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• W2890318636 abstract "To understand why the magnetic fields of many planets are axial dipoles, the evolution in time of a seed magnetic field is studied using a dynamo model. The field is shown to excite helical convection, and the timescale for the growth in convection matches that for dipole formation." @default.
• W2890318636 created "2018-09-27" @default.
• W2890318636 creator A5051274935 @default.
• W2890318636 creator A5076274286 @default.
• W2890318636 date "2018-09-04" @default.
• W2890318636 modified "2023-10-17" @default.
• W2890318636 title "Scale dependence of kinetic helicity and selection of the axial dipole in rapidly rotating dynamos" @default.
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• W2890318636 doi "https://doi.org/10.1103/physrevfluids.3.093801" @default.
• W2890318636 hasPublicationYear "2018" @default.
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