Abstract
An analysis of the effects of Hall current on hydromagnetic free-convective flow through a porous medium bounded by a vertical plate is theoretically investigated when a strong magnetic field is imposed in a direction which is perpendicular to the free stream and makes an angle α to the vertical direction. The influence of Hall currents on the flow is studied for various values of α.
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Abbreviations
- c p :
-
specific heat at constant pressure
- e :
-
electrical charge
- E :
-
Eckert number
- E :
-
electrical field intensity
- g :
-
acceleration due to gravity
- G :
-
Grashof number
- H 0 :
-
applied magnetic field
- H :
-
magnetic field intensity
- (j ′x , j ′y , j ′z ):
-
components of current densityJ
- J :
-
current density
- K′ :
-
permeability of porous medium
- M :
-
magnetic parameter
- m :
-
Hall parameter
- n e :
-
electron number density
- P :
-
Prandtl number
- q :
-
velocity vector
- (T′, T ′w , T ′∞ ):
-
temperature
- t :
-
time
- (u, v, w):
-
components of the velocity vectorq
- U 0 :
-
uniform velocity
- v 0 :
-
suction velocity
- (x′, y′, z′):
-
Cartesian coordinates
- α:
-
angle
- β :
-
coefficient of volume expansion
- ωe :
-
cyclotron frequency
- ω:
-
frequency
- Θ:
-
dimensionless temperature
- ϰ:
-
thermal conductivity
- μ:
-
coefficient of viscosity
- μ:
-
magnetic permeability
- ν:
-
kinematic viscosity
- ρ:
-
mass density of fluid
- ρe :
-
charge density
- σ:
-
electrical conductivity
- τe :
-
electron collision time
References
Cowling, T. G.: 1957,Magnetohydrodynamics, Interscience Publishers. New York.
Datta, N. and Mazumder, B. S.: 1976,Int. J. Eng. Sci. 14, 285.
Ram, P. C., Singh, C. B., and Singh, U. S.: 1984,Astrophys. Space Sci. 100, 45.
Raptis, A.: 1984,Arch. Mech. 36, 307.
Raptis, A. and Perdikis, C. P.: 1983,Int. J. Energy Res. 7, 391.
Raptis, A. and Perdikis, C. P.: 1985,Int. J. Eng. Sci. 23, 51.
Soundalgekar, V. M.: 1973a,Proc. Roy. Soc. (London) 333A, 25.
Soundalgekar, V. M.: 1973b,Proc. Roy. Soc. (London) 333A, 38.
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Takhar, H.S., Ram, P.C. Effects of Hall current on hydromagnetic free-convective flow through a porous medium. Astrophys Space Sci 192, 45–51 (1992). https://doi.org/10.1007/BF00653258
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DOI: https://doi.org/10.1007/BF00653258