نتایج جستجو برای: mhd mixed convection

تعداد نتایج: 254020  

Journal: :journal of nanostructures 2012
g. a. sheikhzadeh m. ebrahim qomi n. hajialigol a. fattahi

the fluid flow and heat transfer in a three-dimensional microchannel filled with al2o3- water nanofluid is numerically investigated. the hybrid scheme is used to discretize the convection terms and simpler algorithm is adopted to couple the velocity and pressure field in the momentum equations. the temperature fields, variation of horizontal velocity along the centre line of the channel, averag...

J. Rahmannezhad M. Kalteh,

Magnetohydrodynamic (MHD) mixed convection flow of Cu–water nanofluid inside a two-sided lid-driven square enclosure with adiabatic horizontal walls and differentially heated sidewalls has been investigated numerically. The effects of moving lids direction, variations of Richardson number, Hartmann number, and volume fraction of nanoparticles on flow and temperature fields have been studied. Th...

2013
Ali J. Chamkha Salman Bin Abdul Aziz ALI J. CHAMKHA S. M. M. EL-KABEIR

UNSTEADY HEAT AND MASS TRANSFER BY MHD MIXED CONVECTION FLOW OVER AN IMPULSIVELY STRETCHED VERTICAL SURFACE WITH CHEMICAL REACTION AND SORET AND DUFOUR EFFECTS Ali J. Chamkha a & S. M. M. El-Kabeir b c a Manufacturing Engineering Department , The Public Authority for Applied Education and Training , Shuweikh , Kuwait b Department of Mathematics , Faculty of Science, Aswan University , Aswan , E...

2013
Karunakar Reddy Raja Shekar

The effects of heat and mass transfer on MHD mixed convection flow of a vertical surface with radiation, heat source/absorption and chemical reaction has been is discussed. The resulting set of coupled non-linear ordinary differential equations is solved by perturbation technique and for graphs we used MATLAB software. Approximate solutions have been derived for the velocity, temperature, conce...

Journal: :Entropy 2017
Muhammad Idrees Afridi Muhammad Qasim Ilyas Khan Sharidan Shafie Ali Saleh Alshomrani

This research focuses on entropy generation rate per unit volume in magneto-hydrodynamic (MHD) mixed convection boundary layer flow of a viscous fluid over an inclined stretching sheet. Analysis has been performed in the presence of viscous dissipation and non-isothermal boundary conditions. The governing boundary layer equations are transformed into ordinary differential equations by an approp...

2013
Bhupendra K. Sharma Kailash Yadav Nidhish K. Mishra R. C. Chaudhary

The Soret and Dufour effects on unsteady MHD mixed convection flow past an infinite radiative vertical porous plate embedded in a porous medium in the presence of chemical reaction have been studied. A uniform magnetic field acts perpendicular to the porous surface. The Rosseland approximation has been used to describe the radiative heat flux in energy equation. The governing equations are solv...

Journal: :international journal of industrial mathematics 0
m. abd el-aziz king khaled university, faculty of science, mathematics department, abha 9004, saudi ‎arabia‎‎. department of mathematics, faculty of science, helwan university, cairo, egypt p. o. box 1179‎5‎‎‎.

the effect of partial slip and temperature dependent fluid properties on the mhd mixed convection flow from a heated, non-linearly stretching surface in the presence of radiation and non-uniform internal heat generation/absorption is investigated. the velocity of the stretching surface was assumed to vary according to power-law form. thermal transport is analyzed for two types of non-isothermal...

2009
Ryoji Matsumoto Hiroaki Isobe

By implementing a three-dimensional magnetohydrodynamic (MHD) code based on the CIP-MOCCT scheme, we carried out large scale MHD simulations of the solar atmosphere covering the region from the convection zone to the corona. We found that in regions with weak magnetic fields (B~100G), horizontal magnetic loops created in the upflow regions of the convection generate high frequency waves by reco...

1997
U. Narain P. Agarwal

We have estimated MHD fluxes in the solar convection zone using the best available data on turbulent (convective) velocities in combination with the formulation of Stein (1981) and suitable efficiency factors. The estimated MHD fluxes compare well with the total solar flux.

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