Exact scaling laws and the local structure of isotropic magnetohydrodynamic turbulence

This paper examines the consistency of the exact scaling laws for isotropic MHD turbulence in numerical simulations with large magnetic Prandtl numbers Pm and with Pm=1. The exact laws are used to elucidate the structure of the magnetic and velocity fields. Despite the linear scaling of certain thir...

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Main Authors: Yousef, T, Rincon, F, Schekochihin, A
Format: Journal article
Language:English
Published: 2006
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author Yousef, T
Rincon, F
Schekochihin, A
author_facet Yousef, T
Rincon, F
Schekochihin, A
author_sort Yousef, T
collection OXFORD
description This paper examines the consistency of the exact scaling laws for isotropic MHD turbulence in numerical simulations with large magnetic Prandtl numbers Pm and with Pm=1. The exact laws are used to elucidate the structure of the magnetic and velocity fields. Despite the linear scaling of certain third-order correlation functions, the situation is not analogous to the case of Kolmogorov turbulence. The magnetic field is adequately described by a model of stripy (folded) field with direction reversals at the resistive scale. At currently available resolutions, the cascade of kinetic energy is short-circuited by the direct exchange of energy between the forcing-scale motions and the stripy magnetic fields. This nonlocal interaction is the defining feature of isotropic MHD turbulence.
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spelling oxford-uuid:a7777eb1-2536-403d-a203-dd77d5b4c3462022-03-27T02:54:51ZExact scaling laws and the local structure of isotropic magnetohydrodynamic turbulenceJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:a7777eb1-2536-403d-a203-dd77d5b4c346EnglishSymplectic Elements at Oxford2006Yousef, TRincon, FSchekochihin, AThis paper examines the consistency of the exact scaling laws for isotropic MHD turbulence in numerical simulations with large magnetic Prandtl numbers Pm and with Pm=1. The exact laws are used to elucidate the structure of the magnetic and velocity fields. Despite the linear scaling of certain third-order correlation functions, the situation is not analogous to the case of Kolmogorov turbulence. The magnetic field is adequately described by a model of stripy (folded) field with direction reversals at the resistive scale. At currently available resolutions, the cascade of kinetic energy is short-circuited by the direct exchange of energy between the forcing-scale motions and the stripy magnetic fields. This nonlocal interaction is the defining feature of isotropic MHD turbulence.
spellingShingle Yousef, T
Rincon, F
Schekochihin, A
Exact scaling laws and the local structure of isotropic magnetohydrodynamic turbulence
title Exact scaling laws and the local structure of isotropic magnetohydrodynamic turbulence
title_full Exact scaling laws and the local structure of isotropic magnetohydrodynamic turbulence
title_fullStr Exact scaling laws and the local structure of isotropic magnetohydrodynamic turbulence
title_full_unstemmed Exact scaling laws and the local structure of isotropic magnetohydrodynamic turbulence
title_short Exact scaling laws and the local structure of isotropic magnetohydrodynamic turbulence
title_sort exact scaling laws and the local structure of isotropic magnetohydrodynamic turbulence
work_keys_str_mv AT youseft exactscalinglawsandthelocalstructureofisotropicmagnetohydrodynamicturbulence
AT rinconf exactscalinglawsandthelocalstructureofisotropicmagnetohydrodynamicturbulence
AT schekochihina exactscalinglawsandthelocalstructureofisotropicmagnetohydrodynamicturbulence