Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
760097 | Communications in Nonlinear Science and Numerical Simulation | 2007 | 21 Pages |
Abstract
The magnetohydrodynamic (MHD) flow due to non-coaxial rotations of a porous disk, moving with uniform acceleration in its own plane and a second grade fluid at infinity is examined. The fluid is electrically conducting in the presence of a uniform magnetic field. The effects of non-Newtonian fluid characteristics and uniform acceleration of the disk on the velocity field are presented both analytically and numerically. A very good accuracy has been seen.
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Authors
S. Asghar, K. Hanif, T. Hayat, C.M. Khalique,