Electron parameter correlations in high-speed streams and heat flux instabilities

Details Electron parameter correlations in high-speed streams and heat flux instabilities Electron parameter correlations in high-speed streams and heat flux instabilities

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jgr....81.2377f&link_type=abstract

Journal of Geophysical Research, vol. 81, May 1, 1976, p. 2377-2382. ERDA-NASA-sponsored research.

Physics

11

Electron Flux Density, Heat Flux, Magnetohydrodynamic Stability, Solar Wind Velocity, Statistical Analysis, Anisotropy, Electron Energy, Proton Energy, Satellite Observation, Signature Analysis, Whistlers

Scientific paper

Statistical electron parameter correlations associated with high-speed streams are determined with the aim of identifying one or more locally active solar wind heat flux instabilities. Evidence that points toward local regulation of the heat flux at 1 AU is presented, and the results of a search for special signatures expected from the action of the Alfven, magnetosonic, and whistler flux instabilities are discussed. It is shown that under certain conditions, the whistler mode can be active in regulating the heat flux at 1 AU.

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