Non-axisymmetric instabilities in magnetic spherical Couette flow

We investigate numerically the flow of an electrically conducting fluid confined in a spherical shell, with the outer sphere stationary, the inner sphere rotating and a magnetic field imposed parallel to the rotation axis. We compute both the axisymmetric basic states and their non-axisymmetric inst...

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Veröffentlicht in:Proceedings of the Royal Society. A, Mathematical and physical sciences Mathematical and physical sciences, 2009-07, Vol.465 (2107), p.2003-2013
1. Verfasser: Hollerbach, Rainer
Format: Artikel
Sprache:eng
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Zusammenfassung:We investigate numerically the flow of an electrically conducting fluid confined in a spherical shell, with the outer sphere stationary, the inner sphere rotating and a magnetic field imposed parallel to the rotation axis. We compute both the axisymmetric basic states and their non-axisymmetric instabilities. Two distinct instability classes emerge, one connected to previous non-magnetic results, the other to previous strongly magnetic results. Both instabilities arise from the basic state's meridional circulation, but are otherwise very different from one another, and are separated by a region of stability that persists even for large Reynolds numbers. Finally, we compute the fully three-dimensional nonlinear equilibration of both instabilities. The second class exhibits a rich variety of secondary bifurcations, involving mode transitions between different azimuthal wave numbers.
ISSN:1364-5021
0962-8444
1471-2946
DOI:10.1098/rspa.2009.0004