Towards the circuit theory of solar flares

Physics

Scientific paper

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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.

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