CDPP / CNES

Commit bbd4e7f047fac0fc72ae162918e5be0b52784228

Authored by Benjamin Renard
1 parent 5df14d57
Exists in juice_jdc and in 1 other branch amdadev

Merge master into amdadev

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Instrument/CDPP-AMDA/ARTEMIS/P1/Models.xml
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5 5 <ResourceID>spase://CNES/Instrument/CDPP-AMDA/ARTEMIS/P1/Models</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>Analytical Models</ResourceName>
8   - <AlternateName>ThemisB different magnetospheric analytical models</AlternateName>
  8 + <AlternateName>Artemis-P1 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Artemis-P1 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
16 16 <InstrumentType>Platform</InstrumentType>
17   - <InvestigationName>ThemisB different magnetospheric analytical models</InvestigationName>
  17 + <InvestigationName>Artemis-P1 different magnetospheric analytical models</InvestigationName>
18 18 <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP1</ObservatoryID>
19 19 </Instrument>
20 20 </Spase>
... ...
Instrument/CDPP-AMDA/ARTEMIS/P2/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>Artemis-P2 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Artemis-P2 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/Cluster1/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>Mars crustal magnetic field analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Mars crustal magnetic field analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/Cluster2/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>Cluster2 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Cluster2 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/Cluster3/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>Cluster3 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Cluster3 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/Cluster4/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>Cluster4 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Cluster4 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/Comets.xml
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... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Comets</ResourceName>
8 8 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Comet Churyumov-Gerasimenko (C-G; P67) - Ephemeris</Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
Instrument/CDPP-AMDA/Ephemerides.xml
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... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Planets and Moons</ResourceName>
8 8 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Planets/Moons Orbitography</Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
Instrument/CDPP-AMDA/Geotail/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>Geotail different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Geotail different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/Giotto/JPA.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>JPA</ResourceName>
8 8 <AlternateName>Johnstone Plasma Analyser</AlternateName>
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>One of two plasma experiments to study the solar wind and charged particles. This instrument measures the three-dimensional energy distribution of positive ions in order to study the interaction between the solar wind and ionised cometary particles.</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Alan.D.Johnstone</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
Instrument/CDPP-AMDA/Giotto/MAG.xml
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... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>MAG</ResourceName>
8 8 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Investigation of the interaction between Comet Halley and the solar wind during the encounter, as well as a study of the interplanetary magnetic field.</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Fritz.M.Neubauer</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
Instrument/CDPP-AMDA/Giotto/RPA.xml
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... ... @@ -7,7 +7,8 @@
7 7 <ResourceName>RPA</ResourceName>
8 8 <AlternateName>Reme Copernic Plasma Experiment</AlternateName>
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>One of two plasma experiments to study the solar wind and charged particles.
  11 + The RPA measured velocity distributions of electrons and composition/distribution of thermal positive ions close to the cometary object.</Description>
11 12 <Contact>
12 13 <PersonID>spase://SMWG/Person/Henri.Reme</PersonID>
13 14 <Role>PrincipalInvestigator</Role>
... ...
Instrument/CDPP-AMDA/ICE/MAG.xml
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... ... @@ -5,8 +5,15 @@
5 5 <ResourceID>spase://CNES/Instrument/CDPP-AMDA/ICE/MAG</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>MAG</ResourceName>
  8 + <AlternateName>Vector Helium Magnetometer</AlternateName>
8 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
9   - <Description>ToDo</Description>
  10 + <Description>The vector helium magnetometer is mounted on the end of a 3 m boom and makes in-situ measurements of
  11 + the ambient magnetic field vector in the frequency range 0-3 Hz. The instrument automatically chooses
  12 + one of eight ranges in which to operate, the four lowest full-scale ranges being +/-4, +/- 14, +/-42,
  13 + and +/- 146 nT. The precision of measurement is 1/256 of the full-scale field values (0.016, 0.055nT, etc.). The absolute accuracy is limited by
  14 + knowledge of the spacecraft magnetic field, which is presently known to better than 0.1 nT. The time
  15 + resolution corresponds to three triaxial samples per second at 1024 bit/s . The magnetometer contains a three- channel spectrum analyzer which
  16 + is connected to the search-coil sensor of the plasma- wave investigation.</Description>
10 17 <Contact>
11 18 <PersonID>spase://SMWG/Person/Edward.J.Smith</PersonID>
12 19 <Role>PrincipalInvestigator</Role>
... ...
Instrument/CDPP-AMDA/Interball-1/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>Interball-1 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Interball-1 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/MAVEN/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>MAVEN : Mars crustal magnetic field analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>MAVEN : Mars crustal magnetic field analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/MEX/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>MEX : Mars crustal magnetic field analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>MEX : Mars crustal magnetic field analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/MGS/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>MGS : Mars crustal magnetic field analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>MGS : Mars crustal magnetic field analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/MMS1/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>MMS1 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>MMS1 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/MMS2/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>MMS2 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>MMS2 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/MMS3/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>MMS3 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>MMS3 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/MMS4/Models.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>MMS4 different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>MMS4 different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/POLAR/Models.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>Polar different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Polar different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/Phobos2/MAG.xml
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... ... @@ -7,7 +7,8 @@
7 7 <ResourceName>MAG</ResourceName>
8 8 <AlternateName>MAGMA</AlternateName>
9 9 <ReleaseDate>2019-11-18T16:00:05Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>The magnetometers on board the Phobos 2 spacecraft provided the opportunity to study the magnetic environment around Mars,
  11 + including regions which have never been explored before, such as at low altitudes (down to 850 km above the surface of Mars) and in the tail. </Description>
11 12 <Contact>
12 13 <PersonID>spase://SMWG/Person/Konrad.Schwingenschuh</PersonID>
13 14 <Role>PrincipalInvestigator</Role>
... ...
Instrument/CDPP-AMDA/Pioneer10/CPI.xml
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... ... @@ -7,7 +7,13 @@
7 7 <ResourceName>CPI</ResourceName>
8 8 <AlternateName>Charged Particle Instrument</AlternateName>
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>This experiment (carried also on Pioneer 11) measured charged-particle composition and spectra using four detector systems:
  11 + (1) the main telescope, consisting of seven elements and providing energy spectra (approximately 3 to 68 MeV for protons and 10 to 150 MeV/nucleon for oxygen), element resolution (through oxygen), and isotope resolution (for H and He);
  12 + (2) the low-energy subsystem telescope, consisting of two elements and using a very small thin first element to extend the high-sensitivity proton measurements below 1 MeV (0.3 to 9 MeV) in the presence of a high gamma-ray background aboard the spacecraft;
  13 + (3) the electron-current detector (ECG), consisting of a beryllium-shield silicon detector operated in current mode to measure high fluxes of electrons with energies above 3 MeV; and
  14 + (4) the fission cell detector, recording fission fragments from the nucleon-induced fission of thorium 232 sandwiched between two large-area silicon detectors to measure fluxes of protons (above 30 MeV) in the presence of high fluxes of electrons.
  15 +
  16 + The experiment sample time was synchronized with the spacecraft spin, permitting sectoring of the readout of the main and low-energy telescopes into eight octants about the spin axis. Data also include the interplanetary region.</Description>
11 17 <Contact>
12 18 <PersonID>spase://SMWG/Person/John.A.Simpson</PersonID>
13 19 <Role>PrincipalInvestigator</Role>
... ...
Instrument/CDPP-AMDA/Pioneer11/CPI.xml
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... ... @@ -7,7 +7,13 @@
7 7 <ResourceName>CPI</ResourceName>
8 8 <AlternateName>Charged Particle Instrument</AlternateName>
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>This experiment (carried also on Pioneer 10) measured charged-particle composition and spectra using four detector systems:
  11 + (1) the main telescope, consisting of seven elements and providing energy spectra (approximately 3 to 68 MeV for protons and 10 to 150 MeV/nucleon for oxygen), element resolution (through oxygen), and isotope resolution (for H and He);
  12 + (2) the low-energy subsystem telescope, consisting of two elements and using a very small thin first element to extend the high-sensitivity proton measurements below 1 MeV (0.3 to 9 MeV) in the presence of a high gamma-ray background aboard the spacecraft;
  13 + (3) the electron-current detector (ECG), consisting of a beryllium-shield silicon detector operated in current mode to measure high fluxes of electrons with energies above 3 MeV; and
  14 + (4) the fission cell detector, recording fission fragments from the nucleon-induced fission of thorium 232 sandwiched between two large-area silicon detectors to measure fluxes of protons (above 30 MeV) in the presence of high fluxes of electrons.
  15 +
  16 + The experiment sample time was synchronized with the spacecraft spin, permitting sectoring of the readout of the main and low-energy telescopes into eight octants about the spin axis. Data also include the interplanetary region.</Description>
11 17 <Contact>
12 18 <PersonID>spase://SMWG/Person/John.A.Simpson</PersonID>
13 19 <Role>PrincipalInvestigator</Role>
... ...
Instrument/CDPP-AMDA/SWARM-A/GNSS.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>GNSS</ResourceName>
8 8 <AlternateName>Global Navigation Satellite System</AlternateName>
9 9 <ReleaseDate>2016-11-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Global Navigation Satellite System</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/R.Haagmans</PersonID>
13 13 <Role>ProjectScientist</Role>
... ...
Instrument/CDPP-AMDA/SWARM-B/GNSS.xml
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... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>GNSS</ResourceName>
8 8 <AlternateName>Global Navigation Satellite System</AlternateName>
9 9 <ReleaseDate>2016-11-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Global Navigation Satellite System</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/R.Haagmans</PersonID>
13 13 <Role>ProjectScientist</Role>
... ...
Instrument/CDPP-AMDA/SWARM-C/GNSS.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>GNSS</ResourceName>
8 8 <AlternateName>Global Navigation Satellite System</AlternateName>
9 9 <ReleaseDate>2016-11-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Global Navigation Satellite System</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/R.Haagmans</PersonID>
13 13 <Role>ProjectScientist</Role>
... ...
Instrument/CDPP-AMDA/THEMIS/A/Models.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>ThemisA different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>ThemisA different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/THEMIS/B/Models.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>ThemisB different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>ThemisB different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/THEMIS/C/Models.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>ThemisC different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>ThemisC different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/THEMIS/D/Models.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>ThemisD different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>ThemisD different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
Instrument/CDPP-AMDA/THEMIS/E/Models.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>Analytical Models</ResourceName>
8 8 <AlternateName>ThemisE different magnetospheric analytical models</AlternateName>
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>ThemisE different magnetospheric analytical models</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/ACE/MFI/ace-mag-real.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>real time</ResourceName>
8 8 <AlternateName>Interplanetary Magnetic Field 60-sec real time Data</AlternateName>
9   - <ReleaseDate>2024-05-22T09:07:09Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T07:07:27Z</ReleaseDate>
10 10 <Description>
11 11 ACE Magnetometer real time, 60-second averages of field magnitude and vectors in GSE and GSM coordinates systems.
12 12 </Description>
... ... @@ -66,7 +66,7 @@
66 66 <TemporalDescription>
67 67 <TimeSpan>
68 68 <StartDate>2024-01-15T00:00:00Z</StartDate>
69   - <StopDate>2024-05-22T08:59:59Z</StopDate>
  69 + <StopDate>2024-05-23T06:59:59Z</StopDate>
70 70 </TimeSpan>
71 71 <Cadence>PT60S</Cadence>
72 72 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/ACE/SWEPAM/ace-swepam-real.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>sw : real time</ResourceName>
8 8 <AlternateName>Solar wind 60-sec real time data</AlternateName>
9   - <ReleaseDate>2024-05-22T09:04:00Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T07:04:14Z</ReleaseDate>
10 10 <Description>
11 11 The ram pressure is calculated using P=rho*Np*Vpยฒ, where rho=1.672622*(1+4*(1/(1-He++_ratio)-1)).
12 12 We use rho=2 here, which corresponds to a ratio of He++ between 4% and 5%.
... ... @@ -63,7 +63,7 @@
63 63 <TemporalDescription>
64 64 <TimeSpan>
65 65 <StartDate>2024-01-15T00:00:00Z</StartDate>
66   - <StopDate>2024-05-22T07:59:59Z</StopDate>
  66 + <StopDate>2024-05-23T05:59:59Z</StopDate>
67 67 </TimeSpan>
68 68 <Cadence>PT60S</Cadence>
69 69 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2e.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2e</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>electron full mode</ResourceName>
8   - <ReleaseDate>2024-05-22T02:00:23Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:00:23Z</ReleaseDate>
  9 + <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron full mode</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
12 12 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2i.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,7 +5,7 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2i</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>ion full mode</ResourceName>
8   - <ReleaseDate>2024-05-22T02:00:23Z</ReleaseDate>
  8 + <ReleaseDate>2024-05-23T02:00:23Z</ReleaseDate>
9 9 <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>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peem-all.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peem-all</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>electron onboard moments</ResourceName>
8   - <ReleaseDate>2024-05-22T02:01:22Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:01:21Z</ReleaseDate>
  9 + <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peim-all.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peim-all</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>ion onboard moments</ResourceName>
8   - <ReleaseDate>2024-05-22T02:01:22Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:01:21Z</ReleaseDate>
  9 + <Description>Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P1/Ephemeris/athp1-orb-all.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,7 +5,7 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/Ephemeris/athp1-orb-all</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>orbit</ResourceName>
8   - <ReleaseDate>2024-05-22T02:03:30Z</ReleaseDate>
  8 + <ReleaseDate>2024-05-23T02:03:23Z</ReleaseDate>
9 9 <Description>
10 10 ARTEMIS P1 ephemeris
11 11 </Description>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-l.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-l</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>0.25 sec (low)</ResourceName>
8   - <ReleaseDate>2024-05-22T02:03:30Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:03:23Z</ReleaseDate>
  9 + <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
12 12 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-s.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-s</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>3 sec (spin)</ResourceName>
8   - <ReleaseDate>2024-05-22T02:03:32Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:03:26Z</ReleaseDate>
  9 + <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
12 12 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2e.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2e</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>electron full mode</ResourceName>
8   - <ReleaseDate>2024-05-22T02:00:29Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:00:29Z</ReleaseDate>
  9 + <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron full mode</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
12 12 <Role>TechnicalContact</Role>
... ... @@ -48,7 +48,7 @@
48 48 <TemporalDescription>
49 49 <TimeSpan>
50 50 <StartDate>2011-07-17T00:00:00Z</StartDate>
51   - <StopDate>2024-05-18T22:01:44Z</StopDate>
  51 + <StopDate>2024-05-20T16:42:11Z</StopDate>
52 52 </TimeSpan>
53 53 <CadenceMin>PT96.27S</CadenceMin>
54 54 <CadenceMax>PT551.0S</CadenceMax>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2i.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,7 +5,7 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2i</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>ion full mode</ResourceName>
8   - <ReleaseDate>2024-05-22T02:00:28Z</ReleaseDate>
  8 + <ReleaseDate>2024-05-23T02:00:29Z</ReleaseDate>
9 9 <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>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
... ... @@ -52,7 +52,7 @@
52 52 <TemporalDescription>
53 53 <TimeSpan>
54 54 <StartDate>2011-07-17T00:00:00Z</StartDate>
55   - <StopDate>2024-05-18T22:00:05Z</StopDate>
  55 + <StopDate>2024-05-20T16:43:25Z</StopDate>
56 56 </TimeSpan>
57 57 <CadenceMin>PT96.27S</CadenceMin>
58 58 <CadenceMax>PT551.0S</CadenceMax>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peem-all.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peem-all</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>electron onboard moments</ResourceName>
8   - <ReleaseDate>2024-05-22T02:01:33Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:01:31Z</ReleaseDate>
  9 + <Description>Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ... @@ -48,7 +48,7 @@
48 48 <TemporalDescription>
49 49 <TimeSpan>
50 50 <StartDate>2011-07-17T00:00:00Z</StartDate>
51   - <StopDate>2024-05-18T21:54:28Z</StopDate>
  51 + <StopDate>2024-05-19T00:00:29Z</StopDate>
52 52 </TimeSpan>
53 53 <Cadence>PT3S</Cadence>
54 54 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peim-all.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peim-all</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>ion onboard moments</ResourceName>
8   - <ReleaseDate>2024-05-22T02:01:32Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:01:30Z</ReleaseDate>
  9 + <Description>Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Vassilis.Angelopoulos</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ... @@ -48,7 +48,7 @@
48 48 <TemporalDescription>
49 49 <TimeSpan>
50 50 <StartDate>2011-07-17T00:00:00Z</StartDate>
51   - <StopDate>2024-05-18T21:54:28Z</StopDate>
  51 + <StopDate>2024-05-19T00:00:29Z</StopDate>
52 52 </TimeSpan>
53 53 <Cadence>PT3S</Cadence>
54 54 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-l.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-l</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>0.25 sec (low)</ResourceName>
8   - <ReleaseDate>2024-05-22T02:03:48Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:03:39Z</ReleaseDate>
  9 + <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
12 12 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-s.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,8 +5,8 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-s</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>3 sec (spin)</ResourceName>
8   - <ReleaseDate>2024-05-22T02:03:50Z</ReleaseDate>
9   - <Description>ToDo</Description>
  8 + <ReleaseDate>2024-05-23T02:03:42Z</ReleaseDate>
  9 + <Description>Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Uli.Auster</PersonID>
12 12 <Role>TechnicalContact</Role>
... ... @@ -47,7 +47,7 @@
47 47 <TemporalDescription>
48 48 <TimeSpan>
49 49 <StartDate>2011-07-17T00:00:00Z</StartDate>
50   - <StopDate>2024-05-18T18:17:41Z</StopDate>
  50 + <StopDate>2024-05-19T00:02:50Z</StopDate>
51 51 </TimeSpan>
52 52 <Cadence>PT4S</Cadence>
53 53 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MGF/bepi-mgf-venus2.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,9 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Venus flyby #2</ResourceName>
8 8 <ReleaseDate>2021-10-12T14:05:27Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region.
  10 +
  11 +Magnetic field.</Description>
10 12 <Contact>
11 13 <PersonID>spase://SMWG/Person/Wolfgang.Baumjohann</PersonID>
12 14 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>prime parameters : electrons</ResourceName>
8 8 <AlternateName>Cluster 1 Prime Parameter RAPID Data</AlternateName>
9 9 <ReleaseDate>2012-03-06T17:14:59Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Prime Parameters RAPID Electron Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>prime parameters : protons</ResourceName>
8 8 <AlternateName>Cluster 1 Prime Parameter RAPID Data</AlternateName>
9 9 <ReleaseDate>2012-03-06T17:15:38Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Prime Parameters RAPID Protons Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>prime parameters : electrons</ResourceName>
8 8 <AlternateName>Cluster 2 Prime Parameter RAPID Data</AlternateName>
9 9 <ReleaseDate>2012-03-06T19:01:05Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Prime Parameters RAPID Electron Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,13 +7,7 @@
7 7 <ResourceName>prime parameters : protons</ResourceName>
8 8 <AlternateName>Cluster 2 Prime Parameter RAPID Data</AlternateName>
9 9 <ReleaseDate>2012-03-06T19:01:43Z</ReleaseDate>
10   - <Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
11   - Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV
12   - for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. For more details of the
13   - Cluster mission, the spacecraft, and its instruments, see the report Cluster: mission,
14   - payload and supporting activities, March 1993, ESA SP-1159, and the included article RAPID:
15   - The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
16   - this information was obtained.</Description>
  10 + <Description>Prime Parameters RAPID Protons Data</Description>
17 11 <Contact>
18 12 <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
19 13 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>electrons</ResourceName>
8 8 <AlternateName>Cluster 3 Prime Parameter RAPID Data</AlternateName>
9 9 <ReleaseDate>2012-03-06T16:11:35Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Prime Parameters RAPID Electron Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>protons</ResourceName>
8 8 <AlternateName>Cluster 3 Prime Parameter RAPID Data</AlternateName>
9 9 <ReleaseDate>2012-03-06T16:12:23Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Prime Parameters RAPID Protons Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>electrons</ResourceName>
8 8 <AlternateName>Cluster 4 Prime Parameter RAPID Data</AlternateName>
9 9 <ReleaseDate>2012-03-06T19:39:56Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Prime Parameters RAPID Electron Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>protons</ResourceName>
8 8 <AlternateName>Cluster 4 Prime Parameter RAPID Data</AlternateName>
9 9 <ReleaseDate>2012-03-06T19:40:38Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Prime Parameters RAPID Protons Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
13 13 <Role>TechnicalContact</Role>
... ...
NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-1m.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>sw : 1 m</ResourceName>
8 8 <AlternateName>solar wind parameters</AlternateName>
9   - <ReleaseDate>2024-05-22T02:12:40Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T02:12:59Z</ReleaseDate>
10 10 <Description>Faraday Cup (FC) measures the solar wind bulk properties (wind speed, density and temperature).
11 11 The ram pressure is calculated using P=rho*Np*Vpยฒ, where rho=1.672622*(1+4*(1/(1-He++_ratio)-1)).
12 12 We use rho=2 here, which corresponds to a ratio of He++ between 4% and 5%.</Description>
... ... @@ -61,7 +61,7 @@
61 61 <TemporalDescription>
62 62 <TimeSpan>
63 63 <StartDate>2016-08-01T00:00:00Z</StartDate>
64   - <StopDate>2024-05-20T23:59:00Z</StopDate>
  64 + <StopDate>2024-05-21T23:59:00Z</StopDate>
65 65 </TimeSpan>
66 66 <Cadence>PT60S</Cadence>
67 67 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-3s.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>sw : 3 s</ResourceName>
8 8 <AlternateName>solar wind parameters</AlternateName>
9   - <ReleaseDate>2024-05-22T02:14:11Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T02:14:27Z</ReleaseDate>
10 10 <Description>Faraday Cup (FC) measures the solar wind bulk properties (wind speed, density and temperature).
11 11 The ram pressure is calculated using P=rho*Np*Vpยฒ, where rho=1.672622*(1+4*(1/(1-He++_ratio)-1)).
12 12 We use rho=2 here, which corresponds to a ratio of He++ between 4% and 5%.</Description>
... ... @@ -61,7 +61,7 @@
61 61 <TemporalDescription>
62 62 <TimeSpan>
63 63 <StartDate>2016-08-01T00:00:00Z</StartDate>
64   - <StopDate>2024-05-20T23:59:40Z</StopDate>
  64 + <StopDate>2024-05-21T23:59:40Z</StopDate>
65 65 </TimeSpan>
66 66 <Cadence>PT3S</Cadence>
67 67 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1m.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>1 m</ResourceName>
8 8 <AlternateName>interplanetary magnetic field</AlternateName>
9   - <ReleaseDate>2024-05-22T02:06:13Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T02:06:26Z</ReleaseDate>
10 10 <Description>Solar wind magnetic field vector (sampling 60s)</Description>
11 11 <Acknowledgement>NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.</Acknowledgement>
12 12 <Contact>
... ... @@ -60,7 +60,7 @@
60 60 <TemporalDescription>
61 61 <TimeSpan>
62 62 <StartDate>2016-08-01T00:00:00Z</StartDate>
63   - <StopDate>2024-05-20T23:59:00Z</StopDate>
  63 + <StopDate>2024-05-21T23:59:00Z</StopDate>
64 64 </TimeSpan>
65 65 <Cadence>PT60S</Cadence>
66 66 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1s.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>1 s</ResourceName>
8 8 <AlternateName>interplanetary magnetic field</AlternateName>
9   - <ReleaseDate>2024-05-22T02:11:27Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T02:11:47Z</ReleaseDate>
10 10 <Description>Solar wind magnetic field vector (sampling 1s)</Description>
11 11 <Acknowledgement>NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.</Acknowledgement>
12 12 <Contact>
... ... @@ -58,7 +58,7 @@
58 58 <TemporalDescription>
59 59 <TimeSpan>
60 60 <StartDate>2016-08-01T00:00:00Z</StartDate>
61   - <StopDate>2024-05-20T23:59:59Z</StopDate>
  61 + <StopDate>2024-05-21T23:59:59Z</StopDate>
62 62 </TimeSpan>
63 63 <Cadence>PT60S</Cadence>
64 64 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/Ephemerides/mars-deimos-orb.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Deimos</ResourceName>
8 8 <ReleaseDate>2022-03-10T10:35:55Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Deimos is the smaller and outer of the two natural satellites of Mars.</Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Phobos - 1 min</ResourceName>
8 8 <ReleaseDate>2022-03-10T09:51:00Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Phobos is the innermost and larger of the two natural satellites of Mars.</Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb1s.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Phobos - 1 sec</ResourceName>
8 8 <ReleaseDate>2022-03-18T08:45:15Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Phobos is the innermost and larger of the two natural satellites of Mars.</Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/Ephemerides/moon-earth-all.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Earth Moon</ResourceName>
8 8 <ReleaseDate>2019-08-23T15:34:00Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>The Moon is Earth's only natural satellite. It orbits at an average distance of 384,400 km (238,900 mi), about 30 times the diameter of Earth.</Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/Giotto/Ephemeris/gio-orb-comet.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>flyby comet/halley</ResourceName>
8 8 <ReleaseDate>2014-06-18T12:59:54Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Giotto spacecraft positions in various coordinate systems</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
12 12 <Role>MetadataContact</Role>
... ...
NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-a.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>alphas</ResourceName>
8 8 <AlternateName>HERS</AlternateName>
9 9 <ReleaseDate>2014-06-16T12:53:01Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>ION MASS SPECTROMETER - High-Energy Range Spectrometer - Alphas data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>GeneralContact</Role>
... ...
NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-his.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>heavy ions countrate</ResourceName>
8 8 <AlternateName>HIS</AlternateName>
9 9 <ReleaseDate>2014-06-17T16:59:11Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>ION MASS SPECTROMETER - High Intensity Spectrometer - Heavy ions countrate data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>GeneralContact</Role>
... ...
NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-p.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>protons</ResourceName>
8 8 <AlternateName>HERS</AlternateName>
9 9 <ReleaseDate>2014-06-16T12:46:56Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>ION MASS SPECTROMETER - High-Energy Range Spectrometer - Protons data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>GeneralContact</Role>
... ...
NumericalData/CDPP-AMDA/Giotto/JPA/gio-jpa-psa.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>protons</ResourceName>
8 8 <ReleaseDate>2014-06-13T14:06:35Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Johnstone Plasma Analyser - protons data.</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
12 12 <Role>GeneralContact</Role>
... ...
NumericalData/CDPP-AMDA/Giotto/MAG/gio-mag-psa.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>magnetic field</ResourceName>
8 8 <ReleaseDate>2014-06-12T09:43:08Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Giotto Magnetometer Experiment data</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
12 12 <Role>GeneralContact</Role>
... ...
NumericalData/CDPP-AMDA/Giotto/RPA/gio-rpa1-corr.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>density elec</ResourceName>
8 8 <ReleaseDate>2014-05-27T15:16:06Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>RPA-(Reme) Copernic Plasma Experiment - Eletrons density</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
12 12 <Role>MetadataContact</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/CORALL/intt-crl-kp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>key parameters</ResourceName>
8 8 <ReleaseDate>2013-05-24T11:06:59Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>CORALL is the ion spectrometer with energy range 30eV - 25keV onboard INTERBALL/TAIL satellite. It has a fan-shape aperture wich plane has a sunward spin axis of spacecraft. The full distribution function is obtained for one spacecraft revolution. So for every revolution plasma parameters ( V, T, N) can be calculated. </Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Andrey.Fedorov</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1s.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>spectra : sunward</ResourceName>
8 8 <AlternateName>Electron Spectra : Sunward Flow</AlternateName>
9 9 <ReleaseDate>2004-12-16T17:44:55Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1t.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>time profiles : sunward</ResourceName>
8 8 <AlternateName>Electron Time Profiles : Sunward Flow</AlternateName>
9 9 <ReleaseDate>2004-12-02T19:47:03Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2s.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>spectra : tailward</ResourceName>
8 8 <AlternateName>Electron Spectra : Tailward Flow</AlternateName>
9 9 <ReleaseDate>2004-12-16T16:51:20Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2t.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>time profiles : tailward</ResourceName>
8 8 <AlternateName>Electron Time Profiles : Tailward Flow</AlternateName>
9 9 <ReleaseDate>2004-12-02T14:45:57Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3s.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>spectra : sunward</ResourceName>
8 8 <AlternateName>Ion Spectra : Sunward Flow</AlternateName>
9 9 <ReleaseDate>2004-12-16T17:45:33Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3t.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>time profiles : sunward</ResourceName>
8 8 <AlternateName>Ion Time Profiles : Sunward Flow</AlternateName>
9 9 <ReleaseDate>2004-12-02T19:48:02Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4s.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>spectra : tailward</ResourceName>
8 8 <AlternateName>Ion Spectra : Tailward Flow</AlternateName>
9 9 <ReleaseDate>2004-12-16T17:46:24Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4t.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>time profiles : tailward</ResourceName>
8 8 <AlternateName>Ion Time Profiles : Tailward Flow</AlternateName>
9 9 <ReleaseDate>2004-12-02T19:49:42Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.</Description>
11 11 <Contact>
12 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/iball-mif-hr.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>high resolution</ResourceName>
8 8 <ReleaseDate>2020-07-10T10:55:42Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>This data set contains the DC/AC Magnetic Field (0-64 Hz and 1 Hz - 40 kHz) in GSM from the MIF-M magnetometer on board Interball-Tail.</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Stanislav.A.Romanov</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/intt-fm-kp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>key parameters</ResourceName>
8 8 <ReleaseDate>2012-03-06T15:38:45Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Interball Tail Magnetic Field 2-min key parameters, GSE and GSM Coordinates</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/Ramona.L.Kessel</PersonID>
12 12 <Role>DataProducer</Role>
... ...
NumericalData/CDPP-AMDA/IRM/ORBIT/irm-orb-all.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>orbit</ResourceName>
8 8 <AlternateName>ephemeris</AlternateName>
9 9 <ReleaseDate>2020-02-07T15:35:31Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>AMPTE/IRM spacecraft positions in various coordinate systems</Description>
11 11 <Acknowledgement>User will acknowledge the AMPTE/IRM team in any publication resulting from the use of these data.
12 12 </Acknowledgement>
13 13 <Contact>
... ...
NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-aa.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>aa</ResourceName>
8 8 <AlternateName>aa IAGA-endorsed magnetic activity index</AlternateName>
9   - <ReleaseDate>2024-05-22T02:04:57Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T02:05:03Z</ReleaseDate>
10 10 <Description>Index which purpose is to measure the amplitude of global geomagnetic activity during 3-hour intervals normalized to geomagnetic latitude ยฑ50ยฐ. aa was introduced to monitor geomagnetic activity over the longest possible time period.</Description>
11 11 <Acknowledgement>ISGI website at EOST; License: CC BY-NC https://creativecommons.org/licenses/by-nc/4.0/</Acknowledgement>
12 12 <Contact>
... ... @@ -53,7 +53,7 @@
53 53 <TemporalDescription>
54 54 <TimeSpan>
55 55 <StartDate>1975-01-01T00:00:00Z</StartDate>
56   - <StopDate>2024-05-19T21:00:00Z</StopDate>
  56 + <StopDate>2024-05-20T21:00:00Z</StopDate>
57 57 </TimeSpan>
58 58 <Cadence>PT3H</Cadence>
59 59 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-am.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>am</ResourceName>
8 8 <AlternateName>am IAGA-endorsed magnetic activity index</AlternateName>
9   - <ReleaseDate>2024-05-22T02:04:57Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T02:05:04Z</ReleaseDate>
10 10 <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>
11 11 <Acknowledgement>ISGI website at EOST; License: CC BY-NC https://creativecommons.org/licenses/by-nc/4.0/</Acknowledgement>
12 12 <Contact>
... ... @@ -55,7 +55,7 @@
55 55 <TemporalDescription>
56 56 <TimeSpan>
57 57 <StartDate>1975-01-01T00:00:00Z</StartDate>
58   - <StopDate>2024-05-19T21:00:00Z</StopDate>
  58 + <StopDate>2024-05-20T21:00:00Z</StopDate>
59 59 </TimeSpan>
60 60 <Cadence>PT3H</Cadence>
61 61 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-dst.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Dst</ResourceName>
8 8 <AlternateName>Disturbance Stormtime index</AlternateName>
9   - <ReleaseDate>2024-05-22T02:04:58Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T02:05:04Z</ReleaseDate>
10 10 <Description> Dst index is taken from the WDC (World Data Center) at Kyoto.
11 11 Processing Level :
12 12 * FINAL : 1970 - 2014
... ... @@ -66,7 +66,7 @@
66 66 <TemporalDescription>
67 67 <TimeSpan>
68 68 <StartDate>1970-01-01T00:00:00Z</StartDate>
69   - <StopDate>2024-05-19T23:00:00Z</StopDate>
  69 + <StopDate>2024-05-20T23:00:00Z</StopDate>
70 70 </TimeSpan>
71 71 <Cadence>PT1H</Cadence>
72 72 </TemporalDescription>
... ...
NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ele.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,7 +5,7 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ele</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>electron counts</ResourceName>
8   - <ReleaseDate>2024-05-22T03:17:19Z</ReleaseDate>
  8 + <ReleaseDate>2024-05-23T03:12:49Z</ReleaseDate>
9 9 <Description>High resolution particle count rate data from AMBRE instruments ELE1, ELE2, ELE3 and ELE4 detection heads onboard JASON3 satellite </Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/Denis.Payan</PersonID>
... ...
NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ion.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,7 +5,7 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ion</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>ion counts</ResourceName>
8   - <ReleaseDate>2024-05-22T03:17:20Z</ReleaseDate>
  8 + <ReleaseDate>2024-05-23T03:12:50Z</ReleaseDate>
9 9 <Description>High resolution particle count rate data from AMBRE instruments ION1, ION2, ION3 and ION4 detection heads onboard JASON3 satellite </Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/Denis.Payan</PersonID>
... ...
NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-mag.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,7 +5,7 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-mag</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>mag</ResourceName>
8   - <ReleaseDate>2024-05-22T03:17:19Z</ReleaseDate>
  8 + <ReleaseDate>2024-05-23T03:12:48Z</ReleaseDate>
9 9 <Description>Calculated magnetic field using ONERA-DESP library internal fields: DGRF/IGRF External field (Olson and Pfitzer, 1974)</Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/Denis.Payan</PersonID>
... ...
NumericalData/CDPP-AMDA/JASON3/Ephemeris/jason-amb-pos.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>orbit</ResourceName>
8 8 <AlternateName>JASON3 position in GEO coordinates, L and L* parameters</AlternateName>
9   - <ReleaseDate>2024-05-22T03:17:21Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T03:12:50Z</ReleaseDate>
10 10 <Description>xyz in GEO : Origin = Earth's center of mass. X = Intersec
11 11 tion of Greenwich meridian and geographic equator. Z = Geographic North Pole. Y = c
12 12 ompletes a right-handed Cartesian triad</Description>
... ...
NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep1-clb.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,9 @@
6 6 <ResourceHeader>
7 7 <ResourceName>diff fluxes</ResourceName>
8 8 <ReleaseDate>2024-04-02T00:23:56Z</ReleaseDate>
9   - <Description>MAVEN SEP 1 Calibrated Ion (without mass discrimination) and Electron Spectra in Forward/Rear look directions (#/cm^2/sec/ster/keV) : Parker / anti-Parker spiral and perpendicular directions
  9 + <Description>MAVEN SEP 1 Calibrated Ion (without mass discrimination) and Electron Spectra in Forward/Rear look directions (#/cm^2/sec/ster/keV) : Parker / anti-Parker spiral and perpendicular directions.
  10 +
  11 + Attenuator state: 0=error, 1=open, 2=closed, 3=mixed
10 12 </Description>
11 13 <Acknowledgement>Principal Investigator : Davin Larson, SSL, Berkeley</Acknowledgement>
12 14 <Contact>
... ...
NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep2-clb.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,6 +7,8 @@
7 7 <ResourceName>diff fluxes</ResourceName>
8 8 <ReleaseDate>2024-04-02T00:29:52Z</ReleaseDate>
9 9 <Description>MAVEN SEP 1 Calibrated Ion (without mass discrimination) and Electron Spectra in Forward/Rear look directions (#/cm^2/sec/ster/keV) : Parker / anti-Parker spiral and perpendicular directions
  10 +
  11 + Attenuator state: 0=error, 1=open, 2=closed, 3=mixed
10 12 </Description>
11 13 <Acknowledgement>Principal Investigator : Davin Larson, SSL, Berkeley</Acknowledgement>
12 14 <Contact>
... ...
NumericalData/CDPP-AMDA/MGS/MAG/mgs-mag-mso.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>orbit mars</ResourceName>
8 8 <ReleaseDate>2014-05-02T16:10:17Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>Calibrated data set from the Magnetometer instrument on the Mars Global Surveyor spacecraft, collected during the Mapping phase of the mission and expressed in Sun-State and Planetocentric coordinates.</Description>
10 10 <Contact>
11 11 <PersonID>spase://SMWG/Person/John.E.P.Connerney</PersonID>
12 12 <Role>GeneralContact</Role>
... ...
NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-dce-brst.xml
  Diff comments   View file @bbd4e7f
... ... @@ -7,7 +7,7 @@
7 7 <ResourceName>dc e-field</ResourceName>
8 8 <AlternateName>dc electric field / burst / l2</AlternateName>
9 9 <ReleaseDate>2024-03-26T05:27:41Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>Electric Double Probe, Three-Dimensional Electric Field, Level 2, Burst Mode Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-dce.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,8 +6,8 @@
6 6 <ResourceHeader>
7 7 <ResourceName>dc e-field</ResourceName>
8 8 <AlternateName>dc electric field / fast / l2</AlternateName>
9   - <ReleaseDate>2024-05-22T02:39:41Z</ReleaseDate>
10   - <Description>ToDo</Description>
  9 + <ReleaseDate>2024-05-23T02:39:00Z</ReleaseDate>
  10 + <Description>Electric Double Probe, Quick-Look Three-Dimensional Electric Field, Level 2, Fast Survey Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-hfesp.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,8 +6,8 @@
6 6 <ResourceHeader>
7 7 <ResourceName>e spectral density</ResourceName>
8 8 <AlternateName>ac electric field spectral density / srvy / l2</AlternateName>
9   - <ReleaseDate>2024-05-22T02:39:24Z</ReleaseDate>
10   - <Description>ToDo</Description>
  9 + <ReleaseDate>2024-05-23T02:38:45Z</ReleaseDate>
  10 + <Description>Electric Double Probe, High-Frequency AC Electric Field Spectra, Level 2, Survey Data, Level 1B AC Electric Field Data</Description>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-scpot.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,8 +6,8 @@
6 6 <ResourceHeader>
7 7 <ResourceName>scpot</ResourceName>
8 8 <AlternateName>sc potential / fast / l2</AlternateName>
9   - <ReleaseDate>2024-05-22T02:39:56Z</ReleaseDate>
10   - <Description>ToDo</Description>
  9 + <ReleaseDate>2024-05-23T02:39:15Z</ReleaseDate>
  10 + <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>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/MMS/MMS1/Ephemeris/mms1-orb-t89d.xml
  Diff comments   View file @bbd4e7f
... ... @@ -5,7 +5,7 @@
5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS1/Ephemeris/mms1-orb-t89d</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>orbit t89d</ResourceName>
8   - <ReleaseDate>2024-05-22T02:42:18Z</ReleaseDate>
  8 + <ReleaseDate>2024-05-23T02:41:26Z</ReleaseDate>
9 9 <Description>MMS1 position</Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/M.G.Henderson</PersonID>
... ...
NumericalData/CDPP-AMDA/MMS/MMS1/FGM/mms1-fgm-srvy.xml
  Diff comments   View file @bbd4e7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>survey</ResourceName>
8 8 <AlternateName>survey</AlternateName>
9   - <ReleaseDate>2024-05-22T02:41:16Z</ReleaseDate>
  9 + <ReleaseDate>2024-05-23T02:40:31Z</ReleaseDate>
10 10 <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
11 11 from AFG. Because AFG and DFG are cross-calibrated on an orbit-averaged basis,
12 12 small differences in offset may be observed between Level2 burst and survey mode
... ...