Why, how and when MHD turbulence at low becomes three-dimensional
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Publication:5175708
DOI10.1017/jfm.2014.620zbMath1308.76334arXiv1305.7105OpenAlexW3099049853MaRDI QIDQ5175708
Publication date: 24 February 2015
Published in: Journal of Fluid Mechanics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1305.7105
Related Items (14)
Variable energy flux in turbulence ⋮ Exact two-dimensionalization of low-magnetic-Reynolds-number flows subject to a strong magnetic field ⋮ Secondary optimal energy growth and magnetic damping of turbulence in Hartmann channel flow ⋮ Subcritical transition to turbulence in quasi-two-dimensional shear flows ⋮ Effects of horizontal magnetic fields on turbulent Rayleigh–Bénard convection in a cuboid vessel with aspect ratio Γ = 5 ⋮ Inertial regimes in a curved electromagnetically forced flow ⋮ Turbulence in electromagnetically driven Keplerian flows ⋮ From three-dimensional to quasi-two-dimensional: transient growth in magnetohydrodynamic duct flows ⋮ Dimensionality, secondary flows and helicity in low-Rm MHD vortices ⋮ Mean flow anisotropy without waves in rotating turbulence ⋮ Transition between advection and inertial wave propagation in rotating turbulence ⋮ Combining an obstacle and electrically driven vortices to enhance heat transfer in a quasi-two-dimensional MHD duct flow ⋮ Direct numerical simulation of quasi-two-dimensional MHD turbulent shear flows ⋮ Decay of turbulence in a liquid metal duct flow with transverse magnetic field
Cites Work
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