Frequency changes and refraction during radio wave propagation through solar wind plasma

Details Frequency changes and refraction during radio wave propagation through solar wind plasma Frequency changes and refraction during radio wave propagation through solar wind plasma

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990raf....33.1007e&link_type=abstract

Radiofizika (ISSN 0021-3462), vol. 33, Sept. 1990, p. 1007-1012, 1. In Russian.

Physics

Decimeter Waves, Radio Wave Refraction, Solar Wind, Space Plasmas, Wave Propagation, Electron Density (Concentration), Frequency Ranges, Radio Probing, Venera Satellites

Scientific paper

Results of measurements of radio wave frequencies in the decimeter range in solar wind radio probing experiments aboard the Venera 15 and 16 satellites are analyzed. It is shown that the radio wave frequency increases as the ray line moves in the direction of the increasing electron concentration and decreases as the ray line moves away from the sun. The frequency shifts of the decimeter radio waves are typically 2.5-3 Hz at a distance of 3 solar radii from the sun. The refraction angle of the radio waves is determined as a function of the distance from the sun.

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