Title of article
The Evolution of a Double Diffusive Magnetic Buoyancy Instability
Author/Authors
Lara J. Silvers، نويسنده , , Geoffrey M. Vasil، نويسنده , , Nicholas H. Brummell، نويسنده , , Michael R. E. Proctor، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2010
Pages
9
From page
218
To page
226
Abstract
Recently, Silvers et al. (2009b), using numerical simulations, confirmed the existence of a double diffusive magnetic buoyancy instability of a layer of horizontal magnetic field produced by the interaction of a shear velocity field with a weak vertical field. Here, we demonstrate the longer term nonlinear evolution of such an instability in the simulations. We find that a quasi two-dimensional interchange instability rides (or “surfs”) on the growing shear-induced background downstream field gradients. The region of activity expands since three-dimensional perturbations remain unstable in the wake of this upward-moving activity front, and so the three-dimensional nature becomes more noticeable with time.
Keywords
instabilities , MHD , Sun: magnetic fields
Journal title
Proceedings of the International Astronomical Union
Serial Year
2010
Journal title
Proceedings of the International Astronomical Union
Record number
667757
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