Frequency drift of type III bursts and a solar-corona model

Details Frequency drift of type III bursts and a solar-corona model Frequency drift of type III bursts and a solar-corona model

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..420t&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Mar.-Apr. 1990, p. 420-427. In Russian.

Astronomy and Astrophysics

Astronomy

4

Frequency Distribution, Solar Corona, Stellar Models, Type 3 Bursts, Electron Density (Concentration), Plasma Density, Solar Electrons

Scientific paper

The frequency dependence of the mean drift rate of type III radio bursts appears to have a singularity at about 25 MHz owing to the fact that the plasma density decreases differently in the inner and outer corona. An analysis of this finding in the framework of various models of the corona does not confirm the hypothesis of a local source moving away from the sun within a dense streamer. Rather, the observations favor an optical model of the quiet corona.

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