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首页> 外文期刊>International Review of Aerospace Engineering >Formation and Dissipation of Karman Vortex Street in an Accelerating Flow Past a Circular Cylinder
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Formation and Dissipation of Karman Vortex Street in an Accelerating Flow Past a Circular Cylinder

机译:绕圆柱加速流中的卡曼涡街的形成与耗散

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Prediction of Karman vortex street in a flow past circular cylinder has become a benchmark problem and many new numerical methods are validated by reproducing the phenomena. The formation and dissipation of Karman vortex street occurs in a range of Reynolds number. But, the conventional Navier-Stokes equations derived in inertial frame of reference based on constant relative velocity are limited to fluid flow problem at a given freestream velocity or Reynolds number. Therefore, in order to capture the formation and dissipation of karman vortex street, several simulations are to be carried out at different freestream velocites. Even then, such simulations will not reveal the continous phenomena of formation and dissipation of vortices. In this work, Navier-Stokes equations are obtained from first principles for fluid flow problems with linear external acceleration in relative acceleration frame of reference, in a form most suited for numerical study. Using these equations, numerical simulation of accelerating flow over circular cylinder is carried out for Reynolds number range, 68 to 1360. The formation and dissipation of Karman vortex street is captured in a single simulation and the results are compared with conventional simulations at various Reynolds numbers. The issues in physical modeling and numerics of using constant freestream acceleration are also discussed in brief. From these simulations, it is demonstrated that the physical phenomena obtained by solving conventional Navier-Stokes equations at various freestream velocities can obtained in a single simulation by using the Navier-Stokes equations written in relative acceleration frame of reference. These equation can be used to explore the physics of accelerating flows in a continuous scenario, without undertaking numerous conventional simulations at various constant freestream velocities.
机译:通过圆柱流的卡曼涡街的预测已成为一个基准问题,并且通过再现该现象验证了许多新的数值方法。 Karman涡街的形成和消散发生在雷诺数范围内。但是,在惯性参考系中基于恒定相对速度导出的常规Navier-Stokes方程仅限于给定的自由流速度或雷诺数下的流体流动问题。因此,为了捕获卡尔曼涡街的形成和消散,将在不同的自由流速度下进行若干模拟。即使这样,这种模拟也不会揭示涡旋形成和消散的连续现象。在这项工作中,Navier-Stokes方程是以最适合数值研究的形式,从相对原理的相对加速度框架中具有线性外部加速度的流体流动问题的第一原理获得的。使用这些方程式,对雷诺数范围为68到1360的圆柱体上的加速流动进行了数值模拟。在单个模拟中捕获了卡曼涡街的形成和消散,并将结果与​​不同雷诺数下的常规模拟进行了比较。 。还简要讨论了物理建模和使用恒定自由流加速的数值问题。从这些模拟中,证明了通过使用相对加速度参考系中编写的Navier-Stokes方程式,可以在单个模拟中获得通过在各种自由流速度下求解常规Navier-Stokes方程式而获得的物理现象。这些方程式可用于探索连续场景中加速流动的物理原理,而无需在各种恒定自由流速度下进行大量常规模拟。

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