Dissipation in Compressible Magnetohydrodynamic Turbulence

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Published 1998 October 21 © 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation James M. Stone et al 1998 ApJ 508 L99 DOI 10.1086/311718

1538-4357/508/1/L99

Abstract

We report results of a three-dimensional, high resolution (up to 5123) numerical investigation of supersonic compressible magnetohydrodynamic turbulence. We consider both forced and decaying turbulence. The model parameters are appropriate to conditions found in Galactic molecular clouds. We find that the dissipation time of turbulence is of the order of the flow crossing time or smaller, even in the presence of strong magnetic fields. About half of the dissipation occurs in shocks. Weak magnetic fields are amplified and tangled by the turbulence, while strong fields remain well ordered.

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10.1086/311718