Dynamics of double layers, ion acceleration and heat flux suppression during solar flares
T. C. Li, J. F. Drake, M. Swisdak

TL;DR
This study uses large-scale PIC simulations to investigate how multiple double layers in the solar corona influence electron confinement, ion acceleration, and heat flux suppression during solar flares, providing insights into solar wind formation.
Contribution
It reveals the dynamics of multiple double layers in larger systems, showing their role in electron confinement and ion acceleration, which was not previously understood in smaller-scale models.
Findings
Multiple double layers generate high-velocity electron beams.
Double layers trap electrons, suppressing transport.
Ion acceleration occurs over extended regions.
Abstract
Observations of flare-heated electrons in the corona typically suggest confinement of electrons. The confinement mechanism, however, remains unclear. The transport of coronal hot electrons into ambient plasma was recently investigated by particle-in-cell (PIC) simulations. Electron transport was significantly suppressed by the formation of a highly localized, nonlinear electrostatic electric potential in the form of a double layer (DL). In this work large-scale PIC simulations are performed to explore the dynamics of DLs in larger systems where, instead of a single DL, multiple DLs are generated. The primary DL accelerates return current electrons, resulting in high velocity electron beams that interact with ambient ions. This forms a Buneman unstable system that spawns more DLs. Trapping of heated return current electrons between multiple DLs strongly suppresses electron transport. DLs…
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