Compressible sub-Alfvénic MHD turbulence in low-beta plasmas.

Phys Rev Lett

Astronomy Department, University of Wisconsin, Madison, WI 53706, USA.

Published: June 2002

We present a model for compressible sub-Alfvénic isothermal magnetohydrodynamic (MHD) turbulence in low- beta 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.

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http://dx.doi.org/10.1103/PhysRevLett.88.245001DOI Listing

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