Near-solar plasma turbulence and solar-wind velocity from Venera 10 radio-occultation data

Details Near-solar plasma turbulence and solar-wind velocity from Venera 10 radio-occultation data Near-solar plasma turbulence and solar-wind velocity from Venera 10 radio-occultation data

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..322e&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, July 1977, p. 322-325. In Russian.

Astronomy and Astrophysics

Astronomy

7

Energy Spectra, Plasma Turbulence, Radio Occultation, Solar Wind Velocity, Nonuniform Plasmas, Plasma Diagnostics, Plasma Spectra, Venera Satellites

Scientific paper

Observations of variations in the energy spectrum of Venera 10 radio signals during their propagation in the inhomogeneous solar plasma at elongations of 0.6 to 6 deg are analyzed. It is shown that the spatial turbulence spectrum of the near-solar plasma is similar to a Kolmogorov spectrum, that this plasma is strongly turbulent, and that the degree of inhomogeneity increases at distances of 2 to 5 and 12 to 20 solar radii. The values determined for the solar-wind velocity are found to be close to those given by Parker's theory.

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