Directionality of continuum gamma rays from solar flares

Details Directionality of continuum gamma rays from solar flares Directionality of continuum gamma rays from solar flares

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8915884b&link_type=abstract

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Physics

Continuous Radiation, Directivity, Gamma Rays, Solar Flares, Solar Radiation, Electron Distribution, Limb Brightening, Solar Limb, Solar X-Rays

Scientific paper

The hard X-ray spectrometer total counts are used as calibration to investigate how the brightness of gamma rays above 300 keV changes as a function of the heliocentric angle of a flare. The normalized gamma-ray brightness, on the average, increases with the heliocentric angle; a flare at the limb is estimated to be 13 times brighter in gamma-rays than a similar flare near the central meridian. Both pancake-like electron distributions and downward beam distributions can be adjusted to produce the deduced limb brightening.

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