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NUMERICAL STUDY OF BUOYANCY-DRIVEN CONVECTION OF MOLTEN GALLIUM UNDER MAGNETIC FIELD

机译:磁场作用下浮选镓对流驱动的数值研究

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This paper focuses on the convection of molten gallium contained in an enclosure of aspect ratios 5:1:1.3 subject to horizontal temperature gradient and an external constant magnetic field. Flows without magnetic field are also solved for comparisons by the spectral method. Steady flows and oscillatory flows show different flow structures. The symmetries are strictly maintained for steady flow and the symmetries are broken for oscillatory flow. Near the onset, stable periodical oscillations appear and the symmetries are satisfied between the present state and the state half a period later, which agrees well with the analytical results. The phase characters agree well with the experimental results. Energy analysis shows that the production of fluctuating kinetic energy by shear of mean flow is the main production to the change of the total fluctuating kinetic energy, while viscous effects give the main dissipation term. The dissipation of the fluctuating kinetic energy by magnetic field keeps negative.
机译:本文的重点是在水平温度梯度和外部恒定磁场的作用下,长宽比为5:1:1.3的外壳中包含的熔融镓的对流。无磁场的流动也可以通过光谱法解决,以进行比较。稳定流和振荡流显示不同的流结构。严格保持对称性以实现稳定流动,而对称性则因振荡流动而破裂。在开始附近,出现稳定的周期性振荡,并且在当前状态和半个周期后的状态之间满足对称性,这与分析结果非常吻合。相位特性与实验结果吻合良好。能量分析表明,平均流量切变产生的波动动能是总波动动能变化的主要产物,而粘滞效应是主要的耗散项。磁场对波动动能的耗散保持为负。

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