Electron-density fluctuations in a region where a supersonic stream of the solar wind is formed

Details Electron-density fluctuations in a region where a supersonic stream of the solar wind is formed Electron-density fluctuations in a region where a supersonic stream of the solar wind is formed

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984rael...29..943b&link_type=abstract

Radiotekhnika i Elektronika (ISSN 0033-8494), vol. 29, May 1984, p. 943-947. In Russian.

Physics

Electron Density (Concentration), Interplanetary Medium, Radial Distribution, Solar Wind, Supersonic Flow, Water Masers, Plasma Turbulence, Radio Telescopes, Scintillation, Water Vapor

Scientific paper

Electron-density fluctuations in the interplanetary medium were studied on the basis of RT-22 telescope observations of scintillations of the S252A water-vapor maser source. Regions close to the sun were investigated in the regime of faint scintillations. A set of data on the radial dependence of the scintillation index made it possible to analyze the radial dependence of electron-density fluctuations in the region of solar-wind acceleration. Three characteristic regions are delineated, corresponding to subsonic flow, a transition region, and supersonic flow.

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