Wave growth in an oscillating model of pulsar magnetospheres

被引：0
|
作者：
Verdon, M. W. [1 ]
Melrose, D. B. [1 ]
机构：
[1] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia
来源：
40 YEARS OF PULSARS: MILLISECOND PULSARS, MAGNETARS AND MORE | 2007年 / 983卷
关键词：
pulsars : electrodynamics; radiation mechanisms;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The pulsar radio emission mechanism has yet to be identified unambiguously. The counter-strearning instability is a possible wave growth mechanism, but the growth rate in conventional models is too low. Here we argue that the growth rate in an oscillating model of the pulsar magnetosphere is much higher than in conventional models, and might account for the observed emission.
引用
收藏
页码：133 / 135
页数：3
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