clust2-rap-psp.xml
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<?xml version="1.0" encoding="UTF-8"?>
<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2.4.1.xsd">
<Version>2.4.1</Version>
<NumericalData>
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp</ResourceID>
<ResourceHeader>
<ResourceName>prime parameters : protons</ResourceName>
<AlternateName>Cluster 2 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2012-03-06T19:01:43Z</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>
<Contact>
<PersonID>spase://SMWG/Person/Peter.W.Daly</PersonID>
<Role>TechnicalContact</Role>
</Contact>
<InformationURL>
<Name>NSSDC Master Catalog listing for Cluster II Salsa 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 Salsa Research with Adaptive Particle Imaging Detectors Instrument.</Description>
</InformationURL>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Restricted</AccessRights>
<AccessURL>
<Name>CDPP/AMDA HAPI Server</Name>
<URL>http://amda.irap.omp.eu/service/hapi</URL>
<Style>HAPI</Style>
<Description>Web Service to this product using the HAPI interface.</Description>
</AccessURL>
<Format>CSV</Format>
<Acknowledgement>Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.</Acknowledgement>
</AccessInformation>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Restricted</AccessRights>
<AccessURL>
<Name>CDPP/AMDA Web application</Name>
<URL>http://amda.cdpp.eu</URL>
<Description>Access to Data via CDPP/AMDA Web application.</Description>
</AccessURL>
<Format>CSV</Format>
<Format>VOTable</Format>
<Format>CDF</Format>
<Format>PNG</Format>
<Acknowledgement>Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.</Acknowledgement>
</AccessInformation>
<ProcessingLevel>Calibrated</ProcessingLevel>
<ProviderName>CSA</ProviderName>
<ProviderResourceName>Cluster II Salsa Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ProviderResourceName>
<ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Cluster2/RAPID</InstrumentID>
<MeasurementType>EnergeticParticles</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2001-01-01T00:00:03Z</StartDate>
<StopDate>2006-12-31T23:59:58Z</StopDate>
</TimeSpan>
<Cadence>PT4S</Cadence>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosheath</ObservedRegion>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
<ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
<ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
<ObservedRegion>Earth.Magnetosphere.RadiationBelt</ObservedRegion>
<ObservedRegion>Earth.NearSurface.AuroralRegion</ObservedRegion>
<ObservedRegion>Earth.NearSurface.Ionosphere</ObservedRegion>
<ObservedRegion>Earth.NearSurface.Plasmasphere</ObservedRegion>
<ObservedRegion>Earth.NearSurface.PolarCap</ObservedRegion>
<ObservedRegion>Heliosphere.NearEarth</ObservedRegion>
<Keyword>4 second</Keyword>
<Keyword>magnetosphere</Keyword>
<Keyword>auroral region</Keyword>
<Keyword>polar cap</Keyword>
<Keyword>cusp</Keyword>
<Keyword>bow shock</Keyword>
<Keyword>solar wind</Keyword>
<Keyword>magnetosheath</Keyword>
<Keyword>Cluster</Keyword>
<Keyword>magnetotail</Keyword>
<Keyword>lobe</Keyword>
<Parameter>
<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>
<Cadence>PT4S</Cadence>
<Units>1/cm^2_sr_s_keV</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<FillValue>-1.0000e+31</FillValue>
<Particle>
<ParticleType>Proton</ParticleType>
<Qualifier>Scalar</Qualifier>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
</NumericalData>
</Spase>