{
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  "contactPoint": {
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    "hasEmail": "mailto:NASA-SPDF-Support@nasa.onmicrosoft.com"
  },
  "description": "data designed to reveal the variations in solar K-corona via a subtraction of a \"background\" model (L2b data; see below) that primarily removes the dominant F-coronal signal. These data are usually in units of MSB, though this should be verified by inspection of the FITS headers. We do not provide L3 data for the high-cadence observations. Important: please see our disclaimer about the L3 data product.",
  "distribution": [
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      "format": "BIN",
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  "identifier": "https://doi.org/10.48322/4hzk-mn18",
  "keyword": [
    "imageintensity"
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  "landingPage": "https://doi.org/10.48322/4hzk-mn18",
  "license": "https://www.usa.gov/government-works",
  "modified": "2026-09-08",
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  "publisher": {
    "@type": "org:Organization",
    "name": "NRL"
  },
  "theme": [
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  "title": "Parker Solar Probe, WISPR Level 3 Data"
}