RELATION BETWEEN SOLAR-WIND STRUCTURE AND SOLAR-WIND ROTATIONAL AND TANGENTIAL DISCONTINUITIES

被引：10

作者：

TURNER, JM ^{[1
]}

机构：

[1] MIT, CTR SPACE RES, CAMBRIDGE, MA 02139 USA

来源：

JOURNAL OF GEOPHYSICAL RESEARCH | 1973年 / 78卷 / 01期

关键词：

D O I：

10.1029/JA078i001p00059

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：59 / 70

页数：12

共 9 条

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[3] LARGE-AMPLITUDE ALFVEN WAVES IN INTERPLANETARY MEDIUM .2. [J].

BELCHER, JW ;

DAVIS, L .

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[4] SIMULTANEOUS PLASMA AND MAGNETIC-FIELD MEASUREMENTS OF PROBABLE TANGENTIAL DISCONTINUITIES IN SOLAR WIND [J].

SISCOE, GL ;

TURNER, JM ;

LAZARUS, AJ .

SOLAR PHYSICS, 1969, 6 (03) :456-&

[5] AN EAST-WEST ASYMMETRY IN SOLAR WIND VELOCITY [J].

SISCOE, GL ;

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LAZARUS, AJ .

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[6] SIGNIFICANCE CRITERIA FOR VARIANCE MATRIX APPLICATIONS [J].

SISCOE, GL ;

SUEY, RW .

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[7]

SISCOE GL, 1969, SOL PHYS, V6, P415

[8] ORIENTATIONS OF ROTATIONAL AND TANGENTIAL DISCONTINUITIES IN SOLAR WIND [J].

TURNER, JM ;

SISCOE, GL .

JOURNAL OF GEOPHYSICAL RESEARCH, 1971, 76 (07) :1816-+

[9]

TURNER JM, 1971, CSRP7159 REP

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