Spherical dynamos with anisotropic α-effect
- 1 January 1979
- journal article
- research article
- Published by Taylor & Francis in Geophysical & Astrophysical Fluid Dynamics
- Vol. 14 (1) , 167-181
- https://doi.org/10.1080/03091927908244537
Abstract
The mean field induction equation of Steenbeck, Krause and Rädler (1966) is solved for anisotropic α ik -tensors of varying anisotropy. The attention is restricted to α2-dynamos in spheres with steady axisymmetric magnetic fields. The ratio of the electrical conductivity outside and inside the sphere is varied, but in all cases it is found that a steady dynamo does not exist when the anisotropy of the α ik -tensor exceeds a critical value. Such a critical value does not exist in the exceptional case of the Fermi boundary condition. The results emphasize the important effect of boundaries on the existence of solutions of the dynamo problem.Keywords
This publication has 12 references indexed in Scilit:
- On the α‐effect for slow and fast rotationAstronomische Nachrichten, 1978
- The role of mean circulation in parity selection by planetary magnetic fieldsGeophysical & Astrophysical Fluid Dynamics, 1977
- Generation of planetary magnetism by convectionPhysics of the Earth and Planetary Interiors, 1976
- A Model of the GeodynamoGeophysical Journal of the Royal Astronomical Society, 1975
- Kinematic dynamo modelsPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1972
- Zur Dynamotheorie stellarer und planetarer Magnetfelder I. Berechnung sonnenähnlicher WechselfeldgeneratorenAstronomische Nachrichten, 1969
- Zur Elektrodynamik turbulent bewegter leitender MedienZeitschrift für Naturforschung A, 1968
- Berechnung der mittleren Lorentz-Feldstärke für ein elektrisch leitendes Medium in turbulenter, durch Coriolis-Kräfte beeinflußter BewegungZeitschrift für Naturforschung A, 1966
- A class of self-sustaining dissipative spherical dynamosAnnals of Physics, 1958
- Hydromagnetic Dynamo Models.The Astrophysical Journal, 1955