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MHD flow and heat transfer in a backward-facing step

机译:MHD向后流动和传热

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The laminar flow of a viscous incompressible electrically conducting fluid in a backward-facing step is investigated under the usual magnetohydrodynamic (MHD) hypothesis. Numerical simulations are performed for Reynolds numbers less then Re = 380 in the range of 0 ≤ N ≤ 0.2, where N is the Stuart number or interaction parameter which is the ratio of electromagnetic force to inertia force. Heat transfer is investigated for Prandtl number ranging from Pr = 0.02 corresponding to liquid metal, to Pr = 7 corresponding to water. It is found through the calculation of the reattachment length that external magnetic field acts to decrease the size of the recirculation zone. Velocity profiles show that, out of the recirculation zone, the basic flow is damped by the magnetic induced force, whereas flow near the walls channel is accelerated. Heat transfer is significantly enhanced by the magnetic field in the case of fluids of high Prandtl numbers.
机译:在通常的磁流体动力学(MHD)假设下,研究了向后步骤中粘性不可压缩导电流体的层流。在0≤N≤0.2的范围内,对小于Re = 380的雷诺数进行数值模拟,其中N是Stuart数或相互作用参数,即电磁力与惯性力的比。研究了传热的普朗特数,其范围从对应于液态金属的Pr = 0.02到对应于水的Pr = 7。通过重新连接长度的计算发现,外部磁场起到减小再循环区域的尺寸的作用。速度曲线显示,在再循环区域之外,基本流被磁感应力衰减,而壁通道附近的流被加速。在高普朗特数流体的情况下,磁场会大大增强传热。

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