Cross-diffusion of the stagnation-point solar radiated micropolar liquid flow through a convected surface

Abstract

The aim of the present analysis was to the best part of the effect of a magnetohydrodynamic micropolar fluid over the convective surface boundary condition into cross-diffusion and linear radiative heats were assumed. The impact on chemical reaction and viscous dissipation is considered. This governing equation about flow fields was transformed with a non-dimensional design to apply relevant correlation variables. That ODE was defined with the bvp4c method. This result is entrusted into plots and tables about the consequence of diverse flow variables in the flow fields. They observed into appreciative temperature in the increase in the Dufour number, although the unfavorable force was recognized in the Richardson number. It was noticed that the higher velocity was placed on the Newtonian liquid on difference into that micropolar liquid. Concentration was the reducing function on chemical reaction parameters and Schmidt number.