{
  "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/OAC/OACT",
      "ResourceHeader": {
        "ResourceName": "OACT (VSO notation)",
        "ReleaseDate": "2012-04-12T00:00:00Z",
        "Description": "The Catania Astrophysicsl Observatory (OAC)\r\nTelescope (OACT) used for solar observations has a\r\nHa Lyot-filter (bandwidth of 0.25 - 0.50 Angstrom, tunable filter \r\nrange +/- 16 Angstrom) and a 1360 x 1200 Astromed TE4 CCD array. \r\nIn patrol full-disk mode the camera can taken images every 60 s, \r\nwith a dynamical range of 16 bit.  It has an H-alpha Halle filter\r\nwith a camera for limb observations.  It has a 150 mm refractor \r\nwith a focal length of 230 cm.  A Cook refractor is used to make \r\ndaily drawings of sunspot-groups from visual observation.  See \r\nhttp://web.ct.astro.it/sun/instrument.htm.",
        "Contact": {
          "PersonID": "spase://SMWG/Person/Francesca.Zuccarelli",
          "Role": "GeneralContact"
        },
        "PriorID": "spase://vspo/instrument/171"
      },
      "InstrumentType": "Imager",
      "InvestigationName": "OACT (VSO notation) on OAC",
      "ObservatoryID": "spase://SMWG/Observatory/OAC"
    }
  }
}