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Numerical Solutions of Radiation Effect on Magnetohydrodynamic Free Convection Boundary Layer Flow about a Solid Sphere with Newtonian Heating

In this paper, the effect of radiation on magnetohydrodynamic free convection boundary of a solid sphere with Newtonian heating has been investigated. The basic equations of boundary layer are transformed into a non-dimensional form and reduced to nonlinear systems of partial differential equations...

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Main Authors: Alkasasbeh, Hamzeh Taha, Mohd Zuki, Salleh
Format: Article
Language:English
English
Published: Hikari Ltd 2014
Subjects:
Q Science (General)
Online Access:http://umpir.ump.edu.my/id/eprint/8276/1/Numerical_Solutions_of_Radiation_Effect_on_Magnetohydrodynamic_Free_Convection_Boundary_Layer_Flow_about_a_Solid_Sphere_with_Newtonian_Heating.pdf
http://umpir.ump.edu.my/id/eprint/8276/4/Numerical%20Solutions%20of%20Radiation%20Effect%20on%20Magnetohydrodynamic%20Free%20Convection%20Boundary%20%20Layer%20Flow%20about%20a%20Solid%20Sphere%20with%20Newtonian%20Heating.pdf
http://umpir.ump.edu.my/id/eprint/8276/
http://dx.doi.org/10.12988/ams.2014.48649
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spelling my.ump.umpir.82762018-01-09T00:57:38Z http://umpir.ump.edu.my/id/eprint/8276/ Numerical Solutions of Radiation Effect on Magnetohydrodynamic Free Convection Boundary Layer Flow about a Solid Sphere with Newtonian Heating Alkasasbeh, Hamzeh Taha Mohd Zuki, Salleh Q Science (General) In this paper, the effect of radiation on magnetohydrodynamic free convection boundary of a solid sphere with Newtonian heating has been investigated. The basic equations of boundary layer are transformed into a non-dimensional form and reduced to nonlinear systems of partial differential equations are solved numerically using an implicit finite difference scheme known as the Keller-box method. Numerical solutions are obtained for the wall temperature, the local skin friction coefficient and the local Nusselt number, as well as the velocity and temperature profiles. The features of the flow and heat transfer characteristics for various values of magnetic parameter M, radiation parameter R N and the coordinate running along the surface of the sphere, x are analyzed and discussed. Hikari Ltd 2014 Article PeerReviewed application/pdf en http://umpir.ump.edu.my/id/eprint/8276/1/Numerical_Solutions_of_Radiation_Effect_on_Magnetohydrodynamic_Free_Convection_Boundary_Layer_Flow_about_a_Solid_Sphere_with_Newtonian_Heating.pdf application/pdf en http://umpir.ump.edu.my/id/eprint/8276/4/Numerical%20Solutions%20of%20Radiation%20Effect%20on%20Magnetohydrodynamic%20Free%20Convection%20Boundary%20%20Layer%20Flow%20about%20a%20Solid%20Sphere%20with%20Newtonian%20Heating.pdf Alkasasbeh, Hamzeh Taha and Mohd Zuki, Salleh (2014) Numerical Solutions of Radiation Effect on Magnetohydrodynamic Free Convection Boundary Layer Flow about a Solid Sphere with Newtonian Heating. Applied Mathematical Sciences, 8 (140). pp. 6989-7000. ISSN 1314-7552 (print); 1312-885X (online). (Published) http://dx.doi.org/10.12988/ams.2014.48649 DOI: 10.12988/ams.2014.48649
institution Universiti Malaysia Pahang Al-Sultan Abdullah
building UMPSA Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Malaysia Pahang Al-Sultan Abdullah
content_source UMPSA Institutional Repository
url_provider http://umpir.ump.edu.my/
language English
English
topic Q Science (General)
spellingShingle Q Science (General)
Alkasasbeh, Hamzeh Taha
Mohd Zuki, Salleh
Numerical Solutions of Radiation Effect on Magnetohydrodynamic Free Convection Boundary Layer Flow about a Solid Sphere with Newtonian Heating
description In this paper, the effect of radiation on magnetohydrodynamic free convection boundary of a solid sphere with Newtonian heating has been investigated. The basic equations of boundary layer are transformed into a non-dimensional form and reduced to nonlinear systems of partial differential equations are solved numerically using an implicit finite difference scheme known as the Keller-box method. Numerical solutions are obtained for the wall temperature, the local skin friction coefficient and the local Nusselt number, as well as the velocity and temperature profiles. The features of the flow and heat transfer characteristics for various values of magnetic parameter M, radiation parameter R N and the coordinate running along the surface of the sphere, x are analyzed and discussed.
format Article
author Alkasasbeh, Hamzeh Taha
Mohd Zuki, Salleh
author_facet Alkasasbeh, Hamzeh Taha
Mohd Zuki, Salleh
author_sort Alkasasbeh, Hamzeh Taha
title Numerical Solutions of Radiation Effect on Magnetohydrodynamic Free Convection Boundary Layer Flow about a Solid Sphere with Newtonian Heating
title_short Numerical Solutions of Radiation Effect on Magnetohydrodynamic Free Convection Boundary Layer Flow about a Solid Sphere with Newtonian Heating
title_full Numerical Solutions of Radiation Effect on Magnetohydrodynamic Free Convection Boundary Layer Flow about a Solid Sphere with Newtonian Heating
title_fullStr Numerical Solutions of Radiation Effect on Magnetohydrodynamic Free Convection Boundary Layer Flow about a Solid Sphere with Newtonian Heating
title_full_unstemmed Numerical Solutions of Radiation Effect on Magnetohydrodynamic Free Convection Boundary Layer Flow about a Solid Sphere with Newtonian Heating
title_sort numerical solutions of radiation effect on magnetohydrodynamic free convection boundary layer flow about a solid sphere with newtonian heating
publisher Hikari Ltd
publishDate 2014
url http://umpir.ump.edu.my/id/eprint/8276/1/Numerical_Solutions_of_Radiation_Effect_on_Magnetohydrodynamic_Free_Convection_Boundary_Layer_Flow_about_a_Solid_Sphere_with_Newtonian_Heating.pdf
http://umpir.ump.edu.my/id/eprint/8276/4/Numerical%20Solutions%20of%20Radiation%20Effect%20on%20Magnetohydrodynamic%20Free%20Convection%20Boundary%20%20Layer%20Flow%20about%20a%20Solid%20Sphere%20with%20Newtonian%20Heating.pdf
http://umpir.ump.edu.my/id/eprint/8276/
http://dx.doi.org/10.12988/ams.2014.48649
_version_ 1822916681572286464
score 13.251813

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