toroidal component, but decreases by increasing the other components. This figure demonstrates that the disc thickness increases by increasing s. Equation 39, is clearly shows that the vertical thickness posses a complicated dependencies with our input parameters. This figure reveal that the magnetic diffusion has not a obvious effect on the thickness of disc.

In figure 5. we have plotted the convection parameter $\alpha_c $ versus the components of magnetic field for several values of s. The results are compatible with AM12. As it is seen, the convective parameter decrease, if the radial and toroidal magnetic field parameter become stronger although by adding z-component of magnetic field the convective parameter $\alpha_c$ increases. Larger values of wind parameter, $s$, cause the strong convection in the disc. It is obviously seen, the effect magnetic resistivity on the convection parameter is more important for the large vertical magnetic field. The results of wind and resistivity on the convection is the same.

In figure 6. the surface temperature ($T_{eff}$ ) is plotted as a function of the dimensionless radius ($\frac{r}{R_s}$). It is obvious that the surface temperature is monotonically decreasing with $\frac{r}{R_s}$. We see that the surface temperature increases by adding wind parameter $s$, 