Some aspects of radio and hard X-ray emissions of solar flares

Details Some aspects of radio and hard X-ray emissions of solar flares Some aspects of radio and hard X-ray emissions of solar flares

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pbeio..37...75k&link_type=abstract

Astrophysics Reports. Publications of the Beijing Astronomical Observatory, No. 37, p. 75 - 80 (2001). In: Proceedings of the Ei

Astronomy and Astrophysics

Astrophysics

Solar Flares, Solar Radio Emission, Solar Hard X-Ray Emission

Scientific paper

Two examples of the 1-2 GHz radio observations made by the Ondrejov radiospectrograph are shown: a) The October 5, 1992 drifting pulsation structure, and b) the November 9, 1998 high-frequency type II-like burst. We propose a model in which the drifting pulsations are caused by quasi-periodic particle accelerations in the magnetic reconnection in space under the ejected plasmoid. Then a new model of the electron component heating during the neutral beam bombardment of the dense atmospheric layers is presented and its relevance to the hard X-ray emission is discussed.

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