Abstract
Collisionless shocks undergo structural changes with the increase of Mach number. Observations and numerical simulations indicate development of time-dependent rippling. It is not known at present what causes the rippling. However, effects of such rippling on the field pattern and ion motion and distributions can be studied without precise knowledge of the causes and detailed shape. It is shown that deviations of the normal component of the magnetic field from the constant value indicate certain spatial dependence of the rippling. Deviations of the motional electric field from the constant value indicate time dependence. It is argued that whistler waves should propagate towards upstream and downstream regions from the rippled ramp. It is shown that the downstream pattern of the fields and ion distributions should follow the rippling pattern, while collisionless relaxation should be faster than in the stationary planar case.
Original language | English |
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Article number | 905880301 |
Journal | Journal of Plasma Physics |
Volume | 88 |
Issue number | 3 |
DOIs | |
State | Published - 10 Jun 2022 |
Keywords
- astrophysical plasmas
- space plasma physics
ASJC Scopus subject areas
- Condensed Matter Physics