{
  "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/BepiColombo/Mio/MGF",
      "ResourceHeader": {
        "ResourceName": "MGF",
        "AlternateName": "Mercury Fluxgate Magnetometer",
        "ReleaseDate": "2020-09-22T16:02:13Z",
        "Description": "The Fluxgate Magnetometer onboard Mio (MGF) measures the magnetic field to study various magnetospheric processes \n      (such as magnetic reconnection, field-aligned currents etc.) in Mercury’s magnetosphere, physics of bowshock and magnetosheath, \n      also magnetic field properties in the inner-heliosphere. It consists of two tir-axial fluxgate magnetometers and power supply units. \n      The magnetometer is able to observe the magnetic field with a vector rate of maximum 128 Hz. ",
        "Contact": [
          {
            "PersonID": "spase://SMWG/Person/Wolfgang.Baumjohann",
            "Role": "PrincipalInvestigator"
          },
          {
            "PersonID": "spase://SMWG/Person/Ayako.Matsuoka",
            "Role": "CoPI"
          }
        ],
        "InformationURL": [
          {
            "Name": "Mio Science Center",
            "URL": "https://miosc.isee.nagoya-u.ac.jp/about/satellite/mgf.php"
          },
          {
            "Name": "Baumjohann, W., Matsuoka, A., Narita, Y. et al. The BepiColombo–Mio Magnetometer en Route to Mercury. Space Sci Rev 216, 125 (2020).",
            "URL": "https://doi.org/10.1007/s11214-020-00754-y",
            "Description": "Reference paper"
          }
        ]
      },
      "InstrumentType": "Magnetometer",
      "InvestigationName": "Mercury Magnetometer on Mio",
      "ObservatoryID": "spase://CNES/Observatory/CDPP-AMDA/BepiColombo/Mio"
    }
  }
}