具有热辐射、多孔介质和可变热通量的非稳态拉伸薄板引起的磁流体动力学流动

IF 1.6 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Advances in Astronomy Pub Date : 2021-01-31 DOI:10.1155/2021/6686883
A. Megahed, N. Ghoneim, M. G. Reddy, M. El-Khatib
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引用次数: 9

摘要

介绍了一种确定牛顿磁流体动力学层流流动常微分方程的数值解的射击方法,该方程是由于非定常拉伸片以及热辐射和变热流通量的存在而引起的。考虑了变粘度和变电导率。在一些研究中,磁场的缺失限制了节能换热机制的发展,而这在许多应用中是需要的。本研究包括非定常参数、多孔参数、粘度参数、磁数、辐射参数、电导率参数等参数。实验结果表明,该模型优于现有的工业流体模型。
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Magnetohydrodynamic Fluid Flow due to an Unsteady Stretching Sheet with Thermal Radiation, Porous Medium, and Variable Heat Flux
A shooting method has been introduced for determining the numerical solution of the ordinary differential equations which describe the Newtonian magnetohydrodynamic laminar fluid flow due to an unsteady stretching sheet together with the presence of thermal radiation and variable heat flux. The variable viscosity and variable conductivity are taken into consideration. Absence of magnetic field in some studies restricts the development of the energy-efficient heat transfer mechanism as is desired in numerous applications. The present study encompasses parameters such as unsteadiness parameter, porous parameter, viscosity parameter, magnetic number, radiation parameter, and conductivity parameter. It has been consummated that the proposed model is superior to other existing models for the industrial fluid.
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来源期刊
Advances in Astronomy
Advances in Astronomy ASTRONOMY & ASTROPHYSICS-
CiteScore
2.70
自引率
7.10%
发文量
10
审稿时长
22 weeks
期刊介绍: Advances in Astronomy publishes articles in all areas of astronomy, astrophysics, and cosmology. The journal accepts both observational and theoretical investigations into celestial objects and the wider universe, as well as the reports of new methods and instrumentation for their study.
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