Free convection effects and radiative heat transfer in MHD Stokes problem for the flow of dusty conducting fluid through porous medium

被引:0
|
作者
OM PRAKASH
DEVENDRA KUMAR
Y K DWIVEDI
机构
[1] Hindustan College of Science & Technology,Department of Mathematics
[2] Sachdeva Institute of Technology,Department of Mathematics
[3] Ganjdundwara P.G. College,Department of Mathematics
来源
Pramana | 2012年 / 78卷
关键词
MHD flow; finite difference technique; porosity; radiative heat transfer; free convection; 47; 47.11. Bc; 47.10.Ad;
D O I
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学科分类号
摘要
The present note deals with the effects of radiative heat transfer and free convection in MHD for a flow of an electrically conducting, incompressible, dusty viscous fluid past an impulsively started vertical non-conducting plate, under the influence of transversely applied magnetic field. The heat due to viscous dissipation and induced magnetic field is assumed to be negligible. The governing linear partial differential equations are solved by finite difference technique. The effects of various parameters (like radiation parameter N, Prandtl number Pr, porosity parameter K) entering into the MHD Stokes problem for flow of dusty conducting fluid have been examined on the temperature field and velocity profile for both the dusty fluid and dust particles.
引用
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页码:429 / 438
页数:9
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