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Magnetoconvection and dynamo coefficients: II. Field-direction dependent pumping of magnetic field

ASTRONOMY & ASTROPHYSICS, no. 2 (2002): 735-745

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We study the pumping of magnetic flux in three-dimensional compressible magnetoconvection in the context of stellar dynamos. The simulation domain represents a rectangular section from the lower part of a stellar convection zone plus the underlying stably stratified layer, with a total depth of up to five pressure scale heights. Once conv...更多

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