A numerical simulation of impulsive growth and sudden disruption of a thin current sheet due to inward boundary flows in a collisionless plasma, governed by the equations of Hall magnetohydrodynamics, is presented. After a period of slow growth followed by a much shorter period of impulsive enhancement, the thin current sheet becomes unstable to secondary tearing instabilities which produce multiple islands. These secondary islands coalesce to form a large plasmoid. Much of the thin current sheet disrupts rapidly to produce magnetic turbulence in less than a characteristic Alfven time. Possible implications for magnetotail substorms are discussed.
|Original language||English (US)|
|Number of pages||4|
|Journal||Geophysical Research Letters|
|State||Published - Nov 15 1999|
All Science Journal Classification (ASJC) codes
- Earth and Planetary Sciences(all)