Spectral line broadening of radio waves in the near-solar plasma

Details Spectral line broadening of radio waves in the near-solar plasma Spectral line broadening of radio waves in the near-solar plasma

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981rael...26.2241l&link_type=abstract

Radiotekhnika i Elektronika, vol. 26, Nov. 1981, p. 2241-2245. In Russian.

Physics

1

Cosmic Plasma, Plasma Spectra, Radio Spectra, Solar Atmosphere, Spectral Line Width, Correlation, Permittivity, Solar Wind

Scientific paper

An analysis is presented of conditions under which the hypothesis of a 'frozen-in' plasma in the near-solar medium is valid. It is shown that at radii less than 10 solar radii, this hypothesis is invalid; the spectral line shape of radio waves that have passed through the turbulent medium is determined by the temporal correlation function of permittivity fluctuations. Experimental data obtained by radio occultation agree with the exponential form of this function.

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