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Updated: May 14, 2026

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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Transitions in rapidly rotating convection driven dynamos
1Institute of Geophysics, University of Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany.
Physical Review Letters
|February 2, 2013
Abstract:
Numerical simulations of dynamos in rotating Rayleigh-Bénard convection in plane layers are presented. Two different types of dynamos exist which obey different scaling laws for the amplitude of the magnetic field. The transition between the two occurs within a hydrodynamically uniform regime which can be classified as rapidly rotating convection.
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