Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003apj...599..715d&link_type=abstract
The Astrophysical Journal, Volume 599, Issue 1, pp. 715-722.
Astronomy and Astrophysics
Astronomy
20
Methods: Numerical, Magnetohydrodynamics: Mhd, Turbulence
Scientific paper
Spectral anisotropy within decaying incompressible electron magnetohydrodynamics turbulence is investigated by two-dimensional fluid simulations. An initially isotropic turbulent spectrum exhibits anisotropy in the spectral cascade because of the presence of a self-consistent large-scale or an externally imposed magnetic field. Our simulations show that the anisotropy scales linearly with the strength of the ambient magnetic field. The linear scaling of the anisotropic spectral cascades appears to be rather generic as turbulent excitation scales larger than kde<1 as well as those smaller than kde>1, the collisionless electron inertial or skin depth length scale (de), follow a similar trend.
Dastgeer Sheikh
Zank Gary P.
No associations
LandOfFree
Anisotropic Turbulence in Two-dimensional Electron Magnetohydrodynamics does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Anisotropic Turbulence in Two-dimensional Electron Magnetohydrodynamics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Anisotropic Turbulence in Two-dimensional Electron Magnetohydrodynamics will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1652108