Modeling of unsteady processes in the solar wind

Details Modeling of unsteady processes in the solar wind Modeling of unsteady processes in the solar wind

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21..968v&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 21, Nov.-Dec. 1981, p. 968-972. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Collisionless Plasmas, Magnetohydrodynamic Flow, Solar Wind, Unsteady Flow, Pioneer Space Probes, Plasma Density, Plasma Temperature, Supersonic Flow, Temporal Distribution

Scientific paper

The paper considers a collisionless model of the unsteady solar wind, with allowance for the supersonic character of the flow. A zero small-parameter approximation (the small parameter being the inverse of the Mach number) is used to qualitatively describe the evolution of unsteady disturbances. This approximation takes into account the basic factor of the evolution: the supersonic radial expansion of the plasma. The model is applied to Pioneer-11 data on solar-wind velocity, density, and temperature.

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