@inproceedings{f5d024dbfeb74dfb87128937f3908c91,
title = "Weak turbulence of anisotropic shear-Alfv{\'e}n waves",
abstract = "We review recent results obtained in [14] on weak turbulence of shear-Alfv{\'e}n waves in the limit of strongly anisotropic pulsations that are elongated along a strong external magnetic field. The kinetic equation for energy is presented at the level of three-wave interactions. It is in agreement with the Galtier et al. [13] formulation of the full three-dimensional helical case when taking the proper limit. The simplified formalism induced by the new approach renders the applicability conditions for weak turbulence more transparent. It provides an attractive theoretical framework for describing anisotropic MHD turbulence in astrophysical contexts where a strong magnetic field is present and for which shear-Alfv{\'e}n waves are important.",
author = "S. Galtier and Nazarenko, {S. V.} and Newell, {A. C.} and A. Pouquet",
note = "Funding Information: Grants from CNRS (PNST and PCMI) and from EC (FMRX-CT98-0175) are gratefully acknowledged. Publisher Copyright: {\textcopyright} 2003 American Institute of Physics.; 10th International Solar Wind Conference ; Conference date: 17-06-2002 Through 21-06-2002",
year = "2003",
month = sep,
day = "2",
doi = "10.1063/1.1618648",
language = "English (US)",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics Inc.",
pages = "518--521",
editor = "Marco Velli and Roberto Bruno and Francesco Malara",
booktitle = "Solar Wind Ten",
}