Electron scattering on small-scale electrostatic fields in the shock front

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Abstract

Electron heating and acceleration in collisionless shocks is a long-standing problem. Rapid isotropization of heated electrons cannot be explained solely by the cross-shock potential. In addition, the macroscopic cross-shock potential prevents efficient reflection and injection into the diffusive acceleration regime. Recent observations have shown that small-scale electric fields are present in the shock front, together with the large-scale cross-shock potential. These small-scale fields have been found also in the upstream and downstream regions. Electron heating in shocks is produced by the combined action of the large- and small-scale fields. The large-scale potential determines the energy transferred to the electrons. The small-scale electrostatic fields scatter electrons. Here we study the scattering of electrons on the typical waveforms, namely solitary bipolar spikes and wavepackets. The main effect is the generation of backstreaming electrons with large pitch angles. It is found that wavepackets are more efficient in electron reflection in the interaction of electrons both with a single spike and with multiple spikes.

Original languageAmerican English
Article number905900509
JournalJournal of Plasma Physics
Volume90
Issue number5
DOIs
StatePublished - 25 Oct 2024

Keywords

  • astrophysical plasmas
  • space plasma physics

All Science Journal Classification (ASJC) codes

  • Condensed Matter Physics

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