首页> 外文期刊>International Journal of Heat and Mass Transfer >The effects of radiation optical properties on the unsteady 2D boundary layer MHD flow and heat transfer over a stretching plate
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The effects of radiation optical properties on the unsteady 2D boundary layer MHD flow and heat transfer over a stretching plate

机译:辐射光学特性对二维非定常边界层MHD流动和在拉伸板上传热的影响

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In this work, the effects of radiation optical properties and Lorentz force on the 2D unsteady laminar boundary magnetohydrodynamic (MHD) fluid flow and heat transfer along a semi-infinite stretching plate are numerically investigated, the Joule heating effect and viscous dissipation are considered. The heat flux caused by the thermal radiation is obtained by solving the radiation transfer equation (RTE) instead of the Rosseland approximation. All the governing equations, including continuous equation, momentum equation, energy equation, and RTE subject to the boundary radiative emission, are transformed into dimensionless forms. The dimensionless governing equations together with the corresponding boundary conditions are solved numerically via Chebyshev collocation spectral method (CCSM). The effects of various physical parameters, say, Ha, Pr, Ec and Pl, especially the optical properties such as the optical thickness, the scattering albedo, and the wall emissivity of the plate, on the flow and heat transfer are depicted graphically and analyzed in detail. It is found that, due to the thermal radiation, the overall average temperature within the boundary layer becomes much higher and the boundary layer becomes thicker. The magnetic force can suppress the fluid flow significantly and stop the convective heat transfer effectively. Viscous dissipation and Joule heating greatly enhance the temperature distribution with the help of the magnetic field.
机译:在这项工作中,数值研究了辐射光学特性和洛伦兹力对二维非定常层流边界磁流体动力学(MHD)流体沿半无限拉伸板流动和传热的影响,并考虑了焦耳热效应和粘性耗散。通过求解辐射传递方程(RTE)而不是Rosseland逼近来获得由热辐射引起的热通量。所有的控制方程,包括连续方程,动量方程,能量方程和受边界辐射发射影响的RTE,都转换为无量纲形式。通过切比雪夫搭配谱法(CCSM)数值求解无量纲控制方程以及相应的边界条件。图形化地描述并分析了各种物理参数(例如,Ha,Pr,Ec和Pl),特别是光学特性(例如光学厚度,散射反照率和板的壁发射率)对流动和传热的影响。详细。已经发现,由于热辐射,边界层内的整体平均温度变得更高并且边界层变得更厚。磁力可以显着抑制流体流动,并有效地阻止对流传热。借助磁场,粘性耗散和焦耳加热极大地提高了温度分布。

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