Effect of thermal radiation on MHD flow

Raptis, A.; Perdikis, C.; Takhar, H. S.

doi:10.1016/s0096-3003(03)00657-x

Cited by 165 publications

(115 citation statements)

References 8 publications

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“…The free convection flow in the presence of radiation has been previously studied by Ali et al [1], Seddeek and Abdelmeguid [2], Raptis and Toki [3], and Malekzadeh et al [4]. The magnetohydrodynamic (MHD) flow in the presence of radiation has been investigated by Chamkha et al [5], Raptis et al [6], Duwairi [7], Ouaf [8], Abd-El Aziz [9], Pal and Mondal [10] and Shit and Haldar [11]. The flow through a porous medium in the presence of radiation has been studied by Murthy et al [12], Al-Harbi [13], Al-Odat et al [14], Raptis and Perdikis [15], Duwairi [16] and Badruddin et al [17], and Awad et al [18].…”

Section: Introductionmentioning

confidence: 99%

Radiation Effects on Flow past a Stretching Plate with Temperature Dependent Viscosity

Xenos¹

2013

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The effect of radiation on the flow over a stretching plate of an optically thin gray, viscous and incompressible fluid is studied. The fluid viscosity is assumed to vary as an inverse linear function of the temperature. The partial differential equations (PDEs) and their boundary conditions, describing the problem under consideration, are dimensionalized and the numerical solution is obtained by using the finite volume discretization methodology which is suitable for fluid mechanics applications. The numerical results for the velocity and temperature profiles are shown for different dimensionless parameters entering the problem under consideration, such as the temperature parameter, θ r , the radiation parameter, S, and the Prandtl number, Pr. The numerical results indicate a strong influence of these parameters on the non-dimensional velocity and temperature profiles in the boundary layer.

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Section: Introductionmentioning

confidence: 99%

Radiation Effects on Flow past a Stretching Plate with Temperature Dependent Viscosity

Xenos¹

2013

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“…9 Gretler and Regenfelder 10 obtained similarity solution for laser-driven shock waves in a dust-laden gas with internal heat transfer effects. Raptis et al 11 of an electrically conducting fluid past a semi-infinite stationary plate in presence of radiation. Heat and mass transfer effects on moving plate in the presence of thermal radiation using Laplace technique have been studied by Muthukumarswamy and Senthil.…”

Section: Introductionmentioning

confidence: 99%

MHD free convection flow of a visco-elastic (Kuvshiniski type) dusty gas through a semi infinite plate moving with velocity decreasing exponentially with time and radiative heat transfer

Prakash

Kumar²,

Dwivedi³

2011

AIP Advances

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The present paper is concerned with the study of MHD free convective flow of a visco-elastic (Kuvshinski type) dusty gas through a porous medium induced by the motion of a semi-infinite flat plate under the influence of radiative heat transfer moving with velocity decreasing exponentially with time. The expressions for velocity distribution of a dusty gas and dust particles, concentration profile and temperature field are obtained. The effect of Schmidt number (Sc), Magnetic field parameter (M) and Radiation parameter (N) on velocity distribution of dusty gas and dust particles, concentration and temperature distribution are discussed graphically

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“…Ghosh and Pop [10] have studied thermal radiation of an optically thick gray gas in the presence of indirect natural convection. Recently, several studies on radiative heat transfer have been reported by Raptis et al [11], Duwairi and duwairi [12], Vasil'ev and Nesterov [13], Duwairi [14], Quaf MEM [15], Ghosh [16,17], Zueco [18], Samad and Rahman [19] and Beg and Ghosh [20]. In the light of Ghosh and Pop [10] work it is stated that the effect of pressure on velocity remains present at y   for > 0 t so that the pressure rise region near the leading edge of the hot plate leads to increase the velocity .Thus it comes to a justification of this problem leading to a fact that the pressure becomes absent due to a stagnation point flow.…”

Section: Introductionmentioning

confidence: 99%

Radiative Heat Transfer of an Optically Thick Gray Gas in The Presence of Indirect Natural Convection

Jana¹,

Ghosh²

2011

WJM

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We study the effects of thermal radiation of a viscous incompressible fluid occupying a semi-infinite region of space bounded by an infinite horizontal moving hot flat plate in the presence of indirect natural convection by way of an induced pressure gradient. The fluid is a gray, absorbing emitting radiation but a non scattering medium. An exact solution is obtained by employing Laplace transform technique. Since temperature field depends on Reynold number the flow is considered to be non-isothermal case (the temperature of the plate T w ≠ constant) and for an isothermal case (T w = constant) the flow is determined by the Reynold number which is equal to 1.

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Effect of thermal radiation on MHD flow

Cited by 165 publications

References 8 publications

Radiation Effects on Flow past a Stretching Plate with Temperature Dependent Viscosity

Radiation Effects on Flow past a Stretching Plate with Temperature Dependent Viscosity

MHD free convection flow of a visco-elastic (Kuvshiniski type) dusty gas through a semi infinite plate moving with velocity decreasing exponentially with time and radiative heat transfer

Radiative Heat Transfer of an Optically Thick Gray Gas in The Presence of Indirect Natural Convection

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