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- W2314473022 abstract "We describe a nonlinear, axisymmetric, spherical-shell model of a planetary dynamo. This intermediate-type dynamo model requires a prescribed helicity field (the alpha effect) and a prescribed buoyancy force or thermal wind (the omega effect) and solves for the axisymmetric time-dependent magnetic and velocity fields. Three very different time dependent solutions are obtained from different prescribed sets of alpha and omega fields." @default.
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- W2314473022 date "1993-01-01" @default.
- W2314473022 modified "2023-10-14" @default.
- W2314473022 title "Intermediate Dynamo Models" @default.
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- W2314473022 doi "https://doi.org/10.5636/jgg.45.1605" @default.
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