Exact two-dimensionalization of low-magnetic-Reynolds-number flows subject to a strong magnetic field
We investigate the behaviour of flows, including turbulent flows, driven by a horizontal body force and subject to a vertical magnetic field, with the following question in mind: for a very strong applied magnetic field, is the flow mostly two-dimensional, with remaining weak three-dimensional fluct...
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Published in | Journal of fluid mechanics Vol. 773; pp. 154 - 177 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Cambridge, UK
Cambridge University Press
25.06.2015
Cambridge University Press (CUP) |
Subjects | |
Online Access | Get full text |
ISSN | 0022-1120 1469-7645 |
DOI | 10.1017/jfm.2015.232 |
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Abstract | We investigate the behaviour of flows, including turbulent flows, driven by a horizontal body force and subject to a vertical magnetic field, with the following question in mind: for a very strong applied magnetic field, is the flow mostly two-dimensional, with remaining weak three-dimensional fluctuations, or does it become exactly 2-D, with no dependence along the vertical direction? We first focus on the quasi-static approximation, i.e. the asymptotic limit of vanishing magnetic Reynolds number,
$\mathit{Rm}\ll 1$
: we prove that the flow becomes exactly 2-D asymptotically in time, regardless of the initial condition and provided that the interaction parameter
$N$
is larger than a threshold value. We call this property absolute two-dimensionalization: the attractor of the system is necessarily a (possibly turbulent) 2-D flow. We then consider the full magnetohydrodynamic (MHD) equations and prove that, for low enough
$\mathit{Rm}$
and large enough
$N$
, the flow becomes exactly 2-D in the long-time limit provided the initial vertically dependent perturbations are infinitesimal. We call this phenomenon linear two-dimensionalization: the (possibly turbulent) 2-D flow is an attractor of the dynamics, but it is not necessarily the only attractor of the system. Some 3-D attractors may also exist and be attained for strong enough initial 3-D perturbations. These results shed some light on the existence of a dissipation anomaly for MHD flows subject to a strong external magnetic field. |
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AbstractList | We investigate the behaviour of flows, including turbulent flows, driven by a horizontal body force and subject to a vertical magnetic field, with the following question in mind: for a very strong applied magnetic field, is the flow mostly two-dimensional, with remaining weak three-dimensional fluctuations, or does it become exactly 2-D, with no dependence along the vertical direction? We first focus on the quasi-static approximation, i.e. the asymptotic limit of vanishing magnetic Reynolds number,
$\mathit{Rm}\ll 1$
: we prove that the flow becomes exactly 2-D asymptotically in time, regardless of the initial condition and provided that the interaction parameter
$N$
is larger than a threshold value. We call this property absolute two-dimensionalization: the attractor of the system is necessarily a (possibly turbulent) 2-D flow. We then consider the full magnetohydrodynamic (MHD) equations and prove that, for low enough
$\mathit{Rm}$
and large enough
$N$
, the flow becomes exactly 2-D in the long-time limit provided the initial vertically dependent perturbations are infinitesimal. We call this phenomenon linear two-dimensionalization: the (possibly turbulent) 2-D flow is an attractor of the dynamics, but it is not necessarily the only attractor of the system. Some 3-D attractors may also exist and be attained for strong enough initial 3-D perturbations. These results shed some light on the existence of a dissipation anomaly for MHD flows subject to a strong external magnetic field. We investigate the behaviour of flows, including turbulent flows, driven by a horizontal body force and subject to a vertical magnetic field, with the following question in mind: for a very strong applied magnetic field, is the flow mostly two-dimensional, with remaining weak three-dimensional fluctuations, or does it become exactly 2-D, with no dependence along the vertical direction? We first focus on the quasi-static approximation, i.e. the asymptotic limit of vanishing magnetic Reynolds number, [formula omitted: see PDF] : we prove that the flow becomes exactly 2-D asymptotically in time, regardless of the initial condition and provided that the interaction parameter [formula omitted: see PDF] is larger than a threshold value. We call this property absolute two-dimensionalization: the attractor of the system is necessarily a (possibly turbulent) 2-D flow. We then consider the full magnetohydrodynamic (MHD) equations and prove that, for low enough [formula omitted: see PDF] and large enough [formula omitted: see PDF] , the flow becomes exactly 2-D in the long-time limit provided the initial vertically dependent perturbations are infinitesimal. We call this phenomenon linear two-dimensionalization: the (possibly turbulent) 2-D flow is an attractor of the dynamics, but it is not necessarily the only attractor of the system. Some 3-D attractors may also exist and be attained for strong enough initial 3-D perturbations. These results shed some light on the existence of a dissipation anomaly for MHD flows subject to a strong external magnetic field. We investigate the behaviour of flows, including turbulent flows, driven by a horizontal body force and subject to a vertical magnetic field, with the following question in mind: for a very strong applied magnetic field, is the flow mostly two-dimensional, with remaining weak three-dimensional fluctuations, or does it become exactly 2-D, with no dependence along the vertical direction? We first focus on the quasi-static approximation, i.e. the asymptotic limit of vanishing magnetic Reynolds number, Rm 1: we prove that the flow becomes exactly 2-D asymptotically in time, regardless of the initial condition and provided that the interaction parameter N is larger than a threshold value. We call this property absolute two-dimensionalization: the attractor of the system is necessarily a (possibly turbulent) 2-D flow. We then consider the full magnetohydrodynamic (MHD) equations and prove that, for low enough Rm and large enough N, the flow becomes exactly 2-D in the long-time limit provided the initial vertically dependent perturbations are infinitesimal. We call this phenomenon linear two-dimensionalization: the (possibly turbulent) 2-D flow is an attractor of the dynamics, but it is not necessarily the only attractor of the system. Some 3-D attractors may also exist and be attained for strong enough initial 3-D perturbations. These results shed some light on the existence of a dissipation anomaly for MHD flows subject to a strong external magnetic field. |
Author | Doering, Charles R. Gallet, Basile |
Author_xml | – sequence: 1 givenname: Basile surname: Gallet fullname: Gallet, Basile email: basile.gallet@gmail.com organization: Service de Physique de l’État Condensé, DSM, CNRS UMR 3680, CEA Saclay, 91191 Gif-sur-Yvette, France – sequence: 2 givenname: Charles R. surname: Doering fullname: Doering, Charles R. organization: Department of Physics, Department of Mathematics and Center for the Study of Complex Systems, University of Michigan, Ann Arbor, MI 48109, USA |
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Cites_doi | 10.1017/S0022112086000836 10.1063/1.1601222 10.1017/S0022112002001386 10.1063/1.3194304 10.1146/annurev.fluid.39.050905.110231 10.1209/0295-5075/82/29001 10.1017/S0022112004007992 10.1146/annurev.fluid.31.1.273 10.1017/S0022112097008239 10.1103/PhysRevE.84.056330 10.1017/jfm.2014.620 10.1103/PhysRevLett.104.034502 10.1080/03091929.2011.648629 10.1209/0295-5075/97/69001 10.1016/j.physleta.2006.07.048 10.1017/S0022112082001177 10.1063/1.870068 10.1017/S0022112007005277 10.1103/PhysRevE.90.033015 10.1017/jfm.2013.233 10.1103/PhysRevE.83.026405 |
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SubjectTerms | Flow velocity Fluid mechanics Magnetic fields Physics Reynolds number Turbulent flow |
Title | Exact two-dimensionalization of low-magnetic-Reynolds-number flows subject to a strong magnetic field |
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