English

Electron heating at quasi-perpendicular collisionless shocks

Space Physics 2024-02-27 v1

Abstract

Adiabatic and non-adiabatic electron dynamics have been proposed to explain electron heating across collisionless shocks. We analyze the evolution of the suprathermal electrons across 310 quasi-perpendicular shocks with 1.7<MA<481.7<M_A<48 using in-situ measurements. We show that the electron heating mechanism shifts from predominantly adiabatic to non-adiabatic for the Alfv\'enic Mach number in the de Hoffman-Teller 30\gtrsim 30 with the latter constituting 48\% of the analyzed shocks. The observed non-adiabatic heating is consistent with the stochastic shock drift acceleration mechanism.

Keywords

Cite

@article{arxiv.2402.16564,
  title  = {Electron heating at quasi-perpendicular collisionless shocks},
  author = {Ahmad Lalti and Yuri V. Khotyaintsev and Daniel B. Graham},
  journal= {arXiv preprint arXiv:2402.16564},
  year   = {2024}
}
R2 v1 2026-06-28T15:00:17.885Z