{
  "Spase": {
    "xmlns": "http://www.spase-group.org/data/schema",
    "xmlns:xsi": "http://www.w3.org/2001/XMLSchema-instance",
    "xsi:schemaLocation": "https://www.spase-group.org/data/schema  https://www.spase-group.org/data/schema/spase-2.7.1.xsd",
    "Version": "2.7.1",
    "MetadataRightsList": {
      "Rights": {
        "SchemeURI": "https://spdx.org/licenses/",
        "RightsIdentifierScheme": "SPDX",
        "RightsIdentifier": "CC0-1.0",
        "RightsURI": "https://spdx.org/licenses/CC0-1.0.html",
        "RightsName": "Creative Commons Zero v1.0 Universal",
        "Note": "CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions"
      }
    },
    "Instrument": {
      "ResourceID": "spase://NASA/Instrument/STEREO-A/SECCHI/Cor1",
      "NamingAuthority": "NASA",
      "ResourceType": "Instrument",
      "ResourceHeader": {
        "ResourceName": "STEREO-A SECCHI Cor1 Coronagraph",
        "ReleaseDate": "2026-02-02T13:11:23Z",
        "RevisionHistory": {
          "RevisionEvent": [
            {
              "ReleaseDate": "2023-10-28T00:08:46Z",
              "Note": "Only known prior ReleaseDate of the metadata"
            },
            {
              "ReleaseDate": "2023-11-02T00:08:46",
              "Note": "Changed the ResourceID Naming Authority from SMWG to NASA"
            },
            {
              "ReleaseDate": "2026-02-02T13:11:23Z",
              "Note": "Added MetadataRightsList. Added ResourceType and NamingAuthority. Updated to 2.7.1. Changed http to https in top-level schemaLocation attribute. ZCB"
            }
          ]
        },
        "Description": "The COR1 telescope is the inner coronagraph of the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) instrument suite aboard the twin Solar Terrestrial Relations Observatory (STEREO) spacecraft. Like all coronagraphs, COR1 is designed to measure the weak light from the solar corona in the presence of scattered light from the much brighter solar photosphere. It designed to observe the white light corona from \n1.4 to 4 R☉.\nhttps://stereo-ssc.nascom.nasa.gov/publications/CMAD/secchi/STEREO_SECCHI_COR1_CMAD_20211206.pdf",
        "Contact": [
          {
            "PersonID": "spase://SMWG/Person/Charles.N.Arge",
            "Role": [
              "ProgramScientist",
              "PrincipalInvestigator"
            ]
          },
          {
            "PersonID": "spase://SMWG/Person/O.Chris.St.Cyr",
            "Role": "CoInvestigator"
          },
          {
            "PersonID": "spase://SMWG/Person/William.T.Thompson",
            "Role": "CoInvestigator"
          },
          {
            "PersonID": "spase://SMWG/Person/Nat.Gopalswamy",
            "Role": "CoInvestigator"
          },
          {
            "PersonID": "spase://SMWG/Person/Barbara.J.Thompson",
            "Role": "CoInvestigator"
          },
          {
            "PersonID": "spase://SMWG/Person/Hong.Xie",
            "Role": "CoInvestigator"
          }
        ],
        "PriorID": "spase://SMWG/Instrument/STEREO-A/SECCHI/Cor1"
      },
      "InstrumentType": "Coronograph",
      "InvestigationName": "SECCHI",
      "ObservatoryID": "spase://SMWG/Observatory/STEREO-A"
    }
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}