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- W4237488568 abstract "The problem of preferential excitation of non-axially symmetric magnetic fields in most of the observed spiral galaxies and in planets as Uranus and Neptune is studied. It is suggested that a dynamo acting in a thin conductive shell is possible in these objects. It is shown that in this thin shell axisymmetric and non-axisymmetric magnetic field modes can be excited with equal efficiency. The preferential excitation of non-axially symmetric magnetic fields is possible, when the gradient of the angular velocity of rotation is comparatively small and has an essential component perpendicular to the shell." @default.
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- W4237488568 date "1993-01-01" @default.
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- W4237488568 title "Non-Axisymmetric Magnetic Structure Generation in Planets Sun and Galaxies" @default.
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- W4237488568 doi "https://doi.org/10.1017/s007418090017425x" @default.
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