{
  "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",
    "Instrument": {
      "ResourceID": "spase://CNES/Instrument/CDPP-AMDA/DSCOVR/FC",
      "ResourceHeader": {
        "ResourceName": "Faraday Cup",
        "ReleaseDate": "2017-10-16T15:10:29Z",
        "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.",
        "Acknowledgement": "NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.",
        "Contact": {
          "PersonID": "spase://CNES/Person/CDPP-AMDA/Justin.Kasper",
          "Role": "PrincipalInvestigator"
        },
        "InformationURL": {
          "Name": "NOAA Satellite and Information Service DSCOVR PLASMA-MAGNETOMETER",
          "URL": "https://en.wikipedia.org/wiki/Deep_Space_Climate_Observatory",
          "Description": "As general description of the DSCOVR Faraday cup."
        }
      },
      "InstrumentType": "FaradayCup",
      "InvestigationName": "PlasmaProbe",
      "ObservatoryID": "spase://CNES/Observatory/CDPP-AMDA/DSCOVR"
    }
  }
}