Impacts of radiative heat flux and heat acquisition on steady Magneto hydrodynamics with viscous and ohmic dissipation, Free convection casson fluid flow between porous plates

Usman M.A, Lawal O.W, Peter B.A.
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Abstract

An investigation was conducted on a steady magnetohydrodynamic (MHD) free convection flow of a Casson fluid across a parallel vertical plate immersed in a porous medium with viscous and magnetic dissipation. In addition, the energy equation contains terms for radiational heat flow, heat injection, and suction. The perturbation approach provides an analytical solution to the governing nonlinear partial differential equations underlying this phenomenon. The numerical approach in the Maple program was used to verify the correctness of the outcomes produced by the perturbation technique. The Grashof and Prandtl numbers, Casson fluid, magnetic field, and porosity parameters as well as radiation parameter, and heat injection/suction parameter impact on the flow is discussed graphically. Skin friction coefficient and Nusselt number are tabulated for a range of magnetic and radiative parameter values. The other physical factors listed above accelerate the fluid velocity, but the magnetic field decreases it. Furthermore, the wall shear stress and heat transfer were significantly impacted by the magnetic and radiative factors.
辐射热通量和热获取对具有粘性和欧姆耗散的稳定磁流体力学的影响,多孔板之间的自由对流卡松流体流动
研究了卡松流体穿过浸没在多孔介质中的平行垂直板的稳定磁流体力学(MHD)自由对流,该流体具有粘性和磁性耗散。此外,能量方程还包含辐射热流、热注入和吸力等项。扰动法为这一现象背后的非线性偏微分方程提供了解析解。我们使用 Maple 程序中的数值方法来验证扰动技术所产生结果的正确性。图解讨论了格拉肖夫数和普朗特尔数、卡森流体、磁场和孔隙度参数以及辐射参数和注热/吸热参数对流动的影响。表中列出了一系列磁场和辐射参数值下的表皮摩擦系数和努塞尔特数。上述其他物理因素加速了流体速度,但磁场降低了流体速度。此外,壁面剪应力和传热也受到磁场和辐射因素的显著影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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