From 51690af93a934b3be539fa98bfabd41e1b67bab6 Mon Sep 17 00:00:00 2001
From: Elena.Budnik <ebudnik@irap.omp.eu>
Date: Thu, 7 Jul 2016 17:48:59 +0200
Subject: [PATCH] work
---
NumericalData/AMDA/Cluster/Cluster1/FGM/clust1-fgm-high.xml | 2 +-
NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml | 18 ++++++------------
NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml | 20 +++++++-------------
NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml | 22 ++++++----------------
NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml | 12 ++++--------
NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml | 23 +++++++++--------------
NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml | 19 +++++++------------
NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml | 25 ++++++++++++-------------
NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml | 23 +++++++++++------------
9 files changed, 63 insertions(+), 101 deletions(-)
diff --git a/NumericalData/AMDA/Cluster/Cluster1/FGM/clust1-fgm-high.xml b/NumericalData/AMDA/Cluster/Cluster1/FGM/clust1-fgm-high.xml
index 99686f1..7226e3d 100644
--- a/NumericalData/AMDA/Cluster/Cluster1/FGM/clust1-fgm-high.xml
+++ b/NumericalData/AMDA/Cluster/Cluster1/FGM/clust1-fgm-high.xml
@@ -7,7 +7,7 @@
<ResourceName>0.2 sec (5vps)</ResourceName>
<AlternateName>Cluster 1 5-vector-per-spin FGM Data</AlternateName>
<ReleaseDate>2015-10-16T15:36:00Z</ReleaseDate>
- <Description>This dataset contains spin resolution measurements of the magnetic field vector from the fluxgate magnetometer (FGM) instrument
+ <Description>This dataset contains 5Hz resolution measurements of the magnetic field vector from the fluxgate magnetometer (FGM) instrument
on the Cluster Rumba spacecraft.</Description>
<Acknowledgement>NASA, Andre Balogh, Elizabeth E. Lucek</Acknowledgement>
<Contact>
diff --git a/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml b/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml
index 9cf66d7..d9560d9 100644
--- a/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml
@@ -4,19 +4,13 @@
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp</ResourceID>
<ResourceHeader>
- <ResourceName>Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ResourceName>
+ <ResourceName>prime parameters : electrons</ResourceName>
<AlternateName>Cluster 1 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2015-10-16T16:01:46Z</ReleaseDate>
- <Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
- Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV
- for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. 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 RAPID:
- The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
- this information was obtained.</Description>
- <Acknowledgement>NASA, Dr. Berend Wilken, European Space Agency</Acknowledgement>
+ <Description/>
+ <Acknowledgement/>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
+ <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
<Role>TechnicalContact</Role>
</Contact>
<InformationURL>
@@ -34,7 +28,7 @@
<URL>http://amda.cdpp.eu</URL>
</AccessURL>
<Format>NetCDF</Format>
- <Acknowledgement>NASA, Dr. Berend Wilken</Acknowledgement>
+ <Acknowledgement/>
</AccessInformation>
<ProviderName>CSA</ProviderName>
<ProcessingLevel>Calibrated</ProcessingLevel>
@@ -72,7 +66,7 @@
<Keyword>magnetotail</Keyword>
<Keyword>lobe</Keyword>
<Parameter>
- <Name>Electron Flux </Name>
+ <Name>diff flux</Name>
<ParameterKey>c1_rap_e</ParameterKey>
<Description>Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux at spin time resolution</Description>
<Ucd>phys.flux.density;phys.count;phys.electron</Ucd>
diff --git a/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml b/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml
index ad7684e..8f180b3 100644
--- a/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml
@@ -4,19 +4,13 @@
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp</ResourceID>
<ResourceHeader>
- <ResourceName>Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ResourceName>
+ <ResourceName>prime parameters : protons</ResourceName>
<AlternateName>Cluster 1 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2015-10-16T16:11:46Z</ReleaseDate>
- <Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
- Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV
- for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. 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 RAPID:
- The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
- this information was obtained.</Description>
- <Acknowledgement>NASA, Dr. Berend Wilken, European Space Agency</Acknowledgement>
+ <Description/>
+ <Acknowledgement/>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
+ <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
<Role>TechnicalContact</Role>
</Contact>
<InformationURL>
@@ -34,9 +28,9 @@
<URL>http://amda.cdpp.eu</URL>
</AccessURL>
<Format>NetCDF</Format>
- <Acknowledgement>NASA, Dr. Berend Wilken</Acknowledgement>
+ <Acknowledgement/>
</AccessInformation>
- <ProviderName>CSA</ProviderName>
+ <ProviderName>CSA </ProviderName>
<ProcessingLevel>Calibrated</ProcessingLevel>
<ProviderResourceName>Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ProviderResourceName>
<ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
@@ -72,7 +66,7 @@
<Keyword>magnetotail</Keyword>
<Keyword>lobe</Keyword>
<Parameter>
- <Name>Proton Flux </Name>
+ <Name>diff flux</Name>
<ParameterKey>c1_rap_p</ParameterKey>
<Description>Cluster II Rumba Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux at spin time resolution</Description>
<Ucd>phys.flux.density;phys.count;phys.atmol.ionStage</Ucd>
diff --git a/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml b/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml
index 2058b3f..bae22f5 100644
--- a/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml
@@ -4,19 +4,13 @@
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp</ResourceID>
<ResourceHeader>
- <ResourceName>Cluster II Salsa Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ResourceName>
+ <ResourceName>prime parameters : electrons</ResourceName>
<AlternateName>Cluster 2 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2015-10-19T15:51:46Z</ReleaseDate>
- <Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
- Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV
- for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. 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 RAPID:
- The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
- this information was obtained.</Description>
- <Acknowledgement>NASA, Dr. Berend Wilken, European Space Agency</Acknowledgement>
+ <Description/>
+ <Acknowledgement/>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
+ <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
<Role>TechnicalContact</Role>
</Contact>
<InformationURL>
@@ -24,10 +18,6 @@
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-06</URL>
<Description>This site provides information concerning the Cluster II Salsa Research with Adaptive Particle Imaging Detectors Instrument.</Description>
</InformationURL>
- <Association>
- <AssociationID>spase://SMWG/Observatory/Cluster-Salsa</AssociationID>
- <AssociationType>ObservedBy</AssociationType>
- </Association>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -38,7 +28,7 @@
<URL>http://amda.cdpp.eu</URL>
</AccessURL>
<Format>NetCDF</Format>
- <Acknowledgement>NASA, Dr. Berend Wilken</Acknowledgement>
+ <Acknowledgement/>
</AccessInformation>
<ProviderName>CSA</ProviderName>
<ProcessingLevel>Calibrated</ProcessingLevel>
@@ -76,7 +66,7 @@
<Keyword>magnetotail</Keyword>
<Keyword>lobe</Keyword>
<Parameter>
- <Name>Electron Flux </Name>
+ <Name>diff flux</Name>
<ParameterKey>c2_rap_e</ParameterKey>
<Description>Cluster II Salsa Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux at spin time resolution</Description>
<Ucd>phys.flux.density;phys.count;phys.electron</Ucd>
diff --git a/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml b/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml
index 2b79a54..6b5318a 100644
--- a/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml
@@ -4,7 +4,7 @@
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp</ResourceID>
<ResourceHeader>
- <ResourceName>Cluster II Salsa Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ResourceName>
+ <ResourceName>prime parameters : protons</ResourceName>
<AlternateName>Cluster 2 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2015-10-19T15:51:46Z</ReleaseDate>
<Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
@@ -14,9 +14,9 @@
payload and supporting activities, March 1993, ESA SP-1159, and the included article RAPID:
The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
this information was obtained.</Description>
- <Acknowledgement>NASA, Dr. Berend Wilken, European Space Agency</Acknowledgement>
+ <Acknowledgement/>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
+ <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
<Role>TechnicalContact</Role>
</Contact>
<InformationURL>
@@ -24,10 +24,6 @@
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-06</URL>
<Description>This site provides information concerning the Cluster II Salsa Research with Adaptive Particle Imaging Detectors Instrument.</Description>
</InformationURL>
- <Association>
- <AssociationID>spase://SMWG/Observatory/Cluster-Salsa</AssociationID>
- <AssociationType>ObservedBy</AssociationType>
- </Association>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -76,7 +72,7 @@
<Keyword>magnetotail</Keyword>
<Keyword>lobe</Keyword>
<Parameter>
- <Name>Proton Flux </Name>
+ <Name>diff flux</Name>
<ParameterKey>c2_rap_p</ParameterKey>
<Description>Cluster II Salsa Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux at spin time resolution</Description>
<Ucd>phys.flux.density;phys.count;phys.atmol.ionStage</Ucd>
diff --git a/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml b/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml
index d2002ba..49c54ca 100644
--- a/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml
@@ -4,29 +4,24 @@
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp</ResourceID>
<ResourceHeader>
- <ResourceName>Cluster II Samba Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ResourceName>
+ <ResourceName>electrons</ResourceName>
<AlternateName>Cluster 3 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2015-10-19T15:51:46Z</ReleaseDate>
- <Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
- Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV
- for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. 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 RAPID:
- The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
- this information was obtained.</Description>
- <Acknowledgement>NASA, Dr. Berend Wilken, European Space Agency</Acknowledgement>
+ <Description></Description>
+ <Acknowledgement/>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
+ <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
<Role>TechnicalContact</Role>
</Contact>
<InformationURL>
<Name>NSSDC Master Catalog listing for Cluster II Samba Research with Adaptive Particle Imaging Detectors (RAPID)</Name>
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-06</URL>
<Description>This site provides information concerning the Cluster II Samba Research with Adaptive Particle Imaging Detectors Instrument.</Description>
- </InformationURL>
+ </InformationURL>
<Association>
- <AssociationID>spase://SMWG/Observatory/Cluster-Rumba</AssociationID>
- <AssociationType>ObservedBy</AssociationType>
+ <AssociationID>cluster3-rap-pp</AssociationID>
+ <AssociationType>PartOf</AssociationType>
+ <Note>prime parameters</Note>
</Association>
</ResourceHeader>
<AccessInformation>
@@ -76,7 +71,7 @@
<Keyword>magnetotail</Keyword>
<Keyword>lobe</Keyword>
<Parameter>
- <Name>Electron Flux </Name>
+ <Name>diff flux</Name>
<ParameterKey>c3_rap_e</ParameterKey>
<Description>Cluster II Samba Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux at spin time resolution</Description>
<Ucd>phys.flux.density;phys.count;phys.electron</Ucd>
diff --git a/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml b/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml
index 5de3aa9..9f1d916 100644
--- a/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml
@@ -4,19 +4,13 @@
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp</ResourceID>
<ResourceHeader>
- <ResourceName>Cluster II Samba Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ResourceName>
+ <ResourceName>protons</ResourceName>
<AlternateName>Cluster 3 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2015-10-19T15:51:46Z</ReleaseDate>
- <Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
- Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV
- for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. 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 RAPID:
- The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
- this information was obtained.</Description>
- <Acknowledgement>NASA, Dr. Berend Wilken, European Space Agency</Acknowledgement>
+ <Description/>
+ <Acknowledgement/>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
+ <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
<Role>TechnicalContact</Role>
</Contact>
<InformationURL>
@@ -25,8 +19,9 @@
<Description>This site provides information concerning the Cluster II Samba Research with Adaptive Particle Imaging Detectors Instrument.</Description>
</InformationURL>
<Association>
- <AssociationID>spase://SMWG/Observatory/Cluster-Samba</AssociationID>
- <AssociationType>ObservedBy</AssociationType>
+ <AssociationID>cluster3-rap-pp</AssociationID>
+ <AssociationType>PartOf</AssociationType>
+ <Note>prime parameters</Note>
</Association>
</ResourceHeader>
<AccessInformation>
diff --git a/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml b/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml
index 759fe68..2cedcfb 100644
--- a/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml
@@ -4,26 +4,25 @@
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp</ResourceID>
<ResourceHeader>
- <ResourceName>Cluster II Tango Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ResourceName>
+ <ResourceName>electrons</ResourceName>
<AlternateName>Cluster 4 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2015-10-16T16:51:46Z</ReleaseDate>
- <Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
- Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV
- for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. 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 RAPID:
- The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
- this information was obtained.</Description>
- <Acknowledgement>NASA, Dr. Berend Wilken, European Space Agency</Acknowledgement>
+ <Description></Description>
+ <Acknowledgement></Acknowledgement>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
+ <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
<Role>TechnicalContact</Role>
</Contact>
<InformationURL>
<Name>NSSDC Master Catalog listing for Cluster II Tango Research with Adaptive Particle Imaging Detectors (RAPID)</Name>
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-06</URL>
<Description>This site provides information concerning the Cluster II Tango Research with Adaptive Particle Imaging Detectors Instrument.</Description>
- </InformationURL>
+ </InformationURL>
+ <Association>
+ <AssociationID>cluster4-rap-pp</AssociationID>
+ <AssociationType>PartOf</AssociationType>
+ <Note>prime parameters</Note>
+ </Association>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -34,7 +33,7 @@
<URL>http://amda.cdpp.eu</URL>
</AccessURL>
<Format>NetCDF</Format>
- <Acknowledgement>NASA, Dr. Berend Wilken</Acknowledgement>
+ <Acknowledgement></Acknowledgement>
</AccessInformation>
<ProviderName>CSA</ProviderName>
<ProcessingLevel>Calibrated</ProcessingLevel>
@@ -72,7 +71,7 @@
<Keyword>magnetotail</Keyword>
<Keyword>lobe</Keyword>
<Parameter>
- <Name>Electron Flux </Name>
+ <Name>diff flux</Name>
<ParameterKey>c4_rap_e</ParameterKey>
<Description>Cluster II Tango Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux at spin time resolution</Description>
<Ucd>phys.flux.density;phys.count;phys.electron</Ucd>
diff --git a/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml b/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml
index 8352ed6..ecfe5a0 100644
--- a/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml
@@ -4,26 +4,25 @@
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp</ResourceID>
<ResourceHeader>
- <ResourceName>Cluster II Tango Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ResourceName>
+ <ResourceName>protons</ResourceName>
<AlternateName>Cluster 4 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2015-10-16T16:51:46Z</ReleaseDate>
- <Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
- Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV
- for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. 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 RAPID:
- The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
- this information was obtained.</Description>
- <Acknowledgement>NASA, Dr. Berend Wilken, European Space Agency</Acknowledgement>
+ <Description></Description>
+ <Acknowledgement></Acknowledgement>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
+ <PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
<Role>TechnicalContact</Role>
</Contact>
<InformationURL>
<Name>NSSDC Master Catalog listing for Cluster II Tango Research with Adaptive Particle Imaging Detectors (RAPID)</Name>
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-06</URL>
<Description>This site provides information concerning the Cluster II Tango Research with Adaptive Particle Imaging Detectors Instrument.</Description>
- </InformationURL>
+ </InformationURL>
+ <Association>
+ <AssociationID>cluster4-rap-pp</AssociationID>
+ <AssociationType>PartOf</AssociationType>
+ <Note>prime parameters</Note>
+ </Association>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -72,7 +71,7 @@
<Keyword>magnetotail</Keyword>
<Keyword>lobe</Keyword>
<Parameter>
- <Name>Proton Flux </Name>
+ <Name>diff flux</Name>
<ParameterKey>c4_rap_p</ParameterKey>
<Description>Cluster II Tango Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux at spin time resolution</Description>
<Ucd>phys.flux.density;phys.count;phys.atmol.ionStage</Ucd>
--
libgit2 0.21.2