NDLI: Magnetohydrodynamic effects on natural convection flow of a nanofluid in the presence of heat source due to solar energy

Content Provider	Springer Nature Link
Author	Anbuchezhian, N. Srinivasan, K. Chandrasekaran, K. Kandasamy, R.
Copyright Year	2012
Abstract	The objective of the present work is to investigate theoretically the MHD convective flow and heat transfer of an incompressible viscous nanofluid past a porous vertical stretching sheet in the presence of variable stream condition due to solar radiation (incident radiation). The governing equations are derived using the usual boundary-layer and Boussinesq approximations and accounting for the presence of an applied magnetic field and incident radiation flux. The absorbed radiation acts as a distributed source which initiates buoyancy-driven flow and convection in the absorbed layer. The partial differential equations governing the problem under consideration are transformed by a special form of Lie symmetry group transformations viz. one-parameter group of transformation into a system of ordinary differential equations which are solved numerically using Runge Kutta Gill based shooting method. The conclusion is drawn that the flow field and temperature are significantly influenced by radiation, heat source and magnetic field.
Starting Page	307
Ending Page	321
Page Count	15
File Format	PDF
ISSN	00256455
Journal	Meccanica
Volume Number	48
Issue Number	2
e-ISSN	15729648
Language	English
Publisher	Springer Netherlands
Publisher Date	2012-10-03
Publisher Place	Dordrecht
Access Restriction	One Nation One Subscription (ONOS)
Subject Keyword	Lie symmetry group transformation Nanofluids Porous media Magnetic field Convective radiation Heat source Mechanics Civil Engineering Automotive Engineering Mechanical Engineering
Content Type	Text
Resource Type	Article
Subject	Mechanics of Materials Condensed Matter Physics Mechanical Engineering

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Comment on the paper “Magnetohydrodynamic effects on natural convection flow of a nanofluid in the presence of heat source due to solar energy, N. Anbuchezhian, K. Srinivasan, K. Chandrasekaran, R. Kandasamy, Meccanica (2013) 48:307–321”

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Comment on the paper “Magnetohydrodynamic effects on natural convection flow of a nanofluid in the presence of heat source due to solar energy, N. Anbuchezhian, K. Srinivasan, K. Chandrasekaran, R. Kandasamy, Meccanica (2013) 48:307–321”

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