Reproducible characteristic features of the formation of supersonic solar wind

Details Reproducible characteristic features of the formation of supersonic solar wind Reproducible characteristic features of the formation of supersonic solar wind

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993geoae..33...10l&link_type=abstract

Geomagnetizm i Aehronomiya, vol. 33, p. 10

Computer Science

1

Solar Wind Velocity, Plasma Turbulence, Plasma Density, Solar Transition Region, Radio Occultation, Electron Density Profiles, Radial Distribution

Scientific paper

The large body of the available experimental data on the solar plasma, obtained by various versions of the radio occultation method, are analyzed in a comprehensive manner. Particular attention is given to the study of the transition region of solar wind. It is shown that the process of solar wind acceleration is characterized by a stably reproducible set of interrelated changes in the medium parameters with increasing distance from the sun.

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