The role of plasma turbulence in the development of solar flares

Details The role of plasma turbulence in the development of solar flares The role of plasma turbulence in the development of solar flares

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...47...79k&link_type=abstract

(NASA, IAU, IUGG, and International Council of Scientific Unions, Workshop on Flare Build-up Study, Falmouth, Mass., Sept. 8-11,

Physics

24

Magnetohydrodynamic Stability, Plasma Turbulence, Solar Activity Effects, Solar Flares, Electrical Resistivity, Magnetic Field Configurations, Particle Acceleration, Plasma Conductivity, Solar Physics

Scientific paper

The amount of energy released during a solar flare and the relatively short time scale in which all the flare-associated events occur lead to the conclusion that a solar flare is a magnetohydrodynamic instability taking place in a strongly turbulent plasma. The main effect of plasma turbulence is a strong reduction of the electrical conductivity, resulting in rapid heating and expansion of the flare plasma. The acceleration of particles during these processes can be understood with present-day knowledge of nonlinear plasma physics. The advantages of a supertwisted flux tube as a model field configuration for a solar flare are discussed.

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