ELECTRIC GAPS IN PULSAR MAGNETOSPHERES

被引：2
|
作者：
MESTEL, L
机构：
[1] Astronomy Centre, University of Sussex, Brighton, BN1 9QH, Falmer
来源：
SPACE SCIENCE REVIEWS | 1994年 / 68卷 / 1-4期
关键词：
D O I：
10.1007/BF00749162
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Two contrasting models of the magnetosphere are studied: a classical, quasi-mhd model, in which it is the component E(perpendicular-to) that accelerates electrons to relativistic energies; and a model with e+-e- production, in which the component E(parallel-to) is locally crucial, both in an acceleration domain near the star and in a dissipation domain beyond the light-cylinder.
引用
收藏
页码：337 / 348
页数：12
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