{
  "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_0_0.xsd",
    "Version": "2.0.0",
    "Instrument": {
      "ResourceID": "spase://SMWG/Instrument/Ulysses/SCE",
      "ResourceHeader": {
        "ResourceName": "Coronal Sounding (radio science) (SCE)",
        "AlternateName": "SCE",
        "ReleaseDate": "2019-05-05T12:34:56Z",
        "Description": "The objective of this radio science investigation is to determine the density, turbulence spectrum, and velocity of the coronal plasma in the acceleration regime of the solar wind. Dual-frequency ranging and Doppler data are recorded during phases of the ULYSSES superior conjunction using the spacecraft transmitters and the NASA DSN.",
        "Contact": {
          "PersonID": "spase://SMWG/Person/Michael.K.Bird",
          "Role": "PrincipalInvestigator"
        },
        "InformationURL": {
          "Name": "NSSDC's Master Catalog",
          "URL": "https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=1990-090B&ex=10",
          "Description": "Information about the Coronal Sounding (radio science) (SCE) experiment on the Ulysses mission."
        }
      },
      "InstrumentType": "Sounder",
      "InvestigationName": "Coronal Sounding (radio science) (SCE) on Ulysses",
      "ObservatoryID": "spase://SMWG/Observatory/Ulysses"
    }
  }
}