<?xml version="1.0" encoding="UTF-8"?>

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  <Version>2.4.1</Version>

  <Instrument>

    <ResourceID>spase://CNES/Instrument/CDPP-AMDA/DSCOVR/FC</ResourceID>

    <ResourceHeader>
      <ResourceName>Faraday Cup</ResourceName>          
      <ReleaseDate>2017-10-16T15:10:29Z</ReleaseDate>

      <Description>The PlasMag Faraday Cup provides very high time resolution (0.5 second) solar wind bulk properties in three dimensions, which coupled with magnetic field data (20 vectors/second), allows the investigation of solar wind waves and turbulence at unprecedented time resolution. This, in turn, allows new insights into the basic plasma properties: the process of turbulent cascade and the rate of reconnection. Both topics are critical in understanding the nature of coronal heating.</Description>

      <Acknowledgement>NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.</Acknowledgement>
      <Contact>      

        <PersonID>spase://CNES/Person/CDPP-AMDA/Justin.Kasper</PersonID>

        <!--<Role>InstrumentLead</Role>-->
        <Role>PrincipalInvestigator</Role>
      </Contact>     
      <InformationURL>

        <Name>NOAA Satellite and Information Service DSCOVR PLASMA-MAGNETOMETER</Name>
        <URL>https://en.wikipedia.org/wiki/Deep_Space_Climate_Observatory</URL>
        <Description>As general description of the DSCOVR Faraday cup.</Description>

      </InformationURL>
    </ResourceHeader>
    <InstrumentType>FaradayCup</InstrumentType>

    <InvestigationName>PlasmaProbe</InvestigationName>

    <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/DSCOVR</ObservatoryID>

  </Instrument>
</Spase>