Transfer of Energy, Potential, and Current by Alfvén Waves in Solar Flares
arXiv:1304.1938 · doi:10.1007/s11207-013-0305-9
Abstract
Alfvén waves play three related roles in the impulsive phase of a solar flare: they transport energy from a generator region to an acceleration region; they map the cross-field potential (associated with the driven energy release) from the generator region onto the acceleration region; and within the acceleration region they damp by setting up a parallel electric field that accelerates electrons and transfers the wave energy to them. The Alfvén waves may also be regarded as setting up new closed current loops, with field-aligned currents that close across field lines at boundaries. A model is developed for large-amplitude Alfvén waves that shows how Alfvén waves play these roles in solar flares. A picket-fence structure for the current flow is incorporated into the model to account for the "number problem" and the energy of the accelerated electrons.
References in corpus (3)
Cited by in corpus (6)
- Is Cyclotron Maser Emission in Solar Flares Driven by a Horseshoe Distribution?
- Current-driven flare and CME models
- Bulk Energization of Electrons in Solar Flares by Alfvén Waves
- Plasma acceleration by the interaction of parallel propagating Alfvén waves
- Photospheric response to a flare
- Rethinking the solar flare paradigm