Formation of non-thermal, high energy particles in relativistic magnetosonic shock waves

被引：2

作者：

Hoshino, M ^{[1
]}

Lembege, B ^{[1
]}

机构：

[1] CTR ETUD ENVIRONM TERR & PLANETAIRES,F-92131 ISSY MOULINEAUX,FRANCE

来源：

PHYSICS OF COLLISIONLESS SHOCKS | 1995年 / 15卷 / 8-9期

关键词：

D O I：

10.1016/0273-1177(94)00086-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：

We study the kinetic nature of the relativistic, perpendicular shocks in electron-ion plasmas and discuss the origin of non-thermal high energy particles, using the full particle simulation code including the relativistic Lorentz equation. We find that the electron can be accelerated up to the upstream ion kinetic energy in the form of non-thermal high energy tail.

引用

页码：67 / 70

页数：4

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