<?xml version="1.0" encoding="UTF-8"?>
<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" 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>
  <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>