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contributor authorSiddiqa, Sadia
contributor authorBegum, Naheed
contributor authorHossain, Md. Anwar
contributor authorAl-Rashed, Abdullah A. A. A.
date accessioned2019-02-28T11:08:11Z
date available2019-02-28T11:08:11Z
date copyright8/29/2017 12:00:00 AM
date issued2018
identifier issn1948-5085
identifier othertsea_010_02_021005.pdf
identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4253062
description abstractIn this paper, numerical solutions to thermally radiating Marangoni convection of dusty fluid flow along a vertical wavy surface are established. The results are obtained with the understanding that the dust particles are of uniform size and dispersed in optically thick fluid. The numerical solutions of the dimensionless transformed equations are obtained through straightforward implicit finite difference scheme. In order to analyze the influence of various controlling parameters, results are displayed in the form of rate of heat transfer, skin friction coefficient, velocity and temperature profiles, streamlines, and isotherms. It is observed that the variation in thermal radiation parameter significantly alters the corresponding particle pattern and extensively promotes the heat transfer rate.
publisherThe American Society of Mechanical Engineers (ASME)
titleNumerical Estimation of Thermal Radiation Effects on Marangoni Convection of Dusty Fluid
typeJournal Paper
journal volume10
journal issue2
journal titleJournal of Thermal Science and Engineering Applications
identifier doi10.1115/1.4037209
journal fristpage21005
journal lastpage021005-7
treeJournal of Thermal Science and Engineering Applications:;2018:;volume( 010 ):;issue: 002
contenttypeFulltext


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