2008
DOI: 10.1063/1.2975988
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Magnetohydrodynamic turbulence in a channel with spanwise magnetic field

Abstract: The effect of a uniform spanwise magnetic field on a turbulent channel flow is investigated for the case of a low magnetic Reynolds number. Direct numerical simulation ͑DNS͒ and large eddy simulation ͑LES͒ computations are performed for two values of the hydrodynamic Reynolds number ͑10 4 and 2 ϫ 10 4 ͒ and with the Hartmann number varying in a wide range. It is shown that the main effect of the magnetic field is the suppression of turbulent velocity fluctuations and momentum transfer in the wall-normal direct… Show more

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Cited by 64 publications
(89 citation statements)
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References 43 publications
(60 reference statements)
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“…This appears to be the reason for the reduced slope of the mean velocity profile in the cross-section Sh-Sh illustrated in figure 5. The same effect has been detected by Krasnov et al (2008) in a channel with spanwise magnetic field. For τ 13 , an interesting feature is that at its peak near the Hartmann wall, the transport rate is higher in the MHD flow at Ha = 100 than it is in the flow with Ha = 0.…”
Section: Turbulent Fluctuationssupporting
confidence: 62%
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“…This appears to be the reason for the reduced slope of the mean velocity profile in the cross-section Sh-Sh illustrated in figure 5. The same effect has been detected by Krasnov et al (2008) in a channel with spanwise magnetic field. For τ 13 , an interesting feature is that at its peak near the Hartmann wall, the transport rate is higher in the MHD flow at Ha = 100 than it is in the flow with Ha = 0.…”
Section: Turbulent Fluctuationssupporting
confidence: 62%
“…We see that when the Hartmann number increases from 0 to 100 and then to 200, the centreline velocity increases (see figures 4 and 5 and table 2). The distribution takes a form similar to the chisel-like form found earlier in the simulations of channel flow with a spanwise magnetic field (Krasnov et al 2008). This has been attributed to reduction of the wall-normal turbulent transport of momentum caused by the suppression of turbulence by the magnetic field.…”
Section: Mean Flowsupporting
confidence: 56%
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“…Between the two limits, the flows have the transitional form discussed below. It is known from [18][19][20][21] and confirmed by our computations that the suppression of turbulence and reduction of momentum transport by the magnetic field result, in the considered range of Re and Ha, in a decrease of C f . After the flow becomes laminar, increase of Ha means thinner Hartmann and sidewall layers and, thus, stronger gradient of mean velocity near the walls and higher C f .…”
supporting
confidence: 71%
“…The Lorentz force density in the fluid is f = j × B. The interaction between a laminar duct flow and a magnetic dipole is studied by direct numerical simulations with a highly conservative finite-difference method on a structured mesh [5]. Our code solves the incompressible Navier-Stokes equations together with the induction equation in the quasistatic approximation.…”
mentioning
confidence: 99%