Process of the formation of the supersonic solar wind

Details Process of the formation of the supersonic solar wind Process of the formation of the supersonic solar wind

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ge%26ae..32...78l&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 32, no. 3, May-June 1992, p. 78-84. In Russian.

Physics

2

Interplanetary Medium, Radio Wave Refraction, Solar Wind Velocity, Supersonic Flow, Radio Telescopes, Solar Flares

Scientific paper

Results of the probing of the circumsolar plasma at a wavelength of 2.9 m using 10 natural sources (quasars) are presented. It is shown that the formation of the supersonic solar-wind stream does not end within the limits of the SW transition region. Local increases of scattering in the plasma were also observed at distances of 50 and 70 solar radii from the sun.

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