@inproceedings{ef35ddaeecea43a589e689577a29cdd4,
title = "Anisotropic MHD Turbulence in the Interstellar Medium and Solar Wind",
abstract = "A theoretical model is given of anisotropic magnetohydrodynamic turbulence in the interstellar medium and the solar wind. The model is motivated by observations that show significant deviations from the Kolmogorov power-law. Dimensional and heuristic arguments are given and critically assessed. On the basis of the weak turbulence approximation in which three-wave interactions dominate, analytical and numerical results are obtained for the anisotropic energy spectrum produced by the random scattering of shear Alfv{\'e}n waves propagating parallel to a large-scale magnetic field. The energy spectrum is shown to be proportional to k⊥-2, qualitatively consistent with some observations and wave kinetic theory.",
author = "A. Bhattacharjee and Ng, {C. S.}",
note = "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 = "10.1063/1.1618628",
language = "English (US)",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics Inc.",
pages = "433--438",
editor = "Marco Velli and Roberto Bruno and Francesco Malara",
booktitle = "Solar Wind Ten",
}