CONVECTION DRIVEN MAGNETOHYDRODYNAMIC DYNAMOS IN ROTATING SPHERICAL-SHELLS

被引：96

作者：

ZHANG, KK ^{[1
]}

BUSSE, FH ^{[1
]}

机构：

[1] UNIV CALIF LOS ANGELES,INST GEOPHYS & PLANETARY PHYS,LOS ANGELES,CA 90024

来源：

GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS | 1989年 / 49卷 / 1-4期

关键词：

D O I：

10.1080/03091928908243466

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：97 / 116

页数：20

共 12 条

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[2]

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[3]

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[7] ON THE COMPUTATION OF STEADY, SELF-CONSISTENT SPHERICAL DYNAMOS [J].

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[8] DYNAMICALLY CONSISTENT NON-LINEAR DYNAMOS DRIVEN BY CONVECTION IN A ROTATING SPHERICAL-SHELL .2. DYNAMOS WITH CYCLES AND STRONG FEEDBACKS [J].

GILMAN, PA .

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[9] NUMERICAL SIMULATIONS OF STELLAR CONVECTIVE DYNAMOS .2. FIELD PROPAGATION IN THE CONVECTION ZONE [J].

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[10] KINEMATIC DYNAMO MODELS [J].

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