Propagation of energetic electron streams in solar flares

Details Propagation of energetic electron streams in solar flares Propagation of energetic electron streams in solar flares

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...95..181m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 95, Jan. 1985, p. 181-188. NASA-supported research.

Physics

3

Coronal Loops, High Energy Electrons, Particle Motion, Solar Electrons, Solar Flares, Electron Scattering, Magnetohydrodynamic Stability, Photosphere, Plasma Waves, Propagation Modes

Scientific paper

The microscopic stability of an electron stream flowing down to the photosphere from the corona is examined. It is found that, while a power-law distribution is stable in the low-density corona, it is unstable against the generation of magnetized electron plasma waves in the high-density photosphere. The scattering of these energetic electrons may alter their radiation signatures.

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