SOLAR WIND STRUCTURE DETERMINED BY COROTATING CORONAL INHOMOGENEITIES .1. VELOCITY-DRIVEN PERTURBATIONS

被引：35

作者：

SISCOE, GL

FINLEY, LT

机构：

来源：

JOURNAL OF GEOPHYSICAL RESEARCH | 1970年 / 75卷 / 10期

关键词：

D O I：

10.1029/JA075i010p01817

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

引用

页码：1817 / +

页数：1

共 19 条

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[3]

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[6]

LYON E, 1968, SPACE RES 8

[7] MARINER 2 OBSERVATIONS OF SOLAR WIND .I. AVERAGE PROPERTIES [J].

NEUGEBAUER, M ;

SNYDER, CW .

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[8] MARINER 2 OBSERVATIONS OF SOLAR WIND .2. RELATION OF PLASMA PROPERTIES TO MAGNETIC FIELD [J].

NEUGEBAUER, M ;

SNYDER, CW .

JOURNAL OF GEOPHYSICAL RESEARCH, 1967, 72 (07) :1823-+

[9] CONDUCTIVE HEATING OF SOLAR WIND .1. [J].

NOBLE, LM ;

SCARF, FL .

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[10]

OLBERT S, 1968, PHYSICS MAGNETOSPHER

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