Kinetic theory of weak disturbances in the solar wind

Details Kinetic theory of weak disturbances in the solar wind Kinetic theory of weak disturbances in the solar wind

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..769v&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 20, Sept.-Oct. 1980, p. 769-776. In Russian.

Physics

1

Kinetic Theory, Plasma Oscillations, Solar Wind, Boundary Value Problems, Collisionless Plasmas, Heat Flux, Ion Distribution

Scientific paper

Unsteady processes in the solar wind are studied on the basis of a kinetic description of the plasma in the collisionless neutral-gas approximation. The boundary value problem is solved and the ion distribution function is determined for spherically symmetric disturbances. Density, velocity, and temperature disturbances are analyzed; and the heat flux transferred by ions is studied.

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