{
  "@type": "dcat:Dataset",
  "accessLevel": "public",
  "accrualPeriodicity": "irregular",
  "bureauCode": [
    "026:00"
  ],
  "contactPoint": {
    "@type": "vcard:Contact",
    "fn": "Thomas Morgan",
    "hasEmail": "mailto:thomas.h.morgan@nasa.gov"
  },
  "description": "This data set contains solar wind plasma data upstream of Jupiter before the Voyager 2 encounter. Fit and moment parameters are given; the fit parameters assume a convected isotropic proton Maxwellian distribution. Use of fit parameters is recommended as these are normally more accurate. Since only the first 72 or last 72 energy/charge channels are telemetered to Earth from each M-mode spectra, derived parameters change significantly only every other set of spectra so the effective time resolution is 196 s.",
  "identifier": "urn:nasa:pds:context_pds3:data_set:data_set.vg2-j-pls-5-summ-ion-inbndswind-96s-v1.0_ksiv-4tc4",
  "issued": "2021-05-21",
  "keyword": [
    "jupiter",
    "voyager"
  ],
  "landingPage": "https://pds.nasa.gov/ds-view/pds/viewDataset.jsp?dsid=VG2-J-PLS-5-SUMM-ION-INBNDSWIND-96S-V1.0",
  "license": "http://www.usa.gov/publicdomain/label/1.0/",
  "modified": "2025-07-17",
  "programCode": [
    "026:005"
  ],
  "publisher": {
    "@type": "org:Organization",
    "name": "National Aeronautics and Space Administration"
  },
  "references": [
    "https://pds.nasa.gov"
  ],
  "theme": [
    "Earth Science"
  ],
  "title": "VG2 JUP PLS DERIVED ION INBOUND SOLAR\nWIND 96SEC V1.0"
}