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Do magnetic fields enhance turbulence at low magnetic Reynolds number ?
by
Pothérat, Alban
, Klein, Rico
in
Accretion disks
/ Anisotropy
/ Conducting fluids
/ Energy dissipation
/ Fluid dynamics
/ Fluid flow
/ Magnetic fields
/ Metallurgy
/ Nuclear engineering
/ Nuclear power plants
/ Phenomenology
/ Reynolds number
/ Systems (metallurgical)
/ Turbulence
/ Turbulent flow
/ Variations
2017
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Do magnetic fields enhance turbulence at low magnetic Reynolds number ?
by
Pothérat, Alban
, Klein, Rico
in
Accretion disks
/ Anisotropy
/ Conducting fluids
/ Energy dissipation
/ Fluid dynamics
/ Fluid flow
/ Magnetic fields
/ Metallurgy
/ Nuclear engineering
/ Nuclear power plants
/ Phenomenology
/ Reynolds number
/ Systems (metallurgical)
/ Turbulence
/ Turbulent flow
/ Variations
2017
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While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
Do magnetic fields enhance turbulence at low magnetic Reynolds number ?
by
Pothérat, Alban
, Klein, Rico
in
Accretion disks
/ Anisotropy
/ Conducting fluids
/ Energy dissipation
/ Fluid dynamics
/ Fluid flow
/ Magnetic fields
/ Metallurgy
/ Nuclear engineering
/ Nuclear power plants
/ Phenomenology
/ Reynolds number
/ Systems (metallurgical)
/ Turbulence
/ Turbulent flow
/ Variations
2017
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Do magnetic fields enhance turbulence at low magnetic Reynolds number ?
Paper
Do magnetic fields enhance turbulence at low magnetic Reynolds number ?
2017
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Overview
Imposing a magnetic field on a turbulent flow of electrically conducting fluid incurs the Joule effect. A current paradigm is that the corresponding dissipation increases with the intensity of the magnetic field, and as a result turbulent fluctuations are all the more damped as the magnetic field is strong. While this idea finds apparent support in the phenomenology of decaying turbulence, measurements of turbulence in duct flows and other, more complex configurations have produced seemingly contradicting results. The root of the controversy is that magnetic fields promote sufficient scale-dependent anisotropy to profoundly reorganise the structure of turbulence, so their net effect cannot be understood in terms of the additional dissipation only. Here we show that when turbulence is forced in a magnetic field that acts on turbulence itself rather than on the mechanisms that generate it, the field promotes large, nearly 2D structures capturing sufficient energy to offset the loss due to Joule dissipation, with the net effect of increasing the intensity of turbulent fluctuations. This change of paradigm potentially carries important consequences for systems as diverse as the liquid cores of planets, accretion disks and a wide range of metallurgical and nuclear engineering applications.
Publisher
Cornell University Library, arXiv.org
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