CONVECTION IN PRESENCE OF MAGNETIC-FIELDS

被引：16

作者：

PECKOVER, RS

WEISS, NO

机构：

[1] UNITED KINGDOM ATOM ENERGY AUTHOR,CULHAM LAB,ABINGDON,BERKSHIRE,ENGLAND

[2] UNIV CAMBRIDGE,DEPT APPL MATH & THEORET PHYS,CAMBRIDGE,ENGLAND

来源：

COMPUTER PHYSICS COMMUNICATIONS | 1972年 / 4卷 / 03期

关键词：

D O I：

10.1016/0010-4655(72)90095-1

中图分类号：

TP39 [计算机的应用];

学科分类号：

081203 ; 0835 ;

摘要：

引用

页码：339 / 344

页数：6

共 23 条

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[13] INFLUENCE OF A POLOIDAL MAGNETIC FIELD ON CONVECTION IN SPHERICAL SHELLS [J].

MOSS, DL ;

TAYLER, RJ .

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[14] A NUMERICAL MODEL OF HYDROMAGNETIC TURBULENCE [J].

MOSS, DL .

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[15] KINEMATICAL HYDROMAGNETIC THEORY AND ITS APPLICATION TO LOW SOLAR PHOTOSPHERE [J].

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[16]

PECKOVER RS, 1971, THESIS U CAMBRIDGE

[17]

THOMPSON WB, 1951, PHILOS MAG, V42, P1417

[18] MAGNETIC FLUX TUBES AND CONVECTION IN THE SUN [J].

WEISS, NO .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1964, 128 (03) :225-235

[19] EXPULSION OF MAGNETIC FLUX BY EDDIES [J].

WEISS, NO .

PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1966, 293 (1434) :310-+

[20]

WEISS NO, 1971, QUART J ROY ASTRON S, V12, P572

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