Convection-driven quadrupolar dynamos in rotating spherical shells.
It is found that for Taylor numbers of the order 10(8) quadrupolar dynamos aligned with the axis of rotation are preferred in comparison with dipolar dynamos. This preference holds for a range of Prandtl numbers P and magnetic Prandtl numbers P(m) in the neighborhood of unity. The main time-dependent feature of the quadrupolar dynamos are polward traveling waves.
Grote
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Institute of Physics, University of Bayreuth, D-95440 Bayreuth, Germany.
Busse
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FH
Tilgner
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