Stochastic and quasi-adiabatic electron heating in quasi-parallel shocks

Krzysztof Stasiewicz, Bengt Eliasson

Research output: Contribution to journalArticlepeer-review

3 Citations (Scopus)

Abstract

Using Magnetospheric Multiscale observations at the Earth's quasi-parallel bow shock we demonstrate that electrons are heated by two different mechanisms: A quasi-adiabatic heating process during magnetic field compression, characterized by the isotropic temperature relation with = 2/3 when the electron heating function and a stochastic heating process when Both processes are controlled by the value of the stochastic heating function for particles with mass m j and charge q j in the electric and magnetic fields. Test-particle simulations are used to show that the stochastic electron heating and acceleration in the studied shock are accomplished by waves at frequencies (0.4-5) f ce (electron gyrofrequency) for bulk heating, and waves for acceleration of the tail of the distribution function. Stochastic heating can give rise to flat-top electron distribution functions, frequently observed near shocks. It is also shown that obliquely polarized electric fields of electron cyclotron drift and ion acoustic instabilities scatter the electrons into the parallel direction and keep the isotropy of the electron distribution. The results reported in this paper may be relevant to electron heating and acceleration at interplanetary shocks and other astrophysical shocks.

Original languageEnglish
Article number173
JournalAstrophysical Journal
Volume904
Issue number2
DOIs
Publication statusPublished - 2 Dec 2020

Keywords

  • electron heating
  • quasi-parallel shocks

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