![]() ![]() Number, and Eckert number are stable at the point of convergence. Observed that several parameters such as Casson fluid parameter, radiation parameter, Prandtl Velocity profile of the Casson fluid flow is directly related to several parameters. With higher values of the magnetic field as well as the radiation. ![]() After simulation, it is found that the heat transfer rate decreases Technique is used for finding the solutions and results are presented in the form of tables and ![]() Ordinary differential equations by using similarity transformations. Mathematical model as a platform non-linier differential equation have been reduced to By considering governing equations of the ![]() An explicit Finite difference method is appliedįor the solution of governing equations. In this paper, the behavior of the non-Newtonian fluid and heat transfer is considered in anĮxponentially stretching surface in the occurrence of porous magnetic field, as it has vastĪpplications in the field of several industries. EFFECT OF SOLAR THERMAL RADIATION AND MAGNETIC FIELD ON THE FLOW OF CASSON FLUID ![]()
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