@prefix skos: <http://www.w3.org/2004/02/skos/core#> .

<https://gcmd.earthdata.nasa.gov/kms/concept/2e83362e-d8f8-4bca-83fd-bae360ebe94b>
  skos:prefLabel "SOLAR ACTIVITY"@en ;
  a skos:Concept ;
  skos:narrower <https://gcmd.earthdata.nasa.gov/kms/concept/a15e514b-4b44-4587-a857-34ab7e2d357e> .

<https://gcmd.earthdata.nasa.gov/kms/concept/a15e514b-4b44-4587-a857-34ab7e2d357e>
  skos:definition """Solar X-Ray emissions can consist of X-Ray background flux or X-Ray bursts. A
daily average background X-ray flux is in the 1 to 8 angstrom range.  It is a
midday minimum designed to reduce the effects of flares. X-Ray burstsare a
temporary enhancement of the X-ray emission of the sun.  The time-intensity
profile of soft X-ray bursts is similar to that of the H-Alpha profile of an
associated flare. Bursts last from minutes to several hours."""@en ;
  skos:prefLabel "SOLAR X-RAY EMISSIONS"@en ;
  skos:inScheme <https://gcmd.earthdata.nasa.gov/kms/concepts/concept_scheme/sciencekeywords> ;
  skos:broader <https://gcmd.earthdata.nasa.gov/kms/concept/2e83362e-d8f8-4bca-83fd-bae360ebe94b> ;
  a skos:Concept .

