cass-rpws-neproxy.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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
<Version>2.3.1</Version>
<NumericalData>
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Cassini/RPWS/cass-rpws-neproxy</ResourceID>
<ResourceHeader>
<ResourceName>electron proxy</ResourceName>
<AlternateName>Langmuir Probe : electron proxy</AlternateName>
<ReleaseDate>2017-10-19T17:01:00</ReleaseDate>
<Description>Cassini RPWS Neproxy data contains all available RPWS Langmuir probe (LP) floating potentials and secondary products.
Cassini RPWS Langmuir Probe proxy electron density data are derived
using an empirical relation between the floating potential and CAPS
measured densities, for the entire mission. Spacecraft potential data
are also derived from LP floating potential.
</Description>
<Contact>
<PersonID>spase://SMWG/Person/William.S.Kurth</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<Contact>
<PersonID>spase://CNES/Person/J.Wahlund</PersonID>
<Role>DataProducer</Role>
</Contact>
<InformationURL>
<Name>PDS home page</Name>
<URL>https://pds-ppi.igpp.ucla.edu/data/CO-SS_S-RPWS-5-NEPROXY-V1.0/CATALOG/NEPROXYDS.CAT</URL>
</InformationURL>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CNES/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-SS_S-RPWS-5-NEPROXY-V1.0</ProviderResourceName>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Cassini/RPWS</InstrumentID>
<MeasurementType>ThermalPlasma</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2004-08-27T00:03:27Z</StartDate>
<StopDate>2015-12-31T22:28:25Z</StopDate>
</TimeSpan>
<Cadence>PT640S</Cadence>
</TemporalDescription>
<ObservedRegion>Saturn</ObservedRegion>
<Caveats>Occasional RPWS Langmuir probe voltage sweeps have interference in
individual sweep samples. These samples have been filtered away before
analysis and should not pose a problem for the delivered output
parameters. The Ufloat proxy method for this data set is applicable only
for densities below 5 cm^-3. To avoid uncertainty of the transition
region, data are limited to radial distance beyond 7 Rs from Saturn and
absolute magnetic latitude above 15 degrees. Also the data inside 10 Rt
from Titan are not included for the same reason. The proxy method uses
the photoelectron condition directly measured by the instrument and
therefore not available when LP is totally in shadow.</Caveats>
<Parameter>
<Name>floating potential</Name>
<ParameterKey>cass_neproxy_fpot</ParameterKey>
<Ucd>phys.potential;phys.elecField;instr.obsty</Ucd>
<Units>V</Units>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Support>
<SupportQuantity>Other</SupportQuantity>
</Support>
</Parameter>
<Parameter>
<Name>s/c potential</Name>
<ParameterKey>cass_neproxy_scpot</ParameterKey>
<Ucd>phys.potential;phys.elecField;instr.obsty</Ucd>
<Units>V</Units>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Support>
<SupportQuantity>Other</SupportQuantity>
</Support>
</Parameter>
<Parameter>
<Name>density e-</Name>
<ParameterKey>cass_neproxy_e</ParameterKey>
<Ucd>phys.density;phys.electron</Ucd>
<Units>cm-3</Units>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Particle>
<ParticleType>Electron</ParticleType>
<ParticleQuantity>NumberDensity</ParticleQuantity>
</Particle>
</Parameter>
</NumericalData>
</Spase>