{
  "id": "SX_K0_30F",
  "url": "http://hpde.io/NASA/NumericalData/SAMPEX/PT30.00S",
  "data-file": "./data/spase_hpde_io/info/SX_K0_30F.json",
  "data": {
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      "NumericalData": {
        "ResourceID": "spase://NASA/NumericalData/SAMPEX/PT30.00S",
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        "ResourceType": "NumericalData",
        "ResourceHeader": {
          "ResourceName": "SAMPEX Fluxes, all instruments",
          "DOI": "https://doi.org/10.48322/2x9v-jv02",
          "ReleaseDate": "2025-12-04T13:31:22Z",
          "RevisionHistory": {
            "RevisionEvent": [
              {
                "ReleaseDate": "2021-04-27T15:38:11",
                "Note": "Only known prior ReleaseDate of the metadata"
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              {
                "ReleaseDate": "2023-07-30T12:34:56.789",
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          },
          "Description": "This set of 30-s averaged fluxes are derived from measurements made by all 4 instruments (HILT, LICA, MAST and PET) onboard the Solar Anomalous and Magnetospheric Particle Explorer (SAMPEX). Each file covers one full day of 30-s averaged fluxes of cosmic rays from selected channels from all experiments. There are 156 variables per record, and the file size is about 4 MB. After an extensive list of ancillary data, the particle fluxes follow. (1) LICA provides fluxes of electrons and protons in the energy range of about >0.7 Mev, of (mainly) helium in the range 0.49-8.3 MeV/nucleon. (2) HILT provides fluxes of helium from two channels, 4-9 and 9-38, of Z > 5 from two channels, 8.2-42 and 41-220 MeV/n. (3) MAST provides fluxes protons (mainly) in 5-12 MeV range, of helium in 8-15, and of Z > 5 in 19.3-22.8, 22.8-31.0, 31.0-51.7, 51.7-76.2, 76.2-113, 113-156 MeV/n. (4) PET provides fluxes of electrons in the ranges 1.5-6, and 2.5-14 MeV, and of (mainly) protons in 19-27 MeV/n. All flux values are accompanied by their standard deviations and quality flags. The fluxes available in this file are from a subset of (30-s resolution) rate channels. Energy spectra are assembled by pick-and-choose across instrument boundaries; an example is the eight-element array of Z>3 fluxes that have contributions from all four instruments",
          "PublicationInfo": {
            "Authors": "Mason, Glenn, M.; Parthasarathy, R.",
            "PublicationDate": "2023-01-01T00:00:00",
            "PublishedBy": "Space Physics Data Facility"
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          "Contact": [
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              "PersonID": "spase://SMWG/Person/Glenn.M.Mason",
              "Role": "PrincipalInvestigator"
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              "PersonID": "spase://SMWG/Person/R.Parthasarathy",
              "Role": "GeneralContact"
            },
            {
              "PersonID": "spase://SMWG/Person/Lee.Frost.Bargatze",
              "Role": "MetadataContact"
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          ],
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              "URL": "ftps://spdf.gsfc.nasa.gov/pub/data/sampex/combined_cdaweb/30f/"
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            "AccessURL": {
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              "URL": "ftps://spdf.gsfc.nasa.gov/pub/data/sampex/"
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        "ProviderProcessingLevel": "CALIBRATED",
        "InstrumentID": [
          "spase://SMWG/Instrument/SAMPEX/MAST",
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          "spase://SMWG/Instrument/SAMPEX/PET",
          "spase://SMWG/Instrument/SAMPEX/LICA"
        ],
        "MeasurementType": [
          "EnergeticParticles",
          "IonComposition"
        ],
        "TemporalDescription": {
          "TimeSpan": {
            "StartDate": "1992-07-06T00:00:00",
            "StopDate": "2004-06-30T23:59:59"
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          "Cadence": "PT30.00S"
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        "ObservedRegion": "Earth.Magnetosphere"
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  }
}