Compressible Sub-Alfvénic MHD Turbulence in Low- β Plasmas

Jungyeon Cho and A. Lazarian
Phys. Rev. Lett. 88, 245001 – Published 31 May 2002
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Abstract

We present a model for compressible sub-Alfvénic isothermal magnetohydrodynamic (MHD) turbulence in low- β plasmas and numerically test it. We separate MHD fluctuations into three distinct families: Alfvén, slow, and fast modes. We find that production of slow and fast modes by Alfvénic turbulence is suppressed. As a result, Alfvén modes in compressible regime exhibit scalings and anisotropy similar to those in incompressible regime. Slow modes passively mimic Alfvén modes. However, fast modes show isotropy and a scaling similar to acoustic turbulence.

  • Received 1 March 2002

DOI:https://doi.org/10.1103/PhysRevLett.88.245001

©2002 American Physical Society

Authors & Affiliations

Jungyeon Cho* and A. Lazarian

  • Astronomy Department, University of Wisconsin, Madison, Wisconsin 53706

  • *Email address: cho@astro.wisc.edu
  • Email address: lazarian@astro.wisc.edu

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Vol. 88, Iss. 24 — 17 June 2002

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