Analytical solutions for MHD flow at a rectangular duct with unsymmetrical walls of arbitrary conductivity

For MHD flows in a rectangular duct with unsymmetrical walls, two analytical solutions have been obtained by solving the gov- erning equations in the liquid and in the walls coupled with the boundary conditions at fluid-wall interface. One solution of ＇Case I＇ is for MHD flows in a duct with side walls insulated and unsymmetrical Hartmann walls of arbitrary conductivity, and another one of ＇Case II＇ is for the flows with unsymmetrical side walls of arbitrary conductivity and Hartmann walls perfectly conductive. The walls are unsymmetrical with either the conductivity or the thickness different from each other. The solutions, which include three parts, well reveal the wall effects on MHD. The first part represents the contribution from insulated walls, the second part represents the contribution from the conductivity of the walls and the third part represents the contribution from the unsymmetri- cal walls. The solution is reduced to the Hunt＇s analytical solutions when the walls are symmetrical and thin enough. With wall thickness runs from 0 to co, there exist many solutions for a fixed conductance ratio. The unsymmetrical walls have great effects on velocity distribution. Unsymmetrical jets may form with a stronger one near the low conductive wall, which may introduce stronger MHD instability. The pressure gradient distributions as a function of Hartmann number are given, in which the wall effects on the distributions are well illustrated.

For MHD flows in a rectangular duct with unsymmetrical walls, two analytical solutions have been obtained by solving the governing equations in the liquid and in the walls coupled with the boundary conditions at fluid-wall interface. One solution of 'Case I' is for MHD flows in a duct with side walls insulated and unsymmetrical Hartmann walls of arbitrary conductivity, and another one of 'Case II' is for the flows with unsymmetrical side walls of arbitrary conductivity and Hartmann walls perfectly conductive.The walls are unsymmetrical with either the conductivity or the thickness different from each other. The solutions, which include three parts, well reveal the wall effects on MHD. The first part represents the contribution from insulated walls, the second part represents the contribution from the conductivity of the walls and the third part represents the contribution from the unsymmetrical walls. The solution is reduced to the Hunt's analytical solutions when the walls are symmetrical and thin enough. With wall thickness runs from 0 to∞, there exist many solutions for a fixed conductance ratio. The unsymmetrical walls have great effects on velocity distribution. Unsymmetrical jets may form with a stronger one near the low conductive wall, which may introduce stronger MHD instability. The pressure gradient distributions as a function of Hartmann number are given, in which the wall effects on the distributions are well illustrated.