Colliding plasma structures: Current sheet and perpendicular shock
- 1 October 1988
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 93 (A10) , 11327-11340
- https://doi.org/10.1029/ja093ia10p11327
Abstract
We present results of a one‐dimensional simulation of the interaction of a current sheet and a supercritical perpendicular shock in a collisionless plasma. The low‐field region of the current sheet passes through the shock, allowing, for a short time, the complete reflection of the incident flow at the transition of the magnetic field to its downstream value. The counterstreaming ion beams relaunch the shock, while the low‐field region remains downstream. The plasma in the low field region is unshocked but develops a complex multistream configuration, which in time develops to a more uniform distribution. We discuss the implications of the simulation results for observations within the magnetosheath and of active current sheets upstream of the bow shock.Keywords
This publication has 34 references indexed in Scilit:
- The interaction of quasiperpendicular shock waves in a collisionless plasmaPhysics of Fluids, 1987
- Fast shocks at the edges of hot diamagnetic cavities upstream from the Earth's bow shockJournal of Geophysical Research, 1987
- A parametric survey of the first critical Mach number for a fast MHD shockJournal of Plasma Physics, 1984
- Electron velocity distributions near the Earth's bow shockJournal of Geophysical Research, 1983
- Energetic magnetosheath ions and the interplanetary magnetic field orientationJournal of Geophysical Research, 1981
- Fine‐scale characteristics of interplanetary sector boundariesJournal of Geophysical Research, 1981
- Structure of current sheets in magnetic holes at 1 AUJournal of Geophysical Research, 1978
- Interplanetary magnetic holes: TheoryJournal of Geophysical Research, 1978
- Average and unusual locations of the Earth's magnetopause and bow shockJournal of Geophysical Research, 1971
- Micro-scale structures in the interplanetary mediumSolar Physics, 1968