Computer Science
Scientific paper
Oct 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21..769e&link_type=abstract
Geomagnetizm i Aeronomiia, vol. 21, Sept.-Oct. 1981, p. 769-774. In Russian.
Computer Science
Interplanetary Medium, Plasma Acceleration, Plasma Drift, Radio Occultation, Solar Wind Velocity, Fluctuation Theory, Plasma Composition, Radio Signals, Scintillation, Space Probes, Spectral Line Width
Scientific paper
Scintillation observations of the near-solar plasma made using interplanetary probes (Mariner, Helios, and Venera) are analyzed on the basis of a method that takes into account the proper motions of the radio source relative to the solar-wind inhomogeneities. It is shown that data on the frequency fluctuations and spectral line broadening of the radio signals can be used to determine the drift velocity of solar-wind inhomogeneities in the acceleration region.
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