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Numerical Analysis of Double-Diffusive Convection/Solidification Under g-Jitter/Magnetic Fields

机译:g抖动/磁场作用下双扩散对流/固溶的数值分析

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摘要

A finite element model is presented for the g-jitter induced double-diffusive convection and solidification phenomena with and without the presence of magnetic fields in an Sn-doped Bi crystal growth system planned for space experiments. The model is developed based on the deforming finite element formulation with the penalty formulation for pressure approximation. An isothermal front tracking algorithm is used to predict the solid-liquid interface. Extensive numerical simulations are carried out and parameters studied include the solute concentration dependent melting temperature and magnetic field strength under both steady state and g-jitter conditions. Both synthesized g-jitter and real g-jitter data taken from space flights are used. Computed results show that the concentration effects on interface morphology must be considered for an accurate prediction of solidification interface morphology, and g-jitter can induce significant convective flows in the liquid pool, which, in turn, cause solute concentration nonuniformity during the space crystal growth. The use of an applied magnetic field can be effective in suppressing the deleterious g-jitter induced convection and solute nonuniformity and their effects on solidification.
机译:提出了一个有限元模型,用于在计划用于空间实验的Sn掺杂Bi晶体生长系统中存在和不存在磁场的情况下,由g抖动引起的双扩散对流和凝固现象。基于变形有限元公式和用于压力逼近的惩罚公式开发模型。等温前沿跟踪算法用于预测固液界面。进行了广泛的数值模拟,所研究的参数包括在稳态和g抖动条件下与溶质浓度有关的熔化温度和磁场强度。从太空飞行中获取的合成g抖动数据和实际g抖动数据均被使用。计算结果表明,为了准确预测凝固界面形态,必须考虑浓度对界面形态的影响,并且g抖动会在液池中引起明显的对流,从而在空间晶体生长过程中导致溶质浓度不均匀。 。使用施加的磁场可以有效地抑制有害的g-抖动引起的对流和溶质不均匀性及其对固化的影响。

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