   * - **latest update:**
-    - 2024-03-29 12:01:32
+    - 2024-04-15 03:38:59
 
 Columns specification
 ~~~~~~~~~~~~~~~~~~~~~