MHD convection flow due to a rotating disk with hall effect
KA Maleque, MA Sattar - 2005 - dspace.aiub.edu
A steady three-dimensional MHD convective laminar incompressible boundary layer flow
due to an infinite rotating disk in an axial uniform magnetic field is studied taking the effect of
Hall current. It is assumed that the flow is laminar and the boundary layer thickness depends
on the radial distance. Then, by introducing suitable similarity variable η, which is a function
of≅ and r, the governing partial differential equations are reduced to nonlinear ordinary
differential equations. The similarity equations are then solved numerically by Nachtsheim …
due to an infinite rotating disk in an axial uniform magnetic field is studied taking the effect of
Hall current. It is assumed that the flow is laminar and the boundary layer thickness depends
on the radial distance. Then, by introducing suitable similarity variable η, which is a function
of≅ and r, the governing partial differential equations are reduced to nonlinear ordinary
differential equations. The similarity equations are then solved numerically by Nachtsheim …
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