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arxiv: 1506.00399 · v2 · pith:WCH6KQ7Qnew · submitted 2015-06-01 · ⚛️ physics.flu-dyn · astro-ph.SR

Destabilization of rotating flows with positive shear by azimuthal magnetic fields

classification ⚛️ physics.flu-dyn astro-ph.SR
keywords flowsinstabilityangularazimuthalfieldsfluidmagneticoutward
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According to Rayleigh's criterion, rotating flows are linearly stable when their specific angular momentum increases radially outward. The celebrated magnetorotational instability opens a way to destabilize those flows, as long as the angular velocity is decreasing outward. Using a short-wavelength approximation we demonstrate that even flows with very steep positive shear can be destabilized by azimuthal magnetic fields which are current-free within the fluid. We illustrate the transition of this instability to a rotationally enhanced kink-type instability in case of a homogeneous current in the fluid, and discuss the prospects for observing it in a magnetized Taylor-Couette flow.

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