CDPP / CNES

Commit 4ad9254658841632bf9e6568b93d4ace60e39cd3

Authored by Elena.Budnik
1 parent 6418c374
Exists in master and in 12 other branches amdadev, aschulz, autocommit, bepi_master, bepi_update, branch_q, cleanup_registry, cleanup_registry_master, cleanup_registry_merged, juice_jdc, juno_jade, soar

cis

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Instrument/AMDA/Cluster-Rumba/CIS-HIA.xml
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... ... @@ -6,21 +6,31 @@
6 6 <ResourceHeader>
7 7 <ResourceName>CIS-HIA</ResourceName>
8 8 <AlternateName>Cluster Ion Spectrometry : Hot Ion Analyser</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>
  9 + <ReleaseDate>2016-10-04T15:37:46Z</ReleaseDate>
  10 + <Description>The HIA is a symmetric quadrispherical analyzer of top-hat geometry, and uses microchannel-plate electron multipliers and position encoding by discrete anodes. A 2D distribution is obtained once per 62.5 ms, and a full 3D distribution of ions in the energy range ~5 eV/charge to 32 KeV/charge is obtained every 4 s. For more details of the Cluster mission, the spacecraft, and its instruments, see the report ``Cluster: mission, payload and supporting activities,'' March 1993, ESA SP-1159, and the included article ``The Cluster Ion Spectrometry Experiment,'' by H. Reme et al., from which this information was obtained.</Description>
  11 + <Acknowledgement>Principal Investigator: Iannis Dandouras</Acknowledgement>
11 12 <Contact>
12   - <PersonID>spase://SMWG/Person/Henri.Reme</PersonID>
  13 + <PersonID>spase://CDPP/Person/Jannis.Dandouras</PersonID>
13 14 <Role>PrincipalInvestigator</Role>
14 15 </Contact>
15 16 <InformationURL>
  17 + <Name>ESA web page</Name>
  18 + <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
  19 + <Description>CIS: Cluster Ion Spectrometry experiment</Description>
  20 + </InformationURL>
  21 + <InformationURL>
16 22 <Name>NSSDC's Master Catalog</Name>
17 23 <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&amp;ex=2</URL>
18 24 <Description>Information about the Cluster Ion Spectrometry (CIS) experiment on the Cluster 2/FM5 (Rumba) mission.</Description>
19 25 </InformationURL>
20 26 <PriorID>spase://SMWG/Instrument/Cluster2-Rumba/CIS</PriorID>
21 27 </ResourceHeader>
22   - <InstrumentType>EnergeticParticleInstrument</InstrumentType>
23   - <InvestigationName>Cluster Ion Spectrometry (CIS) on Cluster 2/FM5 (Rumba)</InvestigationName>
  28 + <InstrumentType>ElectrostaticAnalyser</InstrumentType>
  29 + <InvestigationName>CIS</InvestigationName>
  30 + <OperatingSpan>
  31 + <StartDate>2000-12-01T00:00:00</StartDate>
  32 + <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
  33 + </OperatingSpan>
24 34 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Rumba</ObservatoryID>
25 35 </Instrument>
26 36 </Spase>
... ...
Instrument/AMDA/Cluster-Rumba/CIS.xml
  Diff comments   View file @4ad9254
... ... @@ -25,7 +25,7 @@
25 25 </InformationURL>
26 26 <PriorID>spase://SMWG/Instrument/Cluster2-Rumba/CIS</PriorID>
27 27 </ResourceHeader>
28   - <InstrumentType>ThermalPlasma</InstrumentType>
  28 + <InstrumentType></InstrumentType>
29 29 <InvestigationName></InvestigationName>
30 30 <OperatingSpan>
31 31 <StartDate>2000-12-01T00:00:00</StartDate>
... ...
Instrument/AMDA/Cluster-Samba/CIS-HIA.xml
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... ... @@ -6,21 +6,32 @@
6 6 <ResourceHeader>
7 7 <ResourceName>CIS-HIA</ResourceName>
8 8 <AlternateName>Cluster Ion Spectrometry : Hot Ion Analyser</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>
  9 + <ReleaseDate>2016-10-04T15:37:46Z</ReleaseDate>
  10 + <Description>The HIA is a symmetric quadrispherical analyzer of top-hat geometry, and uses microchannel-plate electron multipliers and position encoding by discrete anodes. A 2D distribution is obtained once per 62.5 ms, and a full 3D distribution of ions in the energy range ~5 eV/charge to 32 KeV/charge is obtained every 4 s. For more details of the Cluster mission, the spacecraft, and its instruments, see the report ``Cluster: mission, payload and supporting activities,'' March 1993, ESA SP-1159, and the included article ``The Cluster Ion Spectrometry Experiment,'' by H. Reme et al., from which this information was obtained.</Description>
  11 + <Acknowledgement>Principal Investigator: Iannis Dandouras</Acknowledgement>
11 12 <Contact>
12   - <PersonID>spase://SMWG/Person/Henri.Reme</PersonID>
  13 + <PersonID>spase://CDPP/Person/Jannis.Dandouras</PersonID>
13 14 <Role>PrincipalInvestigator</Role>
14 15 </Contact>
15 16 <InformationURL>
  17 + <Name>ESA web page</Name>
  18 + <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
  19 + <Description>CIS: Cluster Ion Spectrometry experiment</Description>
  20 + </InformationURL>
  21 + <InformationURL>
16 22 <Name>NSSDC's Master Catalog</Name>
17 23 <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&amp;ex=2</URL>
18 24 <Description>Information about the Cluster Ion Spectrometry (CIS) experiment on the Cluster 2/FM5 (Rumba) mission.</Description>
19   - </InformationURL>
  25 + </InformationURL>
20 26 <PriorID>spase://SMWG/Instrument/Cluster2-Samba/CIS</PriorID>
21 27 </ResourceHeader>
22   - <InstrumentType>EnergeticParticleInstrument</InstrumentType>
23   - <InvestigationName>Cluster Ion Spectrometry (CIS) on Cluster 2/FM7 (Samba)</InvestigationName>
  28 + <InstrumentType>ElectrostaticAnalyser</InstrumentType>
  29 + <InvestigationName>CIS</InvestigationName>
  30 + <OperatingSpan>
  31 + <StartDate>2000-12-01T00:00:00</StartDate>
  32 + <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
  33 + <Note>C3 spacecraft tilt by 40° during one month: 2008-05-01T00:00:00</Note>
  34 + </OperatingSpan>
24 35 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Samba</ObservatoryID>
25 36 </Instrument>
26 37 </Spase>
... ...
Instrument/AMDA/Cluster-Samba/CIS.xml
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... ... @@ -25,7 +25,7 @@
25 25 </InformationURL>
26 26 <PriorID>spase://SMWG/Instrument/Cluster2-Samba/CIS</PriorID>
27 27 </ResourceHeader>
28   - <InstrumentType>ThermalPlasma</InstrumentType>
  28 + <InstrumentType></InstrumentType>
29 29 <InvestigationName></InvestigationName>
30 30 <OperatingSpan>
31 31 <StartDate>2000-12-01T00:00:00</StartDate>
... ...
Instrument/AMDA/Cluster-Tango/CIS.xml
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... ... @@ -25,7 +25,7 @@
25 25 </InformationURL>
26 26 <PriorID>spase://SMWG/Instrument/Cluster2-Tango/CIS</PriorID>
27 27 </ResourceHeader>
28   - <InstrumentType>ThermalPlasma</InstrumentType>
  28 + <InstrumentType></InstrumentType>
29 29 <InvestigationName></InvestigationName>
30 30 <OperatingSpan>
31 31 <StartDate>2000-12-01T00:00:00</StartDate>
... ...
NumericalData/AMDA/ACE/MFI/ace-imf-all.xml
  Diff comments   View file @4ad9254
... ... @@ -58,7 +58,7 @@
58 58 <TemporalDescription>
59 59 <TimeSpan>
60 60 <StartDate>1997-09-02T00:00:12Z</StartDate>
61   - <StopDate>2016-10-01T23:59:52Z</StopDate>
  61 + <StopDate>2016-10-15T23:59:49Z</StopDate>
62 62 </TimeSpan>
63 63 <Cadence>PT16S</Cadence>
64 64 </TemporalDescription>
... ...
NumericalData/AMDA/ACE/MFI/ace-mag-real.xml
  Diff comments   View file @4ad9254
... ... @@ -51,7 +51,7 @@
51 51 <TemporalDescription>
52 52 <TimeSpan>
53 53 <StartDate>2014-01-06T00:00:00Z</StartDate>
54   - <StopDate>2016-10-11T23:59:59Z</StopDate>
  54 + <StopDate>2016-10-25T23:59:59Z</StopDate>
55 55 </TimeSpan>
56 56 <Cadence>PT60S</Cadence>
57 57 </TemporalDescription>
... ...
NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml
  Diff comments   View file @4ad9254
... ... @@ -44,7 +44,7 @@
44 44 <TemporalDescription>
45 45 <TimeSpan>
46 46 <StartDate>2014-01-06T00:00:00Z</StartDate>
47   - <StopDate>2016-10-11T23:59:59Z</StopDate>
  47 + <StopDate>2016-10-25T23:59:59Z</StopDate>
48 48 </TimeSpan>
49 49 <Cadence>PT60S</Cadence>
50 50 </TemporalDescription>
... ...
NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml
  Diff comments   View file @4ad9254
... ... @@ -59,7 +59,7 @@
59 59 <TemporalDescription>
60 60 <TimeSpan>
61 61 <StartDate>2001-01-01T00:00:00Z</StartDate>
62   - <StopDate>2016-10-01T23:55:00Z</StopDate>
  62 + <StopDate>2016-10-15T23:55:00Z</StopDate>
63 63 </TimeSpan>
64 64 <Cadence>PT5M</Cadence>
65 65 </TemporalDescription>
... ...
NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-mom.xml
  Diff comments   View file @4ad9254
... ... @@ -5,23 +5,31 @@
5 5 <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-mom</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>ion moments</ResourceName>
8   - <AlternateName> </AlternateName>
9   - <ReleaseDate>2015-10-19T10:51:45Z</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   - <Acknowledgement>NASA, Prof. Henri Reme, European Space Agency</Acknowledgement>
  8 + <AlternateName>HIA onboard hot ion moments</AlternateName>
  9 + <ReleaseDate>2016-10-19T10:51:45Z</ReleaseDate>
  10 + <Description>
  11 + HIA ion moments are onboard calculated, then reprocessed on ground with the following steps:
  12 + * detection efficiency correction using total efficiency calibration coefficients (from calibration files)
  13 + * coordinate transformations to ISR2 and GSE systems (for ion bulk velocity)
  14 + * parallel and perpendicular temperature calculations using the B-field vector (FGM-CAA spin resolution)
  15 +
  16 + They have 1-spin time resolution (~4 s), and are calculated from the full angular and energy resolution 3-D ion distributions.
  17 + They include ion density, bulk velocity vector (in both GSE and GSM frame), pressure tensor, total pressure, and temperatures (parallel and perpendicular to the magnetic field, and total temperature</Description>
  18 + <Acknowledgement>Principal Investigator: Dr. Iannis Dandouras</Acknowledgement>
12 19 <Contact>
13   - <PersonID>spase://SMWG/Person/Henri.Reme</PersonID>
  20 + <PersonID>spase://CDPP/Person/Jannis.Dandouras</PersonID>
14 21 <Role>PrincipalInvestigator</Role>
15 22 </Contact>
16   - <Contact>
17   - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
18   - <Role>TechnicalContact</Role>
19   - </Contact>
20 23 <InformationURL>
21   - <Name>NSSDC Master Catalog listing for Cluster II Rumba Cluster Ion Spectrometry (CIS)</Name>
  24 + <Name>CSA Instrument User Guides</Name>
  25 + <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
  26 + <Description>This site provides information concerning the Cluster Instruments.</Description>
  27 + </InformationURL>
  28 + <InformationURL>
  29 + <Name>NSSDC Master Catalog listing for Cluster Ion Spectrometry (CIS)</Name>
22 30 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-02</URL>
23   - <Description>This site provides information concerning the Cluster II Rumba Cluster Ion Spectrometry Instrument.</Description>
24   - </InformationURL>
  31 + <Description>This site provides information concerning the Cluster Ion Spectrometry Instrument.</Description>
  32 + </InformationURL>
25 33 </ResourceHeader>
26 34 <AccessInformation>
27 35 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ... @@ -31,12 +39,11 @@
31 39 <Name>AMDA at CDPP</Name>
32 40 <URL>http://amda.cdpp.eu</URL>
33 41 </AccessURL>
34   - <Format>NetCDF</Format>
35   - <Acknowledgement>NASA, Prof. Henri Reme</Acknowledgement>
  42 + <Format>NetCDF</Format>
36 43 </AccessInformation>
37 44 <ProviderName>CSA</ProviderName>
38 45 <ProcessingLevel>Calibrated</ProcessingLevel>
39   - <ProviderResourceName>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry (CIS) Data</ProviderResourceName>
  46 + <ProviderResourceName>C1_CP_CIS-HIA_ONBOARD_MOMENTS</ProviderResourceName>
40 47 <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
41 48 <ProviderVersion>1</ProviderVersion>
42 49 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/CIS-HIA</InstrumentID>
... ... @@ -73,14 +80,14 @@
73 80 <Parameter>
74 81 <Name>density</Name>
75 82 <ParameterKey>c1_hia_dens</ParameterKey>
76   - <Description>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry hot ion number density at spin time resolution</Description>
  83 + <Description>Hot ion number density at spin time resolution</Description>
77 84 <Ucd>phys.density;phys.atmol.ionStage</Ucd>
78 85 <Cadence>PT4S</Cadence>
79 86 <Units>cm^-3</Units>
80 87 <UnitsConversion>1.0e6&gt;m^-3</UnitsConversion>
81 88 <RenderingHints>
82 89 <DisplayType>TimeSeries</DisplayType>
83   - <AxisLabel>n(HIA)</AxisLabel>
  90 + <AxisLabel>n(ion)</AxisLabel>
84 91 <ScaleMin>0.0010</ScaleMin>
85 92 <ScaleMax>1000</ScaleMax>
86 93 </RenderingHints>
... ... @@ -96,7 +103,7 @@
96 103 <Parameter>
97 104 <Name>v_gse</Name>
98 105 <ParameterKey>c1_hia_v</ParameterKey>
99   - <Description>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry hot ion bulk velocity at spin time resolution</Description>
  106 + <Description>Hot ion bulk velocity at spin time resolution in GSE</Description>
100 107 <Ucd>phys.veloc;phys.atmol.ionStage</Ucd>
101 108 <Cadence>PT4S</Cadence>
102 109 <Units>km/s</Units>
... ... @@ -143,7 +150,7 @@
143 150 <Parameter>
144 151 <Name>v_gsm</Name>
145 152 <ParameterKey>c1_hia_v_gsm</ParameterKey>
146   - <Description>Cluster II Rumba Prime Parameter Cluster Ion Spectrometry hot ion bulk velocity at spin time resolution</Description>
  153 + <Description>Hot ion bulk velocity at spin time resolution in GSM</Description>
147 154 <Ucd>phys.veloc;phys.atmol.ionStage</Ucd>
148 155 <Cadence>PT4S</Cadence>
149 156 <Units>km/s</Units>
... ... @@ -190,10 +197,11 @@
190 197 <Parameter>
191 198 <Name>|v|</Name>
192 199 <ParameterKey>c1_hia_vtot</ParameterKey>
193   - <Description>Cluster Rumba Fluxgate Magnetometer Velocity magnitude at spin time resolution</Description>
  200 + <Description> Hot ion bulk velocity magnitude at spin time resolution</Description>
194 201 <Ucd>phys.veloc;phys.atmol.ionStage</Ucd>
195 202 <Cadence>PT4S</Cadence>
196   - <Units>nT</Units>
  203 + <Units>km/s</Units>
  204 + <UnitsConversion>1.0e3&gt;m s^-1</UnitsConversion>
197 205 <RenderingHints>
198 206 <DisplayType>TimeSeries</DisplayType>
199 207 </RenderingHints>
... ... @@ -205,10 +213,10 @@
205 213 </Particle>
206 214 </Parameter>
207 215 <Parameter>
208   - <Name>temperature</Name>
  216 + <Name>temperature total</Name>
209 217 <ParameterKey>c1_hia_t</ParameterKey>
210 218 <Description>
211   - Cluster II Tango Prime Parameter Cluster Ion Spectrometry hot ion parallel temperature at spin time resolution
  219 + Hot ion temperature at spin time resolution
212 220 </Description>
213 221 <Ucd>phys.temperature;phys.atmol.ionStage</Ucd>
214 222 <Cadence>PT4S</Cadence>
... ... @@ -216,7 +224,7 @@
216 224 <RenderingHints>
217 225 <DisplayType>TimeSeries</DisplayType>
218 226 </RenderingHints>
219   - <FillValue>-8.62069e+32</FillValue>
  227 + <FillValue>-1.e+31</FillValue>
220 228 <Particle>
221 229 <ParticleType>Ion</ParticleType>
222 230 <Qualifier>Scalar</Qualifier>
... ... @@ -227,7 +235,7 @@
227 235 <Name>t_para</Name>
228 236 <ParameterKey>c1_hia_tpar</ParameterKey>
229 237 <Description>
230   - Cluster II Tango Prime Parameter Cluster Ion Spectrometry hot ion parallel temperature at spin time resolution
  238 + Hot ion parallel temperature at spin time resolution
231 239 </Description>
232 240 <Ucd>phys.temperature;phys.atmol.ionStage</Ucd>
233 241 <Cadence>PT4S</Cadence>
... ... @@ -235,7 +243,7 @@
235 243 <RenderingHints>
236 244 <DisplayType>TimeSeries</DisplayType>
237 245 </RenderingHints>
238   - <FillValue>-8.62069e+32</FillValue>
  246 + <FillValue>-1.e+31</FillValue>
239 247 <Particle>
240 248 <ParticleType>Ion</ParticleType>
241 249 <Qualifier>Scalar</Qualifier>
... ... @@ -246,7 +254,7 @@
246 254 <Name>t_perp</Name>
247 255 <ParameterKey>c1_hia_tperp</ParameterKey>
248 256 <Description>
249   - Cluster II Tango Prime Parameter Cluster Ion Spectrometry hot ion perpendicular temperature at spin time resolution
  257 + Hot ion perpendicular temperature at spin time resolution
250 258 </Description>
251 259 <Ucd>phys.temperature;phys.atmol.ionStage</Ucd>
252 260 <Cadence>PT4S</Cadence>
... ... @@ -254,7 +262,7 @@
254 262 <RenderingHints>
255 263 <DisplayType>TimeSeries</DisplayType>
256 264 </RenderingHints>
257   - <FillValue>-8.62069e+32</FillValue>
  265 + <FillValue>-1.e+31</FillValue>
258 266 <Particle>
259 267 <ParticleType>Ion</ParticleType>
260 268 <Qualifier>Scalar</Qualifier>
... ... @@ -262,8 +270,11 @@
262 270 </Particle>
263 271 </Parameter>
264 272 <Parameter>
265   - <Name>pressure</Name>
  273 + <Name>pressure total</Name>
266 274 <ParameterKey>c1_hia_press</ParameterKey>
  275 + <Description>
  276 + Hot ion pressure (scalar) at spin time resolution
  277 + </Description>
267 278 <Ucd>phys.pressure;phys.atmol.ionStage</Ucd>
268 279 <Cadence>PT4S</Cadence>
269 280 <Units>nPa</Units>
... ... @@ -277,8 +288,11 @@
277 288 </Particle>
278 289 </Parameter>
279 290 <Parameter>
280   - <Name>pressure_gse</Name>
  291 + <Name>pressure tensor gse</Name>
281 292 <ParameterKey>c1_hia_prest</ParameterKey>
  293 + <Description>
  294 + Hot ion pressure (tensor) at spin time resolution in GSE
  295 + </Description>
282 296 <Ucd>phys.pressure;phys.atmol.ionStage</Ucd>
283 297 <Cadence>PT4S</Cadence>
284 298 <Units>nPa</Units>
... ... @@ -290,7 +304,7 @@
290 304 <DisplayType>TimeSeries</DisplayType>
291 305 </RenderingHints>
292 306 <Structure>
293   - <Size>3</Size>
  307 + <Size>9</Size>
294 308 <Element>
295 309 <Name>xx</Name>
296 310 <Index>1</Index>
... ...
NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml
  Diff comments   View file @4ad9254
... ... @@ -27,7 +27,7 @@
27 27 <TemporalDescription>
28 28 <TimeSpan>
29 29 <StartDate>2004-01-10T07:54:21Z</StartDate>
30   - <StopDate>2016-11-21T01:30:23Z</StopDate>
  30 + <StopDate>2016-12-09T17:13:35Z</StopDate>
31 31 </TimeSpan>
32 32 <Cadence>PT60S</Cadence>
33 33 </TemporalDescription>
... ...
NumericalData/AMDA/OMNI/omni-5min-all.xml
  Diff comments   View file @4ad9254
... ... @@ -47,7 +47,7 @@ for creating the OMNI data set.&lt;/Acknowledgement&gt;
47 47 <TemporalDescription>
48 48 <TimeSpan>
49 49 <StartDate>1981-01-01T00:00:00Z</StartDate>
50   - <StopDate>2016-09-26T23:55:00Z</StopDate>
  50 + <StopDate>2016-09-30T23:55:00Z</StopDate>
51 51 </TimeSpan>
52 52 <Cadence>PT5M</Cadence>
53 53 </TemporalDescription>
... ...
NumericalData/AMDA/OMNI/omni-hour-all.xml
  Diff comments   View file @4ad9254
... ... @@ -47,7 +47,7 @@ for creating the OMNI data set.&lt;/Acknowledgement&gt;
47 47 <TemporalDescription>
48 48 <TimeSpan>
49 49 <StartDate>1970-01-01T00:00:00Z</StartDate>
50   - <StopDate>2016-09-27T14:00:00Z</StopDate>
  50 + <StopDate>2016-10-11T15:00:00Z</StopDate>
51 51 </TimeSpan>
52 52 <Cadence>PT1H</Cadence>
53 53 </TemporalDescription>
... ...
Observatory/AMDA/Cluster-Rumba.xml
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... ... @@ -13,7 +13,6 @@
13 13 <Description>Cluster II is part of an international collaboration to investigate the physical connection between the Sun and Earth. Flying in a tetrahedral (triangular pyramid) formation, the four spacecraft collect the most detailed data yet on small-scale changes in near-Earth space and the interaction between the charged particles of the solar wind and Earth's atmosphere.
14 14 This enables scientists to build a three-dimensional model of the magnetosphere and to better understand the processes taking place inside it. </Description>
15 15 <Acknowledgement>C. Philippe Escoubet (ESA Project Scientist)</Acknowledgement>
16   - <InformationURL>
17 16 <Contact>
18 17 <PersonID>spase://SMWG/Person/Christophe.Philippe.Escoubet</PersonID>
19 18 <Role>ProjectScientist</Role>
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Observatory/AMDA/Cluster-Salsa.xml
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... ... @@ -14,11 +14,11 @@
14 14 <Description>
15 15 Cluster II is part of an international collaboration to investigate the physical connection between the Sun and Earth. Flying in a tetrahedral (triangular pyramid) formation, the four spacecraft collect the most detailed data yet on small-scale changes in near-Earth space and the interaction between the charged particles of the solar wind and Earth's atmosphere. This enables scientists to build a three-dimensional model of the magnetosphere and to better understand the processes taking place inside it.
16 16 </Description>
  17 + <Acknowledgement>C. Philippe Escoubet (ESA Project Scientist)</Acknowledgement>
17 18 <Contact>
18 19 <PersonID>spase://SMWG/Person/Christophe.Philippe.Escoubet</PersonID>
19 20 <Role>ProjectScientist</Role>
20   - </Contact>
21   - <Acknowledgement>C. Philippe Escoubet (ESA Project Scientist)</Acknowledgement>
  21 + </Contact>
22 22 <InformationURL>
23 23 <Name>Fact Sheet of the Cluster mission</Name>
24 24 <URL>http://sci.esa.int/jump.cfm?oid=47348</URL>
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Person/Jannis.Dandouras 0 → 100644
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... ... @@ -0,0 +1,10 @@
  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_0.xsd">
  3 + <Version>2.2.0</Version>
  4 + <Person>
  5 + <ResourceID>spase://CDPP/Person/Jannis.Dandouras</ResourceID>
  6 + <PersonName>Dr. Iannis S. Dandouras</PersonName>
  7 + <OrganizationName>IRAP, Toulouse</OrganizationName>
  8 + <Email>Iannis.Dandouras@irap.omp.eu</Email>
  9 + </Person>
  10 +</Spase>
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