In this study, the effects of temperature dependent viscosity on MHD natural convection flow past an isothermal sphere are determined. The uniformly heated sphere is immersed in a viscous and incompressible fluid where viscosity of the fluid is taken as a non-linear function of temperature. The Partial Differential Equations governing the flow are transformed into non dimensional form and solved using the Direct Numerical Scheme and implemented in MATLAB. The numerical results obtained are presented graphically and in tables and are discussed. In this study, it has been observed that increasing the Magnetic parameter M leads to decrease in velocity, temperature, skin friction and the rate of heat transfer. It has also been noted that increase in the Grashof number Gr leads to increase in velocity and temperature whereas increase in the values of eta η leads to increase in temperature but there is a decrease in velocity. These results are applicable to engineers in designing electricity plants which have higher life expectancy.
Published in | American Journal of Applied Mathematics (Volume 4, Issue 1) |
DOI | 10.11648/j.ajam.20160401.15 |
Page(s) | 53-61 |
Creative Commons |
This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited. |
Copyright |
Copyright © The Author(s), 2016. Published by Science Publishing Group |
Natural Convection Flow, Temperature Dependent Viscosity, Magnetohydrodynamic (MHD), Isothermal Sphere
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APA Style
Mwangi Wanjiku Lucy, Mathew Ngugi Kinyanjui, Surindar Mohan Uppal. (2016). Effects of Temperature Dependent Viscosity on Magnetohydrodynamic Natural Convection Flow Past an Isothermal Sphere. American Journal of Applied Mathematics, 4(1), 53-61. https://doi.org/10.11648/j.ajam.20160401.15
ACS Style
Mwangi Wanjiku Lucy; Mathew Ngugi Kinyanjui; Surindar Mohan Uppal. Effects of Temperature Dependent Viscosity on Magnetohydrodynamic Natural Convection Flow Past an Isothermal Sphere. Am. J. Appl. Math. 2016, 4(1), 53-61. doi: 10.11648/j.ajam.20160401.15
AMA Style
Mwangi Wanjiku Lucy, Mathew Ngugi Kinyanjui, Surindar Mohan Uppal. Effects of Temperature Dependent Viscosity on Magnetohydrodynamic Natural Convection Flow Past an Isothermal Sphere. Am J Appl Math. 2016;4(1):53-61. doi: 10.11648/j.ajam.20160401.15
@article{10.11648/j.ajam.20160401.15, author = {Mwangi Wanjiku Lucy and Mathew Ngugi Kinyanjui and Surindar Mohan Uppal}, title = {Effects of Temperature Dependent Viscosity on Magnetohydrodynamic Natural Convection Flow Past an Isothermal Sphere}, journal = {American Journal of Applied Mathematics}, volume = {4}, number = {1}, pages = {53-61}, doi = {10.11648/j.ajam.20160401.15}, url = {https://doi.org/10.11648/j.ajam.20160401.15}, eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajam.20160401.15}, abstract = {In this study, the effects of temperature dependent viscosity on MHD natural convection flow past an isothermal sphere are determined. The uniformly heated sphere is immersed in a viscous and incompressible fluid where viscosity of the fluid is taken as a non-linear function of temperature. The Partial Differential Equations governing the flow are transformed into non dimensional form and solved using the Direct Numerical Scheme and implemented in MATLAB. The numerical results obtained are presented graphically and in tables and are discussed. In this study, it has been observed that increasing the Magnetic parameter M leads to decrease in velocity, temperature, skin friction and the rate of heat transfer. It has also been noted that increase in the Grashof number Gr leads to increase in velocity and temperature whereas increase in the values of eta η leads to increase in temperature but there is a decrease in velocity. These results are applicable to engineers in designing electricity plants which have higher life expectancy.}, year = {2016} }
TY - JOUR T1 - Effects of Temperature Dependent Viscosity on Magnetohydrodynamic Natural Convection Flow Past an Isothermal Sphere AU - Mwangi Wanjiku Lucy AU - Mathew Ngugi Kinyanjui AU - Surindar Mohan Uppal Y1 - 2016/02/25 PY - 2016 N1 - https://doi.org/10.11648/j.ajam.20160401.15 DO - 10.11648/j.ajam.20160401.15 T2 - American Journal of Applied Mathematics JF - American Journal of Applied Mathematics JO - American Journal of Applied Mathematics SP - 53 EP - 61 PB - Science Publishing Group SN - 2330-006X UR - https://doi.org/10.11648/j.ajam.20160401.15 AB - In this study, the effects of temperature dependent viscosity on MHD natural convection flow past an isothermal sphere are determined. The uniformly heated sphere is immersed in a viscous and incompressible fluid where viscosity of the fluid is taken as a non-linear function of temperature. The Partial Differential Equations governing the flow are transformed into non dimensional form and solved using the Direct Numerical Scheme and implemented in MATLAB. The numerical results obtained are presented graphically and in tables and are discussed. In this study, it has been observed that increasing the Magnetic parameter M leads to decrease in velocity, temperature, skin friction and the rate of heat transfer. It has also been noted that increase in the Grashof number Gr leads to increase in velocity and temperature whereas increase in the values of eta η leads to increase in temperature but there is a decrease in velocity. These results are applicable to engineers in designing electricity plants which have higher life expectancy. VL - 4 IS - 1 ER -