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Solar flare hard X-ray observations

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Abstract

Recent hard X-ray observations of solar flares are reviewed with emphasis on results obtained with instruments on the Solar Maximum Mission satellite. Flares with three different sets of characteristics, designated as Type A, Type B, and Type C, are discussed and hard X-ray temporal, spatial, spectral, and polarization measurements are reviewed in this framework. Coincident observations are reviewed at other wavelengths including the UV, microwaves, and soft X-rays, with discussions of their interpretations. In conclusion, a brief outline is presented of the potential of future hard X-ray observations with sub-second time resolution, arcsecond spatial resolution, and keV energy resolution, and polarization measurements at the few percent level up to 100 keV.

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  1. Solar Physics Branch, Laboratory for Astronomy and Solar Physics, NASA-Goddard Space Flight Center, 20771, Greenbelt, MD, U.S.A.

    Brian R. Dennis

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Dennis, B.R. Solar flare hard X-ray observations. Sol Phys 118, 49–94 (1988). https://doi.org/10.1007/BF00148588

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