Solar flare hard X-ray observations

Details Solar flare hard X-ray observations Solar flare hard X-ray observations

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..118...49d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 118, no. 1-2, 1988, p. 49-94.

Physics

137

Particle Acceleration, Solar Flares, Solar X-Rays, Power Spectra, Solar Electrons, Solar Maximum Mission, Spatial Resolution, Temporal Resolution

Scientific paper

Recent hard X-ray observations of solar flares are reviewed with emphasis on results obtained with instruments on the solar maximum satellite. Flares with three 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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