field parameters, $\beta_{r, \phi, z}, P_{m}$ and also parameters, $s, l$, on the dynamical and observational appearance of CDAF in presence of all components of magnetic field. In this study constant values for some parameters like $\alpha=0.5$, $f=1$, $\gamma=1.01$, $g=-\frac{1}{3}$, $\zeta=1$, $\eta_c=1$ and $\epsilon_c=0.0045$ have been adopted.\
Figures 1,2,3 show the self similar coefficient $c_0$ (the surface density), $c_1$ ( the radial velocity) and $c_2$ (the rotational velocity) as a functions of the three components of magnetic field for different values of wind parameter $s (=0, 0.1, 0.2)$. By adding the all components of magnetic field $(\beta_{r,\varphi,z})$ which indicate the role of magnetic field on the dynamics of accretion disc, we see that the surface density and rotational velocity of the disc gradually increase, although the radial speed decreases. This results are qualitatively consistent with results presented by AM12 and FO12. In these figures we also studied the effect of parameter, $s$ which measures the strength of wind, on physical coefficients. Generally, when the exponent $s$ increases, the flow will rotate slower than that without wind. Also radial and rotational velocities in Figure 1, 2 and 3 represent significant deviations from non-wind solutions. Consequently, CDAFs in the presence of wind 