Radio spectrum and model of white-light flare of July 4, 1974

Details Radio spectrum and model of white-light flare of July 4, 1974 Radio spectrum and model of white-light flare of July 4, 1974

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983baicz..34..355k&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 34, Sept. 1983, p. 355-360.

Astronomy and Astrophysics

Astronomy

1

Radio Spectra, Solar Flares, Solar Radio Bursts, Continuous Spectra, Electrohydrodynamics, Photosphere, Plasma Currents, Solar Electrons, Solar Spectra

Scientific paper

The paper suggests a model of the white-light flare of July 4, 1974 which satisfies both the theoretical considerations and the actual observations. The observed radio spectrum is interpreted as an eruptive process that started at heights of more than 50000 km above the photosphere and was activated by an electron beam. The radio spectrum further shows that the activation is followed by a dissipation-spreading process (Heyvaerts, 1981) propagating through an electric current system towards the photosphere, to the place of the emission in continuum. In conclusion the radio spectrum of the white-light flare (1353 UT, July 4, 1974) is compared with the radio spectrum of its "homologous" flare (0647 UT, July 4, 1974).

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