We calculated line profiles of 32 Cyg with an assumed $str{"{o}}mgren$ sphere at orbital phases 0.06 and 0.78. The wind models with $Alfv'{e}n$ waves show diminished line profiles compared to those of the models using power velocity laws. The reduced density of absorbers in HII region produce weak profiles, but line profiles at ${phi}=0.06$ do not show the differences except in the red edge of absorption. At ${phi}=0.78$ however, we could reproduce the line profiles of Alfven waves model by the power law models with two velocity gradients. It suggests that the power law model with 2 acceleration regions could reduce the errors in the theoretical line formation with no consideration of wind acceleration mechanism.nism.