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arxiv: 1108.1116 · v1 · pith:4EC6UTORnew · submitted 2011-08-04 · 🌌 astro-ph.SR · physics.flu-dyn

The Evolution of a Double Diffusive Magnetic Buoyancy Instability

classification 🌌 astro-ph.SR physics.flu-dyn
keywords fieldinstabilitymagneticactivitybuoyancydiffusivedoubleevolution
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Recently, Silvers, Vasil, Brummell, & Proctor (2009), 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.

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