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Updated: Jun 25, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Large-scale dynamo action driven by velocity shear and rotating convection
David W Hughes1, Michael R E Proctor
1Department of Applied Mathematics, University of Leeds, Leeds LS2 9JT, UK. d.w.hughes@leeds.ac.uk
Abstract:
By incorporating a large-scale shear flow into turbulent rotating convection, we show that a sufficiently strong shear can promote dynamo action in flows that are otherwise nondynamos. Our results are consistent with a dynamo driven either by the shear-current effect or by a fluctuating alpha effect interacting with the shear, but not with either a classical alpha(2) or alpha omega dynamo.
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