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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/11119
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dc.contributor.authorSharma, Bhupendra Kumar-
dc.date.accessioned2023-08-03T05:24:03Z-
dc.date.available2023-08-03T05:24:03Z-
dc.date.issued2017-
dc.identifier.urihttps://link.springer.com/article/10.1007/s10891-017-1710-y-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/xmlui/handle/123456789/11119-
dc.description.abstractA numerical study of an oscillatory unsteady MHD flow and heat and mass transfer in a vertical rotating channel with an inclined uniform magnetic field and the Hall effect is carried out. The conservation equations of momentum, energy, and species are formulated in a rotating frame of reference with inclusion of the buoyancy effects and Lorentz forces. The Lorentz forces are determined by using the generalized Ohm law with the Hall parameter taken into account. The obtained coupled partial differential equations are nondimensionalized and solved numerically by using the explicit finite difference method. The effects of various model parameters, like the Hall parameter, Hartmann number, wall suction/injection parameter, rotation parameter, angle of magnetic field inclination, Prandtl number, Schmidt number, etc., on the channel velocities, skin friction coefficients, Nusselt number, and the Sherwood number are examined. It is found that the influence of the Hartmann number and Hall parameter on the channel velocities and skin friction coefficients is dependent on the value of the wall suction/injection parameteren_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectMagnetic fielden_US
dc.subjectMathematicsen_US
dc.subjectHall effecten_US
dc.titleMHD Mixed Convection Flow in a Rotating Channel in the Presence of an Inclined Magnetic Field with the Hall Effecten_US
dc.typeArticleen_US
Appears in Collections:Department of Mathematics

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