{
  "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/Ground/MaunaLoaSO/ACOS",
      "ResourceHeader": {
        "ResourceName": "MLSO_ACOS",
        "ReleaseDate": "2015-10-23T00:00:00Z",
        "Description": "ACOS is the Advanced Coronal Observation System at\nMauna Loa Solar Observatory.  It is a suite of instruments designed to \nobserve the solar atmosphere, including the Chromospheric Helium Imaging \nPhotometer (CHIP, 1083.0nm), H-alpha prominence and solar disk monitor \n(PICS, 656.3nm), and the Mk4 K-coronameter, which observes the white \nlight K-corona from 1.12-2.79 solar radii (700-950 nm).",
        "Contact": {
          "PersonID": "spase://SMWG/Person/Thomas.E.Holzer",
          "Role": "GeneralContact"
        },
        "PriorID": "spase://SMWG/Instrument/MaunaLoaSO/ACOS"
      },
      "InstrumentType": "Imager",
      "InvestigationName": "ACOS at MLSO",
      "ObservatoryID": "spase://SMWG/Observatory/Ground/MaunaLoaSO"
    }
  }
}