ALIGNED ROTATING MAGNETOSPHERES .1. GENERAL ANALYSIS

被引：148

作者：

SCHARLEMANN, ET

WAGONER, RV

机构：

[1] CORNELL UNIV, DEPT ASTRON, ITHACA, NY 14850 USA

[2] LAWRENCE LIVERMORE LAB, LIVERMORE, CA USA

[3] CORNELL UNIV, CTR RADIOPHYS & SPACE RES, ITHACA, NY 14850 USA

来源：

关键词：

D O I：

10.1086/152195

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：951 / 960

页数：10

共 12 条

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[3] PULSAR ELECTRODYNAMICS
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JULIAN, WH
[J]. ASTROPHYSICAL JOURNAL, 1969, 157 (2P1) : 869 - +
[4] Goldreich P., 1972, Comments on Astrophysics and Space Physics, V4, P23
[5] GOLDREICH P, 1971, COMMENTS ASTROPHYS S, V3, P185
[6] PULSAR MAGNETOSPHERE
MESTEL, L
[J]. NATURE-PHYSICAL SCIENCE, 1971, 233 (43): : 149 - &
[7] ROTATING MAGNETOSPHERE - SIMPLE RELATIVISTIC MODEL
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[8] ARE QUASI-STELLAR RADIO SOURCES GIANT PULSARS
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[J]. ASTROPHYSICAL JOURNAL, 1969, 157 (2P2) : L73 - &
[9] MORSE PM, 1953, METHODS THEORETICAL, pCH5
[10] MORSE PM, 1953, METHODS THEORETICAL, pCH6