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Cremer & Scholer 1999
Cremer, M. and Scholer, M. (1999). Collisionless slow shocks in magnetotail reconnection. Geophysical Research Letters 26: doi: 10.1029/1999GL900592. issn: 0094-8276.

The kinetic structure of collisionless slow shocks in the magnetotail is studied by solving the Riemann problem of the collapse of a current sheet with a normal magnetic field component using 2-D hybrid simulations. The collapse results in a current layer with a hot isotropic distribution and backstreaming ions in a boundary layer. The lobe plasma outside and within the boundary layer exhibits a large perpendicular to parallel temperature anisotropy. Waves in both regions propagate parallel to the magnetic field. In a second experiment a spatially limited high density beam is injected into a low beta background plasma and the subsequent wave excitation is studied. A model for slow shocks bounding the reconnection layer in the magnetotail is proposed where backstreaming ions first excite obliquely propagating waves by the electromagnetic ion/ion cyclotron instability, which lead to perpendicular heating. The T/T temperature anisotropy subsequently excites parallel propagating Alfv¿n ion cyclotron waves, which are convected into the slow shock and are refracted in the downstream region. ¿ 1999 American Geophysical Union

BACKGROUND DATA FILES

Abstract

Keywords
Magnetospheric Physics, Magnetotail, Space Plasma Physics, Magnetic reconnection, Space Plasma Physics, Numerical simulation studies, Space Plasma Physics, Waves and instabilities
Journal
Geophysical Research Letters
http://www.agu.org/journals/gl/
Publisher
American Geophysical Union
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