Abstract
The structure of a collisionless shock affects ion motion in the shock front and is affected by the formed ion distribution. In high-Mach-number shocks, a significant fraction of incident ions are reflected by the macroscopic electric and magnetic fields in the shock front. Ions are non-specularly reflected by the combined electric deceleration and magnetic deflection. Here, a first analytical description of the non-specular reflection is presented. The contribution of the increasing magnetic field is evaluated and shown to enhance reflection. The distribution of non-specularly reflected ions ahead of the ramp is calculated and their velocities at the re-entry to the shock are found numerically. Dependence on the angle between the shock normal and the upstream magnetic field vector is illustrated.
| Original language | American English |
|---|---|
| Article number | 905890505 |
| Journal | Journal of Plasma Physics |
| Volume | 89 |
| Issue number | 5 |
| DOIs | |
| State | Published - 18 Sep 2023 |
Keywords
- astrophysical plasmas
- plasma heating
- space plasma physics
All Science Journal Classification (ASJC) codes
- Condensed Matter Physics
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