Fix JASON3 + Bepi/MPO/MAG

Myriam Bouchemit
1 parent 11d33980
Showing 110 changed files with 178 additions and 178 deletions Show diff stats
NumericalData/CDPP-AMDA/ACE/MFI/ace-mag-real.xml
NumericalData/CDPP-AMDA/ACE/SWEPAM/ace-swepam-real.xml
NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2e.xml
NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2i.xml
NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peem-all.xml
NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peim-all.xml
NumericalData/CDPP-AMDA/ARTEMIS/P1/Ephemeris/athp1-orb-all.xml
NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-l.xml
NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-s.xml
NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2e.xml
NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2i.xml
NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peem-all.xml
NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peim-all.xml
NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-l.xml
NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-s.xml
NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-1m.xml
NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-3s.xml
NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1m.xml
NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1s.xml
NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-aa.xml
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>real time</ResourceName>
       <AlternateName>Interplanetary Magnetic Field 60-sec real time Data</AlternateName>
-      <ReleaseDate>2024-10-03T15:03:38Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:03:44Z</ReleaseDate>
       <Description>
              ACE Magnetometer real time, 60-second averages of field magnitude and vectors in GSE and GSM coordinates systems.             
          </Description>
@@ -66,7 +66,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2024-07-07T00:00:00Z</StartDate>
-        <StopDate>2024-10-03T12:59:59Z</StopDate>
+        <StopDate>2024-10-04T02:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT60S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>sw : real time</ResourceName>
       <AlternateName>Solar wind 60-sec real time data</AlternateName>
-      <ReleaseDate>2024-10-03T15:02:02Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:02:05Z</ReleaseDate>
       <Description>
          The ram pressure is calculated using P=rho*Np*Vp², where rho=1.672622*(1+4*(1/(1-He++_ratio)-1)). 
          We use rho=2 here, which corresponds to a ratio of He++ between 4% and 5%.
@@ -63,7 +63,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2024-07-07T00:00:00Z</StartDate>
-        <StopDate>2024-10-03T11:59:59Z</StopDate>
+        <StopDate>2024-10-04T01:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT60S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2e</ResourceID>
     <ResourceHeader>
       <ResourceName>electron full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:25Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:27Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron full mode</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-06-29T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T22:55:33Z</StopDate>
+        <StopDate>2024-10-01T19:28:58Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2i</ResourceID>
     <ResourceHeader>
       <ResourceName>ion full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:24Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:26Z</ReleaseDate>
       <Description>"Full Mode" is a low-time-resolution data product useful for large-scale surveys of THEMIS data. It generally maintains the "full" 32 energies sampled, and have an 88 solid-angle map. Full distribution data are 1-spin snapshots of the plasma with a measurement cadence of either 32 spins (in "Fast-Survey Spacecraft Mode") or 128 spins ("Slow-Survey Spacecraft Mode").&gt;</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -52,7 +52,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-06-29T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T22:53:32Z</StopDate>
+        <StopDate>2024-10-01T19:37:51Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peem-all</ResourceID>
     <ResourceHeader>
       <ResourceName>electron onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:29Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:39Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-06-29T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T22:53:19Z</StopDate>
+        <StopDate>2024-10-01T19:30:02Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peim-all</ResourceID>
     <ResourceHeader>
       <ResourceName>ion onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:28Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:38Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-06-29T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T22:53:19Z</StopDate>
+        <StopDate>2024-10-01T19:30:02Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/Ephemeris/athp1-orb-all</ResourceID>
     <ResourceHeader>
       <ResourceName>orbit</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:33Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:02Z</ReleaseDate>
       <Description>
                 ARTEMIS P1 ephemeris
 	    </Description>
@@ -50,7 +50,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-06-29T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T17:25:46Z</StopDate>
+        <StopDate>2024-10-01T19:29:30Z</StopDate>
       </TimeSpan>
       <Cadence>PT60S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-l</ResourceID>
     <ResourceHeader>
       <ResourceName>0.25 sec (low)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:33Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:02Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-06-29T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T17:25:46Z</StopDate>
+        <StopDate>2024-10-01T19:29:30Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.25S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-s</ResourceID>
     <ResourceHeader>
       <ResourceName>3 sec (spin)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:37Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:06Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-06-29T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T17:32:54Z</StopDate>
+        <StopDate>2024-10-01T17:19:06Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2e</ResourceID>
     <ResourceHeader>
       <ResourceName>electron full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:30Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:34Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron full mode</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-07-17T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T09:13:58Z</StopDate>
+        <StopDate>2024-10-01T18:39:28Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2i</ResourceID>
     <ResourceHeader>
       <ResourceName>ion full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:29Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:34Z</ReleaseDate>
       <Description>"Full Mode" is a low-time-resolution data product useful for large-scale surveys of THEMIS data. It generally maintains the "full" 32 energies sampled, and have an 88 solid-angle map. Full distribution data are 1-spin snapshots of the plasma with a measurement cadence of either 32 spins (in "Fast-Survey Spacecraft Mode") or 128 spins ("Slow-Survey Spacecraft Mode").</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -52,7 +52,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-07-17T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T09:21:55Z</StopDate>
+        <StopDate>2024-10-01T18:40:42Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peem-all</ResourceID>
     <ResourceHeader>
       <ResourceName>electron onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:39Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:52Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-07-17T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T09:15:04Z</StopDate>
+        <StopDate>2024-10-01T18:40:34Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peim-all</ResourceID>
     <ResourceHeader>
       <ResourceName>ion onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:39Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:51Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-07-17T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T09:15:04Z</StopDate>
+        <StopDate>2024-10-01T18:40:34Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-l</ResourceID>
     <ResourceHeader>
       <ResourceName>0.25 sec (low)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:51Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:25Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-07-17T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T09:14:23Z</StopDate>
+        <StopDate>2024-10-01T18:40:15Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.25S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-s</ResourceID>
     <ResourceHeader>
       <ResourceName>3 sec (spin)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:53Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:27Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2011-07-17T00:00:00Z</StartDate>
-        <StopDate>2024-09-29T07:13:24Z</StopDate>
+        <StopDate>2024-10-01T15:47:44Z</StopDate>
       </TimeSpan>
       <Cadence>PT4S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>sw : 1 m</ResourceName>
       <AlternateName>solar wind parameters</AlternateName>
-      <ReleaseDate>2024-10-03T04:12:16Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:13:19Z</ReleaseDate>
       <Description>Faraday Cup (FC)  measures the solar wind bulk properties (wind speed, density and temperature). 
               The ram pressure is calculated using P=rho*Np*Vp², where rho=1.672622*(1+4*(1/(1-He++_ratio)-1)). 
               We use rho=2 here, which corresponds to a ratio of He++ between 4% and 5%.</Description>
@@ -61,7 +61,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-08-01T00:00:00Z</StartDate>
-        <StopDate>2024-10-01T23:59:00Z</StopDate>
+        <StopDate>2024-10-02T23:59:00Z</StopDate>
       </TimeSpan>
       <Cadence>PT60S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>sw : 3 s</ResourceName>
       <AlternateName>solar wind parameters</AlternateName>
-      <ReleaseDate>2024-10-03T04:13:13Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:14:25Z</ReleaseDate>
       <Description>Faraday Cup (FC)  measures the solar wind bulk properties (wind speed, density and temperature).  
              The ram pressure is calculated using P=rho*Np*Vp², where rho=1.672622*(1+4*(1/(1-He++_ratio)-1)). 
              We use rho=2 here, which corresponds to a ratio of He++ between 4% and 5%.</Description>
@@ -61,7 +61,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-08-01T00:00:00Z</StartDate>
-        <StopDate>2024-10-01T23:59:40Z</StopDate>
+        <StopDate>2024-10-02T23:59:40Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>1 m</ResourceName>
       <AlternateName>interplanetary magnetic field</AlternateName>
-      <ReleaseDate>2024-10-03T04:08:33Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:09:14Z</ReleaseDate>
       <Description>Solar wind magnetic field vector (sampling 60s)</Description>
       <Acknowledgement>NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.</Acknowledgement>
       <Contact>
@@ -60,7 +60,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-08-01T00:00:00Z</StartDate>
-        <StopDate>2024-10-01T23:59:00Z</StopDate>
+        <StopDate>2024-10-02T23:59:00Z</StopDate>
       </TimeSpan>
       <Cadence>PT60S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>1 s</ResourceName>
       <AlternateName>interplanetary magnetic field</AlternateName>
-      <ReleaseDate>2024-10-03T04:11:29Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:12:24Z</ReleaseDate>
       <Description>Solar wind magnetic field vector (sampling 1s)</Description>
       <Acknowledgement>NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.</Acknowledgement>
       <Contact>
@@ -58,7 +58,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-08-01T00:00:00Z</StartDate>
-        <StopDate>2024-10-01T23:59:59Z</StopDate>
+        <StopDate>2024-10-02T23:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT60S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>aa</ResourceName>
       <AlternateName>aa IAGA-endorsed magnetic activity index</AlternateName>
-      <ReleaseDate>2024-10-03T04:07:47Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:08:21Z</ReleaseDate>
       <Description>Index which purpose is to measure the amplitude of global geomagnetic activity during 3-hour intervals normalized to geomagnetic latitude ±50°. aa was introduced to monitor geomagnetic activity over the longest possible time period.</Description>
       <Acknowledgement>ISGI website at EOST; License: CC BY-NC https://creativecommons.org/licenses/by-nc/4.0/</Acknowledgement>
       <Contact>
@@ -53,7 +53,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>1975-01-01T00:00:00Z</StartDate>
-        <StopDate>2024-09-30T21:00:00Z</StopDate>
+        <StopDate>2024-10-01T21:00:00Z</StopDate>
       </TimeSpan>
       <Cadence>PT3H</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>am</ResourceName>
       <AlternateName>am IAGA-endorsed magnetic activity index</AlternateName>
-      <ReleaseDate>2024-10-03T04:07:48Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:08:22Z</ReleaseDate>
       <Description>Index which purpose is to provide a characterization of global geomagnetic activity using a large set of stations representing all longitudes and possible hemispheric discrepancies.</Description>
       <Acknowledgement>ISGI website at EOST; License: CC BY-NC https://creativecommons.org/licenses/by-nc/4.0/</Acknowledgement>
       <Contact>
@@ -55,7 +55,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>1975-01-01T00:00:00Z</StartDate>
-        <StopDate>2024-09-30T21:00:00Z</StopDate>
+        <StopDate>2024-10-01T21:00:00Z</StopDate>
       </TimeSpan>
       <Cadence>PT3H</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>Dst</ResourceName>
       <AlternateName>Disturbance Stormtime index</AlternateName>
-      <ReleaseDate>2024-10-03T04:07:48Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:08:23Z</ReleaseDate>
       <Description> Dst index is taken from the WDC (World Data Center) at Kyoto.
             Processing Level :
             * FINAL : 1970 - 2014
@@ -66,7 +66,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>1970-01-01T00:00:00Z</StartDate>
-        <StopDate>2024-09-30T23:00:00Z</StopDate>
+        <StopDate>2024-10-01T23:00:00Z</StopDate>
       </TimeSpan>
       <Cadence>PT1H</Cadence>
     </TemporalDescription>
@@ -53,7 +53,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-02-08T10:23:43Z</StartDate>
-        <StopDate>2000-01-01T00:00:00Z</StopDate>
+        <StopDate>2023-06-18T23:16:16Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.522S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ion</ResourceID>
     <ResourceHeader>
       <ResourceName>ion counts</ResourceName>
-      <ReleaseDate>2024-10-03T07:08:40Z</ReleaseDate>
+      <ReleaseDate>2024-10-03T17:50:54Z</ReleaseDate>
       <Description>High resolution particle count rate data from AMBRE instruments ION1, ION2, ION3 and ION4 detection heads onboard JASON3 satellite </Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/Denis.Payan</PersonID>
@@ -53,7 +53,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-02-08T10:23:43Z</StartDate>
-        <StopDate>2000-01-01T00:00:00Z</StopDate>
+        <StopDate>2023-06-18T23:16:16Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.522S</Cadence>
     </TemporalDescription>
@@ -57,7 +57,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-02-08T10:23:43Z</StartDate>
-        <StopDate>2000-01-01T00:00:00Z</StopDate>
+        <StopDate>2023-06-18T23:16:16Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.522S</Cadence>
     </TemporalDescription>
@@ -56,7 +56,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-02-08T10:23:43Z</StartDate>
-        <StopDate>2000-01-01T00:00:00Z</StopDate>
+        <StopDate>2023-06-18T23:16:16Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.522S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>dc e-field</ResourceName>
       <AlternateName>dc electric field / fast / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:28:06Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:31:26Z</ReleaseDate>
       <Description>Electric Double Probe, Quick-Look Three-Dimensional Electric Field, Level 2, Fast Survey Data</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>e spectral density</ResourceName>
       <AlternateName>ac electric field spectral density / srvy / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:27:45Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:31:05Z</ReleaseDate>
       <Description>Electric Double Probe, High-Frequency AC Electric Field Spectra, Level 2, Survey Data, Level 1B AC Electric Field Data</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>scpot</ResourceName>
       <AlternateName>sc potential / fast / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:28:21Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:31:41Z</ReleaseDate>
       <Description>Electric Double Probe, Dual Probe Spacecraft Potential, Level 2, Fast Survey Data. Spacecraft potential is etstimatrd by averaging measurements of the probe-to-spacecraft potential from several probes.</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>survey</ResourceName>
       <AlternateName>survey</AlternateName>
-      <ReleaseDate>2024-10-03T05:29:40Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:33:06Z</ReleaseDate>
       <Description>For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken
                 from AFG.  Because AFG and DFG are cross-calibrated on an orbit-averaged basis,
                 small differences in offset may be observed between Level2 burst and survey mode
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>electric current</ResourceName>
       <AlternateName>electric current : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:30:40Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:10Z</ReleaseDate>
       <Description>Derived parameter from electron and ion datasets of FPI instrument in Fast Survey Mode.
  
             Electric current: mms1_fast_jgse = 1.6e-10*(mms1_des_ne+mms1_dis_ni)*0.5*(mms1_dis_vgse-mms1_des_vgse)
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>DES : electrons</ResourceName>
       <AlternateName>Dual Electron Spectrometers : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:30:40Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:10Z</ReleaseDate>
       <Description>FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for  
 the current Mission Phase.  Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made 
  available at survey (4.5 s) resolution.  Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>DIS : ions</ResourceName>
       <AlternateName>Dual Ion Spectrometers : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:30:46Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:17Z</ReleaseDate>
       <Description>FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for  
 the current Mission Phase.  Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made 
  available at survey (4.5 s) resolution.  Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>ion moments : survey</ResourceName>
       <AlternateName>ion moments : survey mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:19Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:56Z</ReleaseDate>
       <Description> </Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-current</ResourceID>
     <ResourceHeader>
       <ResourceName>current</ResourceName>
-      <ReleaseDate>2024-10-03T05:27:38Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:30:57Z</ReleaseDate>
       <Description>Curlometer.</Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/Penou</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>e spectral density</ResourceName>
       <AlternateName>ac electric field spectral density / srvy / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:28:25Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:31:46Z</ReleaseDate>
       <Description>Electric Double Probe, High-Frequency AC Electric Field Spectra, Level 2, Survey Data, Level 1B AC Electric Field Data</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>scpot</ResourceName>
       <AlternateName>sc potential / fast / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:28:35Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:31:57Z</ReleaseDate>
       <Description>Electric Double Probe, Dual Probe Spacecraft Potential, Level 2, Fast Survey Data. Spacecraft potential is etstimatrd by averaging measurements of the probe-to-spacecraft potential from several probes.</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS2/Ephemeris/mms2-orb-t89d</ResourceID>
     <ResourceHeader>
       <ResourceName>orbit t89d</ResourceName>
-      <ReleaseDate>2024-10-03T05:31:22Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:35:00Z</ReleaseDate>
       <Description>MMS2 position</Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/M.G.Henderson</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>survey</ResourceName>
       <AlternateName>survey</AlternateName>
-      <ReleaseDate>2024-10-03T05:29:55Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:33:21Z</ReleaseDate>
       <Description>For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken
                 from AFG.  Because AFG and DFG are cross-calibrated on an orbit-averaged basis,
                 small differences in offset may be observed between Level2 burst and survey mode
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>electric current</ResourceName>
       <AlternateName>electric current : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:30:51Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:22Z</ReleaseDate>
       <Description>Derived parameter from electron and ion datasets of FPI instrument in Fast Survey Mode.
  
             Electric current: mms2_fast_jgse = 1.6e-10*(mms2_des_ne+mms2_dis_ni)*0.5*(mms2_dis_vgse-mms2_des_vgse)
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>DES : electrons</ResourceName>
       <AlternateName>Dual Electron Spectrometers : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:30:51Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:22Z</ReleaseDate>
       <Description>FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for  
 the current Mission Phase.  Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made 
  available at survey (4.5 s) resolution.  Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>DIS : ions</ResourceName>
       <AlternateName>Dual Ion Spectrometers : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:30:56Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:29Z</ReleaseDate>
       <Description>FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for  
 the current Mission Phase.  Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made 
  available at survey (4.5 s) resolution.  Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>distance to neutral sheet</ResourceName>
       <AlternateName>Distance to model neutral sheet</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:22Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:35:00Z</ReleaseDate>
       <Description>
             * Distance (Re) from s/c location to Fairfield1970 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle. Valid for Ysm less than 15 Re.
             * Distance (Re) from s/c location to Fairfield1980 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle.
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>T96 field model</ResourceName>
       <AlternateName>Tsyganenko96 geomagnetospheric magnetic field model</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:22Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:35:00Z</ReleaseDate>
       <Description>A data-based Tsyganenko96 model computes the geomagnetospheric magnetic field with an explicitly defined realistic magnetopause, large-scale Region 1 and 2 Birkeland current systems, and the IMF penetration across the boundary. The model uses the following inputs :
             * solar wind ram pressure
             * IMF Y and Z-component
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>dc e-field</ResourceName>
       <AlternateName>dc electric field / fast / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:28:51Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:32:14Z</ReleaseDate>
       <Description>Electric Double Probe, Quick-Look Three-Dimensional Electric Field, Level 2, Fast Survey Data</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>e spectral density</ResourceName>
       <AlternateName>ac electric field spectral density / srvy / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:28:39Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:32:01Z</ReleaseDate>
       <Description>Electric Double Probe, High-Frequency AC Electric Field Spectra, Level 2, Survey Data, Level 1B AC Electric Field Data</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>scpot</ResourceName>
       <AlternateName>sc potential / fast / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:29:03Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:32:26Z</ReleaseDate>
       <Description>Electric Double Probe, Dual Probe Spacecraft Potential, Level 2, Fast Survey Data. Spacecraft potential is etstimatrd by averaging measurements of the probe-to-spacecraft potential from several probes.</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS3/Ephemeris/mms3-orb-t89d</ResourceID>
     <ResourceHeader>
       <ResourceName>orbit t89d</ResourceName>
-      <ReleaseDate>2024-10-03T05:31:24Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:35:03Z</ReleaseDate>
       <Description>MMS3 position</Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/M.G.Henderson</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>survey</ResourceName>
       <AlternateName>survey</AlternateName>
-      <ReleaseDate>2024-10-03T05:30:10Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:33:37Z</ReleaseDate>
       <Description>For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken
                 from AFG.  Because AFG and DFG are cross-calibrated on an orbit-averaged basis,
                 small differences in offset may be observed between Level2 burst and survey mode
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>electric current</ResourceName>
       <AlternateName>electric current : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:01Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:35Z</ReleaseDate>
       <Description>Derived parameter from electron and ion datasets of FPI instrument in Fast Survey Mode.
  
             Electric current: mms3_fast_jgse = 1.6e-10*(mms3_des_ne+mms3_dis_ni)*0.5*(mms3_dis_vgse-mms3_des_vgse)
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>DES : electrons</ResourceName>
       <AlternateName>Dual Electron Spectrometers : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:01Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:35Z</ReleaseDate>
       <Description>FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for  
 the current Mission Phase.  Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made 
  available at survey (4.5 s) resolution.  Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>DIS : ions</ResourceName>
       <AlternateName>Dual Ion Spectrometers : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:06Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:41Z</ReleaseDate>
       <Description>FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for  
 the current Mission Phase.  Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made 
  available at survey (4.5 s) resolution.  Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>distance to neutral sheet</ResourceName>
       <AlternateName>Distance to model neutral sheet</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:24Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:35:03Z</ReleaseDate>
       <Description>
             * Distance (Re) from s/c location to Fairfield1970 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle. Valid for Ysm less than 15 Re.
             * Distance (Re) from s/c location to Fairfield1980 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle.
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>T96 field model</ResourceName>
       <AlternateName>Tsyganenko96 geomagnetospheric magnetic field model</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:24Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:35:03Z</ReleaseDate>
       <Description>A data-based Tsyganenko96 model computes the geomagnetospheric magnetic field with an explicitly defined realistic magnetopause, large-scale Region 1 and 2 Birkeland current systems, and the IMF penetration across the boundary. The model uses the following inputs :
             * solar wind ram pressure
             * IMF Y and Z-component
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>dc e-field</ResourceName>
       <AlternateName>dc electric field / fast / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:29:19Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:32:44Z</ReleaseDate>
       <Description>Electric Double Probe, Quick-Look Three-Dimensional Electric Field, Level 2, Fast Survey Data</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>e spectral density</ResourceName>
       <AlternateName>ac electric field spectral density / srvy / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:29:06Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:32:31Z</ReleaseDate>
       <Description>Electric Double Probe, High-Frequency AC Electric Field Spectra, Level 2, Survey Data, Level 1B AC Electric Field Data</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>scpot</ResourceName>
       <AlternateName>sc potential / fast / l2</AlternateName>
-      <ReleaseDate>2024-10-03T05:29:27Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:32:53Z</ReleaseDate>
       <Description>Electric Double Probe, Dual Probe Spacecraft Potential, Level 2, Fast Survey Data. Spacecraft potential is etstimatrd by averaging measurements of the probe-to-spacecraft potential from several probes.</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS4/Ephemeris/mms4-orb-t89d</ResourceID>
     <ResourceHeader>
       <ResourceName>orbit t89d</ResourceName>
-      <ReleaseDate>2024-10-03T05:31:26Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:35:05Z</ReleaseDate>
       <Description>MMS4 position</Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/M.G.Henderson</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>survey</ResourceName>
       <AlternateName>survey</AlternateName>
-      <ReleaseDate>2024-10-03T05:30:37Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:06Z</ReleaseDate>
       <Description>For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken
                 from AFG.  Because AFG and DFG are cross-calibrated on an orbit-averaged basis,
                 small differences in offset may be observed between Level2 burst and survey mode
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>DIS : ions</ResourceName>
       <AlternateName>Dual Ion Spectrometers : fast mode</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:12Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:34:48Z</ReleaseDate>
       <Description>FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for  
 the current Mission Phase.  Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made 
  available at survey (4.5 s) resolution.  Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>distance to neutral sheet</ResourceName>
       <AlternateName>Distance to model neutral sheet</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:26Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:35:05Z</ReleaseDate>
       <Description>
             * Distance (Re) from s/c location to Fairfield1970 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle. Valid for Ysm less than 15 Re.
             * Distance (Re) from s/c location to Fairfield1980 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle.
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>T96 field model</ResourceName>
       <AlternateName>Tsyganenko96 geomagnetospheric magnetic field model</AlternateName>
-      <ReleaseDate>2024-10-03T05:31:26Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:35:05Z</ReleaseDate>
       <Description>A data-based Tsyganenko96 model computes the geomagnetospheric magnetic field with an explicitly defined realistic magnetopause, large-scale Region 1 and 2 Birkeland current systems, and the IMF penetration across the boundary. The model uses the following inputs :
             * solar wind ram pressure
             * IMF Y and Z-component
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>position in ITRF</ResourceName>
       <AlternateName>Swarm-A orbital information from FAC dataset</AlternateName>
-      <ReleaseDate>2024-10-03T04:14:33Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:15:50Z</ReleaseDate>
       <Description>Swarm-A orbital information from FAC dataset</Description>
       <Acknowledgement> </Acknowledgement>
       <Contact>
@@ -59,7 +59,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2013-11-26T00:00:00Z</StartDate>
-        <StopDate>2024-09-27T23:59:59Z</StopDate>
+        <StopDate>2024-09-28T23:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT1S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>field-aligned current</ResourceName>
       <AlternateName>Level2daily/Entire_mission_data/FAC dataset</AlternateName>
-      <ReleaseDate>2024-10-03T04:14:32Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:15:49Z</ReleaseDate>
       <Description>field-aligned current</Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/P.Ritter</PersonID>
@@ -55,7 +55,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2013-11-25T11:02:52Z</StartDate>
-        <StopDate>2024-09-27T23:59:59Z</StopDate>
+        <StopDate>2024-09-28T23:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT1S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>field-aligned current (A+C)</ResourceName>
       <AlternateName>Level2daily/Entire_mission_data/FAC dataset</AlternateName>
-      <ReleaseDate>2024-10-02T04:19:02Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:20:04Z</ReleaseDate>
       <Description>field-aligned current (A+C)</Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/P.Ritter</PersonID>
@@ -55,7 +55,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2013-11-26T00:07:47Z</StartDate>
-        <StopDate>2024-09-26T23:59:59Z</StopDate>
+        <StopDate>2024-09-28T23:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT1S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>position in ITRF</ResourceName>
       <AlternateName>Swarm-B orbital information from FAC dataset</AlternateName>
-      <ReleaseDate>2024-10-03T04:15:05Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:17:25Z</ReleaseDate>
       <Description>Swarm-B orbital information from FAC dataset</Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/R.Haagmans</PersonID>
@@ -58,7 +58,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2013-11-28T00:00:00Z</StartDate>
-        <StopDate>2024-09-26T23:59:59Z</StopDate>
+        <StopDate>2024-09-28T23:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT1S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>field-aligned current</ResourceName>
       <AlternateName>Level2daily/Entire_mission_data/FAC dataset</AlternateName>
-      <ReleaseDate>2024-10-03T04:15:04Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:17:23Z</ReleaseDate>
       <Description>field-aligned current</Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/P.Ritter</PersonID>
@@ -55,7 +55,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2013-11-25T11:01:15Z</StartDate>
-        <StopDate>2024-09-26T23:59:59Z</StopDate>
+        <StopDate>2024-09-28T23:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT1S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>position in ITRF</ResourceName>
       <AlternateName>Swarm-C orbital information from FAC dataset</AlternateName>
-      <ReleaseDate>2024-10-02T04:18:00Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:19:01Z</ReleaseDate>
       <Description>Swarm-C orbital information from FAC dataset</Description>
       <Contact>
         <PersonID>spase://CNES/Person/CDPP-AMDA/R.Haagmans</PersonID>
@@ -58,7 +58,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2013-12-04T00:00:00Z</StartDate>
-        <StopDate>2024-09-26T23:59:59Z</StopDate>
+        <StopDate>2024-09-28T23:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT1S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/SWARM-C/MAG/swarmc-fac-all</ResourceID>
     <ResourceHeader>
       <ResourceName>field-aligned current</ResourceName>
-      <ReleaseDate>2024-10-02T04:17:59Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:19:00Z</ReleaseDate>
       <Description>field-aligned current</Description>
       <Acknowledgement> </Acknowledgement>
       <Contact>
@@ -55,7 +55,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2013-11-26T00:00:00Z</StartDate>
-        <StopDate>2024-09-26T23:59:59Z</StopDate>
+        <StopDate>2024-09-28T23:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT1S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/A/ESA/tha-esa-l2e</ResourceID>
     <ResourceHeader>
       <ResourceName>electron full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:16Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:17Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron full mode</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -51,7 +51,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T18:53:59Z</StartDate>
-        <StopDate>2024-09-30T11:09:05Z</StopDate>
+        <StopDate>2024-10-01T18:27:53Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/A/ESA/tha-esa-l2i</ResourceID>
     <ResourceHeader>
       <ResourceName>ion full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:15Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:16Z</ReleaseDate>
       <Description>"Full Mode" is a low-time-resolution data product useful for large-scale surveys of THEMIS data. It generally maintains the "full" 32 energies sampled, and have an 88 solid-angle map. Full distribution data are 1-spin snapshots of the plasma with a measurement cadence of either 32 spins (in "Fast-Survey Spacecraft Mode") or 128 spins ("Slow-Survey Spacecraft Mode").</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -51,7 +51,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T18:53:59Z</StartDate>
-        <StopDate>2024-09-30T11:09:57Z</StopDate>
+        <StopDate>2024-10-01T18:28:09Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/A/ESA/tha-peem-all</ResourceID>
     <ResourceHeader>
       <ResourceName>electron onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:16Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:24Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-02T00:00:30Z</StartDate>
-        <StopDate>2024-09-30T11:10:13Z</StopDate>
+        <StopDate>2024-10-01T18:28:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/A/ESA/tha-peim-all</ResourceID>
     <ResourceHeader>
       <ResourceName>ion onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:15Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:23Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-02T00:00:30Z</StartDate>
-        <StopDate>2024-09-30T11:10:13Z</StopDate>
+        <StopDate>2024-10-01T18:28:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>onboard moments : potential</ResourceName>
       <AlternateName>S/c potential from onboard moments</AlternateName>
-      <ReleaseDate>2024-10-03T04:01:15Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:23Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - S/c potential from onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-02T00:00:30Z</StartDate>
-        <StopDate>2024-09-30T11:10:13Z</StopDate>
+        <StopDate>2024-10-01T18:28:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/A/FGM/tha-fgm-l</ResourceID>
     <ResourceHeader>
       <ResourceName>0.25 sec (low)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:14Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:03:37Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-02-23T03:29:29Z</StartDate>
-        <StopDate>2024-09-30T11:09:34Z</StopDate>
+        <StopDate>2024-10-01T18:28:30Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.25S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/A/FGM/tha-fgm-s</ResourceID>
     <ResourceHeader>
       <ResourceName>3 sec (spin)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:18Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:03:41Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-02-26T23:00:35Z</StartDate>
-        <StopDate>2024-09-30T09:05:09Z</StopDate>
+        <StopDate>2024-10-02T03:41:44Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/B/ESA/thb-esa-l2e</ResourceID>
     <ResourceHeader>
       <ResourceName>electron full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:25Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:27Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron full mode</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T17:55:08Z</StartDate>
-        <StopDate>2024-09-29T22:55:33Z</StopDate>
+        <StopDate>2024-10-01T19:28:58Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/B/ESA/thb-esa-l2i</ResourceID>
     <ResourceHeader>
       <ResourceName>ion full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:24Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:26Z</ReleaseDate>
       <Description>"Full Mode" is a low-time-resolution data product useful for large-scale surveys of THEMIS data. It generally maintains the "full" 32 energies sampled, and have an 88 solid-angle map. Full distribution data are 1-spin snapshots of the plasma with a measurement cadence of either 32 spins (in "Fast-Survey Spacecraft Mode") or 128 spins ("Slow-Survey Spacecraft Mode").&gt;</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -51,7 +51,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T17:55:08Z</StartDate>
-        <StopDate>2024-09-29T22:53:32Z</StopDate>
+        <StopDate>2024-10-01T19:37:51Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/B/ESA/thb-peem-all</ResourceID>
     <ResourceHeader>
       <ResourceName>electron onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:29Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:39Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-10T00:02:05Z</StartDate>
-        <StopDate>2024-09-29T22:53:19Z</StopDate>
+        <StopDate>2024-10-01T19:30:02Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/B/ESA/thb-peim-all</ResourceID>
     <ResourceHeader>
       <ResourceName>ion onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:28Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:38Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-10T00:02:05Z</StartDate>
-        <StopDate>2024-09-29T22:53:19Z</StopDate>
+        <StopDate>2024-10-01T19:30:02Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>onboard moments : potential</ResourceName>
       <AlternateName>S/c potential from onboard moments</AlternateName>
-      <ReleaseDate>2024-10-03T04:01:28Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:38Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - S/c potential from onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-10T00:02:05Z</StartDate>
-        <StopDate>2024-09-29T22:53:19Z</StopDate>
+        <StopDate>2024-10-01T19:30:02Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/B/FGM/thb-fgm-l</ResourceID>
     <ResourceHeader>
       <ResourceName>0.25 sec (low)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:33Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:02Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-02-24T04:42:44Z</StartDate>
-        <StopDate>2024-09-29T17:25:46Z</StopDate>
+        <StopDate>2024-10-01T19:29:30Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.25S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/B/FGM/thb-fgm-s</ResourceID>
     <ResourceHeader>
       <ResourceName>3 sec (spin)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:37Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:06Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-02-26T23:26:57Z</StartDate>
-        <StopDate>2024-09-29T17:32:54Z</StopDate>
+        <StopDate>2024-10-01T17:19:06Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/C/ESA/thc-esa-l2e</ResourceID>
     <ResourceHeader>
       <ResourceName>electron full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:30Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:34Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron full mode</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T15:58:39Z</StartDate>
-        <StopDate>2024-09-29T09:13:58Z</StopDate>
+        <StopDate>2024-10-01T18:39:28Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/C/ESA/thc-esa-l2i</ResourceID>
     <ResourceHeader>
       <ResourceName>ion full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:29Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:34Z</ReleaseDate>
       <Description>"Full Mode" is a low-time-resolution data product useful for large-scale surveys of THEMIS data. It generally maintains the "full" 32 energies sampled, and have an 88 solid-angle map. Full distribution data are 1-spin snapshots of the plasma with a measurement cadence of either 32 spins (in "Fast-Survey Spacecraft Mode") or 128 spins ("Slow-Survey Spacecraft Mode").</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -51,7 +51,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T15:58:39Z</StartDate>
-        <StopDate>2024-09-29T09:21:55Z</StopDate>
+        <StopDate>2024-10-01T18:40:42Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/C/ESA/thc-peem-all</ResourceID>
     <ResourceHeader>
       <ResourceName>electron onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:39Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:52Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-10T00:00:32Z</StartDate>
-        <StopDate>2024-09-29T09:15:04Z</StopDate>
+        <StopDate>2024-10-01T18:40:34Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/C/ESA/thc-peim-all</ResourceID>
     <ResourceHeader>
       <ResourceName>ion onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:39Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:51Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-10T00:00:32Z</StartDate>
-        <StopDate>2024-09-29T09:15:04Z</StopDate>
+        <StopDate>2024-10-01T18:40:34Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>onboard moments : potential</ResourceName>
       <AlternateName>S/c potential from onboard moments</AlternateName>
-      <ReleaseDate>2024-10-03T04:01:39Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:51Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - S/c potential from onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-10T00:00:32Z</StartDate>
-        <StopDate>2024-09-29T09:15:04Z</StopDate>
+        <StopDate>2024-10-01T18:40:34Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/C/FGM/thc-fgm-l</ResourceID>
     <ResourceHeader>
       <ResourceName>0.25 sec (low)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:51Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:25Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -46,7 +46,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-02-22T23:17:57Z</StartDate>
-        <StopDate>2024-09-29T09:14:23Z</StopDate>
+        <StopDate>2024-10-01T18:40:15Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.25S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/C/FGM/thc-fgm-s</ResourceID>
     <ResourceHeader>
       <ResourceName>3 sec (spin)</ResourceName>
-      <ReleaseDate>2024-10-03T04:03:53Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:27Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -46,7 +46,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-02-26T22:17:50Z</StartDate>
-        <StopDate>2024-09-29T07:13:24Z</StopDate>
+        <StopDate>2024-10-01T15:47:44Z</StopDate>
       </TimeSpan>
       <Cadence>PT4S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/D/ESA/thd-esa-l2e</ResourceID>
     <ResourceHeader>
       <ResourceName>electron full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:39Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:43Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron full mode</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T16:54:49Z</StartDate>
-        <StopDate>2024-09-29T01:33:30Z</StopDate>
+        <StopDate>2024-10-02T09:47:49Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/D/ESA/thd-esa-l2i</ResourceID>
     <ResourceHeader>
       <ResourceName>ion full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:39Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:00:43Z</ReleaseDate>
       <Description>"Full Mode" is a low-time-resolution data product useful for large-scale surveys of THEMIS data. It generally maintains the "full" 32 energies sampled, and have an 88 solid-angle map. Full distribution data are 1-spin snapshots of the plasma with a measurement cadence of either 32 spins (in "Fast-Survey Spacecraft Mode") or 128 spins ("Slow-Survey Spacecraft Mode").</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -51,7 +51,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T16:54:49Z</StartDate>
-        <StopDate>2024-09-29T01:33:00Z</StopDate>
+        <StopDate>2024-10-02T09:46:31Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/D/ESA/thd-peem-all</ResourceID>
     <ResourceHeader>
       <ResourceName>electron onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:50Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:02:03Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-09T23:59:56Z</StartDate>
-        <StopDate>2024-09-29T01:28:51Z</StopDate>
+        <StopDate>2024-10-02T09:44:27Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/D/ESA/thd-peim-all</ResourceID>
     <ResourceHeader>
       <ResourceName>ion onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:01:50Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:02:02Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-09T23:59:56Z</StartDate>
-        <StopDate>2024-09-29T01:28:51Z</StopDate>
+        <StopDate>2024-10-02T09:44:27Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>onboard moments : potential</ResourceName>
       <AlternateName>S/c potential from onboard moments</AlternateName>
-      <ReleaseDate>2024-10-03T04:01:50Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:02:02Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - S/c potential from onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-09T23:59:56Z</StartDate>
-        <StopDate>2024-09-29T01:28:51Z</StopDate>
+        <StopDate>2024-10-02T09:44:27Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/D/FGM/thd-fgm-l</ResourceID>
     <ResourceHeader>
       <ResourceName>0.25 sec (low)</ResourceName>
-      <ReleaseDate>2024-10-03T04:04:17Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:52Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-02-23T01:31:22Z</StartDate>
-        <StopDate>2024-09-28T21:44:45Z</StopDate>
+        <StopDate>2024-10-01T23:24:43Z</StopDate>
       </TimeSpan>
       <Cadence>PT0.25S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/D/FGM/thd-fgm-s</ResourceID>
     <ResourceHeader>
       <ResourceName>3 sec (spin)</ResourceName>
-      <ReleaseDate>2024-10-03T04:04:21Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:04:53Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-02-28T02:55:28Z</StartDate>
-        <StopDate>2024-09-28T21:28:52Z</StopDate>
+        <StopDate>2024-10-02T05:12:16Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/E/ESA/the-esa-l2e</ResourceID>
     <ResourceHeader>
       <ResourceName>electron full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:55Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:02Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron full mode</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T19:54:48Z</StartDate>
-        <StopDate>2024-10-01T12:38:27Z</StopDate>
+        <StopDate>2024-10-02T13:48:34Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/E/ESA/the-esa-l2i</ResourceID>
     <ResourceHeader>
       <ResourceName>ion full mode</ResourceName>
-      <ReleaseDate>2024-10-03T04:00:54Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:01:02Z</ReleaseDate>
       <Description>"Full Mode" is a low-time-resolution data product useful for large-scale surveys of THEMIS data. It generally maintains the "full" 32 energies sampled, and have an 88 solid-angle map. Full distribution data are 1-spin snapshots of the plasma with a measurement cadence of either 32 spins (in "Fast-Survey Spacecraft Mode") or 128 spins ("Slow-Survey Spacecraft Mode").</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -51,7 +51,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-03-07T19:54:48Z</StartDate>
-        <StopDate>2024-10-01T12:40:07Z</StopDate>
+        <StopDate>2024-10-02T13:49:14Z</StopDate>
       </TimeSpan>
       <CadenceMin>PT96.27S</CadenceMin>
       <CadenceMax>PT551.0S</CadenceMax>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/E/ESA/the-peem-all</ResourceID>
     <ResourceHeader>
       <ResourceName>electron onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:02:06Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:02:23Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-10T00:00:17Z</StartDate>
-        <StopDate>2024-10-01T12:40:07Z</StopDate>
+        <StopDate>2024-10-02T13:50:18Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/E/ESA/the-peim-all</ResourceID>
     <ResourceHeader>
       <ResourceName>ion onboard moments</ResourceName>
-      <ReleaseDate>2024-10-03T04:02:06Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:02:22Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -47,7 +47,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-10T00:00:17Z</StartDate>
-        <StopDate>2024-10-01T12:40:07Z</StopDate>
+        <StopDate>2024-10-02T13:50:18Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>onboard moments : potential</ResourceName>
       <AlternateName>S/c potential from onboard moments</AlternateName>
-      <ReleaseDate>2024-10-03T04:02:06Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:02:22Z</ReleaseDate>
       <Description>Electrostatic Analyzer (ESA) data - Level 2 - S/c potential from onboard moments</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
@@ -48,7 +48,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2007-08-10T00:00:17Z</StartDate>
-        <StopDate>2024-10-01T12:40:07Z</StopDate>
+        <StopDate>2024-10-02T13:50:18Z</StopDate>
       </TimeSpan>
       <Cadence>PT3S</Cadence>
     </TemporalDescription>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/E/FGM/the-fgm-l</ResourceID>
     <ResourceHeader>
       <ResourceName>0.25 sec (low)</ResourceName>
-      <ReleaseDate>2024-10-03T04:07:32Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:08:12Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -5,7 +5,7 @@
     <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/THEMIS/E/FGM/the-fgm-s</ResourceID>
     <ResourceHeader>
       <ResourceName>3 sec (spin)</ResourceName>
-      <ReleaseDate>2024-10-03T04:07:46Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:08:20Z</ReleaseDate>
       <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field</Description>
       <Contact>
         <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>daily averages</ResourceName>
       <AlternateName>daily averages / level3 / flares excluded</AlternateName>
-      <ReleaseDate>2024-10-03T04:15:53Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:20:13Z</ReleaseDate>
       <Description>
           SEE Level 3 OVERVIEW:  
           The Solar EUV Experiment (SEE) is comprised of two science components: 
@@ -72,7 +72,7 @@ personnel, and funding agencies should be given.
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2002-01-22T12:00:00Z</StartDate>
-        <StopDate>2024-09-29T12:00:00Z</StopDate>
+        <StopDate>2024-09-30T12:00:00Z</StopDate>
       </TimeSpan>
       <Cadence>PT24H</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>3 min averages</ResourceName>
       <AlternateName>3 min averages / level3a / flares included</AlternateName>
-      <ReleaseDate>2024-10-03T05:27:05Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T05:30:50Z</ReleaseDate>
       <Description>
           SEE Level 3A OVERVIEW:  
           The Solar EUV Experiment (SEE) is comprised of two science components: 
@@ -74,7 +74,7 @@ personnel, and funding agencies should be given.
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2002-01-22T00:00:00Z</StartDate>
-        <StopDate>2024-09-30T23:59:59Z</StopDate>
+        <StopDate>2024-10-01T23:59:59Z</StopDate>
       </TimeSpan>
       <Cadence>PT90M</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>input DSCOVR</ResourceName>
       <AlternateName>Ballistic delay from the Earth to Bepi</AlternateName>
-      <ReleaseDate>2024-10-03T04:12:16Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:13:19Z</ReleaseDate>
       <Description>DSCOVR solar wind 1-hour velocity data is used as model input. A sidereal period of 25.38 days is used in the calculations. Calculation : IRAP.
  
          * delay(days)=(r_bepi-r_earth)/dsc_vpr*1731.46 + angle_bepi_earth/14.1844 
@@ -55,7 +55,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-08-01T00:00:00Z</StartDate>
-        <StopDate>2024-10-01T23:59:00Z</StopDate>
+        <StopDate>2024-10-02T23:59:00Z</StopDate>
       </TimeSpan>
       <Cadence>PT1H</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>input DSCOVR</ResourceName>
       <AlternateName>Ballistic delay from the Earth to PSP</AlternateName>
-      <ReleaseDate>2024-10-03T04:12:16Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:13:19Z</ReleaseDate>
       <Description>DSCOVR solar wind 1-hour velocity data is used as model input. A sidereal period of 25.38 days is used in the calculations. Calculation : IRAP.
  
          * delay(days)=(r_psp-r_earth)/dsc_vpr*1731.46 + angle_psp_earth/14.1844 
@@ -55,7 +55,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-08-01T00:00:00Z</StartDate>
-        <StopDate>2024-10-01T23:59:00Z</StopDate>
+        <StopDate>2024-10-02T23:59:00Z</StopDate>
       </TimeSpan>
       <Cadence>PT1H</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>input DSCOVR</ResourceName>
       <AlternateName>Ballistic delay from the Earth to Solar Orbiter</AlternateName>
-      <ReleaseDate>2024-10-03T04:12:16Z</ReleaseDate>
+      <ReleaseDate>2024-10-04T04:13:19Z</ReleaseDate>
       <Description>DSCOVR solar wind 1-min data is used as model input. A sidereal period of 25.38 days is used in the calculations. Calculation : IRAP.
  
          delay(days)=(r_solo-r_earth)/dsc_vpr*1731.46 + angle_solo_earth/14.1844 
@@ -58,7 +58,7 @@
     <TemporalDescription>
       <TimeSpan>
         <StartDate>2016-08-01T00:00:00Z</StartDate>
-        <StopDate>2024-10-01T23:59:00Z</StopDate>
+        <StopDate>2024-10-02T23:59:00Z</StopDate>
       </TimeSpan>
       <Cadence>PT1H</Cadence>
     </TemporalDescription>
@@ -6,7 +6,7 @@
     <ResourceHeader>
       <ResourceName>SW / Input OMNI</ResourceName>
       <AlternateName>Tao SW Venus / Input OMNI</AlternateName>
-      <ReleaseDate>2024-10-02T20:10:03Z</ReleaseDate>
+      <ReleaseDate>2024-10-03T20:10:03Z</ReleaseDate>
       <Description>OMNI solar wind 1-hour data is used as model input. Calculation : IRAP.</Description>
       <Acknowledgement>TBD</Acknowledgement>
       <Contact>