Hard X-rays of solar flares - Thermal versus non-thermal models: A review

Details Hard X-rays of solar flares - Thermal versus non-thermal models: A review Hard X-rays of solar flares - Thermal versus non-thermal models: A review

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ijrsp..18...71r&link_type=abstract

Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 18, June 1989, p. 71-84. Research supported by ISRO.

Physics

Space Physics

Bremsstrahlung, Satellite-Borne Instruments, Solar Flares, Solar Maximum Mission, Solar X-Rays, Electron Distribution, International Sun Earth Explorers, Monte Carlo Method, X Ray Spectroscopy

Scientific paper

The experimental results of X-ray bursts about spectral characteristics, spatial distribution, fast time variations and directivity measurements carried out with PVO/ISEE-3 spacecraft, imaging instrument observations of hard X-ray (HXIS) and hard X-ray burst spectrometer (HXRBS) during solar maximum mission have been reviewed. The observed results about the above characteristics are discussed in detail in terms of thermal and nonthermal models. The results are interpreted in terms of beamed thick target model in which electrons stream down to the loop footpoints and produce hard X-rays through electron-ion bremsstrahlung.

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