Synthetic analysis of observed data of the two-ribbon solar flares and associated phenomena for the event of the 3rd February, 1983.

Details Synthetic analysis of observed data of the two-ribbon solar flares and associated phenomena for the event of the 3rd February, 1983. Synthetic analysis of observed data of the two-ribbon solar flares and associated phenomena for the event of the 3rd February, 1983.

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991chjss..11..142l&link_type=abstract

Chin. J. Space Sci., Vol. 11, No. 2, p. 142 - 151

Other

Solar Flares: Models, Solar Flares: Solar X-Ray Bursts, Solar Flares: Solar Gamma-Ray Bursts

Scientific paper

This paper analyzes synthetically the observed data of two-ribbon flares and associated phenomena on Feb 3, 1983. It is shown that there exists a close connection between the physical processes of nonthermal and thermal emissions in the two-ribbon flares, and, in particular that the nonthermal electrons from source regions of type III, type IVμ and other type IV bursts are responsible for hard X-ray and γ-ray bursts and Hα bright ribbons while the magnetic structures move freely along the vertical and horizontal direction.

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