Generation of density inhomogeneities by magnetohydrodynamic waves in two dimensions
Astrophysics
2009-11-11 v1
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.
Keywords
Cite
@article{arxiv.astro-ph/0605258,
title = {Generation of density inhomogeneities by magnetohydrodynamic waves in two dimensions},
author = {S. Van Loo and S. A. E. G. Falle and T. W. Hartquist},
journal= {arXiv preprint arXiv:astro-ph/0605258},
year = {2009}
}
Comments
6 pages, 7 figures, accepted by MNRAS