Affiliation:
1. ETSI Industriales, Universidad de Castilla-La Mancha , E-13071 Ciudad Real, Spain
2. Instituto de Investigaciones Energéticas y Aplicaciones Industriales, Campus Universitario de Ciudad Real , E-13071 Ciudad Real, Spain
Abstract
ABSTRACTThe properties of collisionless shocks are frequently assessed in the magnetohydrodynamics (MHD) model. Yet, in a collisionless plasma, an ambient magnetic field can sustain a stable anisotropy in the upstream or the downstream, resulting in a departure from the MHD predicted behaviour. We present a model allowing to derive the downstream anisotropy, hence the shock density jump, in terms of the upstream quantities. For simplicity, the case of a parallel shock in pair plasma is considered. Contrary to previous works where the upstream was assumed isotropic, here the upstream anisotropy A = T⊥/T∥ is a free parameter. The strong sonic shock regime is formally identical to the isotropic upstream case. Yet, for intermediate sonic Mach numbers, a variety of behaviours appear as a result of the anisotropy of the upstream.
Funder
Ministerio de Economía y Competitividad
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
2 articles.
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