On the non-linear mirror instability

被引:24
作者
Pantellini, FGE
Burgess, D
Schwartz, SJ
机构
[1] Astronomy Unit, Queen Mary and Westfield College, London, E1 4NS, Mile End Road
来源
PHYSICS OF COLLISIONLESS SHOCKS | 1995年 / 15卷 / 8-9期
关键词
D O I
10.1016/0273-1177(94)00114-G
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
It is argued that quasi-linear theory alone does not provide an adequate description of the non linear evolution of the mirror instability. Based on a simplified model for the motion of particles in a mirror wave, it is found that the main mechanism which ends the linear phase of the instability has to be particle trapping. Quasi-linear effects may still play a role for particles with small velocities perpendicular to the background magnetic field and do probably dominate the late stage of the instability when the wave-particle energy exchange associated with particle trapping becomes inefficient.
引用
收藏
页码:341 / 344
页数:4
相关论文
共 5 条
[1]  
NORTHROP TG, 1963, ADIABATIC MOTION CHA, P12
[2]  
PANTELLINI FGE, 1994, UNPUB J GEOPHYS RES
[3]   GENERAL CRITERION FOR MIRROR INSTABILITY OF A PLASMA [J].
ROSE, DJ .
PHYSICS OF FLUIDS, 1965, 8 (05) :951-&
[4]  
SHAPIRO VD, 1964, SOV PHYS JETP-USSR, V18, P1109
[5]   MIRROR INSTABILITY .1. PHYSICAL-MECHANISM OF LINEAR INSTABILITY [J].
SOUTHWOOD, DJ ;
KIVELSON, MG .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1993, 98 (A6) :9181-9187