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Generation of density inhomogeneities by magnetohydrodynamic waves in two dimensions

S. Van Loo, S. A. E. G. Falle, T. W. Hartquist

astro-pharXiv:astro-ph/0605258

Abstract

Using two dimensional simulations, we study the formation of structures with a high-density contrast by magnetohydrodynamic waves in regions in which the ratio of thermal to magnetic pressure is small. The initial state is a uniform background perturbed by fast-mode wave. Our most significant result is that dense structures persist for far longer in a two-dimensional simulation than in the one-dimensional case. Once formed, these structures persist as long as the fast-mode amplitude remains high.

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