Physics
Scientific paper
Dec 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..155..339g&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 155, no. 2, p. 339-350
Physics
8
Collisionless Plasmas, Current Sheets, Polarization (Waves), Solar Radio Emission, Electromagnetic Fields, Electron Density (Concentration), Faraday Effect, Wave Propagation
Scientific paper
We show that it is possible to account for the polarization features of solar radio emission provided the linear mode coupling theory is properly applied and the presence of current sheets in the corona is taken into account. We present a schematic model, including a current sheet that can explain the polarization features of both the low frequency slowly varying component and the bipolar noise storm radiation; the two radiations face similar propagation conditions through a current sheet and hence display similar polarization behavior. We discuss the applications of the linear mode coupling theory to the following types of solar emission: the slowly varying component, the microwave radio bursts, metric type U bursts, and bipolar noise storms.
Gopalswamy Nat
Kundu Mukul R.
White Stephen M.
Zheleznyakov Vladimir V.
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