M
M. Venkatachalappa
Researcher at Bangalore University
Publications - 17
Citations - 905
M. Venkatachalappa is an academic researcher from Bangalore University. The author has contributed to research in topics: Natural convection & Nusselt number. The author has an hindex of 9, co-authored 17 publications receiving 832 citations.
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Effect of a magnetic field on free convection in a rectangular enclosure
TL;DR: In this paper, a finite difference scheme consisting of modified ADI (Alternating Direction Implicit) method and SLOR (Successive Line Over Relaxation) method is used to solve the vorticity-stream function formulation of the problem.
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Effect of magnetic field on natural convection in a vertical cylindrical annulus
TL;DR: A finite difference scheme consisting of alternating direction implicit (ADI) method and successive line over relaxation (SLOR) method is used to solve the vorticity stream function formulation of the problem as mentioned in this paper.
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Combined surface tension and buoyancy-driven convection in a rectangular open cavity in the presence of a magnetic field
TL;DR: In this paper, the effect of magnetic field on the flow driven by the combined mechanism of buoyancy and thermocapillarity in a rectangular open cavity filled with a low Prandtl number fluid (Pr = 0.054) was studied.
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Natural convection in a rectangular enclosure in the presence of a magnetic field with uniform heat flux from the side walls
TL;DR: In this paper, a numerical study for magnetohydrodynamic free convection of an electrically conducting fluid in a two-dimensional rectangular enclosure in which two side walls are maintained at uniform heat flux condition.
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Effect of magnetic field on the buoyancy and thermocapillary driven convection of an electrically conducting fluid in an annular enclosure
TL;DR: In this paper, the effect of magnetic field on the combined buoyancy and surface tension driven convection in a cylindrical annular enclosure is studied. And the results reveal that, in tall cavities, the axial magnetic field suppresses the surface tension flow more effectively than the radial magnetic field.