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Instabilities of Taylor columns in a rotating stratified fluid. (English) Zbl 1233.76112

Summary: We numerically solve for the flow in a differentially rotating spherical shell, with a stable stratification imposed along the rotation axis. The axisymmetric basic state evolves from a Stewartson layer in the unstratified limit to a Taylor column in the strongly stratified limit. For the Taylor columns, we next compute the linear onset of non-axisymmetric instabilities, and show that small (0.1) and large (10) Prandtl numbers yield very different results. For \(\mathrm{Pr}=10\), positive and negative differential rotations also yield fundamentally different instabilities.

MSC:

76U05 General theory of rotating fluids
76F45 Stratification effects in turbulence
76E07 Rotation in hydrodynamic stability
76M25 Other numerical methods (fluid mechanics) (MSC2010)
Full Text: DOI

References:

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