The system will be unavailable for updates from 12:30 on Tuesday 23 May to prepare for the upgrade of the software platform.

Heat transfer to MHD oscillatory dusty fluid flow in a channel filled with a porous medium

Prakash, O. M. ; Makinde, O. D. ; Kumar, Devendra ; Dwivedi, Y. K. (2015)

CITATION: Prakash, O. M., Makinde, O. D., Kumar, D. & Dwivedi, Y. K. 2015. Heat transfer to MHD oscillatory dusty fluid flow in a channel filled with a porous medium. Sadhana, 40(4):1273–1282, doi:10.1007/s12046-015-0371-9.

The original publication is available at http://link.springer.com/journal/12046

Article

In this paper, we examine the combined effects of thermal radiation, buoyancy force and magnetic field on oscillatory flow of a conducting optically thin dusty fluid through a vertical channel filled with a saturated porous medium. The governing partial differential equations are obtained and solved analytically by variable separable method. Numerical results depicting the effects of various embedded parameters like radiation number, Hartmann number and Grashof number on dusty fluid velocity profiles, temperature profiles, Nusselt number and skin friction coefficient are presented graphically and discussed qualitatively.

Please refer to this item in SUNScholar by using the following persistent URL: http://hdl.handle.net/10019.1/99454


VIEW METADATA
This item appears in the following collections: