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Shearing Instabilities in Magnetoconvection

Published online by Cambridge University Press:  11 May 2010

M. R. E. Proctor
Affiliation:
University of Cambridge
P. C. Matthews
Affiliation:
University of Cambridge
A. M. Rucklidge
Affiliation:
University of Cambridge
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Summary

Recent numerical simulations of two-dimensional convection (compressible and Boussinesq) in the presence of a vertical magnetic field reveal that in some circumstances, narrow rolls are unstable to horizontal shear: tilted rolls are observed, as well as oscillating shearing motion. During the oscillation, the rolls tilt over and are replaced by a vigorous horizontal streaming motion, which decays, and the rolls are reformed, only to tilt over again, either in the same or in the opposite direction. A low-order model of this problem is constructed by truncating the PDEs for Boussinesq magnetoconvection. In the model, oscillatory shearing motion is created either in a ℍ bifurcation from untilted rolls, in which case the rolls tilt first one way and then the other, or in a ℍ bifurcation from tilted rolls, in which case the rolls always tilt in the same direction. Oscillations of the second type are converted into oscillations of the first type in a gluing bifurcation. This scenario is interpreted in terms of a Takens–Bogdanov bifurcation.

MOTIVATION

The interaction between convection and magnetic fields plays a central role in the theory of stellar dynamos. In order to investigate this interaction in detail, we consider a simplified problem: two-dimensional convection in a vertical magnetic field. To represent the astrophysical situation, in which there are no sidewalls, we consider a box with periodic boundary conditions in the horizontal direction, allowing horizontal flows. It is found that convection can be unstable to a horizontal shearing motion.

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Publisher: Cambridge University Press
Print publication year: 1994

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