Outlining the impact of induced magnetic field and thermal radiation on magneto-convection flow of dissipative fluid
In order to deal with many scientific and technological problems such as solar dynamo and planetary problems, magnetohydrodynamics power-generation, plasma confinement, crude oil purification and rotating magnetic stars, we have investigated the steady flow of incompressible, viscous, conducting and...
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Published in: | International journal of thermal sciences Vol. 146; p. 106101 |
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Main Authors: | , , , |
Format: | Journal Article |
Language: | English |
Published: |
Elsevier Masson SAS
01-12-2019
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Subjects: | |
Online Access: | Get full text |
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Summary: | In order to deal with many scientific and technological problems such as solar dynamo and planetary problems, magnetohydrodynamics power-generation, plasma confinement, crude oil purification and rotating magnetic stars, we have investigated the steady flow of incompressible, viscous, conducting and optically thin fluid over a vertical plate with magnetohydrodynamic mixed convection, thermal radiation and viscous dissipation. The solution of governing partial differential equations is obtained by the spectral quasi-linearization method. Apart from finding solution for the induced magnetic field, velocity, and temperature, we have plotted graphs of skin friction and heat transfer coefficients for different pertinent parameters which are mentioned thereat. Results indicate that viscous dissipation has tendency to increase the temperature, induced magnetic field and velocity profiles whereas radiation parameter has opposite effect on it. Viscous dissipation and thermal buoyancy force tend to enhance the skin friction and reduce heat transfer coefficient. However, radiation parameter reduces skin friction and enhances heat transfer coefficient at the surface.
•Using 3-D graphics, the solution of magneto-convection flow of dissipative fluid is presented.•Impact of induced magnetic field is considered.•A very well efficient method i. e. spectral quasilinearization method (SQLM) is used to find out solution of our model.•The induced magnetic field profiles, velocity profiles, temperature profiles are reduced due to thermal radiation.•Thermal buoyancy force has tendency to enhance the skin friction, velocity profiles and induced magnetic field profiles. |
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ISSN: | 1290-0729 1778-4166 |
DOI: | 10.1016/j.ijthermalsci.2019.106101 |