Commit 0bcc4ffffab9c65458ccbd679492c088557909b0
1 parent
f4e63eba
Exists in
master
and in
12 other branches
cluster modifs
Showing
6 changed files
with
71 additions
and
35 deletions
Show diff stats
... | ... | @@ -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&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> | ... | ... |
... | ... | @@ -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&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> | ... | ... |