EGU24-17436, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-17436
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Electron heating at quasi-perpendicular collisionless shocks: adiabatic vs non-adiabatic 

Ahmad Lalti1,2, Yuri V. Khotyaintsev1, and Daniel B. Graham1
Ahmad Lalti et al.
  • 1Swedish Institute of Space Physics, Sweden (ahmadl@irfu.se)
  • 2Department of Physics and Astronomy, Space and Plasma Physics, Uppsala University, Sweden

The mechanism of electron heating across collisionless shocks remains an open question. The mechanisms suggested to address this problem revolve around the adiabatic or the non-adiabatic\stochastic dynamics of electrons across the shock. In this letter, we analyze the evolution of the electron velocity distribution function observed across 313 shocks with 1.7<MA<48. We use a Liouville mapping technique to show that the electron heating mechanism shifts from predominantly adiabatic to predominantly non-adiabatic as the Alfvenic Mach number in the de Hoffmann-Teller frame increases. We also show that for shocks with non-adiabatic heating of electrons, the heating mechanism is consistent with the stochastic shock drift acceleration (SSDA) mechanism.

How to cite: Lalti, A., Khotyaintsev, Y. V., and Graham, D. B.: Electron heating at quasi-perpendicular collisionless shocks: adiabatic vs non-adiabatic , EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-17436, https://doi.org/10.5194/egusphere-egu24-17436, 2024.

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