Density jump as a function of magnetic field strength for parallel collisionless shocks with anisotropic upstream pressure

ABSTRACT The 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...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2023-02, Vol.520 (4), p.6083-6090
Main Author: Bret, Antoine
Format: Article
Language:English
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Summary:ABSTRACT The 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.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stad527