Influence of plasma effects on the conditions for observing lines in the solar spectrum of radio emission

Details Influence of plasma effects on the conditions for observing lines in the solar spectrum of radio emission Influence of plasma effects on the conditions for observing lines in the solar spectrum of radio emission

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sva....21..742k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 54, Nov.-Dec. 1977, p. 1305-1308.) Soviet Astronomy, vol. 21, Nov.-Dec. 1977, p. 742, 743. Tran

Astronomy and Astrophysics

Astronomy

Line Spectra, Plasma-Electromagnetic Interaction, Radio Spectra, Solar Radio Emission, Transition Probabilities, Plasma Turbulence, Plasma Waves

Scientific paper

It is noted that no emission or absorption lines have ever been detected in the solar radio spectrum and that such detection is probably impossible. Calculations are performed which show that the emission of plasma waves by atoms is more effective than the emission of ordinary photons in a turbulent plasma medium. It is concluded that this effect may be one of the reasons why solar radio lines are not observed.

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