CDPP / CNES

Commit ba44a06de823a3bc80e01fe45a558fc9c76fb622

Authored by Benjamin Renard
1 parent 854b25c3
Exists in cleanup_registry_merged and in 2 other branches cleanup_registry, cleanup_registry_master

Move Person/*.xml into Person/CDPP-AMDA/*.xml

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Instrument/CDPP-AMDA/ACE/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>ACE spacecraft positions</Description>
11 11 <Acknowledgement></Acknowledgement>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
14 14 <Role>TechnicalContact</Role>
15 15 </Contact>
16 16 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/ACE/SWEPAM.xml
  Diff comments   View file @ba44a06
... ... @@ -28,7 +28,7 @@
28 28 </Description>
29 29 <Contact>
30 30 <!-- David McComas -->
31   - <PersonID>spase://CNES/Person/David.J.McComas</PersonID>
  31 + <PersonID>spase://CNES/Person/CDPP-AMDA/David.J.McComas</PersonID>
32 32 <Role>CoInvestigator</Role>
33 33 </Contact>
34 34 <Contact>
... ...
Instrument/CDPP-AMDA/ARTEMIS/P1/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/ARTEMIS/P2/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Bepi/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>Bepi Ephemeris are calculated in IRAP by using BepiColombo SPICE kernels</Description>
11 11 <Acknowledgement/>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Marc.Sitja</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Marc.Sitja</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <PriorID/>
... ...
Instrument/CDPP-AMDA/Bepi/MEA1.xml
  Diff comments   View file @ba44a06
... ... @@ -13,11 +13,11 @@
13 13 The Mercury Electron Analyzers have been developed at IRAP with the support of CNES.</Description>
14 14 <Acknowledgement/>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/Yoshifumi.Saito</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yoshifumi.Saito</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 <Contact>
20   - <PersonID>spase://CNES/Person/Nicolas.Andre</PersonID>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Nicolas.Andre</PersonID>
21 21 <Role>CoInvestigator</Role>
22 22 </Contact>
23 23 <PriorID/>
... ...
Instrument/CDPP-AMDA/Bepi/MEA2.xml
  Diff comments   View file @ba44a06
... ... @@ -13,11 +13,11 @@
13 13 The Mercury Electron Analyzers have been developed at IRAP with the support of CNES.</Description>
14 14 <Acknowledgement/>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/Yoshifumi.Saito</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yoshifumi.Saito</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 <Contact>
20   - <PersonID>spase://CNES/Person/Nicolas.Andre</PersonID>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Nicolas.Andre</PersonID>
21 21 <Role>CoInvestigator</Role>
22 22 </Contact>
23 23 <PriorID/>
... ...
Instrument/CDPP-AMDA/Bepi/MIA.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>ToDo</Description>
11 11 <Acknowledgement/>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Yoshifumi.Saito</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yoshifumi.Saito</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <PriorID/>
... ...
Instrument/CDPP-AMDA/Bepi/MPO-MAG.xml
  Diff comments   View file @ba44a06
... ... @@ -29,11 +29,11 @@
29 29 due to magnetospheric processes. </Description>
30 30 <Acknowledgement/>
31 31 <Contact>
32   - <PersonID>spase://CNES/Person/Daniel.Heyner</PersonID>
  32 + <PersonID>spase://CNES/Person/CDPP-AMDA/Daniel.Heyner</PersonID>
33 33 <Role>PrincipalInvestigator</Role>
34 34 </Contact>
35 35 <Contact>
36   - <PersonID>spase://CNES/Person/C.Carr</PersonID>
  36 + <PersonID>spase://CNES/Person/CDPP-AMDA/C.Carr</PersonID>
37 37 <Role>CoInvestigator</Role>
38 38 </Contact>
39 39 <PriorID/>
... ...
Instrument/CDPP-AMDA/Cassini/CAPS.xml
  Diff comments   View file @ba44a06
... ... @@ -13,7 +13,7 @@
13 13 * the Ion Mass Spectrometer (IMS), which provides species-resolved measurements of the flux of positively charged atomic and molecular ions as a function of energy/charge vs. aperture entrydirection. Its energy range is 1 eV to 50 keV. </Description>
14 14 <Acknowledgement/>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/J.Waite</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/J.Waite</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cassini/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -13,7 +13,7 @@
13 13 </Description>
14 14 <Acknowledgement/>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 <Contact>
... ...
Instrument/CDPP-AMDA/Cassini/MAG.xml
  Diff comments   View file @ba44a06
... ... @@ -20,7 +20,7 @@
20 20 orbiter's spacecraft body.</Description>
21 21 <Acknowledgement/>
22 22 <Contact>
23   - <PersonID>spase://CNES/Person/Michele.Dougherty</PersonID>
  23 + <PersonID>spase://CNES/Person/CDPP-AMDA/Michele.Dougherty</PersonID>
24 24 <Role>PrincipalInvestigator</Role>
25 25 </Contact>
26 26 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cassini/Moons_Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>Ephemeris for Saturn moons, some special coordinate systems. 'Regular' ephemeris are in "Astronomical Objects Ephemerides, Saturn Moons" </Description>
11 11 <Acknowledgement/>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <Contact>
... ...
Instrument/CDPP-AMDA/Cluster1/CIS-CODIF.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2011-02-04T15:37:46Z</ReleaseDate>
10 10 <Description>This instrument (CIS: Cluster Ion Spectrometry) is capable of obtaining full 3D ion distributions with high time resolution (in one spacecraft spin) and mass-per-charge resolution. The experiment consists of two different instruments, a Hot Ion Analyzer (HIA) and a time-of-flight Ion Composition and Distribution Function analyzer (CODIF). Extensive on-board processing is done, within its dual-processor Data Processing System (DPS). CODIF determines the distributions of the major ion species with energies from spacecraft potential to 40 KeV/charge with an angular resolution of 22.5 x 10.25 degrees and with two different sensitivities. The CODIF instrument uses electrostatic deflection to select by energy per charge, with subsequent time-of-flight analysis. The sensor primarily covers the energy range 0.02--40 KeV/charge, but with additional pre-acceleration for energies below 25 eV/charge, the range is extended to energies as low as the spacecraft potential. The HIA does not measure mass, but extends the dynamic range to the highest ion fluxes, and has angular resolution capability of 5.6 x 5.6 degrees for ion-beam and solar-wind measurements. The HIA is a symmetric quadrispherical analyzer of top-hat geometry, and uses microchannel-plate electron multipliers and position encoding by discrete anodes. A 2D distribution is obtained once per 62.5 ms, and a full 3D distribution of ions in the energy range ~5 eV/charge to 32 KeV/charge is obtained every 4 s. For more details of the Cluster mission, the spacecraft, and its instruments, see the report ``Cluster: mission, payload and supporting activities,'' March 1993, ESA SP-1159, and the included article ``The Cluster Ion Spectrometry Experiment,'' by H. Reme et al., from which this information was obtained.</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Jannis.Dandouras</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jannis.Dandouras</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster1/CIS-HIA.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>The HIA is a symmetric quadrispherical analyzer of top-hat geometry, and uses microchannel-plate electron multipliers and position encoding by discrete anodes. A 2D distribution is obtained once per 62.5 ms, and a full 3D distribution of ions in the energy range ~5 eV/charge to 32 KeV/charge is obtained every 4 s. For more details of the Cluster mission, the spacecraft, and its instruments, see the report ``Cluster: mission, payload and supporting activities,'' March 1993, ESA SP-1159, and the included article ``The Cluster Ion Spectrometry Experiment,'' by H. Reme et al., from which this information was obtained.</Description>
11 11 <Acknowledgement>Principal Investigator: Iannis Dandouras</Acknowledgement>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Jannis.Dandouras</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jannis.Dandouras</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster1/EFW.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>The EFW (Electric Field and Waves) instrument consists of four orthogonal spherical sensors deployed from 50 m cable booms in the spin plane of the spacecraft, plus four deployment units and a main electronics unit. Each deployment unit deploys a multiconductor cable and tip-mounted spherical sensor. Each opposing pair of cables will be symmetrically deployed to a tip-to-tip distance of approximately 100 m, except for about a week at the beginning of the mission when 70 m will be used for one boom pair (the Z-booms) and 100 m for the other pair. The potentials of the spherical sensor and nearby conductors are controlled by the microprocessor to minimize errors associated with photoelectron fluxes to and from the spheres.
11 11 </Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Mats.Andre</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Mats.Andre</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster1/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description>Cluster 1 spacecraft positions in various coordinate systems</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 <PriorID>spase://SMWG/Instrument/Cluster2-Rumba/Ephemeris</PriorID>
... ...
Instrument/CDPP-AMDA/Cluster1/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Cluster1/WHISPER.xml
  Diff comments   View file @ba44a06
... ... @@ -19,7 +19,7 @@
19 19 * command and data processing systems, which are part of the DWP experiment.</Description>
20 20 <Acknowledgement>Principal Investigator: Jean-Louis Rauch</Acknowledgement>
21 21 <Contact>
22   - <PersonID>spase://CNES/Person/Jean-Louis.Rauch</PersonID>
  22 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jean-Louis.Rauch</PersonID>
23 23 <Role>PrincipalInvestigator</Role>
24 24 </Contact>
25 25 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster2/EFW.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>The EFW (Electric Field and Waves) instrument consists of four orthogonal spherical sensors deployed from 50 m cable booms in the spin plane of the spacecraft, plus four deployment units and a main electronics unit. Each deployment unit deploys a multiconductor cable and tip-mounted spherical sensor. Each opposing pair of cables will be symmetrically deployed to a tip-to-tip distance of approximately 100 m, except for about a week at the beginning of the mission when 70 m will be used for one boom pair (the Z-booms) and 100 m for the other pair. The potentials of the spherical sensor and nearby conductors are controlled by the microprocessor to minimize errors associated with photoelectron fluxes to and from the spheres.
11 11 </Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Mats.Andre</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Mats.Andre</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster2/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:33Z</ReleaseDate>
10 10 <Description>Cluster 2 spacecraft positions in various coordinate systems</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 <PriorID>spase://SMWG/Instrument/Cluster2-Salsa/Ephemeris</PriorID>
... ...
Instrument/CDPP-AMDA/Cluster2/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Cluster2/WHISPER.xml
  Diff comments   View file @ba44a06
... ... @@ -19,7 +19,7 @@
19 19 * command and data processing systems, which are part of the DWP experiment.</Description>
20 20 <Acknowledgement>Principal Investigator: Jean-Louis Rauch</Acknowledgement>
21 21 <Contact>
22   - <PersonID>spase://CNES/Person/Jean-Louis.Rauch</PersonID>
  22 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jean-Louis.Rauch</PersonID>
23 23 <Role>PrincipalInvestigator</Role>
24 24 </Contact>
25 25 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster3/CIS-CODIF.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2011-02-04T15:37:07Z</ReleaseDate>
10 10 <Description>This instrument (CIS: Cluster Ion Spectrometry) is capable of obtaining full 3D ion distributions with high time resolution (in one spacecraft spin) and mass-per-charge resolution. The experiment consists of two different instruments, a Hot Ion Analyzer (HIA) and a time-of-flight Ion Composition and Distribution Function analyzer (CODIF). Extensive on-board processing is done, within its dual-processor Data Processing System (DPS). CODIF determines the distributions of the major ion species with energies from spacecraft potential to 40 KeV/charge with an angular resolution of 22.5 x 10.25 degrees and with two different sensitivities. The CODIF instrument uses electrostatic deflection to select by energy per charge, with subsequent time-of-flight analysis. The sensor primarily covers the energy range 0.02--40 KeV/charge, but with additional pre-acceleration for energies below 25 eV/charge, the range is extended to energies as low as the spacecraft potential. The HIA does not measure mass, but extends the dynamic range to the highest ion fluxes, and has angular resolution capability of 5.6 x 5.6 degrees for ion-beam and solar-wind measurements. The HIA is a symmetric quadrispherical analyzer of top-hat geometry, and uses microchannel-plate electron multipliers and position encoding by discrete anodes. A 2D distribution is obtained once per 62.5 ms, and a full 3D distribution of ions in the energy range ~5 eV/charge to 32 KeV/charge is obtained every 4 s. For more details of the Cluster mission, the spacecraft, and its instruments, see the report ``Cluster: mission, payload and supporting activities,'' March 1993, ESA SP-1159, and the included article ``The Cluster Ion Spectrometry Experiment,'' by H. Reme et al., from which this information was obtained.</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Jannis.Dandouras</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jannis.Dandouras</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster3/CIS-HIA.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>The HIA is a symmetric quadrispherical analyzer of top-hat geometry, and uses microchannel-plate electron multipliers and position encoding by discrete anodes. A 2D distribution is obtained once per 62.5 ms, and a full 3D distribution of ions in the energy range ~5 eV/charge to 32 KeV/charge is obtained every 4 s. For more details of the Cluster mission, the spacecraft, and its instruments, see the report ``Cluster: mission, payload and supporting activities,'' March 1993, ESA SP-1159, and the included article ``The Cluster Ion Spectrometry Experiment,'' by H. Reme et al., from which this information was obtained.</Description>
11 11 <Acknowledgement>Principal Investigator: Iannis Dandouras</Acknowledgement>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Jannis.Dandouras</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jannis.Dandouras</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster3/EFW.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>The EFW (Electric Field and Waves) instrument consists of four orthogonal spherical sensors deployed from 50 m cable booms in the spin plane of the spacecraft, plus four deployment units and a main electronics unit. Each deployment unit deploys a multiconductor cable and tip-mounted spherical sensor. Each opposing pair of cables will be symmetrically deployed to a tip-to-tip distance of approximately 100 m, except for about a week at the beginning of the mission when 70 m will be used for one boom pair (the Z-booms) and 100 m for the other pair. The potentials of the spherical sensor and nearby conductors are controlled by the microprocessor to minimize errors associated with photoelectron fluxes to and from the spheres.
11 11 </Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Mats.Andre</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Mats.Andre</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster3/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:07Z</ReleaseDate>
10 10 <Description>Cluster 3 spacecraft positions in various coordinate systems</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 <PriorID>spase://SMWG/Instrument/Cluster2-Samba/Ephemeris</PriorID>
... ...
Instrument/CDPP-AMDA/Cluster3/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Cluster3/WHISPER.xml
  Diff comments   View file @ba44a06
... ... @@ -19,7 +19,7 @@
19 19 * command and data processing systems, which are part of the DWP experiment.</Description>
20 20 <Acknowledgement>Principal Investigator: Jean-Louis Rauch</Acknowledgement>
21 21 <Contact>
22   - <PersonID>spase://CNES/Person/Jean-Louis.Rauch</PersonID>
  22 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jean-Louis.Rauch</PersonID>
23 23 <Role>PrincipalInvestigator</Role>
24 24 </Contact>
25 25 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster4/CIS-CODIF.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2011-02-04T15:37:19Z</ReleaseDate>
10 10 <Description>This instrument (CIS: Cluster Ion Spectrometry) is capable of obtaining full 3D ion distributions with high time resolution (in one spacecraft spin) and mass-per-charge resolution. The experiment consists of two different instruments, a Hot Ion Analyzer (HIA) and a time-of-flight Ion Composition and Distribution Function analyzer (CODIF). Extensive on-board processing is done, within its dual-processor Data Processing System (DPS). CODIF determines the distributions of the major ion species with energies from spacecraft potential to 40 KeV/charge with an angular resolution of 22.5 x 10.25 degrees and with two different sensitivities. The CODIF instrument uses electrostatic deflection to select by energy per charge, with subsequent time-of-flight analysis. The sensor primarily covers the energy range 0.02--40 KeV/charge, but with additional pre-acceleration for energies below 25 eV/charge, the range is extended to energies as low as the spacecraft potential. The HIA does not measure mass, but extends the dynamic range to the highest ion fluxes, and has angular resolution capability of 5.6 x 5.6 degrees for ion-beam and solar-wind measurements. The HIA is a symmetric quadrispherical analyzer of top-hat geometry, and uses microchannel-plate electron multipliers and position encoding by discrete anodes. A 2D distribution is obtained once per 62.5 ms, and a full 3D distribution of ions in the energy range ~5 eV/charge to 32 KeV/charge is obtained every 4 s. For more details of the Cluster mission, the spacecraft, and its instruments, see the report ``Cluster: mission, payload and supporting activities,'' March 1993, ESA SP-1159, and the included article ``The Cluster Ion Spectrometry Experiment,'' by H. Reme et al., from which this information was obtained.</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Jannis.Dandouras</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jannis.Dandouras</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster4/EFW.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>The EFW (Electric Field and Waves) instrument consists of four orthogonal spherical sensors deployed from 50 m cable booms in the spin plane of the spacecraft, plus four deployment units and a main electronics unit. Each deployment unit deploys a multiconductor cable and tip-mounted spherical sensor. Each opposing pair of cables will be symmetrically deployed to a tip-to-tip distance of approximately 100 m, except for about a week at the beginning of the mission when 70 m will be used for one boom pair (the Z-booms) and 100 m for the other pair. The potentials of the spherical sensor and nearby conductors are controlled by the microprocessor to minimize errors associated with photoelectron fluxes to and from the spheres.
11 11 </Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Mats.Andre</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Mats.Andre</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster4/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:19Z</ReleaseDate>
10 10 <Description>Cluster 4 spacecraft positions in various coordinate systems</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 <PriorID>spase://SMWG/Instrument/Cluster2-Tango/Ephemeris</PriorID>
... ...
Instrument/CDPP-AMDA/Cluster4/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Cluster4/WHISPER.xml
  Diff comments   View file @ba44a06
... ... @@ -19,7 +19,7 @@
19 19 * command and data processing systems, which are part of the DWP experiment.</Description>
20 20 <Acknowledgement>Principal Investigator: Jean-Louis Rauch</Acknowledgement>
21 21 <Contact>
22   - <PersonID>spase://CNES/Person/Jean-Louis.Rauch</PersonID>
  22 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jean-Louis.Rauch</PersonID>
23 23 <Role>PrincipalInvestigator</Role>
24 24 </Contact>
25 25 <InformationURL>
... ...
Instrument/CDPP-AMDA/Comets.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
9 9 <Description></Description>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/DSCOVR/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <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>
13   - <PersonID>spase://CNES/Person/Doug.Biesecker</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Doug.Biesecker</PersonID>
14 14 <Role>DataProducer</Role>
15 15 </Contact>
16 16 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/DSCOVR/FC.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <Description></Description>
10 10 <Acknowledgement>NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.</Acknowledgement>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Justin.Kasper</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Justin.Kasper</PersonID>
13 13 <!--<Role>InstrumentLead</Role>-->
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
... ...
Instrument/CDPP-AMDA/DSCOVR/MAG.xml
  Diff comments   View file @ba44a06
... ... @@ -13,7 +13,7 @@
13 13 </Description>
14 14 <Acknowledgement>NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.</Acknowledgement>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/Adam.Szabo</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Adam.Szabo</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 <InformationURL>
... ...
Instrument/CDPP-AMDA/DoubleStar1/HIA.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10 10 <Description>HIA (Hot Ion Analyzer) meausres the distribution function of ions in the magnetosphere and the solar wind, during each spin period of four seconds.</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Jannis.Dandouras</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jannis.Dandouras</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <InformationURL>
... ...
Instrument/CDPP-AMDA/EISCAT/32M.xml
  Diff comments   View file @ba44a06
... ... @@ -10,11 +10,11 @@
10 10 <ReleaseDate>2018-02-04T12:34:56.789</ReleaseDate>
11 11 <Description> EISCAT incoherent scatter radar in Longyearbyen, Svalbard archipelago. Steerable antenna, 32m in diameter. </Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Assar.Westman</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Assar.Westman</PersonID>
14 14 <Role>Scientist</Role>
15 15 </Contact>
16 16 <Contact>
17   - <PersonID>spase://CNES/Person/Craig.Heinselman</PersonID>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/Craig.Heinselman</PersonID>
18 18 <Role>PrincipalInvestigator</Role>
19 19 </Contact>
20 20 <InformationURL>
... ...
Instrument/CDPP-AMDA/EISCAT/42M.xml
  Diff comments   View file @ba44a06
... ... @@ -10,11 +10,11 @@
10 10 <ReleaseDate>2018-02-04T12:34:56.789</ReleaseDate>
11 11 <Description>EISCAT incoherent scatter radar in Longyearbyen, Svalbard archipelago. field-aligned pointing antenna, 42m in diameter</Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Assar.Westman</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Assar.Westman</PersonID>
14 14 <Role>Scientist</Role>
15 15 </Contact>
16 16 <Contact>
17   - <PersonID>spase://CNES/Person/Craig.Heinselman</PersonID>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/Craig.Heinselman</PersonID>
18 18 <Role>PrincipalInvestigator</Role>
19 19 </Contact>
20 20 <InformationURL>
... ...
Instrument/CDPP-AMDA/EISCAT/UHF.xml
  Diff comments   View file @ba44a06
... ... @@ -10,11 +10,11 @@
10 10 <ReleaseDate>2018-02-04T12:34:56.789</ReleaseDate>
11 11 <Description>EISCAT incoherent scatter radar in Tromso, Norway. Steerable antenna, 32m in diameter.</Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Mike.Rietveld</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Mike.Rietveld</PersonID>
14 14 <Role>Scientist</Role>
15 15 </Contact>
16 16 <Contact>
17   - <PersonID>spase://CNES/Person/Craig.Heinselman</PersonID>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/Craig.Heinselman</PersonID>
18 18 <Role>PrincipalInvestigator</Role>
19 19 </Contact>
20 20 <InformationURL>
... ...
Instrument/CDPP-AMDA/EISCAT/VHF.xml
  Diff comments   View file @ba44a06
... ... @@ -10,11 +10,11 @@
10 10 <ReleaseDate>2018-02-04T12:34:56.789</ReleaseDate>
11 11 <Description>EISCAT incoherent scatter radar in Tromso, Norway. Steerable antenna, 120x40m</Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Mike.Rietveld</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Mike.Rietveld</PersonID>
14 14 <Role>Scientist</Role>
15 15 </Contact>
16 16 <Contact>
17   - <PersonID>spase://CNES/Person/Craig.Heinselman</PersonID>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/Craig.Heinselman</PersonID>
18 18 <Role>PrincipalInvestigator</Role>
19 19 </Contact>
20 20 <InformationURL>
... ...
Instrument/CDPP-AMDA/Ephemerides.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/FERMI/LAT.xml
  Diff comments   View file @ba44a06
... ... @@ -11,7 +11,7 @@
11 11 Such gamma rays are emitted only in the most extreme conditions, by particles moving very nearly at the speed of light.
12 12 The LAT's field of view covers about 20% of the sky at any time, and it scans continuously, covering the whole sky every three hours</Description>
13 13 <Contact>
14   - <PersonID>spase://CNES/Person/Elizabeth.Hays</PersonID>
  14 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elizabeth.Hays</PersonID>
15 15 <Role>ProjectScientist</Role>
16 16 </Contact>
17 17 <InformationURL>
... ...
Instrument/CDPP-AMDA/Galileo/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>Different magnetic parameters calculated basing on Khurana's model</Description>
11 11 <Acknowledgement/>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/Krishan.Khurana</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/Krishan.Khurana</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Galileo/ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -11,7 +11,7 @@
11 11 Special Galileo Ephemeris are calculated by Joseph Groene tool (University of Iowa). Orbits
12 12 during Jupiter moons flybys are obtained from NASA/PDS MAG dataset.</Description>
13 13 <Contact>
14   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  14 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
15 15 <Role>PrincipalInvestigator</Role>
16 16 </Contact>
17 17 <Contact>
... ...
Instrument/CDPP-AMDA/Geotail/EPIC.xml
  Diff comments   View file @ba44a06
... ... @@ -17,11 +17,11 @@
17 17 <Role>FormerPI</Role>
18 18 </Contact>
19 19 <Contact>
20   - <PersonID>spase://CNES/Person/A.T.Lui</PersonID>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/A.T.Lui</PersonID>
21 21 <Role>PrincipalInvestigator</Role>
22 22 </Contact>
23 23 <Contact>
24   - <PersonID>spase://CNES/Person/Stuart.Nyland</PersonID>
  24 + <PersonID>spase://CNES/Person/CDPP-AMDA/Stuart.Nyland</PersonID>
25 25 <Role>DataProducer</Role>
26 26 </Contact>
27 27 <InformationURL>
... ...
Instrument/CDPP-AMDA/Geotail/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios1/AUX.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>
11 11 </Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/David.Stansby</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/David.Stansby</PersonID>
14 14 <Role>DataProducer</Role>
15 15 </Contact>
16 16 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios1/E1.xml
  Diff comments   View file @ba44a06
... ... @@ -20,11 +20,11 @@
20 20 * The I3 instrument measures positive ions. It can select for m/q and velocity.
21 21 </Description>
22 22 <Contact>
23   - <PersonID>spase://CNES/Person/Rosenbauer</PersonID>
  23 + <PersonID>spase://CNES/Person/CDPP-AMDA/Rosenbauer</PersonID>
24 24 <Role>PrincipalInvestigator</Role>
25 25 </Contact>
26 26 <Contact>
27   - <PersonID>spase://CNES/Person/Schwenn</PersonID>
  27 + <PersonID>spase://CNES/Person/CDPP-AMDA/Schwenn</PersonID>
28 28 <Role>PrincipalInvestigator</Role>
29 29 </Contact>
30 30 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios1/E3.xml
  Diff comments   View file @ba44a06
... ... @@ -16,7 +16,7 @@
16 16 At lower bit rates, averages and variances were computed on board for transmission to earth.
17 17 </Description>
18 18 <Contact>
19   - <PersonID>spase://CNES/Person/Norman.F.Ness</PersonID>
  19 + <PersonID>spase://CNES/Person/CDPP-AMDA/Norman.F.Ness</PersonID>
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios1/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2018-10-20T21:10:13Z</ReleaseDate>
10 10 <Description>Helios1 Ephemeris data are calculated using SPICE kernels taken from the https://naif.jpl.nasa.gov/pub/naif/HELIOS/kernels</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios1/MAG.xml
  Diff comments   View file @ba44a06
... ... @@ -31,11 +31,11 @@ E3 : The Romeโ€GSFC magnetic field experiment utilized a triaxial fluxg
31 31 magnetometer. 
32 32 </Description>
33 33 <Contact>
34   - <PersonID>spase://CNES/Person/Musmann</PersonID>
  34 + <PersonID>spase://CNES/Person/CDPP-AMDA/Musmann</PersonID>
35 35 <Role>PrincipalInvestigator</Role>
36 36 </Contact>
37 37 <Contact>
38   - <PersonID>spase://CNES/Person/Mariani</PersonID>
  38 + <PersonID>spase://CNES/Person/CDPP-AMDA/Mariani</PersonID>
39 39 <Role>PrincipalInvestigator</Role>
40 40 </Contact>
41 41 <Contact>
... ... @@ -43,7 +43,7 @@ magnetometer. 
43 43 <Role>PrincipalInvestigator</Role>
44 44 </Contact>
45 45 <Contact>
46   - <PersonID>spase://CNES/Person/F.M.Neubauer</PersonID>
  46 + <PersonID>spase://CNES/Person/CDPP-AMDA/F.M.Neubauer</PersonID>
47 47 <Role>PrincipalInvestigator</Role>
48 48 </Contact>
49 49 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios2/AUX.xml
  Diff comments   View file @ba44a06
... ... @@ -10,7 +10,7 @@
10 10 <Description>
11 11 </Description>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/David.Stansby</PersonID>
  13 + <PersonID>spase://CNES/Person/CDPP-AMDA/David.Stansby</PersonID>
14 14 <Role>DataProducer</Role>
15 15 </Contact>
16 16 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios2/E1.xml
  Diff comments   View file @ba44a06
... ... @@ -19,11 +19,11 @@
19 19 * The I2 instrument measures electrons. It can run in two different modes (A or B), toggled by manual commands sent to the spacecraft. The only difference between the modes is the energy channel spacing. There is only1 elevation bin, so effectively a 2D cut through the electron distribution is measured in the ecliptic.
20 20 * The I3 instrument measures positive ions. It can select for m/q and velocity. </Description>
21 21 <Contact>
22   - <PersonID>spase://CNES/Person/Rosenbauer</PersonID>
  22 + <PersonID>spase://CNES/Person/CDPP-AMDA/Rosenbauer</PersonID>
23 23 <Role>PrincipalInvestigator</Role>
24 24 </Contact>
25 25 <Contact>
26   - <PersonID>spase://CNES/Person/Schwenn</PersonID>
  26 + <PersonID>spase://CNES/Person/CDPP-AMDA/Schwenn</PersonID>
27 27 <Role>PrincipalInvestigator</Role>
28 28 </Contact>
29 29 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios2/E3.xml
  Diff comments   View file @ba44a06
... ... @@ -16,7 +16,7 @@
16 16 At lower bit rates, averages and variances were computed on board for transmission to earth.
17 17 </Description>
18 18 <Contact>
19   - <PersonID>spase://CNES/Person/Norman.F.Ness</PersonID>
  19 + <PersonID>spase://CNES/Person/CDPP-AMDA/Norman.F.Ness</PersonID>
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios2/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2018-10-20T21:10:13Z</ReleaseDate>
10 10 <Description>Helios2 Ephemeris data are calculated using SPICE kernels taken from the https://naif.jpl.nasa.gov/pub/naif/HELIOS/kernels</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios2/MAG.xml
  Diff comments   View file @ba44a06
... ... @@ -31,11 +31,11 @@ E3 : The Romeโ€GSFC magnetic field experiment utilized a triaxial fluxg
31 31 magnetometer. 
32 32 </Description>
33 33 <Contact>
34   - <PersonID>spase://CNES/Person/Musmann</PersonID>
  34 + <PersonID>spase://CNES/Person/CDPP-AMDA/Musmann</PersonID>
35 35 <Role>PrincipalInvestigator</Role>
36 36 </Contact>
37 37 <Contact>
38   - <PersonID>spase://CNES/Person/Mariani</PersonID>
  38 + <PersonID>spase://CNES/Person/CDPP-AMDA/Mariani</PersonID>
39 39 <Role>PrincipalInvestigator</Role>
40 40 </Contact>
41 41 <Contact>
... ... @@ -43,7 +43,7 @@ magnetometer. 
43 43 <Role>PrincipalInvestigator</Role>
44 44 </Contact>
45 45 <Contact>
46   - <PersonID>spase://CNES/Person/F.M.Neubauer</PersonID>
  46 + <PersonID>spase://CNES/Person/CDPP-AMDA/F.M.Neubauer</PersonID>
47 47 <Role>PrincipalInvestigator</Role>
48 48 </Contact>
49 49 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/ISEE1/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,8 +9,7 @@
9 9 <ReleaseDate>2013-04-09T00:00:00Z</ReleaseDate>
10 10 <Description>ISEE1 spacecraft positions in various coordinate systems</Description>
11 11 <Contact>
12   - <PersonID>spase://SMWG/Person/Robert.E.McGuire
13   -</PersonID>
  12 + <PersonID>spase://SMWG/Person/Robert.E.McGuire</PersonID>
14 13 <Role>MetadataContact</Role>
15 14 </Contact>
16 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/ISEE1/FVA.xml
  Diff comments   View file @ba44a06
... ... @@ -14,7 +14,7 @@
14 14 </Description>
15 15 <Acknowledgement/>
16 16 <Contact>
17   - <PersonID>spase://CNES/Person/K.A.Anderson</PersonID>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/K.A.Anderson</PersonID>
18 18 <Role>PrincipalInvestigator</Role>
19 19 </Contact>
20 20 <InformationURL>
... ...
Instrument/CDPP-AMDA/ISEE2/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,8 +9,7 @@
9 9 <ReleaseDate>2013-04-09T00:00:00Z</ReleaseDate>
10 10 <Description>ISEE2 spacecraft positions in various coordinate systems</Description>
11 11 <Contact>
12   - <PersonID>spase://SMWG/Person/Robert.E.McGuire
13   -</PersonID>
  12 + <PersonID>spase://SMWG/Person/Robert.E.McGuire</PersonID>
14 13 <Role>MetadataContact</Role>
15 14 </Contact>
16 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/ISEE2/FVA.xml
  Diff comments   View file @ba44a06
... ... @@ -14,7 +14,7 @@
14 14 </Description>
15 15 <Acknowledgement/>
16 16 <Contact>
17   - <PersonID>spase://CNES/Person/K.A.Anderson</PersonID>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/K.A.Anderson</PersonID>
18 18 <Role>PrincipalInvestigator</Role>
19 19 </Contact>
20 20 <InformationURL>
... ...
Instrument/CDPP-AMDA/Interball-1/CORALL.xml
  Diff comments   View file @ba44a06
... ... @@ -14,7 +14,7 @@
14 14 is equal to about 4 min.
15 15 </Description>
16 16 <Contact>
17   - <PersonID>spase://CNES/Person/Andrey.Fedorov</PersonID>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/Andrey.Fedorov</PersonID>
18 18 <Role>PrincipalInvestigator</Role>
19 19 </Contact>
20 20 <Contact>
... ...
Instrument/CDPP-AMDA/Interball-1/DOK2.xml
  Diff comments   View file @ba44a06
... ... @@ -28,11 +28,11 @@
28 28 All other systems both hardware and software are working normally.
29 29 </Description>
30 30 <Contact>
31   - <PersonID>spase://CNES/Person/Volt.Lutsenko</PersonID>
  31 + <PersonID>spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko</PersonID>
32 32 <Role>PrincipalInvestigator</Role>
33 33 </Contact>
34 34 <Contact>
35   - <PersonID>spase://CNES/Person/Karel.Kudela</PersonID>
  35 + <PersonID>spase://CNES/Person/CDPP-AMDA/Karel.Kudela</PersonID>
36 36 <Role>PrincipalInvestigator</Role>
37 37 </Contact>
38 38 <InformationURL>
... ...
Instrument/CDPP-AMDA/Interball-1/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Juice/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10 10 <Description>Juice orbit</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/ESA.SPICE.Service</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/ESA.SPICE.Service</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Juice/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -15,7 +15,7 @@
15 15 (Juno Reference Model through Perijove 9) of the planetary magnetic field with spherical harmonic coefficients well determined through
16 16 degree and order 10, providing the first detailed view of a planetary dynamo beyond Earth.</Description>
17 17 <Contact>
18   - <PersonID>spase://CNES/Person/Connerney</PersonID>
  18 + <PersonID>spase://CNES/Person/CDPP-AMDA/Connerney</PersonID>
19 19 <Role>PrincipalInvestigator</Role>
20 20 </Contact>
21 21 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Juno/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,11 +9,11 @@
9 9 <ReleaseDate>2017-01-20T21:10:13Z</ReleaseDate>
10 10 <Description>Juno Orbit</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
17 17 <Role>TechnicalContact</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Juno/FGM.xml
  Diff comments   View file @ba44a06
... ... @@ -12,7 +12,7 @@
12 12 Limitations: The Juno magnetic field investigation was designed to measure fields to 16 Gauss per axis over 6 dynamic ranges of the instrument, the most sensitive of which is ยฑ 1600 nT with a quantization step size of 0.05 nT (16 bit A/D). Moreover, the spacecraft magnetic requirement was not to exceed 2 nT static and 0.5 nT variable spacecraft-generated magnetic field. In very weak field environments, such as encountered in outer cruise, accuracy may be expected to be limited by sensor offset and spacecraft magnetic field variations. The combined (static) spacecraft-generated magnetic field and sensor offset may be continuously monitored in flight in the spacecraft x and y axis, since the spacecraft spins (nominally at 1 or 2 RPM) about an axis closely aligned with the spacecraft payload z axis. However, offsets in the z axis need be estimated using the Alfvenic properties in the solar wind (ref. Juno Magnetic field investigation paper in Space Science Reviews). Statistical in nature, estimates of z axis zeros are not continuously available and are less accurate than the x and y zeros. Also, variations in spacecraft field over a time span comparable to a spin period will also lead to larger errors.
13 13 </Description>
14 14 <Contact>
15   - <PersonID>spase://CNES/Person/John.E.P.Connerney</PersonID>
  15 + <PersonID>spase://CNES/Person/CDPP-AMDA/John.E.P.Connerney</PersonID>
16 16 <Role>PrincipalInvestigator</Role>
17 17 </Contact>
18 18 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Juno/JADE.xml
  Diff comments   View file @ba44a06
... ... @@ -22,7 +22,7 @@
22 22 50 amu with m/ฮ” mหœ2.5, which is sufficient to separate the heavy and light ions, as well as
23 23 O+ vs S+, in the Jovian magnetosphere.</Description>
24 24 <Contact>
25   - <PersonID>spase://CNES/Person/Allegrini</PersonID>
  25 + <PersonID>spase://CNES/Person/CDPP-AMDA/Allegrini</PersonID>
26 26 <Role>PrincipalInvestigator</Role>
27 27 </Contact>
28 28 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Juno/JEDI.xml
  Diff comments   View file @ba44a06
... ... @@ -14,7 +14,7 @@ have a time of flight (TOF) and a deposited
14 14 instruments can be operated in a variety of modes, differing in the
15 15 way they use and combine these measurements. </Description>
16 16 <Contact>
17   - <PersonID>spase://CNES/Person/Barry.Mauk</PersonID>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/Barry.Mauk</PersonID>
18 18 <Role>PrincipalInvestigator</Role>
19 19 </Contact>
20 20 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Juno/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -15,7 +15,7 @@
15 15 (Juno Reference Model through Perijove 9) of the planetary magnetic field with spherical harmonic coefficients well determined through
16 16 degree and order 10, providing the first detailed view of a planetary dynamo beyond Earth.</Description>
17 17 <Contact>
18   - <PersonID>spase://CNES/Person/Connerney</PersonID>
  18 + <PersonID>spase://CNES/Person/CDPP-AMDA/Connerney</PersonID>
19 19 <Role>PrincipalInvestigator</Role>
20 20 </Contact>
21 21 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MAVEN/EUV.xml
  Diff comments   View file @ba44a06
... ... @@ -17,7 +17,7 @@
17 17 input to the Flare Irradiance Spectral Model (FISM) model
18 18 </Description>
19 19 <Contact>
20   - <PersonID>spase://CNES/Person/Frank.Eparvier</PersonID>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Frank.Eparvier</PersonID>
21 21 <Role>PrincipalInvestigator</Role>
22 22 </Contact>
23 23 <InformationURL>
... ...
Instrument/CDPP-AMDA/MAVEN/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,11 +9,11 @@
9 9 <ReleaseDate>2016-05-20T21:10:13Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/Elena.Budnik</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
17 17 <Role>TechnicalContact</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MAVEN/MAG.xml
  Diff comments   View file @ba44a06
... ... @@ -13,7 +13,7 @@
13 13 * 32 samples/sec intrinsic sample rate averaged and decimated as necessary
14 14 * Sensor scale factor accuracy of 0.05%</Description>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/John.E.P.Connerney</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/John.E.P.Connerney</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 <InformationURL>
... ...
Instrument/CDPP-AMDA/MAVEN/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MAVEN/SWEA.xml
  Diff comments   View file @ba44a06
... ... @@ -13,7 +13,7 @@
13 13 Measure atmospheric electron impact ionization effects
14 14 </Description>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/David.L.Mitchell</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/David.L.Mitchell</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 <InformationURL>
... ...
Instrument/CDPP-AMDA/MAVEN/SWIA.xml
  Diff comments   View file @ba44a06
... ... @@ -16,7 +16,7 @@
16 16 *Measure basic space plasma phenomena, including reconnection, flux ropes, plasmoids, bulk plasma escape, auroral processes, and boundary instabilities, throughout the Martian system
17 17 </Description>
18 18 <Contact>
19   - <PersonID>spase://CNES/Person/Jasper.S.Halekas</PersonID>
  19 + <PersonID>spase://CNES/Person/CDPP-AMDA/Jasper.S.Halekas</PersonID>
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 <InformationURL>
... ...
Instrument/CDPP-AMDA/MESSENGER/EPS.xml
  Diff comments   View file @ba44a06
... ... @@ -15,7 +15,7 @@ mechanical collimator that delimits the look direction into the instrument. Part
15 15 pass through the collimator then transit through a thin, composite Start foil (polyimide +
16 16 aluminum, 10 ยตg/cm2) and onto the TOF region of the instrument.</Description>
17 17 <Contact>
18   - <PersonID>spase://CNES/Person/George.Ho</PersonID>
  18 + <PersonID>spase://CNES/Person/CDPP-AMDA/George.Ho</PersonID>
19 19 <Role>Scientist</Role>
20 20 </Contact>
21 21 <InformationURL>
... ...
Instrument/CDPP-AMDA/MESSENGER/ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-01-01T21:10:13Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MEX/ELS.xml
  Diff comments   View file @ba44a06
... ... @@ -20,7 +20,7 @@ By varying the electrostatic potential between the hemispheres of the electrosta
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 <Contact>
23   - <PersonID>spase://CNES/Person/Rudy.Frahm</PersonID>
  23 + <PersonID>spase://CNES/Person/CDPP-AMDA/Rudy.Frahm</PersonID>
24 24 <Role>GeneralContact</Role>
25 25 </Contact>
26 26 <InformationURL>
... ...
Instrument/CDPP-AMDA/MEX/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MEX/ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-01-20T21:10:13Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MGS/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-01-20T21:10:13Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/NAIF</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/NAIF</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MGS/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MGS/PROXY.xml
  Diff comments   View file @ba44a06
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10 10 <Description>Several useful MGS proxies</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/David.Brain</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/David.Brain</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 <InformationURL>
... ...
Instrument/CDPP-AMDA/MMS1/EDP.xml
  Diff comments   View file @ba44a06
... ... @@ -16,15 +16,15 @@ giving a 120 m baseline for each of the two spin-plane electric field components
16 16 biased cylindrical probes extended on ~12 m long stiff booms along the spacecraft axis, giving a 29.2
17 17 m baseline for the axial electric field component.</Description>
18 18 <Contact>
19   - <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
  19 + <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 <Contact>
23   - <PersonID>spase://CNES/Person/Robert.E.Ergun</PersonID>
  23 + <PersonID>spase://CNES/Person/CDPP-AMDA/Robert.E.Ergun</PersonID>
24 24 <Role>PrincipalInvestigator</Role>
25 25 </Contact>
26 26 <Contact>
27   - <PersonID>spase://CNES/Person/P.Lindqvist</PersonID>
  27 + <PersonID>spase://CNES/Person/CDPP-AMDA/P.Lindqvist</PersonID>
28 28 <Role>PrincipalInvestigator</Role>
29 29 </Contact>
30 30 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS1/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,11 +9,11 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description></Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/M.G.Henderson</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/M.G.Henderson</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/S.K.Morley</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/S.K.Morley</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS1/FGM.xml
  Diff comments   View file @ba44a06
... ... @@ -18,7 +18,7 @@ rotation axis allows accurate monitoring of the zero levels along the rotation a
18 18 survey (8 samples per second) outside of the Region of Interest (ROI), and fast survey (16 samples per second) inside the ROI.
19 19 Within the ROI burst mode data (128 samples per second) are also acquired.</Description>
20 20 <Contact>
21   - <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
  21 + <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
22 22 <Role>PrincipalInvestigator</Role>
23 23 </Contact>
24 24 <Contact>
... ... @@ -26,7 +26,7 @@ Within the ROI burst mode data (128 samples per second) are also acquired.&lt;/Desc
26 26 <Role>PrincipalInvestigator</Role>
27 27 </Contact>
28 28 <Contact>
29   - <PersonID>spase://CNES/Person/W.Magnus</PersonID>
  29 + <PersonID>spase://CNES/Person/CDPP-AMDA/W.Magnus</PersonID>
30 30 <Role>PrincipalInvestigator</Role>
31 31 </Contact>
32 32 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS1/FPI.xml
  Diff comments   View file @ba44a06
... ... @@ -9,11 +9,11 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description>The Fast Plasma Investigation (FPI) includes four dual electron spectrometers (DES) and four dual ion spectrometers (DIS) per spacecraft. When the data from the two sets of four dual-spectrometers are combined, FPI is able to provide the velocity-space distribution of electrons from 10 eV to 30 keV and ions from 10 eV to 30 keV with a time resolution of 30 ms, and 150 ms, respectively.</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/B.Giles</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/B.Giles</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS1/HPCA.xml
  Diff comments   View file @ba44a06
... ... @@ -9,11 +9,11 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description> </Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/S.Fuselier</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/S.Fuselier</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS1/Models.xml
  Diff comments   View file @ba44a06
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS1234/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,11 +9,11 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description></Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/M.G.Henderson</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/M.G.Henderson</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/S.K.Morley</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/S.K.Morley</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS1234/FGM.xml
  Diff comments   View file @ba44a06
... ... @@ -18,7 +18,7 @@ rotation axis allows accurate monitoring of the zero levels along the rotation a
18 18 survey (8 samples per second) outside of the Region of Interest (ROI), and fast survey (16 samples per second) inside the ROI.
19 19 Within the ROI burst mode data (128 samples per second) are also acquired.</Description>
20 20 <Contact>
21   - <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
  21 + <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
22 22 <Role>ProjectScientist</Role>
23 23 </Contact>
24 24 <Contact>
... ... @@ -26,7 +26,7 @@ Within the ROI burst mode data (128 samples per second) are also acquired.&lt;/Desc
26 26 <Role>PrincipalInvestigator</Role>
27 27 </Contact>
28 28 <Contact>
29   - <PersonID>spase://CNES/Person/W.Magnus</PersonID>
  29 + <PersonID>spase://CNES/Person/CDPP-AMDA/W.Magnus</PersonID>
30 30 <Role>PrincipalInvestigator</Role>
31 31 </Contact>
32 32 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS2/EDP.xml
  Diff comments   View file @ba44a06
... ... @@ -16,15 +16,15 @@ giving a 120 m baseline for each of the two spin-plane electric field components
16 16 biased cylindrical probes extended on ~12 m long stiff booms along the spacecraft axis, giving a 29.2
17 17 m baseline for the axial electric field component.</Description>
18 18 <Contact>
19   - <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
  19 + <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 <Contact>
23   - <PersonID>spase://CNES/Person/Robert.E.Ergun</PersonID>
  23 + <PersonID>spase://CNES/Person/CDPP-AMDA/Robert.E.Ergun</PersonID>
24 24 <Role>PrincipalInvestigator</Role>
25 25 </Contact>
26 26 <Contact>
27   - <PersonID>spase://CNES/Person/P.Lindqvist</PersonID>
  27 + <PersonID>spase://CNES/Person/CDPP-AMDA/P.Lindqvist</PersonID>
28 28 <Role>PrincipalInvestigator</Role>
29 29 </Contact>
30 30 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS2/Ephemeris.xml
  Diff comments   View file @ba44a06
... ... @@ -9,11 +9,11 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description></Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/M.G.Henderson</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/M.G.Henderson</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/S.K.Morley</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/S.K.Morley</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS2/FGM.xml
  Diff comments   View file @ba44a06
... ... @@ -18,7 +18,7 @@ rotation axis allows accurate monitoring of the zero levels along the rotation a
18 18 survey (8 samples per second) outside of the Region of Interest (ROI), and fast survey (16 samples per second) inside the ROI.
19 19 Within the ROI burst mode data (128 samples per second) are also acquired.</Description>
20 20 <Contact>
21   - <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
  21 + <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
22 22 <Role>PrincipalInvestigator</Role>
23 23 </Contact>
24 24 <Contact>
... ... @@ -26,7 +26,7 @@ Within the ROI burst mode data (128 samples per second) are also acquired.&lt;/Desc
26 26 <Role>PrincipalInvestigator</Role>
27 27 </Contact>
28 28 <Contact>
29   - <PersonID>spase://CNES/Person/W.Magnus</PersonID>
  29 + <PersonID>spase://CNES/Person/CDPP-AMDA/W.Magnus</PersonID>
30 30 <Role>PrincipalInvestigator</Role>
31 31 </Contact>
32 32 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS2/FPI.xml
  Diff comments   View file @ba44a06
... ... @@ -9,11 +9,11 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description>The Fast Plasma Investigation (FPI) includes four dual electron spectrometers (DES) and four dual ion spectrometers (DIS) per spacecraft. When the data from the two sets of four dual-spectrometers are combined, FPI is able to provide the velocity-space distribution of electrons from 10 eV to 30 keV and ions from 10 eV to 30 keV with a time resolution of 30 ms, and 150 ms, respectively.</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/B.Giles</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/B.Giles</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS2/HPCA.xml
  Diff comments   View file @ba44a06
... ... @@ -9,11 +9,11 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description>The Hot Plasma Composition Analyzer (HPCA) measures the composition-resolved velocity-space distribution of ions from 1 eV to 40 keV with time resolution of 10 - 15 seconds (Young et al., 2014).</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/James.L.Burch</PersonID>
  12 + <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/S.Fuselier</PersonID>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/S.Fuselier</PersonID>
17 17 <Role>PrincipalInvestigator</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...