CDPP / CNES

Commit eadfc371b71dce980e1fd6ecbe894a4e07f33913

Authored by Benjamin Renard
1 parent d6808d8d
Exists in cleanup_registry_merged and in 1 other branch cleanup_registry_master

Fixes

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Instrument/CDPP-AMDA/ACE/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -10,7 +10,7 @@
10 10 <Description>ACE spacecraft positions</Description>
11 11 <Acknowledgement></Acknowledgement>
12 12 <Contact>
13   - <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
  13 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
14 14 <Role>TechnicalContact</Role>
15 15 </Contact>
16 16 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/ACE/SWEPAM.xml
  Diff comments   View file @eadfc37
... ... @@ -28,7 +28,7 @@
28 28 </Description>
29 29 <Contact>
30 30 <!-- David McComas -->
31   - <PersonID>spase://CNES/Person/CDPP-AMDA/David.J.McComas</PersonID>
  31 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/BepiColombo/MPO/MAG.xml
  Diff comments   View file @eadfc37
... ... @@ -33,7 +33,7 @@
33 33 <Role>PrincipalInvestigator</Role>
34 34 </Contact>
35 35 <Contact>
36   - <PersonID>spase://CNES/Person/CDPP-AMDA/C.Carr</PersonID>
  36 + <PersonID>spase://SMWG/Person/C.Carr</PersonID>
37 37 <Role>CoInvestigator</Role>
38 38 </Contact>
39 39 <PriorID/>
... ...
Instrument/CDPP-AMDA/BepiColombo/Mio/ENA.xml
  Diff comments   View file @eadfc37
... ... @@ -10,7 +10,7 @@
10 10 <Description>ToDo</Description>
11 11 <Acknowledgement/>
12 12 <Contact>
13   - <PersonID></PersonID>
  13 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <PriorID/>
... ...
Instrument/CDPP-AMDA/BepiColombo/Mio/MEA2.xml
  Diff comments   View file @eadfc37
... ... @@ -2,7 +2,7 @@
2 2 <Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2.4.1.xsd">
3 3 <Version>2.4.1</Version>
4 4 <Instrument>
5   - <ResourceID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/MEA2</ResourceID>
  5 + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MEA2</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>MEA2</ResourceName>
8 8 <AlternateName>Mercury Electron Analyzer 2</AlternateName>
... ...
Instrument/CDPP-AMDA/BepiColombo/Mio/MIA.xml
  Diff comments   View file @eadfc37
... ... @@ -2,7 +2,7 @@
2 2 <Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2.4.1.xsd">
3 3 <Version>2.4.1</Version>
4 4 <Instrument>
5   - <ResourceID>spase://CNES/Instrument/CDPP-AMDA/Bepi/MIA</ResourceID>
  5 + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>MIA</ResourceName>
8 8 <AlternateName>Mercury Ion Analyzer</AlternateName>
... ...
Instrument/CDPP-AMDA/BepiColombo/Mio/MSA.xml
  Diff comments   View file @eadfc37
... ... @@ -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://SMWG/Person/Yoshifumi.Saito</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <PriorID/>
... ...
Instrument/CDPP-AMDA/Cluster1/EFW.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Mats.Andre</PersonID>
  13 + <PersonID>spase://SMWG/Person/Mats.Andre</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster1/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  12 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Cluster1/STAFF.xml
  Diff comments   View file @eadfc37
... ... @@ -15,7 +15,7 @@
15 15 Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz.</Description>
16 16 <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
17 17 <Contact>
18   - <PersonID>spase://CNES/Person/CDPP-AMDA/Patrick.Canu</PersonID>
  18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
19 19 <Role>PrincipalInvestigator</Role>
20 20 </Contact>
21 21 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster1/WHISPER.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Jean-Louis.Rauch</PersonID>
  22 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -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/CDPP-AMDA/Mats.Andre</PersonID>
  13 + <PersonID>spase://SMWG/Person/Mats.Andre</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster2/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ... @@ -16,4 +16,4 @@
16 16 <InvestigationName/>
17 17 <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/Cluster2</ObservatoryID>
18 18 </Instrument>
19   -</Spase>
20 19 \ No newline at end of file
  20 +</Spase>
... ...
Instrument/CDPP-AMDA/Cluster2/STAFF.xml
  Diff comments   View file @eadfc37
... ... @@ -15,7 +15,7 @@
15 15 Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz.</Description>
16 16 <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
17 17 <Contact>
18   - <PersonID>spase://CNES/Person/CDPP-AMDA/Patrick.Canu</PersonID>
  18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
19 19 <Role>PrincipalInvestigator</Role>
20 20 </Contact>
21 21 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster2/WHISPER.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Jean-Louis.Rauch</PersonID>
  22 + <PersonID>spase://SMWG/Person/Jean-Louis.Rauch</PersonID>
23 23 <Role>PrincipalInvestigator</Role>
24 24 </Contact>
25 25 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster3/EFW.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Mats.Andre</PersonID>
  13 + <PersonID>spase://SMWG/Person/Mats.Andre</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster3/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ... @@ -16,4 +16,4 @@
16 16 <InvestigationName/>
17 17 <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/Cluster3</ObservatoryID>
18 18 </Instrument>
19   -</Spase>
20 19 \ No newline at end of file
  20 +</Spase>
... ...
Instrument/CDPP-AMDA/Cluster3/STAFF.xml
  Diff comments   View file @eadfc37
... ... @@ -15,7 +15,7 @@
15 15 Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz.</Description>
16 16 <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
17 17 <Contact>
18   - <PersonID>spase://CNES/Person/CDPP-AMDA/Patrick.Canu</PersonID>
  18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
19 19 <Role>PrincipalInvestigator</Role>
20 20 </Contact>
21 21 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster3/WHISPER.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Jean-Louis.Rauch</PersonID>
  22 + <PersonID>spase://SMWG/Person/Jean-Louis.Rauch</PersonID>
23 23 <Role>PrincipalInvestigator</Role>
24 24 </Contact>
25 25 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster4/EFW.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Mats.Andre</PersonID>
  13 + <PersonID>spase://SMWG/Person/Mats.Andre</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15 15 </Contact>
16 16 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster4/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ... @@ -16,4 +16,4 @@
16 16 <InvestigationName/>
17 17 <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/Cluster4</ObservatoryID>
18 18 </Instrument>
19   -</Spase>
20 19 \ No newline at end of file
  20 +</Spase>
... ...
Instrument/CDPP-AMDA/Cluster4/STAFF.xml
  Diff comments   View file @eadfc37
... ... @@ -15,7 +15,7 @@
15 15 Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz.</Description>
16 16 <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
17 17 <Contact>
18   - <PersonID>spase://CNES/Person/CDPP-AMDA/Patrick.Canu</PersonID>
  18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
19 19 <Role>PrincipalInvestigator</Role>
20 20 </Contact>
21 21 <InformationURL>
... ...
Instrument/CDPP-AMDA/Cluster4/WHISPER.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Jean-Louis.Rauch</PersonID>
  22 + <PersonID>spase://SMWG/Person/Jean-Louis.Rauch</PersonID>
23 23 <Role>PrincipalInvestigator</Role>
24 24 </Contact>
25 25 <InformationURL>
... ...
Instrument/CDPP-AMDA/DoubleStar1/FGM.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10 10 <Description>FGM (Flux Gate Magnetometer) is located on a 3.5 meter long boom and measures the magnetic field along the orbit at a rate up to 67 samples per second.</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/unknown</PersonID>
  12 + <PersonID>spase://SMWG/Person/UNKNOWN</PersonID>
13 13 <Role>GeneralContact</Role>
14 14 </Contact>
15 15 <InformationURL>
... ...
Instrument/CDPP-AMDA/Geotail/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ... @@ -16,4 +16,4 @@
16 16 <InvestigationName/>
17 17 <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/Geotail</ObservatoryID>
18 18 </Instrument>
19   -</Spase>
20 19 \ No newline at end of file
  20 +</Spase>
... ...
Instrument/CDPP-AMDA/Giotto/RPA.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10 10 <Description></Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Henri.Reme</PersonID>
  12 + <PersonID>spase://SMWG/Person/Henri.Reme</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios1/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Helios2/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Interball-1/CORALL.xml
  Diff comments   View file @eadfc37
... ... @@ -14,7 +14,7 @@
14 14 is equal to about 4 min.
15 15 </Description>
16 16 <Contact>
17   - <PersonID>spase://CNES/Person/CDPP-AMDA/Andrey.Fedorov</PersonID>
  17 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -32,7 +32,7 @@
32 32 <Role>PrincipalInvestigator</Role>
33 33 </Contact>
34 34 <Contact>
35   - <PersonID>spase://CNES/Person/CDPP-AMDA/Karel.Kudela</PersonID>
  35 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/JASON3/AMBRE.xml
  Diff comments   View file @eadfc37
... ... @@ -26,7 +26,7 @@
26 26 </Description>
27 27 <Acknowledgement/>
28 28 <Contact>
29   - <PersonID>spase://SMWG/Person/Denis.Payan</PersonID>
  29 + <PersonID>spase://CNES/Person/CDPP-AMDA/Denis.Payan</PersonID>
30 30 <Role>PrincipalInvestigator</Role>
31 31 </Contact>
32 32 <Contact>
... ...
Instrument/CDPP-AMDA/JASON3/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -11,7 +11,7 @@
11 11 </Description>
12 12 <Acknowledgement/>
13 13 <Contact>
14   - <PersonID>spase://SMWG/Person/Denis.Payan</PersonID>
  14 + <PersonID>spase://CNES/Person/CDPP-AMDA/Denis.Payan</PersonID>
15 15 <Role>PrincipalInvestigator</Role>
16 16 </Contact>
17 17 <Contact>
... ...
Instrument/CDPP-AMDA/Juno/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -13,7 +13,7 @@
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
  16 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
17 17 <Role>TechnicalContact</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Juno/FGM.xml
  Diff comments   View file @eadfc37
... ... @@ -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 ± 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/CDPP-AMDA/John.E.P.Connerney</PersonID>
  15 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -22,7 +22,7 @@
22 22 50 amu with m/Δ m˜2.5, 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/CDPP-AMDA/Allegrini</PersonID>
  25 + <PersonID>spase://SMWG/Person/David.J.McComas</PersonID>
26 26 <Role>PrincipalInvestigator</Role>
27 27 </Contact>
28 28 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Juno/JEDI.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/Barry.Mauk</PersonID>
  17 + <PersonID>spase://SMWG/Person/Barry.H.Mauk</PersonID>
18 18 <Role>PrincipalInvestigator</Role>
19 19 </Contact>
20 20 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MAVEN/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -13,7 +13,7 @@
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
16   - <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
  16 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
17 17 <Role>TechnicalContact</Role>
18 18 </Contact>
19 19 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MAVEN/LPW.xml
  Diff comments   View file @eadfc37
... ... @@ -19,7 +19,7 @@ Goals:
19 19 * Identify the ionopause and detached, escaping ionosphere clouds
20 20 </Description>
21 21 <Contact>
22   - <PersonID>spase://CNES/Person/CDPP-AMDA/Robert.E.Ergun</PersonID>
  22 + <PersonID>spase://SMWG/Person/Robert.E.Ergun</PersonID>
23 23 <Role>PrincipalInvestigator</Role>
24 24 </Contact>
25 25 <InformationURL>
... ...
Instrument/CDPP-AMDA/MAVEN/MAG.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/John.E.P.Connerney</PersonID>
  16 + <PersonID>spase://SMWG/Person/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 @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  12 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MESSENGER/EPS.xml
  Diff comments   View file @eadfc37
... ... @@ -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 µg/cm2) and onto the TOF region of the instrument.</Description>
17 17 <Contact>
18   - <PersonID>spase://CNES/Person/CDPP-AMDA/George.Ho</PersonID>
  18 + <PersonID>spase://SMWG/Person/George.Ho</PersonID>
19 19 <Role>Scientist</Role>
20 20 </Contact>
21 21 <InformationURL>
... ...
Instrument/CDPP-AMDA/MEX/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  12 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MGS/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
10 10 <Description/>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  12 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/MMS1/EDP.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/James.L.Burch</PersonID>
  19 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 <Contact>
23   - <PersonID>spase://CNES/Person/CDPP-AMDA/Robert.E.Ergun</PersonID>
  23 + <PersonID>spase://SMWG/Person/Robert.E.Ergun</PersonID>
24 24 <Role>PrincipalInvestigator</Role>
25 25 </Contact>
26 26 <Contact>
27   - <PersonID>spase://CNES/Person/CDPP-AMDA/P.Lindqvist</PersonID>
  27 + <PersonID>spase://SMWG/Person/Per-Arne.Lindqvist</PersonID>
28 28 <Role>PrincipalInvestigator</Role>
29 29 </Contact>
30 30 <InformationURL>
... ...
Instrument/CDPP-AMDA/MMS1/FGM.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/James.L.Burch</PersonID>
  21 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
22 22 <Role>PrincipalInvestigator</Role>
23 23 </Contact>
24 24 <Contact>
... ...
Instrument/CDPP-AMDA/MMS1/FPI.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
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/CDPP-AMDA/James.L.Burch</PersonID>
  12 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
... ...
Instrument/CDPP-AMDA/MMS1/HPCA.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
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/CDPP-AMDA/James.L.Burch</PersonID>
  12 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
... ...
Instrument/CDPP-AMDA/MMS1/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ... @@ -16,4 +16,4 @@
16 16 <InvestigationName/>
17 17 <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/MMS1</ObservatoryID>
18 18 </Instrument>
19   -</Spase>
20 19 \ No newline at end of file
  20 +</Spase>
... ...
Instrument/CDPP-AMDA/MMS1234/FGM.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/James.L.Burch</PersonID>
  21 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
22 22 <Role>ProjectScientist</Role>
23 23 </Contact>
24 24 <Contact>
... ...
Instrument/CDPP-AMDA/MMS2/EDP.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/James.L.Burch</PersonID>
  19 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 <Contact>
23   - <PersonID>spase://CNES/Person/CDPP-AMDA/Robert.E.Ergun</PersonID>
  23 + <PersonID>spase://SMWG/Person/Robert.E.Ergun</PersonID>
24 24 <Role>PrincipalInvestigator</Role>
25 25 </Contact>
26 26 <Contact>
27   - <PersonID>spase://CNES/Person/CDPP-AMDA/P.Lindqvist</PersonID>
  27 + <PersonID>spase://SMWG/Person/Per-Arne.Lindqvist</PersonID>
28 28 <Role>PrincipalInvestigator</Role>
29 29 </Contact>
30 30 <InformationURL>
... ...
Instrument/CDPP-AMDA/MMS2/FGM.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/James.L.Burch</PersonID>
  21 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
22 22 <Role>PrincipalInvestigator</Role>
23 23 </Contact>
24 24 <Contact>
... ...
Instrument/CDPP-AMDA/MMS2/FPI.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
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/CDPP-AMDA/James.L.Burch</PersonID>
  12 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
... ...
Instrument/CDPP-AMDA/MMS2/HPCA.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
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/CDPP-AMDA/James.L.Burch</PersonID>
  12 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
... ...
Instrument/CDPP-AMDA/MMS2/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ... @@ -16,4 +16,4 @@
16 16 <InvestigationName/>
17 17 <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/MMS2</ObservatoryID>
18 18 </Instrument>
19   -</Spase>
20 19 \ No newline at end of file
  20 +</Spase>
... ...
Instrument/CDPP-AMDA/MMS3/EDP.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/James.L.Burch</PersonID>
  19 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 <Contact>
23   - <PersonID>spase://CNES/Person/CDPP-AMDA/Robert.E.Ergun</PersonID>
  23 + <PersonID>spase://SMWG/Person/Robert.E.Ergun</PersonID>
24 24 <Role>PrincipalInvestigator</Role>
25 25 </Contact>
26 26 <Contact>
27   - <PersonID>spase://CNES/Person/CDPP-AMDA/P.Lindqvist</PersonID>
  27 + <PersonID>spase://SMWG/Person/Per-Arne.Lindqvist</PersonID>
28 28 <Role>PrincipalInvestigator</Role>
29 29 </Contact>
30 30 <InformationURL>
... ...
Instrument/CDPP-AMDA/MMS3/FGM.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/James.L.Burch</PersonID>
  21 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
22 22 <Role>PrincipalInvestigator</Role>
23 23 </Contact>
24 24 <Contact>
... ...
Instrument/CDPP-AMDA/MMS3/FPI.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
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/CDPP-AMDA/James.L.Burch</PersonID>
  12 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
... ...
Instrument/CDPP-AMDA/MMS3/HPCA.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
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/CDPP-AMDA/James.L.Burch</PersonID>
  12 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
... ...
Instrument/CDPP-AMDA/MMS3/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ... @@ -16,4 +16,4 @@
16 16 <InvestigationName/>
17 17 <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/MMS3</ObservatoryID>
18 18 </Instrument>
19   -</Spase>
20 19 \ No newline at end of file
  20 +</Spase>
... ...
Instrument/CDPP-AMDA/MMS4/EDP.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/James.L.Burch</PersonID>
  19 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
20 20 <Role>PrincipalInvestigator</Role>
21 21 </Contact>
22 22 <Contact>
23   - <PersonID>spase://CNES/Person/CDPP-AMDA/Robert.E.Ergun</PersonID>
  23 + <PersonID>spase://SMWG/Person/Robert.E.Ergun</PersonID>
24 24 <Role>PrincipalInvestigator</Role>
25 25 </Contact>
26 26 <Contact>
27   - <PersonID>spase://CNES/Person/CDPP-AMDA/P.Lindqvist</PersonID>
  27 + <PersonID>spase://SMWG/Person/Per-Arne.Lindqvist</PersonID>
28 28 <Role>PrincipalInvestigator</Role>
29 29 </Contact>
30 30 <InformationURL>
... ...
Instrument/CDPP-AMDA/MMS4/FGM.xml
  Diff comments   View file @eadfc37
... ... @@ -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/CDPP-AMDA/James.L.Burch</PersonID>
  21 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
22 22 <Role>PrincipalInvestigator</Role>
23 23 </Contact>
24 24 <Contact>
... ...
Instrument/CDPP-AMDA/MMS4/FPI.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
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/CDPP-AMDA/James.L.Burch</PersonID>
  12 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
... ...
Instrument/CDPP-AMDA/MMS4/HPCA.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
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/CDPP-AMDA/James.L.Burch</PersonID>
  12 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
... ...
Instrument/CDPP-AMDA/MMS4/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ... @@ -16,4 +16,4 @@
16 16 <InvestigationName/>
17 17 <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/MMS4</ObservatoryID>
18 18 </Instrument>
19   -</Spase>
20 19 \ No newline at end of file
  20 +</Spase>
... ...
Instrument/CDPP-AMDA/POLAR/HYDRA.xml
  Diff comments   View file @eadfc37
... ... @@ -12,7 +12,7 @@
12 12 * (2) to understand the role of field-aligned currents in the auroral zone, their relation to auroral forms and terrestrial kilometric radiation, and their response to magnetotail and solar wind stimuli as monitored by the other ISTP program spacecraft; to ascertain the altitude dependence of the associated electrical potential and the parameters which control its size;
13 13 * (3) to obtain a quantitative, high time resolution definition of the regions associated with the cusp and entry layer including a study of the momentum transfer between magnetosheath and entry layer plasmas. The instrument, named HYDRA, resolves electrons and ions, in three dimensions, with energies between 1 eV and 30 keV with 0.5-s time resolution. HYDRA consists of eight pairs of 127-deg electrostatic analyzer heads. Six pairs are body mounted, and two are on the loss cone platform.</Description>
14 14 <Contact>
15   - <PersonID>spase://CNES/Person/CDPP-AMDA/Jack.D.Scudder</PersonID>
  15 + <PersonID>spase://SMWG/Person/Jack.D.Scudder</PersonID>
16 16 <Role>PrincipalInvestigator</Role>
17 17 </Contact>
18 18 <InformationURL>
... ...
Instrument/CDPP-AMDA/POLAR/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Rosetta/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-05-20T21:10:13Z</ReleaseDate>
10 10 <Description>Rosetta Ephemeris data are calculated using SPICE kernels taken from the ftp://ssols01.esac.esa.int/pub/data/SPICE/ROSETTA/kernels/ (PSA)</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Rosetta/IES.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2017-02-20T21:10:13Z</ReleaseDate>
10 10 <Description>The IES is a plasma instrument consisting of two electrostatic analyzers, one each for electrons and ions. In general, IES acquires ion and electron measurements in 256 bins over an azimuth range of 90 degrees and polar angle of 360 degrees (less spacecraft obstructions). Thus IES collects plasma data roughly in 2.8 π steradians of space, and samples plasma velocity space.</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/James.L.Burch</PersonID>
  12 + <PersonID>spase://SMWG/Person/James.L.Burch</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15 15 <Contact>
... ...
Instrument/CDPP-AMDA/STEREO-A/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2018-10-20T21:10:10Z</ReleaseDate>
10 10 <Description>STEREO-A spacecraft position in various coordinate systems are calculated using SPICE kernels taken from the https://sohowww.nascom.nasa.gov/</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/STEREO-A/IMPACT/SWEA.xml
  Diff comments   View file @eadfc37
... ... @@ -28,7 +28,7 @@ SWEA is designed to measure the distribution function of the solar wind core and
28 28 <Role>CoInvestigator</Role>
29 29 </Contact>
30 30 <Contact>
31   - <PersonID>spase://CNES/Person/CDPP-AMDA/Philippe.Louarn</PersonID>
  31 + <PersonID>spase://SMWG/Person/Philippe.Louarn</PersonID>
32 32 <Role>CoInvestigator</Role>
33 33 </Contact>
34 34 <InformationURL>
... ...
Instrument/CDPP-AMDA/STEREO-B/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2018-10-20T21:10:12Z</ReleaseDate>
10 10 <Description>STEREO-B spacecraft position in various coordinate systems are calculated using SPICE kernels taken from the https://sohowww.nascom.nasa.gov/</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/STEREO-B/IMPACT/SWEA.xml
  Diff comments   View file @eadfc37
... ... @@ -28,7 +28,7 @@ SWEA is designed to measure the distribution function of the solar wind core and
28 28 <Role>CoInvestigator</Role>
29 29 </Contact>
30 30 <Contact>
31   - <PersonID>spase://CNES/Person/CDPP-AMDA/Philippe.Louarn</PersonID>
  31 + <PersonID>spase://SMWG/Person/Philippe.Louarn</PersonID>
32 32 <Role>CoInvestigator</Role>
33 33 </Contact>
34 34 <InformationURL>
... ...
Instrument/CDPP-AMDA/Solar_Orbiter/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2018-10-28T21:10:13Z</ReleaseDate>
10 10 <Description>Calculated at IRAP from SPICE kernels</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>DataProducer</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Solar_Orbiter/PAS.xml
  Diff comments   View file @eadfc37
... ... @@ -33,7 +33,7 @@ continuous sampling at high cadence. The sampling frequency during burst or
33 33 snapshots is generally of 4 distributions / s (4 Hz analysis).</Description>
34 34 <Acknowledgement></Acknowledgement>
35 35 <Contact>
36   - <PersonID>spase://CNES/Person/CDPP-AMDA/Philippe.Louarn</PersonID>
  36 + <PersonID>spase://SMWG/Person/Philippe.Louarn</PersonID>
37 37 <Role>PrincipalInvestigator</Role>
38 38 </Contact>
39 39 <Contact>
... ...
Instrument/CDPP-AMDA/Solar_Orbiter/RPW.xml
  Diff comments   View file @eadfc37
... ... @@ -38,7 +38,7 @@ waves in the solar wind. More precisely, RPW will:
38 38 * Detect on-board in-situ Type III events and store the corresponding data</Description>
39 39 <Acknowledgement/>
40 40 <Contact>
41   - <PersonID>spase://CNES/Person/CDPP-AMDA/Milan.Maksimovic</PersonID>
  41 + <PersonID>spase://SMWG/Person/Milan.Maksimovic</PersonID>
42 42 <Role>PrincipalInvestigator</Role>
43 43 </Contact>
44 44 <InformationURL>
... ...
Instrument/CDPP-AMDA/THEMIS/A/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/THEMIS/B/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/THEMIS/C/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/THEMIS/D/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/THEMIS/E/Models.xml
  Diff comments   View file @eadfc37
... ... @@ -8,7 +8,7 @@
8 8 <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://CNES/Person/CDPP-AMDA/Christian.Jacquey</PersonID>
  11 + <PersonID>spase://SMWG/Person/Christian.Jacquey</PersonID>
12 12 <Role>TechnicalContact</Role>
13 13 </Contact>
14 14 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/VEX/ELS.xml
  Diff comments   View file @eadfc37
... ... @@ -15,7 +15,7 @@ divided into 16 sectors. The sensor is a standard top-hat electrostatic analyzer
15 15 <Role>PrincipalInvestigator</Role>
16 16 </Contact>
17 17 <Contact>
18   - <PersonID>spase://CNES/Person/CDPP-AMDA/Andrew.J.Coates</PersonID>
  18 + <PersonID>spase://SMWG/Person/Andrew.J.Coates</PersonID>
19 19 <Role>GeneralContact</Role>
20 20 </Contact>
21 21 <InformationURL>
... ...
Instrument/CDPP-AMDA/Voyager1/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10 10 <Description>Voyager 1 spacecraft positions</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
Instrument/CDPP-AMDA/Voyager2/Ephemeris.xml
  Diff comments   View file @eadfc37
... ... @@ -9,7 +9,7 @@
9 9 <ReleaseDate>2009-05-20T21:10:14Z</ReleaseDate>
10 10 <Description>Voyager 2 spacecraft positions</Description>
11 11 <Contact>
12   - <PersonID>spase://CNES/Person/CDPP-AMDA/Elena.Budnik</PersonID>
  12 + <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
13 13 <Role>TechnicalContact</Role>
14 14 </Contact>
15 15 </ResourceHeader>
... ...
NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-ca60.xml
  Diff comments   View file @eadfc37
... ... @@ -2,7 +2,7 @@
2 2 <Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
3 3 <Version>2.3.1</Version>
4 4 <NumericalData>
5   - <ResourceID>spase://NASA/NumericalData/ACE/EPAM/ace-epam-ca60</ResourceID>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-ca60</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>CA60</ResourceName>
8 8 <AlternateName>CA60 - ACE Electron Proton Alpha Monitor (EPAM) 5-min Level 2 Data</AlternateName>
... ...
NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-de.xml
  Diff comments   View file @eadfc37
... ... @@ -2,7 +2,7 @@
2 2 <Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
3 3 <Version>2.3.1</Version>
4 4 <NumericalData>
5   - <ResourceID>spase://NASA/NumericalData/ACE/EPAM/ace-epam-de</ResourceID>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-de</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>DE</ResourceName>
8 8 <AlternateName>ACE Electron Proton Alpha Monitor (EPAM) 5-min Level 2 Data</AlternateName>
... ...
NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-lefs150.xml
  Diff comments   View file @eadfc37
... ... @@ -2,7 +2,7 @@
2 2 <Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
3 3 <Version>2.3.1</Version>
4 4 <NumericalData>
5   - <ResourceID>spase://NASA/NumericalData/ACE/EPAM/ace-epam-lefs150</ResourceID>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-lefs150</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>LEFS150</ResourceName>
8 8 <AlternateName>LEFS150 - ACE Electron Proton Alpha Monitor (EPAM) 5-min Level 2 Data</AlternateName>
... ...
NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-lefs60.xml
  Diff comments   View file @eadfc37
... ... @@ -2,7 +2,7 @@
2 2 <Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
3 3 <Version>2.3.1</Version>
4 4 <NumericalData>
5   - <ResourceID>spase://NASA/NumericalData/ACE/EPAM/ace-epam-lefs60</ResourceID>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-lefs60</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>LEFS60</ResourceName>
8 8 <AlternateName>LEFS60 - ACE Electron Proton Alpha Monitor (EPAM) 5-min Level 2 Data</AlternateName>
... ...
NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-lems120.xml
  Diff comments   View file @eadfc37
... ... @@ -2,7 +2,7 @@
2 2 <Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
3 3 <Version>2.3.1</Version>
4 4 <NumericalData>
5   - <ResourceID>spase://NASA/NumericalData/ACE/EPAM/ace-epam-lems120</ResourceID>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-lems120</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>LEMS120</ResourceName>
8 8 <AlternateName>ACE Electron Proton Alpha Monitor (EPAM) 5-min Level 2 Data</AlternateName>
... ...
NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-lems30.xml
  Diff comments   View file @eadfc37
... ... @@ -2,7 +2,7 @@
2 2 <Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
3 3 <Version>2.3.1</Version>
4 4 <NumericalData>
5   - <ResourceID>spase://NASA/NumericalData/ACE/EPAM/ace-epam-lems30</ResourceID>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-lems30</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>LEMS30</ResourceName>
8 8 <AlternateName>ACE Electron Proton Alpha Monitor (EPAM) 5-min Level 2 Data</AlternateName>
... ...
NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-wartd.xml
  Diff comments   View file @eadfc37
... ... @@ -2,7 +2,7 @@
2 2 <Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
3 3 <Version>2.3.1</Version>
4 4 <NumericalData>
5   - <ResourceID>spase://NASA/NumericalData/ACE/EPAM/ace-epam-wartd</ResourceID>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/ACE/EPAM/ace-epam-wartd</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>WARTD</ResourceName>
8 8 <AlternateName>WARTD - ACE Electron Proton Alpha Monitor (EPAM) 5-min Level 2 Data</AlternateName>
... ...
NumericalData/CDPP-AMDA/ACE/SWEPAM/ace-swe-all.xml
  Diff comments   View file @eadfc37
... ... @@ -19,7 +19,7 @@
19 19 </Acknowledgement>
20 20 <Contact>
21 21 <!-- David McComas -->
22   - <PersonID>spase://CNES/Person/CDPP-AMDA/David.J.McComas</PersonID>
  22 + <PersonID>spase://SMWG/Person/David.J.McComas</PersonID>
23 23 <Role>CoInvestigator</Role>
24 24 </Contact>
25 25 <Contact>
... ...
NumericalData/CDPP-AMDA/ACE/SWEPAM/ace-swepam-real.xml
  Diff comments   View file @eadfc37
... ... @@ -16,7 +16,7 @@
16 16 </Acknowledgement>
17 17 <Contact>
18 18 <!-- David McComas -->
19   - <PersonID>spase://CNES/Person/CDPP-AMDA/David.J.McComas</PersonID>
  19 + <PersonID>spase://SMWG/Person/David.J.McComas</PersonID>
20 20 <Role>CoInvestigator</Role>
21 21 </Contact>
22 22 <Contact>
... ...
NumericalData/CDPP-AMDA/ACE/SWEPAM/ace-swepam-stea.xml
  Diff comments   View file @eadfc37
... ... @@ -18,7 +18,7 @@ Also note that the detector gains on the SWEPAM-E instrument change over time, i
18 18 The following would be an appropriate acknowledgement: “We thank the ACE SWEPAM instrument team and the ACE Science Center for providing the ACE data.” We would appreciate preprints/reprints of your papers when they become available.
19 19 </Acknowledgement>
20 20 <Contact>
21   - <PersonID>spase://CNES/Person/CDPP-AMDA/David.J.McComas</PersonID>
  21 + <PersonID>spase://SMWG/Person/David.J.McComas</PersonID>
22 22 <Role>CoInvestigator</Role>
23 23 </Contact>
24 24 <Contact>
... ...