{
  "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_2_2.xsd",
    "Version": "2.2.2",
    "Instrument": {
      "ResourceID": "spase://SMWG/Instrument/OBSPM/OBSPM",
      "ResourceHeader": {
        "ResourceName": "OBSPM Heliograph",
        "ReleaseDate": "2012-04-24T00:00:00Z",
        "Description": "The OBSPM (OBservatoire Solaire de Paris a \r\nMeudon) heliograph provides 3 images every 1.5 minute of the \r\nsolar disk in the H alpha line at 3 wavelengths: line core and \r\nat 0.5 Angstroms from it on each side. A Lyot filter with a \r\n0.5 Angstrom bandpass is used.  The objective is to detect and \r\nobserve solar eruptions at a high temporal cadence.",
        "Contact": {
          "PersonID": "spase://SMWG/Person/Jean-Marie.Malherbe",
          "Role": "GeneralContact"
        },
        "PriorID": "spase://vspo/Instrument/172"
      },
      "InstrumentType": "Imager",
      "InvestigationName": "OBSPM Heliograph",
      "ObservatoryID": "spase://SMWG/Observatory/OBSPM"
    }
  }
}