Kinetic processes in solar flares

Details Kinetic processes in solar flares Kinetic processes in solar flares

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....68..145n&link_type=abstract

Astronomy and Astrophysics, vol. 68, no. 1-2, Aug. 1978, p. 145-155. Research supported by the Miller Foundation and CECAM.

Astronomy and Astrophysics

Astrophysics

35

Electrical Resistivity, Magnetohydrodynamic Stability, Particle Acceleration, Plasma Turbulence, Solar Flares, Dynamic Models, Electric Current, Magnetic Fields, Particle Beams

Scientific paper

Various microscopic processes for the triggering and spreading of anomalous resistivity in the solar-flare flash phase are discussed. Among these processes are low-frequency current-driven instabilities, wave filamentation, and high-frequency parametric instabilities driven by particle beams. The role of these processes in producing runaway and statistical acceleration is discussed. A possible observational test of the state of plasma turbulence in the flare volume is suggested.

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