Heat flux instabilities in the solar wind

Details Heat flux instabilities in the solar wind Heat flux instabilities in the solar wind

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jgr....80.4197g&link_type=abstract

Journal of Geophysical Research, vol. 80, Nov. 1, 1975, p. 4197-4203. ERDA-sponsored research.

Physics

29

Heat Flux, Magnetohydrodynamic Stability, Plasma Waves, Solar Flux, Solar Wind, Cosmic Plasma, Magnetoelastic Waves, Solar Electrons

Scientific paper

The linear dispersion properties of three electron heat flux plasma
instabilities are studied in detail by using parameters appropriate to
average values in the solar wind at 1 AU. Among the (fast) magnetosonic,
Alfven, and whistler instabilities the first one appears most likely to
make a significant contribution to the regulation of the heat flux.

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