On the saturation of non-axisymmetric instabilites of magnetized spherical Couette flow
arXiv:1402.5064 · doi:10.1103/PhysRevE.89.063016
Abstract
We numerically investigate the saturation of the hydromagnetic instabilities of a magnetized spherical Couette flow. Previous simulations [Hollerbach, 2009] demonstrated region where the axisymmetric flow, calculated from a 2-D simulation, was linearly unstable to nonaxisymmetric perturbations. Full, nonlinear, 3d simulations [Hollerbach 2009, Travnikov 2011] showed that the saturated state would consist only of harmonics of one azimuthal wave number, though there were bifurcations and transitions as nondimensional parameters (Re, Ha) were varied. Here, the energy transfer between different aziumthal modes is formulated as a network. This demonstrates a mechanism or the saturation of one mode and for the suppression of other unstable modes. A given mode grows by extracting energy from the axisymmetric flow, and then saturates as the energy transfer to its second harmonic equals this inflow. At the same time, this mode suppresses other unstable modes by facilitating an energy transfer to linearly stable modes.
10 pages, 9 figures
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Cited by in corpus (7)
- Chaotic wave dynamics in weakly magnetised spherical Couette flows
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- Long term time dependent frequency analysis of chaotic waves in the weakly magnetized spherical Couette system
- High dimensional tori and chaotic and intermittent transients in magnetohydrodynamic Couette flows
- Shercliff layers in strongly magnetic cylindrical Taylor-Couette flow
- Transitions in a magnetized quasi-laminar spherical Couette Flow
- Laboratory experiments and numerical simulations on magnetic instabilities