Morphological evolution of X-ray flare structures from the rise through the decay phase

Details Morphological evolution of X-ray flare structures from the rise through the decay phase Morphological evolution of X-ray flare structures from the rise through the decay phase

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199l..57k&link_type=abstract

Astrophysical Journal, vol. 199, July 1, 1975, pt. 2, p. L57-L61.

Astronomy and Astrophysics

Astronomy

61

Solar Flares, Solar X-Rays, Spaceborne Astronomy, X Ray Astronomy, Astronomical Photography, Morphology, Skylab Program, Solar Flux Density

Scientific paper

The morphological evolution of 12 solar X-ray subflares from onset through the decay phase has been studied using photographic X-ray images obtained from Skylab. The spatial configurations are found to vary widely from flare to flare, but they appear to be composed of two basic kinds of structures. The first, termed 'X-ray kernels', are brightest during the rise phase; the second, looplike structures, appear during the maximum and decay phases of the event. The X-ray kernels are small pointlike structures which may be related to the nonthermal phases of flares.

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