{
  "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_1_0.xsd",
    "Version": "2.1.0",
    "Instrument": {
      "ResourceID": "spase://SMWG/Instrument/Wind/SMS",
      "ResourceHeader": {
        "ResourceName": "Solar Wind and Suprathermal Ion Composition Experiment (SMS)",
        "ReleaseDate": "2019-05-05T12:34:56Z",
        "Description": "The Wind SMS instrument suite is composed of three separate instruments.\n\n          * The SupraThermal Ion Composition Spectrometer (STICS) determines the mass, mass per charge, and energy for ions in the energy range of 6-230 keV/e.\n          * The high resolution mass spectrometer (MASS) determines elemental and isotopic abundances from 0.5 to 12 keV/e.\n          * Finally, the Solar Wind Ion Composition Spectrometer (SWICS) determines mass, charge, and energy for ions in the energy range of 0.5 to 30 keV/e. The SWICS \"stop\" MCP experienced a failure resulting in reduced capabilities for this instrument.",
        "Contact": {
          "PersonID": "spase://SMWG/Person/George.Gloeckler",
          "Role": "PrincipalInvestigator"
        },
        "InformationURL": {
          "Name": "Wind spacecraft SMS Documentation",
          "URL": "https://link.springer.com/article/10.1007/BF00751327",
          "Description": "The Space Science Reviews paper describing the Wind SMS instrument suite."
        }
      },
      "InstrumentType": "EnergeticParticleInstrument",
      "InvestigationName": "Solar Wind and Suprathermal Ion Composition Experiment (SMS)",
      "ObservatoryID": "spase://SMWG/Observatory/Wind"
    }
  }
}