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Convective dynamos in spherical wedge geometry

ASTRONOMISCHE NACHRICHTEN, no. 1 (2010): 73-81

Cited: 65|Views27

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Sun: magnetic fieldsmagnetohydrodynamics (MHD)

Abstract

Self-consistent convective dynamo simulations in wedge-shaped spherical shells are presented. Differential rotation is generated by the interaction of convection with rotation. Equatorward acceleration and dynamo action are obtained only for sufficiently rapid rotation. The angular velocity tends to be constant along cylinders. Oscillator...More

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