Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993kfnt....9...16l&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 9, no. 1, p. 16-23.
Astronomy and Astrophysics
Astronomy
Magnetohydrodynamic Turbulence, Radio Astronomy, Solar Wind, Subsonic Flow, Supersonic Flow, Transition Flow, Quasars, Radio Scattering
Scientific paper
The transition zone between subsonic and supersonic solar wind flow is studied using nine natural radio sounding sources. The observations were carried out in June-August 1989. In the interval of the radial distances 5-40 solar radii, the scattering angle radial dependence theta-R was studied. The two-dimensional mapping of the solar wind transonic region was obtained. The large-scale configuration of the medium was reconstructed from the data on the scattering angle theta-R. The relation between the configuration of the solar wind transonic region and that of the solar supercorona has been investigated.
Korelov O. A.
Lotova N. A.
Pisarenko Ya. V.
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