{
  "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/Rosetta/MAG",
      "ResourceHeader": {
        "ResourceName": "MAG",
        "AlternateName": "Fluxgate Magnetometer",
        "ReleaseDate": "2017-01-01T21:10:13Z",
        "Description": "The fluxgate magnetometer experiment onboard the ROSETTA spacecraft aims to measure\nthe magnetic field in the interaction region of the solar wind plasma with comet 67P/Churyumov-\nGerasimenko. It consists of a system of two ultra light (about 28 g each ) triaxial fluxgate magnetometer\nsensors, mounted on the 1.5 m long spacecraft boom. The measurement range of each sensor is\n±16384 nT with quantization steps of 31 pT. The magnetometer sensors are operated with a time\nresolution of up to 0.05 s, corresponding to a bandwidth of 0–10 Hz. This performance of the RPC-\nMAG sensors allows detailed analyses of magnetic field variations in the cometary environment. RPC-\nMAG furthermore is designed to study possible remnant magnetic fields of the nucleus, measurements\nwhich will be done in close cooperation with the ROSETTA lander magnetometer experiment ROMAP.\n",
        "Contact": {
          "PersonID": "spase://SMWG/Person/Karl-Heinz.Glassmeier",
          "Role": "PrincipalInvestigator"
        }
      },
      "InstrumentType": "Magnetometer",
      "InvestigationName": "Fluxgate Magnetometer",
      "ObservatoryID": "spase://CNES/Observatory/CDPP-AMDA/Rosetta"
    }
  }
}