Evolution of strong inhomogeneities in the solar-wind plasma

Details Evolution of strong inhomogeneities in the solar-wind plasma Evolution of strong inhomogeneities in the solar-wind plasma

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ge%26ae..18....3v&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 18, Jan.-Feb. 1978, p. 3-8.) Geomagnetism and Aeronomy, vol. 18, Aug. 1978, p. 1-4. Translatio

Physics

Cold Plasmas, Nonuniform Plasmas, Particle Motion, Solar Wind, Collisionless Plasmas, Flow Velocity, Plasma Density, Time Response

Scientific paper

The approximation of solar-wind plasma as a cold unmagnetized gas of noninteracting particles is used to analyze the evolution and properties of strong inhomogeneities of velocity and density in the solar wind. The main energy of the inhomogeneities is concentrated in the direction of proton motion; the electric fields are weak and have little effect on ion motion; the dynamics of such inhomogeneities is fully determined by ion motion; strong localized disturbances disperse in sufficiently long periods of time.

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