Extended structure of the solar-wind transition region

Details Extended structure of the solar-wind transition region Extended structure of the solar-wind transition region

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..223l&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, Mar.-Apr. 1991, p. 223-227. In Russian.

Physics

2

Rayleigh Scattering, Solar Wind, Supersonic Flow, Transition Flow, Electron Density (Concentration), Flux Density, Radio Scattering, Radio Telescopes, Space Plasmas, Wave Scattering

Scientific paper

The paper presents results of a radio-telescope study of the solar-wind transition region conducted in June 1988. The region in which the supersonic flow was generated was found to be of greater extent than previously thought. A region of increased scattering was observed along with an increase in the scattering properties of the near-solar plasma in the region of R = 20-40 solar radii.

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