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Computational Aspects of High-Speed Flows With Applied Magnetic Field

机译:施加磁场的高速流动的计算方面

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High-speed flows over the surface of hypersonic airfoil subjected to several types of applied magnetic field distributions are numerically simulated. The governing equations are composed of the Euler equation modified to include the effect of magnetic field. In the current applications, the low magnetic Reynolds number approximation is utilized and the Hall effect and ion slip have been neglected. A fourth-order modified Runge-Kutta scheme augmented with the Davis-Yee symmetric Total Variation Diminishing model in post-processing stage is used to solve the magnetogasdynamics equations. The flow simulations are compared to the existing solutions. A good agreement between the present analysis and the available normal shock data is demonstrated. It has been found that the location and distribution of the imposed magnetic field have dominant effects on the flow parameters and the shock standoff distance.
机译:数值模拟了高超声速翼型表面上的高速流动,该高速流受到几种类型的磁场分布的影响。控制方程由经修改以包括磁场影响的欧拉方程组成。在当前的应用中,利用了低磁性的雷诺数近似值,并且忽略了霍尔效应和离子滑移。在后处理阶段,通过在Davis-Yee对称总变化量减小模型的基础上增强的四阶修改过的Runge-Kutta方案来求解磁气动力学方程。将流动模拟与现有解决方案进行比较。证明了本分析与可用的正常冲击数据之间的良好一致性。已经发现,施加的磁场的位置和分布对流动参数和冲击隔离距离具有主要影响。

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