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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 17, issue 10
Ann. Geophys., 17, 1251–1259, 1999
https://doi.org/10.1007/s00585-999-1251-6
© European Geosciences Union 1999
Ann. Geophys., 17, 1251–1259, 1999
https://doi.org/10.1007/s00585-999-1251-6
© European Geosciences Union 1999

  31 Oct 1999

31 Oct 1999

Collisionless electrons in a thin high Mach number shock: dependence on angle and b

M. Gedalin and E. Griv M. Gedalin and E. Griv
  • Department of Physics, Ben-Gurion University, Beer-Sheva, 84105 Israel

Abstract. It is widely believed that electron dynamics in the shock front is essentially collisionless and determined by the quasistationary magnetic and electric fields in the shock. In thick shocks the electron motion is adiabatic: the magnetic moment is conserved throughout the shock and v2^B. In very thin shocks with large cross-shock potential (the last feature is typical for shocks with strong electron heating), electrons may become demagnetized (the magnetic moment is no longer conserved) and their motion may become nonadiabatic. We consider the case of substantial demagnetization in the shock profile with the small-scale internal structure. The dependence of electron dynamics and downstream distributions on the angle between the shock normal and upstream magnetic field and on the upstream electron temperature is analyzed. We show that demagnetization becomes significantly stronger with the increase of obliquity (decrease of the angle) which is related to the more substantial influence of the inhomogeneous parallel electric field. We also show that the demagnetization is stronger for lower upstream electron temperatures and becomes less noticeable for higher temperatures, in agreement with observations. We also show that demagnetization results, in general, in non-gyrotropic down-stream distributions.

Key words. Interplanetary physics (interplanetary shocks; planetary bow shocks)

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