Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-25T15:41:50.755Z Has data issue: false hasContentIssue false
  • English
  • Français

Lack of universality in MHD turbulence, and the possible emergence of a new paradigm?

Published online by Cambridge University Press:  12 August 2011

Annick Pouquet ,
Marc-Etienne Brachet ,
Ed Lee ,
Pablo Mininni ,
Duane Rosenberg  and
Vadim Uritsky
Annick Pouquet
Affiliation:
Geophysical Turbulence Program, National Center for Atmospheric Research, PO Box 3000, Boulder CO 80304USA email: [email protected] and [email protected]
Marc-Etienne Brachet
Affiliation:
École Normale Supérieure, 24 rue Lhomond, 75005 Paris, France email: [email protected]
Ed Lee
Affiliation:
Centrum voor Plasma-Astrofysica, Departement Wiskunde, Katholieke Universiteit Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium email: [email protected]
Pablo Mininni
Affiliation:
Geophysical Turbulence Program, National Center for Atmospheric Research, PO Box 3000, Boulder CO 80304USA email: [email protected] and [email protected] Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria, 1428 Buenos Aires, Argentina email: [email protected]
Duane Rosenberg
Affiliation:
Geophysical Turbulence Program, National Center for Atmospheric Research, PO Box 3000, Boulder CO 80304USA email: [email protected] and [email protected]
Vadim Uritsky
Affiliation:
Physics and Astronomy Department, University of Calgary, Calgary, AB T2N1N4Canada email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We review some of the recent results obtained in MHD turbulence, as encountered in many astrophysical objects. We focus attention on the lack of universality in such flows, including in the simplest case (no externally imposed magnetic field, no forcing, unit magnetic Prandtl number). Several parameters can foster such a breakdown of classical Kolmogorov scaling, such as the presence of velocity-magnetic field correlations, or of magnetic helicity and the role of the interplay between nonlinear eddies and Alfvén waves. A link with avalanche processes is also discussed. These findings have led to the conjecture of the emergence of a new paradigm for MHD turbulence, as a possibly unsettled competition between several dynamical phenomena.

Keywords

turbulencemagnetic fields(magnetohydrodynamics:) MHDwavesSun: flares(Sun:) solar windstars: activityISM: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S271: Astrophysical Dynamics: From Stars to Galaxies , June 2010 , pp. 304 - 316
Copyright
Copyright © International Astronomical Union 2011

References

Plunian, F. & Stepanov, R., 2006 J. Turbulence, 7, 39Google Scholar
Podesta, J. J., Roberts, D. A. & Goldstein, M. L. 2007, Astrophys. J., 664, 543CrossRefGoogle Scholar
Meneguzzi, M., Politano, H., Pouquet, A. & Zolver, M. 1996, J. Comp. Phys., 123, 32CrossRefGoogle Scholar
Kadomtsev, B. B. & Pogutse, O. P. 1974, Z. Eksp. Teor. Fiz., 65, 575Google Scholar
Alexandrova, O., Mangeney, A., Maksimovic, M., Cornilleau-Wehrlin, N., Bosqued, J.-M. & André, M. 2006, J. Geophys. Res., 111, A12208Google Scholar
Lee, E., Brachet, M., Pouquet, A., Mininni, P. & Rosenberg, D. 2008, Phys. Rev.E, 78, 066401CrossRefGoogle Scholar
Whang, Y. C. 2004, Nonlinear Processes Geophys., 11, 259CrossRefGoogle Scholar