Plasma field aspects of the solar wind

Details Plasma field aspects of the solar wind Plasma field aspects of the solar wind

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...26..277c&link_type=abstract

Space Science Reviews, vol. 26, July 1980, p. 277-315.

Physics

9

Dynamic Models, Magnetohydrodynamic Flow, Mathematical Models, Plasma Dynamics, Solar Wind, Density Distribution, Plasma Acceleration, Plasma Density, Radial Flow, Solar Corona, Solar Physics, Thermal Conductivity

Scientific paper

It is noted that while significant progress in the description and understanding of the solar wind has been achieved with fluid models, there is, so far, no general model capable of providing a mathematical solution for the overall solar wind phenomenon. Existing plasma fluid models for the solar wind are presented, including a general characterization and illustration of the capabilities of various models. Insight into fundamental physical processes is provided in such a manner. In conclusion, a sound basis is provided for further physical study of magnetohydrodynamic and/or transient phenomena.

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