SCALE AND STRENGTH OF GALACTIC MAGNETIC-FIELD ACCORDING TO PULSAR DATA

被引：13

作者：

RUZMAIKIN, AA ^{[1
]}

SOKOLOFF, DD ^{[1
]}

机构：

[1] MV LOMONOSOV STATE UNIV,MOSCOW 117234,USSR

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1977年 / 52卷 / 02期

关键词：

D O I：

10.1007/BF01093873

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：365 / 374

页数：10

共 20 条

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[5] FARADAY ROTATION, DISPERSION IN PULSAR SIGNALS, AND TURBULENT STRUCTURE OF GALAXY [J].

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[7]

KUZNETSOVA IP, 1976, ASTRON ZH+, V53, P475

[8] PULSAR ROTATION AND DISPERSION MEASURES AND GALACTIC MAGNETIC-FIELD [J].

MANCHESTER, RN .

ASTROPHYSICAL JOURNAL, 1972, 172 (01) :43-+

[9] STRUCTURE OF LOCAL GALACTIC MAGNETIC-FIELD [J].

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[10]

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