clust4-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/Cluster4/RAPID/clust4-rap-psp</ResourceID>
<ResourceHeader>
<ResourceName>protons</ResourceName>
<AlternateName>Cluster 4 Prime Parameter RAPID Data</AlternateName>
<ReleaseDate>2012-03-06T19:40:38Z</ReleaseDate>
<Description>Prime Parameters RAPID Protons Data</Description>
<Contact>
<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>
<Association>
<AssociationID>cluster4-rap-pp</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>prime parameters</Note>
</Association>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Restricted</AccessRights>
<AccessURL>
<Name>CDPP/AMDA HAPI Server</Name>
<URL>https://amda.irap.omp.eu/service/hapi</URL>
<Style>HAPI</Style>
<ProductKey>clust4-rap-psp</ProductKey>
<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 https://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>https://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 https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.</Acknowledgement>
</AccessInformation>
<ProcessingLevel>Calibrated</ProcessingLevel>
<ProviderName>CSA</ProviderName>
<ProviderResourceName>Cluster II Tango Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ProviderResourceName>
<ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Cluster4/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>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;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>