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The effects of cosmic-ray diffusion and radiative cooling on the structure ofthe Galactic wind are studied using a steady state approximation. It is knownthat realistic cooling processes suppress the wind from launching. The effectsof cosmic-ray diffusion are also supposed to be unfavorable for launching thewind. Both of these effects have not been studied simultaneously in asteady-state approximation of the wind. We find 327,254 solutions of thesteady-state Galactic wind and confirm that: the effect of cosmic-ray pressuredepends on the Alfv{\'e}n Mach number, the mass flux carried by the wind doesnot depend on the cosmic-ray pressure directly (but depends on the thermalpressure), and the typical conditions found in the Galaxy may correspond to thewind solution that provides metal polluted matters at a height of $\sim300$~kpcfrom the disk.

The Effects of Cosmic-Ray Diffusion and Radiative Cooling on the Galactic Wind from the Milky Way