Abstract
Field-aligned and gyrophase bunched ion beams are observed in the foreshock of the Earth bow shock. One of the mechanisms proposed for their production is non-specular reflection at the shock front. We study the distributions which are formed at the stationary quasi-perpendicular shock front within the same process which is responsible for the generation of reflected ions and transmitted gyrating ions. The test particle motion analysis in a model shock allows one to identify the parameters which control the efficiency of the process and the features of the escaping ion distribution. These parameters are: the angle between the shock normal and the upstream magnetic field, the ratio of the ion thermal velocity to the flow velocity upstream, and the cross-shock potential. A typical distribution of escaping ions exhibits a bimodal pitch angle distribution (in the plasma rest frame).
Original language | English |
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Article number | A05101 |
Journal | Journal of Geophysical Research: Space Physics |
Volume | 113 |
Issue number | 5 |
DOIs | |
State | Published - 1 May 2008 |
ASJC Scopus subject areas
- Geophysics
- Space and Planetary Science