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- W44963996 abstract "The preferred structure of dynamo-generated magnetic fields is calculated for a sample of 17 galaxy models. The models are assumed to be axisymmetric in their non-magnetic properties. It is found that the preferred large-scale magnetic fields are of S0-type, i.e. have the symmetry of an axisymmetric quadrupole. Only in two cases, where the alpha-effect is restricted to the rigidly rotating inner part of the galaxy and the differential rotation is rather small, are A0-fields (dipole symmetry) preferred. We do not find non-axisymmetric magnetic fields to be preferred in any example" @default.
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- W44963996 date "1992-09-01" @default.
- W44963996 modified "2023-09-26" @default.
- W44963996 title "Galactic dynamos and their radio signatures" @default.
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