{
  "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_3_1.xsd",
    "Version": "2.3.1",
    "Instrument": {
      "ResourceID": "spase://SMWG/Instrument/Meudon/Heliograph",
      "ResourceHeader": {
        "ResourceName": "Meudon Heliograph",
        "ReleaseDate": "2020-07-01T13:22:00Z",
        "Description": "The Meudon Heliograph provides 3 images every 1.5 minute of the \nsolar disk in the H alpha line at 3 wavelengths: line core and \nat 0.5 Angstroms from it on each side. A Lyot filter with a \n0.5 Angstrom bandpass is used.  The objective is to detect and \nobserve solar eruptions at a high temporal cadence.",
        "Contact": {
          "PersonID": "spase://SMWG/Person/Jean-Marie.Malherbe",
          "Role": "GeneralContact"
        },
        "PriorID": [
          "spase://vspo/Instrument/172",
          "spase://SMWG/Instrument/OBSPM/OBSPM"
        ]
      },
      "InstrumentType": "Imager",
      "InvestigationName": "Meudon Heliograph",
      "OperatingSpan": {
        "StartDate": "1960-01-01T00:00:00.000Z"
      },
      "ObservatoryID": "spase://SMWG/Observatory/Meudon"
    }
  }
}