β-Plane Magnetohydrodynamic Turbulence in the Solar Tachocline

, , and

Published 2007 September 13 © 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Steven M. Tobias et al 2007 ApJ 667 L113 DOI 10.1086/521978

1538-4357/667/1/L113

Abstract

This Letter discusses the role of a weak toroidal magnetic field in modifying the turbulent transport properties of stably stratified rotating turbulence in the tachocline. A local two-dimensional β-plane model is investigated numerically. In the absence of magnetic fields, nonlinear interactions of Rossby waves lead to the formation of strong mean zonal flows. However, the addition of even a very weak toroidal field suppresses the generation of mean flows. We argue that this has serious implications for angular momentum transport in the lower tachocline.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/521978