Shell Models for Magnetohydrodynamic Turbulence
Chaotic Dynamics
2007-05-23 v1
Abstract
We review the main properties of shell models for magnetohydrodynamic (MHD) turbulence. After a brief account on shell models with nearest neighbour interactions, the paper focuses on the most recent results concerning dynamical properties and intermittency of a model which is a generalization to MHD of the Gledzer-Yamada-Okhitani (GOY) model for hydrodynamic. Applications to astrophysical problems are also discussed.
Cite
@article{arxiv.nlin/0107032,
title = {Shell Models for Magnetohydrodynamic Turbulence},
author = {Paolo Giuliani},
journal= {arXiv preprint arXiv:nlin/0107032},
year = {2007}
}