VISCOSITY IN THE SOLAR-WIND

被引：16

作者：

HOLZER, TE

LEER, E

ZHAO, XP

机构：

[1] UNIV TROMSO,INST MATH & PHYS SCI,AURORAL OBSERV,N-9001 TROMSO,NORWAY

[2] BEIJING UNIV,DEPT GEOPHYS,BEIJING,PEOPLES R CHINA

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1986年 / 91卷 / A4期

关键词：

D O I：

10.1029/JA091iA04p04126

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：4126 / 4132

页数：7

共 25 条

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[4] PAPER BY LEER,E AND HOLZER,TE COLLISIONLESS SOLAR-WIND PROTONS - COMPARISON OF KINETIC AND HYDRODYNAMIC DESCRIPTIONS - COMMENTS [J].

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[5] AN ALTERNATIVE DERIVATION OF THE PARALLEL ION VISCOSITY [J].

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[8] THEORY OF STELLAR WINDS AND RELATED FLOWS [J].

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AXFORD, WI .

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1970, 8 :31-&

[9] COLLISIONLESS SOLAR-WIND PROTONS - COMPARISON OF KINETIC AND HYDRODYNAMIC DESCRIPTIONS - REPLY [J].

HOLZER, TE ;

LEER, E .

JOURNAL OF GEOPHYSICAL RESEARCH, 1973, 78 (16) :3199-3201

[10]

LEER E, 1982, SPACE SCI REV, V33, P161, DOI 10.1007/BF00213253

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