{
  "Spase": {
    "xmlns": "http://www.spase-group.org/data/schema",
    "xmlns:xsi": "http://www.w3.org/2001/XMLSchema-instance",
    "xsi:schemaLocation": "http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_4_0.xsd",
    "Version": "2.4.0",
    "Observatory": {
      "ResourceID": "spase://CNES/Observatory/CDPP-Archive/GEOS-1",
      "ResourceHeader": {
        "ResourceName": "GEOS-1",
        "ReleaseDate": "2022-06-09T16:56:58Z",
        "Description": "European GEOS Mission: the Satellites\n\nGeos was designed for geostationary orbit to study the particles, fields and plasmas of the Earth's magnetosphere using seven instruments provided by ten European laboratories. Because of its unique orbit and the sophistication of its payload, Geos was selected as the reference spacecraft for the worldwide 'International Magnetospheric Study'. Unfortunately, Geos-1 was left in a low transfer orbit following launch on 20 April 1977 because of a problem with its US Delta launcher. As a result, the Qualification Model was launched as Geos-2 on 14 July 1978 with an identical payload and successfully reached the planned orbit. In spite of its orbit, Geos-1 made a significant contribution to IMS, and its mission formally ended on 23 June. Geos-2 was highly successful, creating a huge database for magnetospheric studies and plasma research in general.\n\nScience objectives of the European GEOS Mission\n   - to advance our knowledge of the dynamics of the magnetosphere, in particular to study the response of the near-Earth environnment to varying conditions in interplanetary space (nominal objective reached with GEOS-2),\n    -to study of the dayside sector of the magnetosphere : the plasma bulge and the plasmapause have been investigated in detail.(GEOS-1).\n\nGEOS comprises the following seven experiments:\n\nS-300\nAC-magnetic fields up to 30 kHz\nDC/AC electric fields and plasma resonances up to 80 kHz\nMutual and self-impedance\nCRPE, Issy-les-Moulineuax, France\nSpace Science Dept., ESA, ESTAC, Holland\nDanish Space Research Institute, Lyngby, Denmark\nCRPE, Orléans, France\n\nS-302\nThermal plasma up to 500 eV\nMullard Space Science Lab., Dorking, UK\n\nS-303\nComposition (1-140 amu) and energy spectra of ions up to 16 keV\nUniversity of Bern, Switzerland\nMax-Planck-Institut, Garching, Germany\n\nS-310\nPitch-angle distribution of electrons and protons (0.2-20 keV) energy range\nKiruna Geophysical Observatory, Kiruna, Sweden\n\nS-321\nPitch-angle distribution for electrons (20-300 keV) and protons (20 keV-3MeV)\nMax-Planck-Institut, Lindau, Germany\n\nS-329\nDC electric field\nMax-Planck-Institut, Garching, Germany\n\nS-331\nDC and ULF magnetif field\nCNR, Frascaty, Italy\nNASA/GSFC, Greenbelt, Maryland",
        "Contact": {
          "PersonID": "spase://CNES/Person/CDPP-Archive/Karl.Knott",
          "Role": "ProjectScientist"
        }
      },
      "Location": {
        "ObservatoryRegion": "Earth.Magnetosphere.Main"
      },
      "OperatingSpan": {
        "StartDate": "1977-04-20T00:00:00Z",
        "StopDate": "1978-06-23T00:00:00Z"
      }
    }
  }
}