Turbulent MHD transport coefficients
Previous calculations of turbulent magnetohydrodynamic (MHD) eddy viscosity and anomalous resistivity are reviewed. Emphasis is laid on a new approach to fully developed turbulence proposed by Canuto and Dubovikov, containing both systematic and heuristic elements for the ultraviolet (UV) and infrar...
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todo:paper_07413335_v41_n3A_pA635_FerroFontan2023-10-03T15:38:18Z Turbulent MHD transport coefficients Ferro Fontán, C. Approximation theory Differential equations Magnetohydrodynamics Mathematical models Navier Stokes equations Prandtl number Viscosity Direct interaction approximation Renormalization group Plasma turbulence Previous calculations of turbulent magnetohydrodynamic (MHD) eddy viscosity and anomalous resistivity are reviewed. Emphasis is laid on a new approach to fully developed turbulence proposed by Canuto and Dubovikov, containing both systematic and heuristic elements for the ultraviolet (UV) and infrared (IR) parts of the nonlinear interactions in hydrodynamics. Their method is extended so that the magnetic and velocity fluctuations are treated on an equal footing. The effective magnetic Prandtl number is obtained as a function of the residual energy spectral density. © 1999 IOP Publishing Ltd. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_07413335_v41_n3A_pA635_FerroFontan |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Approximation theory Differential equations Magnetohydrodynamics Mathematical models Navier Stokes equations Prandtl number Viscosity Direct interaction approximation Renormalization group Plasma turbulence |
spellingShingle |
Approximation theory Differential equations Magnetohydrodynamics Mathematical models Navier Stokes equations Prandtl number Viscosity Direct interaction approximation Renormalization group Plasma turbulence Ferro Fontán, C. Turbulent MHD transport coefficients |
topic_facet |
Approximation theory Differential equations Magnetohydrodynamics Mathematical models Navier Stokes equations Prandtl number Viscosity Direct interaction approximation Renormalization group Plasma turbulence |
description |
Previous calculations of turbulent magnetohydrodynamic (MHD) eddy viscosity and anomalous resistivity are reviewed. Emphasis is laid on a new approach to fully developed turbulence proposed by Canuto and Dubovikov, containing both systematic and heuristic elements for the ultraviolet (UV) and infrared (IR) parts of the nonlinear interactions in hydrodynamics. Their method is extended so that the magnetic and velocity fluctuations are treated on an equal footing. The effective magnetic Prandtl number is obtained as a function of the residual energy spectral density. © 1999 IOP Publishing Ltd. |
format |
JOUR |
author |
Ferro Fontán, C. |
author_facet |
Ferro Fontán, C. |
author_sort |
Ferro Fontán, C. |
title |
Turbulent MHD transport coefficients |
title_short |
Turbulent MHD transport coefficients |
title_full |
Turbulent MHD transport coefficients |
title_fullStr |
Turbulent MHD transport coefficients |
title_full_unstemmed |
Turbulent MHD transport coefficients |
title_sort |
turbulent mhd transport coefficients |
url |
http://hdl.handle.net/20.500.12110/paper_07413335_v41_n3A_pA635_FerroFontan |
work_keys_str_mv |
AT ferrofontanc turbulentmhdtransportcoefficients |
_version_ |
1782026556926853120 |