The nature of solar microwave pulse bursts with quasi-thermal spectrum

Details The nature of solar microwave pulse bursts with quasi-thermal spectrum The nature of solar microwave pulse bursts with quasi-thermal spectrum

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976azh....53.1041u&link_type=abstract

Astronomicheskii Zhurnal, vol. 53, Sept.-Oct. 1976, p. 1041-1045. In Russian.

Physics

2

Microwave Spectra, Solar Radio Bursts, Solar Spectra, Stellar Models, Chromosphere, Optical Thickness, Shock Fronts, Shock Wave Propagation, Solar Corona, Solar Flares, Solar Physics

Scientific paper

The features of a model of solar microwave pulse bursts with quasi-thermal spectrum are described. The general picture is as follows: The heat released from a chromospheric flare is transported upward by a shock or thermal wave. When the shock front of the hot expanding region reaches optical depths of the order of unity, a radio burst is formed. Absorption by free-free transitions is assumed to be dominant.

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