The large-scale structure of the circumsolar plasma as determined from scintillations

Details The large-scale structure of the circumsolar plasma as determined from scintillations The large-scale structure of the circumsolar plasma as determined from scintillations

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992azh....69..173l&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 69, no. 1, Jan.-Feb. 1992, p. 173-180. In Russian.

Computer Science

Sound

6

Cosmic Plasma, Scintillation, Solar Neighborhood, Solar Wind, Interplanetary Medium, Solar Corona

Scientific paper

An occultation experiment using water vapor maser sources was conducted in December 1987. Five occultation sources were used simultaneously. Circumsolar plasma sounding was performed at the transition zone of the solar wind, where the subsonic outflow becomes supersonic. The large-scale configuration of the medium was reconstructed from results of studies of the scintillation index radial dependence. The relationship between the configuration of the solar wind transonic region and that of the solar corona is investigated.

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