On the Role of Separatrix Instabilities in Heating the Reconnection Outflow Region
arXiv:1808.09849 · doi:10.1063/1.5054100
Abstract
A study of the role of microinstabilities at the reconnection separatrix can play in heating the electrons during the transition from inflow to outflow is being presented. We find that very strong flow shears at the separatrix layer lead to counterstreaming electron distributions in the region around the separatrix, which become unstable to a beam-type instability. Similar to what has been seen in earlier research, the ensuing instability leads to the formation of propagating electrostatic solitons. We show here that this region of strong electrostatic turbulence is the predominant electron heating site when transiting from inflow to outflow. The heating is the result of heating generated by electrostatic turbulence driven by overlapping beams, and its macroscopic effect is a quasi-viscous contribution to the overall electron energy balance. We suggest that instabilities at the separatrix can play a key role in the overall electron energy balance in magnetic reconnection.
References in corpus (4)
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- Width-amplitude relation of Bernstein-Greene-Kruskal solitary waves
- The Physical Foundation of the Reconnection Electric Field
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Cited by in corpus (8)
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- Wave emission of non-thermal electron beams generated by magnetic reconnection
- The dynamics of electron holes in current sheets
- Nonthermal electron velocity distribution functions due to 3D kinetic magnetic reconnection for solar coronal plasma conditions
- Role of ion acoustic instability in magnetic reconnection