{
  "Spase": {
    "xmlns": "http://www.spase-group.org/data/schema",
    "xmlns:xsi": "http://www.w3.org/2001/XMLSchema-instance",
    "xsi:schemaLocation": "http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_3_0.xsd",
    "Version": "2.3.0",
    "NumericalData": {
      "ResourceID": "spase://GBO/NumericalData/NeutronMonitor/FtSmith_Peawanuck_Nain_Inuvik/PT1H",
      "ResourceHeader": {
        "ResourceName": "Cosmic Ray Intensities Hourly  averages from Neutron Monitors at \n         Fort Smith, Peawanuck, Nain, and Inuvik\n       ",
        "ReleaseDate": "2018-05-29T14:44:18Z",
        "Description": "Hourly averages of relativistic cssmic ray intensities from Bartol Research Institute Neutron Monitors at Fort Smith, Peawanuck, Nain, and Inuvik\n       ",
        "Acknowledgement": "Please acknowledge the Principal Investigator  (Dr. John Bieber)",
        "Contact": [
          {
            "PersonID": "spase://SMWG/Person/John.Bieber",
            "Role": [
              "PrincipalInvestigator",
              "DataProducer"
            ]
          },
          {
            "PersonID": "spase://SMWG/Person/K.Roger.Pyle",
            "Role": [
              "DeputyPI",
              "DataProducer"
            ]
          },
          {
            "PersonID": "spase://SMWG/Person/Paul.A.Evenson",
            "Role": "DeputyPI"
          }
        ],
        "InformationURL": {
          "Name": "\n           General ReadMe file for data for the University of Delaware \n           Bartol Research Institute Neutron Monitor Program\n         ",
          "URL": "http://neutronm.bartol.udel.edu/",
          "Description": "\n           This site provides basic information about the Bartol Neutron Monitor Network as well as links to 1) discussions of recent events, 2) an explanation of how neutron monitors work, 3) instructions for downloading of data, 4) listings of personnel and points of contact, and 5) other neutron monitor sites. \n         "
        },
        "PriorID": "spase://VEPO/NumericalData/NeutronMonitor/FtSmith_Peawanuck_Nain_Inuvik/PT1H"
      },
      "AccessInformation": {
        "RepositoryID": "spase://SMWG/Repository/Bartol",
        "Availability": "Online",
        "AccessRights": "Open",
        "AccessURL": {
          "Name": "\n           Plain Text Hourly Data for Download from Bartol-operated Neutron Monitors\n         ",
          "URL": "http://neutronm.bartol.udel.edu/~pyle/bri_table.html",
          "Description": "\n\t   Home page for yearly files of hourly average data from all Bartol Neutron Monitors containing\n           pressure corrected intensities, uncorrected intensities, and measured atmospheric pressure\n           Includes conditions for use of data and descriptions of processing level\n\t   Data are grouped into two sets of files.\n           Set A contains data from neutron monitors at\n             McMurdo: June 24, 1960 - Present\n             Newark: July 1, 1964 - Present\n             South Pole: March 1, 1964 - November 27, 2005\n             Thule: August 13, 1957 - Present\n           Set B contains data from neutron monitors at \n             Fort Smith: October 4, 2000 - Present\n             Peawanuck: September 14, 2000 - February 1, 2009\n             Nain:  November 10, 2000 - Present\n             Inuvik: January 1, 2000 - Present\n           Direct links to yearly files are provided for viewing of one or a few years.  Also provided is\n           a link to the ftp server where the files reside for direct downloading of from one to the total \n           set of yearly files.  On the ftp server, the file naming convention for set A is BRIYYYY.txt.  The\n           file naming convention for set B on the ftp site is BRIYYYYB.txt\n           Additional documentation concerning the specific neutron monitors included in each file is \n           provided at the top of each yearly file.\n           Cutoff rigidities (minimum rigidities) given are for epoch 1965 as calculated by \n           M.A. Shea and  D.F. Smart, Vertical Cutoff Rigidities for cosmic ray stations since 1955, \n           Proc. 27th ICRC, Hamburg, Germany, pp. 4063-4067, 2001.  \n           (available on-line at http://articles.adsabs.harvard.edu/full/2001ICRC...10.4063S) \t \n       \t "
        },
        "Format": "Text",
        "Acknowledgement": "John Bieber, Bartol Research Institute, University of Delaware"
      },
      "InstrumentID": [
        "spase://SMWG/Instrument/NeutronMonitor/Bartol/FortSmith",
        "spase://SMWG/Instrument/NeutronMonitor/Bartol/Peawanuck",
        "spase://SMWG/Instrument/NeutronMonitor/Bartol/Nain",
        "spase://SMWG/Instrument/NeutronMonitor/Bartol/Inuvik"
      ],
      "MeasurementType": "EnergeticParticles",
      "TemporalDescription": {
        "TimeSpan": {
          "StartDate": "2000-01-01T00:00:00.000",
          "RelativeStopDate": "P3M"
        },
        "Cadence": "PT1H"
      },
      "ObservedRegion": "Heliosphere.NearEarth",
      "Parameter": [
        {
          "Name": "Start Time",
          "Cadence": "PT1H",
          "Structure": {
            "Size": "5",
            "Description": "\n           Columns 1-5 containing Nominal Start Time for the average \n           given as \n           YYYY MM DD HH MM2 \n           where \n           YYYY       = Gregorian Year AD\n           MM         = month of year (01-12)\n           DD         = Day of Month (01-31)\n           HH         = Hour of Day (00-23)\n           MM2         = Minute of Hour (00-60)\n         ",
            "Element": [
              {
                "Name": "4 digit year",
                "Index": "1",
                "ValidMin": "1960",
                "ValidMax": "2010"
              },
              {
                "Name": "month of year",
                "Index": "2",
                "ValidMin": "01",
                "ValidMax": "12"
              },
              {
                "Name": "Day of month",
                "Index": "3",
                "ValidMin": "01",
                "ValidMax": "31"
              },
              {
                "Name": "Hour of day",
                "Index": "4",
                "ValidMin": "00",
                "ValidMax": "23"
              },
              {
                "Name": "Minute of hour",
                "Index": "5",
                "ValidMin": "00",
                "ValidMax": "00"
              }
            ]
          },
          "Support": {
            "SupportQuantity": "Temporal"
          }
        },
        {
          "Name": "Column 6: Fort Smith corrected intensities",
          "Description": "\n         Fort Smith neutron monitor ground-level intensities of\n         cosmic-ray produced secondary neutrons, corrected for \n         effects of atmospheric pressure and, if necessary,\n         changes in normalization (see documentation in file header).\n         Intensity is given as counts/100 per hour.\n         Rigidity range (GV) refers to rigidity of primary cosmic rays\n         capable of producing an observable neutron shower.\n       ",
          "Particle": {
            "ParticleType": "Neutron",
            "ParticleQuantity": "CountRate",
            "EnergyRange": {
              "Low": "0.27",
              "High": "1.0e15",
              "Units": "GV"
            }
          }
        },
        {
          "Name": "Column 7: Fort Smith uncorrected intensities",
          "Description": "\n         Fort Smith neutron monitor ground-level cosmic ray intensities\n         as measured, prior to application of corrections.\n         Intensity is given as counts/100 per hour.    \n       ",
          "Particle": {
            "ParticleType": "Neutron",
            "ParticleQuantity": "CountRate",
            "EnergyRange": {
              "Low": "0.27",
              "High": "1.0e15",
              "Units": "GV"
            }
          }
        },
        {
          "Name": "Column 8: Fort Smith barometric pressure",
          "Units": "mm of Hg",
          "Support": {
            "SupportQuantity": "Other"
          }
        },
        {
          "Name": "Column 9: Peawanuck corrected intensities",
          "Description": "\n         Peawanuck neutron monitor ground-level intensities of\n         cosmic-ray produced secondary neutrons, corrected for \n         effects of atmospheric pressure and, if necessary,\n         changes in normalization (see documentation in file header).\n         Intensity is given as counts/100 per hour.\n         Rigidity range (GV) refers to rigidity of primary cosmic rays\n         capable of producing an observable neutron shower.\n       ",
          "Particle": {
            "ParticleType": "Neutron",
            "ParticleQuantity": "CountRate",
            "EnergyRange": {
              "Low": "0.33",
              "High": "1.0e15",
              "Units": "GV"
            }
          }
        },
        {
          "Name": "Column 10: Peawanuck uncorrected intensities",
          "Description": "\n         Peawanuck neutron monitor ground-level cosmic ray intensities\n         as measured, prior to application of corrections.\n         Intensity is given as counts/100 per hour.    \n       ",
          "Particle": {
            "ParticleType": "Neutron",
            "ParticleQuantity": "CountRate",
            "EnergyRange": {
              "Low": "0.33",
              "High": "1.0e15",
              "Units": "GV"
            }
          }
        },
        {
          "Name": "Column 11: Peawanuck barometric pressure",
          "Units": "mm of Hg",
          "Support": {
            "SupportQuantity": "Other"
          }
        },
        {
          "Name": "Column 12: Nain corrected intensities",
          "Description": "\n         Nain neutron monitor ground-level intensities of\n         cosmic-ray produced secondary neutrons, corrected for \n         effects of atmospheric pressure and, if necessary,\n         changes in normalization (see documentation in file header).\n         Intensity is given as counts/100 per hour.\n         Rigidity range (GV) refers to rigidity of primary cosmic rays\n         capable of producing an observable neutron shower.\n       ",
          "Particle": {
            "ParticleType": "Neutron",
            "ParticleQuantity": "CountRate",
            "EnergyRange": {
              "Low": "0.30",
              "High": "1.0e15",
              "Units": "GV"
            }
          }
        },
        {
          "Name": "Column 13: Nain uncorrected intensities",
          "Description": "\n         Nain neutron monitor ground-level cosmic ray intensities\n         as measured, prior to application of corrections.\n         Intensity is given as counts/100 per hour.    \n       ",
          "Particle": {
            "ParticleType": "Neutron",
            "ParticleQuantity": "CountRate",
            "EnergyRange": {
              "Low": "0.30",
              "High": "1.0e15",
              "Units": "GV"
            }
          }
        },
        {
          "Name": "Column 14: Nain barometric pressure",
          "Units": "mm of Hg",
          "Support": {
            "SupportQuantity": "Other"
          }
        },
        {
          "Name": "Column 15: Inuvik corrected intensities",
          "Description": "\n         Inuvik neutron monitor ground-level intensities of\n         cosmic-ray produced secondary neutrons, corrected for \n         effects of atmospheric pressure and, if necessary,\n         changes in normalization (see documentation in file header).\n         Intensity is given as counts/100 per hour.\n         Rigidity range (GV) refers to rigidity of primary cosmic rays\n         capable of producing an observable neutron shower.\n       ",
          "Particle": {
            "ParticleType": "Neutron",
            "ParticleQuantity": "CountRate",
            "EnergyRange": {
              "Low": "0.15",
              "High": "1.0e15",
              "Units": "GV"
            }
          }
        },
        {
          "Name": "Column 16: Inuvik uncorrected intensities",
          "Description": "\n         Inuvik neutron monitor ground-level cosmic ray intensities\n         as measured, prior to application of corrections.\n         Intensity is given as counts/100 per hour.    \n       ",
          "Particle": {
            "ParticleType": "Neutron",
            "ParticleQuantity": "CountRate",
            "EnergyRange": {
              "Low": "0.15",
              "High": "1.0e15",
              "Units": "GV"
            }
          }
        },
        {
          "Name": "Column 17: Inuvik barometric pressure",
          "Units": "mm of Hg",
          "Support": {
            "SupportQuantity": "Other"
          }
        }
      ]
    }
  }
}