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Phys. Rev. Lett. 101, 235003 (2008) [4 pages]

Rapid Generation of Angular Momentum in Bounded Magnetized Plasma

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Wouter J. T. Bos1,2, Salah Neffaa2, and Kai Schneider2
1LMFA, UMR CNRS 5509, Ecole Centrale de Lyon–Université de Lyon, Ecully, France
2M2P2, UMR 6181 CNRS & CMI, Universités d’Aix-Marseille, Marseille, France

Received 17 July 2008; published 2 December 2008

Direct numerical simulations of two-dimensional decaying MHD turbulence in bounded domains show the rapid generation of angular momentum in nonaxisymmetric geometries. It is found that magnetic fluctuations enhance this mechanism. On a larger time scale, the generation of a magnetic angular momentum, or angular field, is observed. For axisymmetric geometries, the generation of angular momentum is absent; nevertheless, a weak magnetic field can be observed. The derived evolution equations for both the angular momentum and angular field yield possible explanations for the observed behavior.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.101.235003
DOI:
10.1103/PhysRevLett.101.235003
PACS:
52.30.Cv, 47.65.−d, 52.65.Kj