clust4-rap-psp.xml 5.47 KB
<?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://cdpp1.cesr.fr/AMDA-NG/public/schemas/spase-amda-1_2_0.xsd">
    <Version>2.2.6</Version>
    <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>
            <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>
            <Contact>
                <PersonID>spase://SMWG/Person/Elena.Budnik</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>
            <Association>
                <AssociationID>spase://SMWG/Observatory/Cluster-Tango</AssociationID>
                <AssociationType>ObservedBy</AssociationType>
            </Association>
         </ResourceHeader>
        <AccessInformation>
            <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
            <Availability>Online</Availability>
            <AccessRights>Open</AccessRights>
            <AccessURL>
                <Name>AMDA at CDPP</Name>
                <URL>http://amda.cdpp.eu</URL>                
            </AccessURL>
            <Format>NetCDF</Format>
            <Acknowledgement>NASA, Dr. Berend Wilken</Acknowledgement>
        </AccessInformation>
        <ProviderName>CSA</ProviderName>
        <ProcessingLevel>Calibrated</ProcessingLevel>
        <ProviderResourceName>Cluster II Tango Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ProviderResourceName>
        <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
        <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Tango/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>Proton 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>
            <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>