Concept information
TERME PRÉFÉRENTIEL
SOLAR X-RAY EMISSIONS
DÉFINITION
- 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.
CONCEPT GÉNÉRIQUE
URI
https://gcmd.earthdata.nasa.gov/kms/concept/a15e514b-4b44-4587-a857-34ab7e2d357e
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