Instability of magnetohydrodynamic flow of Hartmann layers between parallel plates
This study investigates the linear stability of the Hartmann layers of an electrically conductive fluid between parallel plates under the impact of a transverse magnetic field. The corresponding Orr–Sommerfeld equations are numerically solved using Chebyshev’s pseudo-spectral method with Chebyshev p...
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Online Access: | http://dx.doi.org/10.1063/1.5086975 |
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doaj-99b54c182fcf4419a6a113f824525c8c2020-11-24T21:43:37ZengAIP Publishing LLCAIP Advances2158-32262019-05-0195055003055003-810.1063/1.5086975122904ADVInstability of magnetohydrodynamic flow of Hartmann layers between parallel platesZhang Yang0Zakir Hussain1Abid Hussanan2Sultan Hussain3Huisheng Zhang4Department of Biomedical Engineering, School of Medicine, Shenzhen University, Shenzhen 518060, P. R. ChinaDepartment of Biomedical Engineering, School of Medicine, Shenzhen University, Shenzhen 518060, P. R. ChinaCollege of Mathematics and Statistics, Shenzhen University, Shenzhen 518060, P. R. ChinaDepartment of Mathematics, COMSATS University Islamabad, Abbottabad Campus, 22060, PakistanDepartment of Biomedical Engineering, School of Medicine, Shenzhen University, Shenzhen 518060, P. R. ChinaThis study investigates the linear stability of the Hartmann layers of an electrically conductive fluid between parallel plates under the impact of a transverse magnetic field. The corresponding Orr–Sommerfeld equations are numerically solved using Chebyshev’s pseudo-spectral method with Chebyshev polynomial expansion. The QZ algorithm is applied to find neutral linear instability curves. Details of the instability are evaluated by solving the generalized Orr–Sommerfeld system, allowing growth rates to be determined. The results confirm that a magnetic field provides a stabilizing impact to the flow, and the extent of this impact is demonstrated for a range of Reynolds numbers. From numerical simulations, it is observed that a magnetic field with a specific magnitude stabilizes the Hartmann flow. Further, the critical Reynolds number increases rapidly when the Hartmann number is greater than 0.7. Finally, it is shown that a transverse magnetic field overcomes the instability in the flow.http://dx.doi.org/10.1063/1.5086975 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Zhang Yang Zakir Hussain Abid Hussanan Sultan Hussain Huisheng Zhang |
spellingShingle |
Zhang Yang Zakir Hussain Abid Hussanan Sultan Hussain Huisheng Zhang Instability of magnetohydrodynamic flow of Hartmann layers between parallel plates AIP Advances |
author_facet |
Zhang Yang Zakir Hussain Abid Hussanan Sultan Hussain Huisheng Zhang |
author_sort |
Zhang Yang |
title |
Instability of magnetohydrodynamic flow of Hartmann layers between parallel plates |
title_short |
Instability of magnetohydrodynamic flow of Hartmann layers between parallel plates |
title_full |
Instability of magnetohydrodynamic flow of Hartmann layers between parallel plates |
title_fullStr |
Instability of magnetohydrodynamic flow of Hartmann layers between parallel plates |
title_full_unstemmed |
Instability of magnetohydrodynamic flow of Hartmann layers between parallel plates |
title_sort |
instability of magnetohydrodynamic flow of hartmann layers between parallel plates |
publisher |
AIP Publishing LLC |
series |
AIP Advances |
issn |
2158-3226 |
publishDate |
2019-05-01 |
description |
This study investigates the linear stability of the Hartmann layers of an electrically conductive fluid between parallel plates under the impact of a transverse magnetic field. The corresponding Orr–Sommerfeld equations are numerically solved using Chebyshev’s pseudo-spectral method with Chebyshev polynomial expansion. The QZ algorithm is applied to find neutral linear instability curves. Details of the instability are evaluated by solving the generalized Orr–Sommerfeld system, allowing growth rates to be determined. The results confirm that a magnetic field provides a stabilizing impact to the flow, and the extent of this impact is demonstrated for a range of Reynolds numbers. From numerical simulations, it is observed that a magnetic field with a specific magnitude stabilizes the Hartmann flow. Further, the critical Reynolds number increases rapidly when the Hartmann number is greater than 0.7. Finally, it is shown that a transverse magnetic field overcomes the instability in the flow. |
url |
http://dx.doi.org/10.1063/1.5086975 |
work_keys_str_mv |
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