{
  "@type": "dcat:Dataset",
  "accessLevel": "public",
  "bureauCode": [
    "026:00"
  ],
  "contactPoint": {
    "@type": "vcard:Contact",
    "fn": "NASA Space Physics Data Facility",
    "hasEmail": "mailto:NASA-SPDF-Support@nasa.onmicrosoft.com"
  },
  "description": "The vector direction of peak suprathermal electron flux as measured with the Genesis Electron Monitor (GEM) instrument. This direction serves as a proxy for the interplanetary field orientation. The suprathermal electron flux is either parallel or anti-parallel to the interplanetary magnetic field. The true field polarity (+ or -) cannot be determined from GEM. Angles are given in Geocentric Solar Ecliptic (GSE) coordinates.",
  "distribution": [
    {
      "@type": "dcat:Distribution",
      "downloadURL": "ftps://cdaweb.gsfc.nasa.gov/pub/data/genesis/gim/",
      "format": "BIN",
      "mediaType": "application/octet-stream"
    },
    {
      "@type": "dcat:Distribution",
      "downloadURL": "https://helio.data.nasa.gov/dataset/Genesis_GIM_B-Proxy_PT160S",
      "format": "BIN",
      "mediaType": "application/octet-stream"
    },
    {
      "@type": "dcat:Distribution",
      "downloadURL": "https://hpde.io/NASA/NumericalData/Genesis/GIM/B-Proxy/PT160S",
      "format": "BIN",
      "mediaType": "application/octet-stream"
    }
  ],
  "identifier": "https://doi.org/10.48322/9gdf-de47",
  "keyword": [
    "magneticfield"
  ],
  "landingPage": "https://doi.org/10.48322/9gdf-de47",
  "license": "https://www.usa.gov/government-works",
  "modified": "2026-09-08",
  "programCode": [
    "026:000"
  ],
  "publisher": {
    "@type": "org:Organization",
    "name": "GSFC"
  },
  "theme": [
    "Heliophysics"
  ],
  "title": "Genesis interplanetary field orientation proxy"
}