Abstract

An analysis of an unsteady MHD convective flow of an electrically conducting viscous incompressible fluid through porous medium filled in a vertical porous channel is carried out. The two porous plates are subjected to a constant injection and suction velocity as shown in Fig. 1a, b. The temperature of the plate at y*= + 9 2 is assumed to be varying in space and time as T*(y*, z*, t*) = T1 (y*) + (T2 - T1)COS (πz*d -ω*t*). A magnetic field of uniform strength is applied perpendicular to the plates of the channel. The temperature difference between the plates is high enough to induce the heat due to radiation. It is also assumed that the conducting fluid is opticallythin gray gas, absorbing/ emitting radiation and non-scattering. The Hall current effects have also been taken into account. Exact solution of the partial differential equations governing the flow under the prescribed boundary conditions has been obtained for the velocity and the temperature fields. The primary and secondary velocities, temperature and the skin-friction and Nusselt number for the rate of heat transfer in terms of their amplitudes and phase angles have been shown graphically to observe the effects of suction parameter λ, Grashof number Gr, Hartmann number M, Hall parameter H, the permeability of the porous medium K, Prandtl number Pr, radiation parameter N, pressure gradient A and the frequency of oscillation ω. The final results are then discussed in detail in the last section of the paper with the help of figures.

Highlights

  • The study of MHD free convection flow for electrically conducting fluid has attracted the attention of many scholars in view of its applications in many engineering problems such as meteorology, solar physics, motion of earth's core and chemical engineering etc

  • These days the convective flows through porous medium is receiving considerable attention due to its application in geophysical and astrophysical importance

  • YEN and CHANG [29] analyzed the effect of wall electrical conductance on the magnetohydrodynamic Couette flow

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Summary

Introduction

The study of MHD free convection flow for electrically conducting fluid has attracted the attention of many scholars in view of its applications in many engineering problems such as meteorology, solar physics, motion of earth's core and chemical engineering etc. These days the convective flows through porous medium is receiving considerable attention due to its application in geophysical and astrophysical importance. In astrophysics it is applied to study the stellar and solar structure, inter planetary and inter stellar matter, solar storms and flares etc In engineering it finds its application in MHD generators, ion propulsion, MHD bearings, MHD pumps, MHD boundary layer control of re-entryof space vehicles etc. ATTIA [4] discussed unsteady MHD Couette flow of a viscoelastic fluid with heat transfer. ATTIA and KOTB [5] investigated MHD flow between two parallel porous plates with heat transfer. HASSANIEN and MANSOUR [12] studied an unsteady magnetic flow through a porous medium between two infinite parallel plates

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