Physics of the inner heliosphere 1-1OR0 plasma diagnostics and models

Details Physics of the inner heliosphere 1-1OR0 plasma diagnostics and models Physics of the inner heliosphere 1-1OR0 plasma diagnostics and models

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sao..repts....w&link_type=abstract

Semiannual Progress Report, 1 May - 31 Oct. 1984 Smithsonian Astrophysical Observatory, Cambridge, MA.

Physics

Heliosphere, Plasma Diagnostics, Solar Atmosphere, Solar Corona, Solar Wind, Flow Velocity, Magnetohydrodynamic Flow, Plasma Acceleration, Plasma Heating, Plasma Temperature, Ultraviolet Radiation, Ultraviolet Spectra, Wave Propagation

Scientific paper

The physics of solar wind flow in the acceleration region and impulsive phenomena in the solar corona is studied. The study of magnetohydrodynamic wave propagation in the corona and the solutions for steady state and time dependent solar wind equations gives insights concerning the physics of the solar wind acceleration region, plasma heating and plasma acceleration processes and the formation of shocks. Also studied is the development of techniques for placing constraints on the mechanisms responsible for coronal heating.

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