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Stability of MHD Wall driven Flow through a Tube

机译:MHD壁驱动流过管的稳定性

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In this work, wall driven incompressible viscous fluid flow through a tube in the presence of magnetic field is considered. The mathematical model of the problem is formulated and solved using series solution method and Hermite-Pade approximation method. Flow becomes unstable due to movement of wall and existence of magnetic field where critical Reynolds number and critical Hart-mann number indicate the point of flow instability. This critical point for instability in terms of Reynolds number and Hartmann number are determined and described using bifurcation diagrams. The effect of these two dimensionless numbers on flow velocity and their interaction on flow stability are discussed.
机译:在这项工作中,考虑壁驱动的不可压缩的粘性粘性流体在磁场存在下通过管流动。 使用串联解决方案方法和Hermite-Pade近似法制定和解决了问题的数学模型。 由于壁的运动和磁场的存在,流动变得不稳定,其中临界雷诺数和关键的HART-MANN号表示流动不稳定点。 在雷诺数和Hartmann号方面的这种关键点是使用分叉图确定和描述的。 讨论了这两种无量纲数对流速的影响及其对流动稳定性的相互作用。

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