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• W2155432834 abstract "Abstract. We use a quasi-geostrophic numerical model to study the turbulence of rotating flows in a sphere, with realistic Ekman friction and bulk viscous dissipation. The forcing is caused by the destabilization of an axisymmetric Stewartson shear layer, generated by differential rotation, resulting in a forcing at rather large scales. The equilibrium regime is strongly anisotropic and inhomogeneous but exhibits a steep m-5 spectrum in the azimuthal (periodic) direction, at scales smaller than the injection scale. This spectrum has been proposed by Rhines for a Rossby wave turbulence. For some parameter range, we observe a turbulent flow dominated by a large scale vortex located in the shear layer, reminding us of the Great Red Spot of Jupiter." @default.
• W2155432834 created "2016-06-24" @default.
• W2155432834 creator A5046164155 @default.
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• W2155432834 date "2005-11-04" @default.
• W2155432834 modified "2023-10-03" @default.
• W2155432834 title "Rossby-wave turbulence in a rapidly rotating sphere" @default.
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• W2155432834 doi "https://doi.org/10.5194/npg-12-947-2005" @default.
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