{
  "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/PSPT",
      "ResourceHeader": {
        "ResourceName": "MLSO_PSPT",
        "ReleaseDate": "2015-10-23T00:00:00Z",
        "Description": "The Precision Solar Photometric Telescope (PSPT) \nis the centerpiece of the National Science Foundation Radiative \nInputs from Sun to Earth (RISE) program whose aim is to measure \nand understand variability in the solar radiative output. The PSPT \nproduces seeing-limited full-disk (2048x2048 with 1.05\"/pixel) \nimages in the blue continuum (409.4nm, FWHM 0.3nm), red continuum \n(607.1nm, FWHM 0.5nm), CaII K (393.4nm, FWHM 0.3nm), CaII K Narrow \nBand Wing (NBW) (393.6nm, FWHM 0.1nm), and CaII K Narrow Band Core \n(NBC) (393.4nm, FWHM 0.1nm), with an unprecedented 0.1% pixel-to-\npixel relative photometric precision.",
        "Contact": {
          "PersonID": "spase://SMWG/Person/Thomas.E.Holzer",
          "Role": "GeneralContact"
        },
        "PriorID": "spase://SMWG/Instrument/MaunaLoaSO/PSPT"
      },
      "InstrumentType": [
        "MultispectralImager",
        "Photometer"
      ],
      "InvestigationName": "PSPT at MLSO",
      "ObservatoryID": "spase://SMWG/Observatory/Ground/MaunaLoaSO"
    }
  }
}