FILAMENTATION INSTABILITY OF INTERACTING CURRENT SHEETS IN STRIPED RELATIVISTIC WINDS: THE ORIGIN OF LOW SIGMA?

被引：8

作者：

Arons, Jonathan ^{[1
,2
]}

机构：

[1] Univ Calif Berkeley, Dept Phys, Dept Astron, Berkeley, CA 94720 USA

[2] Univ Calif Berkeley, Theoret Astrophys Ctr, Berkeley, CA 94720 USA

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2008年 / 17卷 / 09期

关键词：

Pulsar winds; current sheets;

D O I：

10.1142/S0218271808012991

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

I outline a mechanism, akin to Weibel instabilities of interpenetrating beams, in which the neighboring current sheets in a striped wind from an oblique rotator interact through a two stream-like mechanism (a Weibel instability in flatland), to create an anomalous resistivity that heats the sheets and causes the magnetic field to diffusively annihilate in the wind upstream of the termination shock. The heating has consequences for observable unpulsed emission from pulsars.

引用

页码：1419 / 1430

页数：12

共 34 条

[1]

ARONS J, 2008, SPRINGER LE IN PRESS

[2]

ARONS J, 2008, ASTROPHYS J UNPUB

[3]

Arons J., 1983, P WORKSHOP ELECTRON, P163

[4] A model for the moving "wisps" in the Crab Nebula [J].