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• W1988486572 abstract "We examine kinematic dynamo action in an electrically conducting spherical body of fluid with an overlying shell of differential rotation. It is thought that such flow types could explain the nearly axisymmetric magnetic field of Saturn. Although we find that an outer layer of differential rotation can ‘axisymmetrize’ the exterior magnetic field, surprisingly, sometimes it does not, giving magnetic fields that have no axisymmetric ingredients." @default.
• W1988486572 created "2016-06-24" @default.
• W1988486572 creator A5065260177 @default.
• W1988486572 date "2000-09-15" @default.
• W1988486572 modified "2023-09-26" @default.
• W1988486572 title "Dynamo action and the nearly axisymmetric magnetic field of Saturn" @default.
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• W1988486572 doi "https://doi.org/10.1029/1999gl008466" @default.
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