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Application of Reynolds stress transport turbulence closure models to flows affected by Lorentz and buoyancy forces

机译:雷诺应力传递湍流闭合模型在受洛伦兹和浮力影响的流动中的应用

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The effect of magnetic field strength and orientation on two types of electromagnetically influenced turbulent flows was studied numerically under the Reynolds averaged Navier-Stokes (RANS) framework. Previous work (Wilson et al., 2014) used an electromagnetically extended linear eddy-viscosity model, whilst the current paper focuses on the performance of a more advanced Reynolds stress transport type model both with and without electromagnetic modifications proposed by Kenjeres et al. (2004). First, a fully-developed 2D channel flow is considered with a magnetic field imposed in either the wall-normal or streamwise direction. Both forms of the RSM gave good agreement with the DNS data for the wall-normal magnetic field across the range of Hartmann numbers with the additional electromagnetic terms providing a small, but noticeable, difference. For the streamwise magnetic field, where electromagnetic influence is only through the turbulence, the electromagnetically extended RSM performed well at moderate Hartmann numbers but returned laminar flow at the highest Hartmann number considered, contrary to the DNS. The RSM results were, however, significantly better than the previous eddy-viscosity model predictions. The second case is that of unsteady 3D Rayleigh-Benard convection with a magnetic field imposed in either a horizontal or vertical direction. Results revealed that a significant reorganization of the flow structures is predicted to occur. For a vertically oriented magnetic field, the plume structures increase in number and become thinner and elongated along the magnetic field lines, leading to an increase in thermal mixing within the core in agreement with Hanjalic and Kenjeres (2000). With a horizontal magnetic field, the structures become two-dimensional and a striking realignment of the roll cells' axes with the magnetic field lines occurs. The results demonstrate the capability of the Reynolds stress transport approach in modelling MHD flows that are relevant to industry and offer potential for those wishing to control levels of turbulence, heat transfer or concentration without recourse to mechanical means. (C) 2015 Elsevier Inc. All rights reserved.
机译:在雷诺平均Navier-Stokes(RANS)框架下,数值研究了磁场强度和方向对两种类型的电磁影响的湍流的影响。先前的工作(Wilson等人,2014)使用了电磁扩展的线性涡流-粘度模型,而当前的论文集中于Kenjeres等人提出的具有或不具有电磁修改的更高级的雷诺应力传输类型模型的性能。 (2004)。首先,考虑在壁法线方向或流向方向施加磁场的情况下充分发展的2D通道流。两种形式的RSM与在整个Hartmann数范围内的壁法向磁场的DNS数据都具有很好的一致性,并且附加的电磁项提供了微小但明显的差异。对于仅通过湍流产生电磁影响的流式磁场,与DNS相反,电磁扩展的RSM在中等Hartmann数下表现良好,但在考虑到的最高Hartmann数下返回层流。但是,RSM结果明显优于先前的涡流-粘度模型预测。第二种情况是在水平或垂直方向施加磁场的不稳定3D Rayleigh-Benard对流。结果表明,预计将发生流动结构的重大重组。对于垂直方向的磁场,羽状结构的数量增加,并沿着磁场线变细和拉长,这导致与Hanjalic和Kenjeres(2000)一致的铁心内部的热混合增加。在水平磁场作用下,结构变为二维,并且滚动单元的轴与磁场线发生明显的重新对齐。结果表明,雷诺应力传递方法具有对与工业相关的MHD流动进行建模的能力,并为那些希望在不依靠机械手段的情况下控制湍流,传热或集中水平的人们提供了潜力。 (C)2015 Elsevier Inc.保留所有权利。

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