Solar wind from radio occultation data obtained by Veneras 15 and 16

Details Solar wind from radio occultation data obtained by Veneras 15 and 16 Solar wind from radio occultation data obtained by Veneras 15 and 16

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65.1290i&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Nov.-Dec. 1988, p. 1290-1299. In Russian.

Astronomy and Astrophysics

Astronomy

16

Electron Plasma, Interplanetary Medium, Radio Occultation, Solar Wind, Solar Wind Velocity, Venera Satellites, Cross Correlation, Heliosphere, Nonuniform Plasmas

Scientific paper

Data on solar wind speed, spatial spectrum of plasma irregularities and inner scale of the turbulence are presented. Electron density, degree of plasma inhomogeneity, power of solar wind and the rate of solar mass loss are determined. The dependence of these parameters on heliocentric distance in the interval R = 5 - 100 R_sun; is discussed for two spatial regions. It is shown that at (12 - 25) R_sun; the principal parameters of the solar wind show great variations.

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