Imaging of impulsive solar flare phenomena

Details Imaging of impulsive solar flare phenomena Imaging of impulsive solar flare phenomena

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..279d&link_type=abstract

(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un

Physics

29

Microwave Imagery, Solar Flares, X Ray Imagery, Solar Maximum Mission, Thermal Plasmas, Very Long Base Interferometry

Scientific paper

The present study reviews recent advances in the understanding of impulsive solar flare phenomena investigated using new hard X-ray and microwave imaging instruments: the Hard X-ray Imaging Spectrometer aboard the Solar Maximum Mission satellite and the Solar Hard X-ray Telescope aboard Hinotori, and the VLA and VLBI. The problem of quasi-thermal flares is discussed, and attention is given to the implications of the presence of a hot component (T of about 40-million K) for the flare energy balance.

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