Frequency and phase fluctuations of radio waves during propagation in the Venus atmosphere

Details Frequency and phase fluctuations of radio waves during propagation in the Venus atmosphere Frequency and phase fluctuations of radio waves during propagation in the Venus atmosphere

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982rael...27.2318e&link_type=abstract

Radiotekhnika i Elektronika, vol. 27, Dec. 1982, p. 2318-2322. In Russian.

Physics

Frequency Response, Phase Deviation, Radio Occultation, Venus Atmosphere, Atmospheric Turbulence, Mean Square Values, Time Dependence, Turbulence Effects, Venera 10 Satellite

Scientific paper

Radio-occultation data on the Venus atmosphere obtained with the Venera-10 probe are used to analyze the effect of atmospheric irregularities on frequency and phase fluctuations of radio waves at a wavelength of 32 cm; the experiments were carried out in March 1976. It is shown that, as in the case of amplitude fluctuations, when the line of sight is removed 58-60 km from the Venus surface the frequency and phase fluctuations increase, whereas these fluctuations decrease at a height of 54-56 km. The external turbulence scale of the Venus atmosphere, which amounts to 4.5-6 km, is determined for the upper turbulence region, localized near a height of 60 km.

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