Solar wind dynamics at small distances from the sun

Details Solar wind dynamics at small distances from the sun Solar wind dynamics at small distances from the sun

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984rpesc...2..135l&link_type=abstract

In its USSR Rept.: Earth Sci. (JPRS-UES-84-007) p 135 (SEE N85-15196 06-42) Transl. into ENGLISH from Geomagetizm i Aeronomiya

Astronomy and Astrophysics

Astronomy

Plasma Dynamics, Solar Activity Effects, Solar Wind Velocity, Magnetohydrodynamic Waves, Radio Astronomy, Supersonic Flow

Scientific paper

The dynamics of the solar wind at distances from the Sun that are less than or approximately equal to 30 solar radii was investigated using the scintillation method. It is found that a change in the level of solar activity produces a change in the location of the region where the transition from the subsonic flow of circumsolar plasma to the supersonic solar wind flow occurs. The dynamics of the subsonic/supersonic transition is examined.

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