Commit 0bcc4ffffab9c65458ccbd679492c088557909b0

Authored by Elena.Budnik
1 parent f4e63eba

cluster modifs

Instrument/AMDA/Cluster-Rumba/CIS-CODIF.xml 0 → 100644
... ... @@ -0,0 +1,26 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  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_2_6.xsd">
  3 + <Version>2.2.6</Version>
  4 + <Instrument>
  5 + <ResourceID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-CODIF</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>CIS-CODIF</ResourceName>
  8 + <AlternateName>Cluster Ion Spectrometry (CIS-CODIF)</AlternateName>
  9 + <ReleaseDate>2011-02-04T15:37:46Z</ReleaseDate>
  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 + <Contact>
  12 + <PersonID>spase://SMWG/Person/Henri.Reme</PersonID>
  13 + <Role>PrincipalInvestigator</Role>
  14 + </Contact>
  15 + <InformationURL>
  16 + <Name>NSSDC's Master Catalog</Name>
  17 + <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&amp;ex=2</URL>
  18 + <Description>Information about the Cluster Ion Spectrometry (CIS) experiment on the Cluster 2/FM5 (Rumba) mission.</Description>
  19 + </InformationURL>
  20 + <PriorID>spase://SMWG/Instrument/Cluster2-Rumba/CIS</PriorID>
  21 + </ResourceHeader>
  22 + <InstrumentType>EnergeticParticleInstrument</InstrumentType>
  23 + <InvestigationName>Cluster Ion Spectrometry (CIS) on Cluster 2/FM5 (Rumba)</InvestigationName>
  24 + <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Rumba</ObservatoryID>
  25 + </Instrument>
  26 +</Spase>
... ...
Instrument/AMDA/Cluster-Rumba/CIS-HIA.xml 0 → 100644
... ... @@ -0,0 +1,26 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  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_2_6.xsd">
  3 + <Version>2.2.6</Version>
  4 + <Instrument>
  5 + <ResourceID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-HIA</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>CIS-HIA</ResourceName>
  8 + <AlternateName>Cluster Ion Spectrometry (CIS-HIA)</AlternateName>
  9 + <ReleaseDate>2011-02-04T15:37:46Z</ReleaseDate>
  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 + <Contact>
  12 + <PersonID>spase://SMWG/Person/Henri.Reme</PersonID>
  13 + <Role>PrincipalInvestigator</Role>
  14 + </Contact>
  15 + <InformationURL>
  16 + <Name>NSSDC's Master Catalog</Name>
  17 + <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&amp;ex=2</URL>
  18 + <Description>Information about the Cluster Ion Spectrometry (CIS) experiment on the Cluster 2/FM5 (Rumba) mission.</Description>
  19 + </InformationURL>
  20 + <PriorID>spase://SMWG/Instrument/Cluster2-Rumba/CIS</PriorID>
  21 + </ResourceHeader>
  22 + <InstrumentType>EnergeticParticleInstrument</InstrumentType>
  23 + <InvestigationName>Cluster Ion Spectrometry (CIS) on Cluster 2/FM5 (Rumba)</InvestigationName>
  24 + <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Rumba</ObservatoryID>
  25 + </Instrument>
  26 +</Spase>
... ...
NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp_.xml
... ... @@ -4,7 +4,7 @@
4 4 <NumericalData>
5 5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/CIS-CODIF/clust1-cis-prp_</ResourceID>
6 6 <ResourceHeader>
7   - <ResourceName>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) CODIF Data</ResourceName>
  7 + <ResourceName>CODIF prime parametres</ResourceName>
8 8 <AlternateName>Cluster 1 Prime Parameter CIS data</AlternateName>
9 9 <ReleaseDate>2015-10-19T09:53:45Z</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>
... ... @@ -21,11 +21,7 @@
21 21 <Name>NSSDC Master Catalog listing for Cluster II Rumba Cluster Ion Spectrometry (CIS)</Name>
22 22 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-02</URL>
23 23 <Description>This site provides information concerning the Cluster II Rumba Cluster Ion Spectrometry Instrument.</Description>
24   - </InformationURL>
25   - <Association>
26   - <AssociationID>spase://SMWG/Observatory/Cluster-Rumba</AssociationID>
27   - <AssociationType>ObservedBy</AssociationType>
28   - </Association>
  24 + </InformationURL>
29 25 </ResourceHeader>
30 26 <AccessInformation>
31 27 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ... @@ -43,7 +39,7 @@
43 39 <ProviderResourceName>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data</ProviderResourceName>
44 40 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
45 41 <ProviderVersion>1</ProviderVersion>
46   - <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS</InstrumentID>
  42 + <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-CODIF</InstrumentID>
47 43 <MeasurementType>IonComposition</MeasurementType>
48 44 <TemporalDescription>
49 45 <TimeSpan>
... ... @@ -121,7 +117,7 @@
121 117 </Particle>
122 118 </Parameter>
123 119 <Parameter>
124   - <Name>H Velocity</Name>
  120 + <Name>H Velocity GSE</Name>
125 121 <ParameterKey>c1_h_v</ParameterKey>
126 122 <Description>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution</Description>
127 123 <Ucd>phys.veloc;phys.atmol.ionStage</Ucd>
... ... @@ -168,7 +164,7 @@
168 164 </Particle>
169 165 </Parameter>
170 166 <Parameter>
171   - <Name>H Velocity</Name>
  167 + <Name>H Velocity GSM</Name>
172 168 <ParameterKey>c1_h_v_gsm</ParameterKey>
173 169 <Description>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry H velocity at spin time resolution</Description>
174 170 <Ucd>phys.veloc;phys.atmol.ionStage</Ucd>
... ...
NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-cis-prp.xml
... ... @@ -4,7 +4,7 @@
4 4 <NumericalData>
5 5 <ResourceID>spase://CDPP/NumericalData/AMDA//Cluster/Cluster1/CIS-HIA/clust1-cis-prp</ResourceID>
6 6 <ResourceHeader>
7   - <ResourceName>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data</ResourceName>
  7 + <ResourceName>HIA prime parameters</ResourceName>
8 8 <AlternateName>Cluster 1 Prime Parameter CIS data</AlternateName>
9 9 <ReleaseDate>2015-10-19T10:31:00Z</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>
... ... @@ -21,11 +21,7 @@
21 21 <Name>NSSDC Master Catalog listing for Cluster II Rumba Cluster Ion Spectrometry (CIS)</Name>
22 22 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-02</URL>
23 23 <Description>This site provides information concerning the Cluster II Rumba Cluster Ion Spectrometry Instrument.</Description>
24   - </InformationURL>
25   - <Association>
26   - <AssociationID>spase://SMWG/Observatory/Cluster-Rumba</AssociationID>
27   - <AssociationType>ObservedBy</AssociationType>
28   - </Association>
  24 + </InformationURL>
29 25 </ResourceHeader>
30 26 <AccessInformation>
31 27 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ... @@ -43,7 +39,7 @@
43 39 <ProviderResourceName>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data</ProviderResourceName>
44 40 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
45 41 <ProviderVersion>1</ProviderVersion>
46   - <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS</InstrumentID>
  42 + <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-HIA</InstrumentID>
47 43 <MeasurementType>IonComposition</MeasurementType>
48 44 <TemporalDescription>
49 45 <TimeSpan>
... ...
NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-mom.xml
... ... @@ -4,7 +4,7 @@
4 4 <NumericalData>
5 5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-mom</ResourceID>
6 6 <ResourceHeader>
7   - <ResourceName>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data</ResourceName>
  7 + <ResourceName>HIA moments</ResourceName>
8 8 <AlternateName>Cluster 1 Prime Parameter CIS data</AlternateName>
9 9 <ReleaseDate>2015-10-19T10:51:45Z</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>
... ... @@ -21,11 +21,7 @@
21 21 <Name>NSSDC Master Catalog listing for Cluster II Rumba Cluster Ion Spectrometry (CIS)</Name>
22 22 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-02</URL>
23 23 <Description>This site provides information concerning the Cluster II Rumba Cluster Ion Spectrometry Instrument.</Description>
24   - </InformationURL>
25   - <Association>
26   - <AssociationID>spase://SMWG/Observatory/Cluster-Rumba</AssociationID>
27   - <AssociationType>ObservedBy</AssociationType>
28   - </Association>
  24 + </InformationURL>
29 25 </ResourceHeader>
30 26 <AccessInformation>
31 27 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ... @@ -43,7 +39,7 @@
43 39 <ProviderResourceName>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data</ProviderResourceName>
44 40 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
45 41 <ProviderVersion>1</ProviderVersion>
46   - <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS</InstrumentID>
  42 + <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-HIA</InstrumentID>
47 43 <MeasurementType>IonComposition</MeasurementType>
48 44 <TemporalDescription>
49 45 <TimeSpan>
... ... @@ -98,7 +94,7 @@
98 94 </Particle>
99 95 </Parameter>
100 96 <Parameter>
101   - <Name>Hot Ion Bulk Velocity</Name>
  97 + <Name>Ion Bulk Velocity GSE</Name>
102 98 <ParameterKey>c1_hia_v</ParameterKey>
103 99 <Description>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry hot ion bulk velocity at spin time resolution</Description>
104 100 <Ucd>phys.veloc;phys.atmol.ionStage</Ucd>
... ... @@ -145,7 +141,7 @@
145 141 </Particle>
146 142 </Parameter>
147 143 <Parameter>
148   - <Name>Hot Ion Bulk Velocity</Name>
  144 + <Name>Ion Bulk Velocity GSM</Name>
149 145 <ParameterKey>c1_hia_v_gsm</ParameterKey>
150 146 <Description>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry hot ion bulk velocity at spin time resolution</Description>
151 147 <Ucd>phys.veloc;phys.atmol.ionStage</Ucd>
... ... @@ -209,7 +205,7 @@
209 205 </Particle>
210 206 </Parameter>
211 207 <Parameter>
212   - <Name>Hot Ion Temperature</Name>
  208 + <Name>Ion Temperature</Name>
213 209 <ParameterKey>c1_hia_t</ParameterKey>
214 210 <Description>
215 211 Cluster II Tango Prime Parameter Cluster Ion Spectrometry hot ion parallel temperature at spin time resolution
... ... @@ -228,7 +224,7 @@
228 224 </Particle>
229 225 </Parameter>
230 226 <Parameter>
231   - <Name>Hot Ion Parallel Temperature</Name>
  227 + <Name>Ion Parallel Temperature</Name>
232 228 <ParameterKey>c1_hia_tpar</ParameterKey>
233 229 <Description>
234 230 Cluster II Tango Prime Parameter Cluster Ion Spectrometry hot ion parallel temperature at spin time resolution
... ... @@ -247,7 +243,7 @@
247 243 </Particle>
248 244 </Parameter>
249 245 <Parameter>
250   - <Name>Hot Ion Perpendicular Temperature</Name>
  246 + <Name>Ion Perpendicular Temperature</Name>
251 247 <ParameterKey>c1_hia_tperp</ParameterKey>
252 248 <Description>
253 249 Cluster II Tango Prime Parameter Cluster Ion Spectrometry hot ion perpendicular temperature at spin time resolution
... ...
NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml
... ... @@ -4,7 +4,7 @@
4 4 <NumericalData>
5 5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad</ResourceID>
6 6 <ResourceHeader>
7   - <ResourceName>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data</ResourceName>
  7 + <ResourceName>HIA pad</ResourceName>
8 8 <AlternateName>Cluster 1 Prime Parameter CIS data</AlternateName>
9 9 <ReleaseDate>2015-10-19T10:51:45Z</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>
... ... @@ -21,11 +21,7 @@
21 21 <Name>NSSDC Master Catalog listing for Cluster II Rumba Cluster Ion Spectrometry (CIS)</Name>
22 22 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-02</URL>
23 23 <Description>This site provides information concerning the Cluster II Rumba Cluster Ion Spectrometry Instrument.</Description>
24   - </InformationURL>
25   - <Association>
26   - <AssociationID>spase://SMWG/Observatory/Cluster-Rumba</AssociationID>
27   - <AssociationType>ObservedBy</AssociationType>
28   - </Association>
  24 + </InformationURL>
29 25 </ResourceHeader>
30 26 <AccessInformation>
31 27 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ... @@ -43,7 +39,7 @@
43 39 <ProviderResourceName>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data</ProviderResourceName>
44 40 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
45 41 <ProviderVersion>1</ProviderVersion>
46   - <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS</InstrumentID>
  42 + <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-HIA</InstrumentID>
47 43 <MeasurementType>IonComposition</MeasurementType>
48 44 <TemporalDescription>
49 45 <TimeSpan>
... ...