Physics
Scientific paper
Jun 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..139..343z&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 139, no. 2, June 1992, p. 343-356.
Physics
37
Chromosphere, Ionic Collisions, Lorentz Force, Ohms Law, Solar Flares, Electric Current, Magnetic Flux, Magnetohydrodynamic Waves, Solar Prominences, Wave Propagation
Scientific paper
The coalescence of a flare loop and a filament is presently used to illustrate magnetic-loop reemergence and the correct application of the generalized form of Ohm's law for solar flares. Flare energy release entails large current values, a nonsteady-state process, and the existence of a neutral component in a flare plasma. Current dissipation furnishes effective Joule heating of the plasma and particle acceleration in a solar flare. Due to the decisive role played in the energy release process by ion-atom collisions, flare loop resistance can grow by 8-10 orders of magnitude. The energy release from the upper part of a flare loop stimulates powerful energy release from the chromospheric level.
Stepanov Alexander V.
Zaitsev Valerii V.
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