Stability of the ordinary mode to an electron heat flux

Details Stability of the ordinary mode to an electron heat flux Stability of the ordinary mode to an electron heat flux

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...59..387l&link_type=abstract

Solar Physics, vol. 59, Oct. 1978, p. 387-393. Research supported by the U.S. Department of Energy.

Physics

Collisionless Plasmas, Heat Flux, Magnetohydrodynamic Stability, Solar Electrons, Solar Wind, Electron Distribution, Plasma Oscillations

Scientific paper

Stability equations for the low frequency ordinary mode propagating
perpendicular to a homogeneous magnetic field in the presence of a heat
flux in a collisionless plasma are derived by working within an
appropriate velocity reference frame. Solutions indicate the ordinary
mode is stable under average solar wind conditions at 1 AU.

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