Distribution of velocities in the instantaneous solar wind pattern

Details Distribution of velocities in the instantaneous solar wind pattern Distribution of velocities in the instantaneous solar wind pattern

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ge%26ae..19..788l&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 19, Sept.-Oct. 1979, p. 788-792. In Russian.

Astronomy and Astrophysics

Astronomy

1

Radio Astronomy, Solar Wind Velocity, Velocity Distribution, Distribution Functions, Scintillation, Time Response

Scientific paper

Ground-based radio astronomy observations of interplanetary scintillations contain information that can be used to determine the velocity distribution in the instantaneous solar wind pattern. In the present study, scintillation data obtained from observations at three locations are used to study the distribution of solar wind velocities. The basis parameters of the velocity distribution function are identified. Dispersion curves are plotted for these data.

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