Shell Models for Magnetohydrodynamic Turbulence

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dc.creatorGiuliani, Paolo
dc.date2001-07-14
dc.date.accessioned2026-07-07T05:33:35Z
dc.date.available2026-07-07T05:33:35Z
dc.descriptionWe 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.
dc.identifierhttps://arxiv.org/abs/nlin/0107032
dc.identifierhttp://arxiv.org/abs/nlin/0107032
dc.identifierNonlinear MHD Waves and Turbulence, Eds. T. Passot and P.L. Sulem, Lecture Notes in Physics, Springer, (1999)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/80050
dc.subjectChaotic Dynamics
dc.titleShell Models for Magnetohydrodynamic Turbulence
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