{
  "id": "UY_M0_KET",
  "url": "http://hpde.io/VEPO/NumericalData/Ulysses/COSPIN/KET/RATES/PT10M",
  "data-file": "./data/spase_hpde_io/info/UY_M0_KET.json",
  "data": {
    "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_2_2.xsd'",
      "Version": "2.2.2",
      "NumericalData": {
        "ResourceID": "spase://VEPO/NumericalData/Ulysses/COSPIN/KET/RATES/PT10M",
        "ResourceHeader": {
          "ResourceName": "Ulysses COSPIN/KET Proton, Helium and Electron 10-Minute Average Rates Data",
          "AlternateName": "COSPIN-KET-RAT-10M",
          "ReleaseDate": "2009-06-01T00:00:00Z",
          "Description": "This data set contains 10-Minute averages of:\n\t                (a) spin-integrated count rates of protons (2.7-5.4, 5.4-23.1, 34.1-125.0, 125.0-320.0, 320.0-2100 and >2100.0 MeV),\n\t\t\t\t\t    alpha particles (6.0-20.4, 34.2-125.0, 125.0-320.0, 320.0-2100.0 and >2100.0 MeV/n) and\n\t\t\t\t\t\telectrons (2.5-7.0, 7.0-170.0 and >170.0 MeV).\n\t\t\t\t\t(b)\t8-sectored count rates of protons (5.4-23.1 MeV) and electrons (2.5-7.0 MeV);\n\t\t\t\t\t(c)\tcount rates of D10, D20, C10, C20 and A01 single detector sensors.  The parameter keys in the parameter-level segments below are specifically relevant to the UFA-accessible versions of the data.",
          "Acknowledgement": "Please acknowlegde the COSPIN PI (R.B. McKibben), the KET Co-PI (B. Heber) and the UDS and/or NSSDC",
          "Contact": [
            {
              "PersonID": "spase://SMWG/Person/R.Bruce.McKibben",
              "Role": "PrincipalInvestigator"
            },
            {
              "PersonID": "spase://SMWG/Person/Bernd.Heber",
              "Role": "CoInvestigator"
            },
            {
              "PersonID": "spase://SMWG/Person/Cecil.Tranquille",
              "Role": "ArchiveSpecialist"
            }
          ],
          "InformationURL": {
            "Name": "README file for COSPIN/KET data files",
            "URL": "http://ufa.esac.esa.int/ufa/#instruments",
            "Description": "\n           The README file at the Ulysses Final Archive (UFA) describes the\n\t\t   format of the ASCII data files containing 10-minute average proton,\n\t\t   helium and electron count rates and detector count rates for the COSPIN Kiel\n\t\t   Electron Telescope (KET), and caveats for their use.\n         "
          }
        },
        "AccessInformation": [
          {
            "RepositoryID": "spase://SMWG/Repository/ESA/ESAC/UlyssesFinalArchive",
            "Availability": "Online",
            "AccessRights": "Open",
            "AccessURL": {
              "Name": "Ulysses Final Archive",
              "URL": "http://ufa.esac.esa.int/ufa/#data",
              "Description": "\n\t\t   Parent directory containing compressed Ulysses COSPIN/KET 10-minute average rates\n\t\t   data organised in daily ASCII files ucosketaYYDOY.dat (YY and DOY are the two digit\n\t\t   year and the day of year, respectively) grouped together into yearly files\n\t\t   (cosketYY.zip, where YY is the two digit year).\n         "
            },
            "Format": "Text",
            "Encoding": "ZIP",
            "Acknowledgement": "B. Heber, CAU Kiel"
          },
          {
            "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF",
            "Availability": "Online",
            "AccessRights": "Open",
            "AccessURL": {
              "Name": "FTP access to CDFs at SPDF",
              "URL": "ftp://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin_cdaweb/ket/",
              "Description": "via ftp in CDF from SPDF."
            },
            "Format": "CDF",
            "Acknowledgement": "Space Physics Data Facility at NASA/GSFC"
          },
          {
            "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF",
            "Availability": "Online",
            "AccessRights": "Open",
            "AccessURL": {
              "Name": "HTTP access to CDFs at SPDF",
              "URL": "http://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin_cdaweb/ket/",
              "Description": "In CDF via HTTP from SPDF"
            },
            "Format": "CDF",
            "Acknowledgement": "Space Physics Data Facility at NASA/GSFC"
          },
          {
            "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF",
            "Availability": "Online",
            "AccessRights": "Open",
            "AccessURL": {
              "Name": "CDAWeb",
              "URL": "http://cdaweb.gsfc.nasa.gov/cdaweb/sp_phys/",
              "ProductKey": "UY_M0_KET",
              "Description": "subset, plot, list via CDAWeb"
            },
            "Format": "Text",
            "Acknowledgement": "Space Physics Data Facility at NASA/GSFC"
          },
          {
            "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF",
            "Availability": "Online",
            "AccessRights": "Open",
            "AccessURL": {
              "Name": "FTP access to ASCII files at SPDF",
              "URL": "ftp://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin/ket/10_min/",
              "Description": "via ftp in ASCII from SPDF."
            },
            "Format": "Text",
            "Acknowledgement": "Space Physics Data Facility at NASA/GSFC"
          },
          {
            "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF",
            "Availability": "Online",
            "AccessRights": "Open",
            "AccessURL": {
              "Name": "HTTP access to ASCII files at SPDF",
              "URL": "http://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin/ket/10_min/",
              "Description": "via http in ASCII from SPDF"
            },
            "Format": "Text",
            "Acknowledgement": "Space Physics Data Facility at NASA/GSFC"
          }
        ],
        "InstrumentID": "spase://SMWG/Instrument/Ulysses/COSPIN/KET",
        "MeasurementType": "EnergeticParticles",
        "TemporalDescription": {
          "TimeSpan": {
            "StartDate": "1990-10-23T00:00:00.000",
            "StopDate": "2008-12-31T23:59:59.999"
          },
          "Cadence": "PT10M"
        },
        "ObservedRegion": "Heliosphere.Outer",
        "Parameter": {
          "Time_PG1": {
            "Name": "Time for the record",
            "ParameterKey": "Time_PG1",
            "Description": "Time for the record given in year, day of year, hour, min, seconds and coverage in percent.\n                    The given time represents the start of the averaging interval.",
            "Cadence": "PT10M",
            "Structure": {
              "Size": "6",
              "Element": [
                {
                  "Name": "Year",
                  "Index": "1",
                  "ValidMin": "1990",
                  "ValidMax": "2008"
                },
                {
                  "Name": "Day of year",
                  "Index": "2",
                  "ValidMin": "1",
                  "ValidMax": "366"
                },
                {
                  "Name": "Hour of day",
                  "Index": "3",
                  "ValidMin": "0",
                  "ValidMax": "23"
                },
                {
                  "Name": "Minute of hour",
                  "Index": "4",
                  "ValidMin": "0",
                  "ValidMax": "59"
                },
                {
                  "Name": "Seconds of minute",
                  "Index": "5",
                  "ValidMin": "0",
                  "ValidMax": "59"
                },
                {
                  "Name": "Coverage",
                  "Index": "6",
                  "ValidMin": "0",
                  "ValidMax": "100"
                }
              ]
            },
            "Support": {
              "SupportQuantity": "Temporal"
            }
          },
          "K1": {
            "Name": "COSPIN/KET 10-Minute Average 2.7-5.4 MeV Proton Spin-Averaged Count Rates (K1)",
            "ParameterKey": "K1",
            "Description": "10-minute average KET spin-averaged proton count rates between 2.7 and 5.4 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K1                     18\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.\n\n\t\t\t\tBackground fluxes of K1 are a combination of components, including a high RTG background rate.\n\t\t\t\tThis channel should be used only during event times.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.7",
                "High": "5.4",
                "Units": "MeV"
              }
            }
          },
          "K21": {
            "Name": "COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 1 (K21)",
            "ParameterKey": "K21",
            "Description": "10-minute average KET proton count rates in spin sector 1 (of 8) between 5.4 and 23.1 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K21-K28               120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "5.4",
                "High": "23.1",
                "Units": "MeV"
              }
            }
          },
          "K22": {
            "Name": "COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 2 (K22)",
            "ParameterKey": "K22",
            "Description": "10-minute average KET proton count rates in spin sector 2 (of 8) between 5.4 and 23.1 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K21-K28               120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "5.4",
                "High": "23.1",
                "Units": "MeV"
              }
            }
          },
          "K23": {
            "Name": "COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 3 (K23)",
            "ParameterKey": "K23",
            "Description": "10-minute average KET proton count rates in spin sector 3 (of 8) between 5.4 and 23.1 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K21-K28               120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "5.4",
                "High": "23.1",
                "Units": "MeV"
              }
            }
          },
          "K24": {
            "Name": "COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 4 (K24)",
            "ParameterKey": "K24",
            "Description": "10-minute average KET proton count rates in spin sector 4 (of 8) between 5.4 and 23.1 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K21-K28               120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "5.4",
                "High": "23.1",
                "Units": "MeV"
              }
            }
          },
          "K25": {
            "Name": "COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 5 (K25)",
            "ParameterKey": "K25",
            "Description": "10-minute average KET proton count rates in spin sector 5 (of 8) between 5.4 and 23.1 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K21-K28               120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "5.4",
                "High": "23.1",
                "Units": "MeV"
              }
            }
          },
          "K26": {
            "Name": "COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 6 (K26)",
            "ParameterKey": "K26",
            "Description": "10-minute average KET proton count rates in spin sector 6 (of 8) between 5.4 and 23.1 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K21-K28               120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "5.4",
                "High": "23.1",
                "Units": "MeV"
              }
            }
          },
          "K27": {
            "Name": "COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 7 (K27)",
            "ParameterKey": "K27",
            "Description": "10-minute average KET proton count rates in spin sector 7 (of 8) between 5.4 and 23.1 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K21-K28               120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "5.4",
                "High": "23.1",
                "Units": "MeV"
              }
            }
          },
          "K28": {
            "Name": "COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 8 (K28)",
            "ParameterKey": "K28",
            "Description": "10-minute average KET proton count rates in spin sector 8 (of 8) between 5.4 and 23.1 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K21-K28               120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "5.4",
                "High": "23.1",
                "Units": "MeV"
              }
            }
          },
          "P4": {
            "Name": "COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Spin-Averaged Count Rates (P4)",
            "ParameterKey": "P4",
            "Description": "10-minute average KET spin-averaged proton count rates between 5.4 and 23.1 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   P4                    120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "5.4",
                "High": "23.1",
                "Units": "MeV"
              }
            }
          },
          "K3": {
            "Name": "COSPIN/KET 10-Minute Average 34.1-125.0 MeV Proton Spin-Averaged Count Rates (K3)",
            "ParameterKey": "K3",
            "Description": "10-minute average KET spin-averaged proton count rates between 34.1 and 125.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K3                   70.0\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "34.1",
                "High": "125.0",
                "Units": "MeV"
              }
            }
          },
          "K34": {
            "Name": "COSPIN/KET 10-Minute Average 125.0-320.0 MeV Proton Spin-Averaged Count Rates (K34)",
            "ParameterKey": "K34",
            "Description": "10-minute average KET spin-averaged proton count rates between 125.0 and 320.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K34                  152.0\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "125.0",
                "High": "320.0",
                "Units": "MeV"
              }
            }
          },
          "K12": {
            "Name": "COSPIN/KET 10-Minute Average 320.0-2100.0 MeV Proton Spin-Averaged Count Rates (K12)",
            "ParameterKey": "K12",
            "Description": "10-minute average KET spin-averaged proton count rates between 320.0 and 2100.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K12                  3300.0\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "320.0",
                "High": "2100.0",
                "Units": "MeV"
              }
            }
          },
          "K0": {
            "Name": "COSPIN/KET 10-Minute Average >2100.0 MeV Proton Spin-Averaged Count Rates (K10)",
            "ParameterKey": "K0",
            "Description": "10-minute average KET spin-averaged proton count rates >2100.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K10                   N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Proton",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2100.0",
                "High": "INF",
                "Units": "MeV"
              }
            }
          },
          "K2": {
            "Name": "COSPIN/KET 10-Minute Average 6.0-20.4 MeV/n Helium Spin-Averaged Count Rates (K2)",
            "ParameterKey": "K2",
            "Description": "10-minute average KET spin-averaged helium count rates between 6.0 and 20.4 MeV/n",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K2                    120\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "AlphaParticle",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "6.0",
                "High": "20.4",
                "Units": "MeV/n"
              }
            }
          },
          "K33": {
            "Name": "COSPIN/KET 10-Minute Average 34.2-125.0 MeV/n Helium Spin-Averaged Count Rates (K33)",
            "ParameterKey": "K33",
            "Description": "10-minute average KET spin-averaged helium count rates between 34.2 and 125.0 MeV/n",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K33                  70.0\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "AlphaParticle",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "34.2",
                "High": "125.0",
                "Units": "MeV/n"
              }
            }
          },
          "K29": {
            "Name": "COSPIN/KET 10-Minute Average 125.0-320.0 MeV/n Helium Spin-Averaged Count Rates (K29)",
            "ParameterKey": "K29",
            "Description": "10-minute average KET spin-averaged helium count rates between 125.0 and 320.0 MeV/n",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K29                  88.0\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "AlphaParticle",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "125.0",
                "High": "320.0",
                "Units": "MeV/n"
              }
            }
          },
          "K31": {
            "Name": "COSPIN/KET 10-Minute Average 320.0-2100.0 MeV/n Helium Spin-Averaged Count Rates (K31)",
            "ParameterKey": "K31",
            "Description": "10-minute average KET spin-averaged helium count rates between 320.0 and 2100.0 MeV/n",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K31                 3200.0\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "AlphaParticle",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "320.0",
                "High": "2100.0",
                "Units": "MeV/n"
              }
            }
          },
          "K30": {
            "Name": "COSPIN/KET 10-Minute Average >2100.0 MeV/n Helium Spin-Averaged Count Rates (K30)",
            "ParameterKey": "K30",
            "Description": "10-minute average KET spin-averaged helium count rates >2100.0 MeV/n",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K30                   N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "AlphaParticle",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2100.0",
                "High": "INF",
                "Units": "MeV/n"
              }
            }
          },
          "K13": {
            "Name": "COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 1 (K13)",
            "ParameterKey": "K13",
            "Description": "10-minute average KET electron count rates in spin sector 1 (of 8) between 2.5 and 7.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K13-K20               N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.5",
                "High": "7.0",
                "Units": "MeV"
              }
            }
          },
          "K14": {
            "Name": "COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 2 (K14)",
            "ParameterKey": "K14",
            "Description": "10-minute average KET electron count rates in spin sector 2 (of 8) between 2.5 and 7.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K13-K20               N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.5",
                "High": "7.0",
                "Units": "MeV"
              }
            }
          },
          "K15": {
            "Name": "COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 3 (K15)",
            "ParameterKey": "K15",
            "Description": "10-minute average KET electron count rates in spin sector 3 (of 8) between 2.5 and 7.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K13-K20               N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.5",
                "High": "7.0",
                "Units": "MeV"
              }
            }
          },
          "K16": {
            "Name": "COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 4 (K16)",
            "ParameterKey": "K16",
            "Description": "10-minute average KET electron count rates in spin sector 4 (of 8) between 2.5 and 7.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K13-K20               N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.5",
                "High": "7.0",
                "Units": "MeV"
              }
            }
          },
          "K17": {
            "Name": "COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 5 (K17)",
            "ParameterKey": "K17",
            "Description": "10-minute average KET electron count rates in spin sector 5 (of 8) between 2.5 and 7.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K13-K20               N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.5",
                "High": "7.0",
                "Units": "MeV"
              }
            }
          },
          "K18": {
            "Name": "COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 6 (K18)",
            "ParameterKey": "K18",
            "Description": "10-minute average KET electron count rates in spin sector 6 (of 8) between 2.5 and 7.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K13-K20               N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.5",
                "High": "7.0",
                "Units": "MeV"
              }
            }
          },
          "K19": {
            "Name": "COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 7 (K19)",
            "ParameterKey": "K19",
            "Description": "10-minute average KET electron count rates in spin sector 7 (of 8) between 2.5 and 7.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K13-K20               N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.5",
                "High": "7.0",
                "Units": "MeV"
              }
            }
          },
          "K20": {
            "Name": "COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 8 (K20)",
            "ParameterKey": "K20",
            "Description": "10-minute average KET electron count rates in spin sector 8 (of 8) between 2.5 and 7.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K13-K20               N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.5",
                "High": "7.0",
                "Units": "MeV"
              }
            }
          },
          "E4": {
            "Name": "COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Spin-Averaged Count Rates (E4)",
            "ParameterKey": "E4",
            "Description": "10-minute average KET spin-averaged electron count rates between 2.5 and 7.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   E4                    N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "2.5",
                "High": "7.0",
                "Units": "MeV"
              }
            }
          },
          "K11": {
            "Name": "COSPIN/KET 10-Minute Average 7.0-170.0 MeV Electron Spin-Averaged Count Rates (K11)",
            "ParameterKey": "K11",
            "Description": "10-minute average KET spin-averaged electron count rates between 7.0 and 170.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K11                   N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "7.0",
                "High": "170.0",
                "Units": "MeV"
              }
            }
          },
          "K32": {
            "Name": "COSPIN/KET 10-Minute Average >170.0 MeV Electron Spin-Averaged Count Rates (K32)",
            "ParameterKey": "K32",
            "Description": "10-minute average KET spin-averaged electron count rates >170.0 MeV",
            "Caveats": "Only rates C are given, since no simple estimates of the intensities can be done\n\t            Intensities (I) must be derived by dividing through the integral geometric factor Gi,\n\t\t\t\tand by correcting through Pils Height Analysis.\n\t\t\t\t                   I=C/Gi\n\t\t        Values of the geometrical Factor Gi = (counting rate)/(Intensity):\n\t\t\t\t                   KET Channel           Gi\n\t\t\t\t\t\t\t\t   =============================\n\t\t\t\t\t\t\t\t   K32                   N/A\n\n\t\t\t\tOn 10 min averages some of the channels have limitations because of RTG background.  Very slow\n\t\t\t\tincreases are a sign that backgrounf levels are reached (a few percent per year).\n\n\t\t\t\tGET LOW FLUX VALUES FROM THE PI ON LONGER ACCUMULATION PERIODS\n\n\t\t\t\tTimeperiods when KET is saturated or is working in a \"calibration mode\" have been omitted:\n\t\t\t\t                   eg. March event 1991\n\t\t\t\t\t\t\t\t   peak fluxes in the June to August period 1991\n\t\t\t\t\t\t\t\t   Jovian encounter.",
            "Cadence": "PT10M",
            "Units": "(/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": "Electron",
              "Qualifier": "Average",
              "ParticleQuantity": "CountRate",
              "EnergyRange": {
                "Low": "170.0",
                "High": "INF",
                "Units": "MeV"
              }
            }
          },
          "D10": {
            "Name": "COSPIN/KET 10-Minute Average D10 Detector Counting Rate (D10)",
            "ParameterKey": "D10",
            "Description": "10-minute average KET D10 detector counting rate",
            "Caveats": "Rate channel D10 includes all particles depositing energy greater than the\n\t            minimum discriminator level.",
            "Cadence": "PT10M",
            "Units": "(counts/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": [
                "Proton",
                "AlphaParticle",
                "Ion",
                "Electron"
              ],
              "Qualifier": "Average",
              "ParticleQuantity": "Counts"
            }
          },
          "D20": {
            "Name": "COSPIN/KET 10-Minute Average D20 Detector Counting Rate (D20)",
            "ParameterKey": "D20",
            "Description": "10-minute average KET D20 detector counting rate",
            "Caveats": "Rate channel D20 includes all particles depositing energy greater than the\n\t            minimum discriminator level.",
            "Cadence": "PT10M",
            "Units": "(counts/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": [
                "Proton",
                "AlphaParticle",
                "Ion",
                "Electron"
              ],
              "Qualifier": "Average",
              "ParticleQuantity": "Counts"
            }
          },
          "C10": {
            "Name": "COSPIN/KET 10-Minute Average C10 Detector Counting Rate (D10)",
            "ParameterKey": "C10",
            "Description": "10-minute average KET C10 detector counting rate",
            "Caveats": "Rate channel C10 includes all particles depositing energy greater than the\n\t            minimum discriminator level.",
            "Cadence": "PT10M",
            "Units": "(counts/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": [
                "Proton",
                "AlphaParticle",
                "Ion",
                "Electron"
              ],
              "Qualifier": "Average",
              "ParticleQuantity": "Counts"
            }
          },
          "C20": {
            "Name": "COSPIN/KET 10-Minute Average C20 Detector Counting Rate (D10)",
            "ParameterKey": "C20",
            "Description": "10-minute average KET C20 detector counting rate",
            "Caveats": "Rate channel C20 includes all particles depositing energy greater than the\n\t            minimum discriminator level.",
            "Cadence": "PT10M",
            "Units": "(counts/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": [
                "Proton",
                "AlphaParticle",
                "Ion",
                "Electron"
              ],
              "Qualifier": "Average",
              "ParticleQuantity": "Counts"
            }
          },
          "A01": {
            "Name": "COSPIN/KET 10-Minute Average A01 Detector Counting Rate (A01)",
            "ParameterKey": "A01",
            "Description": "10-minute average KET A01 detector counting rate",
            "Caveats": "Rate channel A01 includes all particles depositing energy greater than the\n\t            minimum discriminator level.",
            "Cadence": "PT10M",
            "Units": "(counts/s)",
            "ValidMin": "0.0",
            "ValidMax": "1.00E+06",
            "FillValue": "-707",
            "Particle": {
              "ParticleType": [
                "Proton",
                "AlphaParticle",
                "Ion",
                "Electron"
              ],
              "Qualifier": "Average",
              "ParticleQuantity": "Counts"
            }
          }
        }
      }
    }
  }
}