Computer Science – Sound
Scientific paper
Jun 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992raf....34..615i&link_type=abstract
Radiofizika (ISSN 0021-3462), vol. 34, no. 6, June 1992, p. 615-623. In Russian.
Computer Science
Sound
Frequency Measurement, Nonuniform Plasmas, Radio Occultation, Solar Corona, Solar Wind Velocity, Autocorrelation, Radio Wave Refraction, Satellite Sounding, Venera Satellites
Scientific paper
The correlation functions for phase and frequency fluctuations are analyzed for the case of two-way propagation of radio waves in the solar corona. It is shown that the correlation function has a distinct maximum at the time shift which depends on the velocity of corona irregularities and the distance between the radio link and the sun. A method for the determination of the solar wind velocity is presented, which is based on phase and frequency measurements during two-way radio occultation experiments. The theoretical data are compared with the experimental data obtained with radio sounding of the solar corona from the Venera-15,-16 spacecraft.
Efimov Alexander I.
Erofeev A. L.
Iakovlev O. I.
Iakubov V. P.
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