cass-mag-jup.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://cdpp.irap.omp.eu/AMDA-NG/public/schemas/spase-amda-1_2_0.xsd">
<Version>2.2.6</Version>
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/Cassini/MAG/cass-mag-jup</ResourceID>
<ResourceHeader>
<ResourceName>flyby jupiter</ResourceName>
<AlternateName>high resolution MAG data during Jupiter flyby</AlternateName>
<ReleaseDate>2015-10-12T15:43:00</ReleaseDate>
<Description>High-resolution magnetic field data from the Cassini magnetometer during the Jupiter flyby in RTN coordinates obtained from NASA/PDS plasma node</Description>
<Contact>
<PersonID>spase://SMWG/Person/David.J.Southwood</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<InformationURL>
<URL>http://www.lesia.obspm.fr/</URL>
</InformationURL>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Open</AccessRights>
<AccessURL>
<Name>AMDA</Name>
<URL>amda.cdpp.eu</URL>
</AccessURL>
<Format>NetCDF</Format>
</AccessInformation>
<ProviderName>PDS</ProviderName>
<ProviderResourceName>CO-E_SW_J_S-MAG-3-RDR-FULL-RES-V1.0</ProviderResourceName>
<InstrumentID>spase://CDPP/Instrument/AMDA/Cassini/MAG</InstrumentID>
<MeasurementType>MagneticField</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2000-10-07T00:01:18Z</StartDate>
<StopDate>2001-05-10T15:25:41Z</StopDate>
</TimeSpan>
<Cadence_Min>PT0.031S</Cadence_Min>
<Cadence_Max>PT8S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Jupiter</ObservedRegion>
<ObservedRegion>Interstellar</ObservedRegion>
<ObservedRegion>Jupiter.Ganymede</ObservedRegion>
<ObservedRegion>Jupiter.Io</ObservedRegion>
<ObservedRegion>Jupiter.Callisto</ObservedRegion>
<ObservedRegion>Jupiter.Europa</ObservedRegion>
<Caveats>These data contain persistent noise signals at 0.2, 8, 16 Hz, and associated
harmonics. This noise was not observed during ground testing of the
instruments and is anticipated to be interference arising from the spacecraft.
Removal of these signals is at the user's discretion.</Caveats>
<Parameter>
<Name>b_rtn</Name>
<ParameterKey>cass_b_jup</ParameterKey>
<Description>Magnetic field vector components in RTN coordinates </Description>
<Ucd>phys.magField</Ucd>
<Units>nT</Units>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Structure>
<Size>3</Size>
<Element>
<Name>br</Name>
<Index>1</Index>
<ParameterKey>cass_b_jup(0)</ParameterKey>
</Element>
<Element>
<Name>bt</Name>
<Index>2</Index>
<ParameterKey>cass_b_jup(1)</ParameterKey>
</Element>
<Element>
<Name>bn</Name>
<Index>3</Index>
<ParameterKey>cass_b_jup(2)</ParameterKey>
</Element>
</Structure>
<Field>
<Qualifier>Vector</Qualifier>
<FieldQuantity>Magnetic</FieldQuantity>
</Field>
</Parameter>
<Parameter>
<Name>|b|</Name>
<ParameterKey>cass_bmag_jup</ParameterKey>
<Description>Magnetic field vector magnitude</Description>
<Ucd>phys.magField</Ucd>
<Units>nT</Units>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Field>
<Qualifier>Magnitude</Qualifier>
<FieldQuantity>Magnetic</FieldQuantity>
</Field>
</Parameter>
</NumericalData>
</Spase>