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Linear stability of magnetohydrodynamic flow in a perfectly conducting rectangular duct

机译:磁流体动力学流动的线性稳定性   矩形管道

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摘要

We analyse numerically the linear stability of a liquid metal flow in arectangular duct with perfectly electrically conducting walls subject to auniform transverse magnetic field. A non-standard three dimensional vectorstream function/vorticity formulation is used with Chebyshev collocation methodto solve the eigenvalue problem for small-amplitude perturbations. A relativelyweak magnetic field is found to render the flow linearly unstable as two weakjets appear close to the centre of the duct at the Hartmann number Ha \approx9.6. In a sufficiently strong magnetic field, the instability following thejets becomes confined in the layers of characteristic thickness \delta \simHa^{-1/2} located at the walls parallel to the magnetic field. In this case theinstability is determined by \delta, which results in both the criticalReynolds and wavenumbers numbers scaling as \sim \delta^{-1}. Instability modescan have one of the four different symmetry combinations along and across themagnetic field. The most unstable is a pair of modes with an even distributionof vorticity along the magnetic field. These two modes represent stronglynon-uniform vortices aligned with the magnetic field, which rotate either inthe same or opposite senses across the magnetic field. The former enhance whilethe latter weaken one another provided that the magnetic field is not toostrong or the walls parallel to the field are not too far apart. In a strongmagnetic field, when the vortices at the opposite walls are well separated bythe core flow, the critical Reynolds and wavenumbers for both of theseinstability modes are the same: Re_c \approx 642Ha^{1/2}+8.9x10^3Ha^{-1/2} andk_c \approx 0.477Ha^{1/2}. The other pair of modes, which differs from theprevious one by an odd distribution of vorticity along the magnetic field, ismore stable with approximately four times higher critical Reynolds number.
机译:我们用数值分析了在均匀横向磁场作用下具有完美导电壁的矩形管道中液态金属流的线性稳定性。非标准三维矢量流函数/涡度公式与Chebyshev搭配方法一起使用,以解决小振幅扰动的特征值问题。发现一个相对较弱的磁场使流动线性不稳定,因为在哈特曼数Ha \ approx9.6处,两个弱射流出现在管道中心附近。在足够强的磁场中,喷射之后的不稳定性被限制在位于平行于磁场的壁处的特征厚度为δdeltasimHa^ {-1/2}的层中。在这种情况下,不稳定性由\ delta决定,这将导致CriticalReynolds和波数均按\ sim \ delta ^ {-1}缩放。不稳定模式具有沿磁场和跨越磁场的四个不同对称组合之一。最不稳定的是一对沿磁场具有均匀涡度分布的模式。这两种模式表示与磁场对准的强烈非均匀涡流,它们在磁场中以相同或相反的方向旋转。前者增强,而后者则彼此弱化,条件是磁场不要太强或平行于磁场的壁相隔不远。在强磁场中,当相对壁的涡流被核心流很好地隔开时,这两种不稳定模式的临界雷诺数和波数都相同:Re_c \ approx 642Ha ^ {1/2} + 8.9x10 ^ 3Ha ^ { -1/2}和k_c \约0.477Ha ^ {1/2}。另一对模式与前一个模式的不同之处在于沿磁场的涡度分布呈奇数分布,它的临界雷诺数大约高四倍,因此更加稳定。

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