Observational and theoretical studies from the last decade have shown that the Viscous Decretion Disk (VDD) scenario, in which turbulent viscosity is the physical mechanism responsible for the transport of material and angular momentum ejected from the star to the outer regions of the disk, is the only viable model for explaining the circumstellar disks of Be stars. In the alpha-disk approach applied to the VDD, the dimensionless parameter a is alpha measure of the turbulent viscosity. Recently, combining the time-dependent evolution of a VDD alpha-disk with non-LTE radiative transfer calculations, the first measurement of the alpha parameter was made, for the disk dissipation of the Be star omega CMa. It was found that alpha approximate to 1 for that Be disk. The main motivation of this present work is the statistical determination of the a parameter. For this purpose, we present a pipeline that will allow the semiautomatic determination of the a parameter of several dozens of light curves of Be stars available from photometric surveys, In this contribution, we describe the pipeline, outlining the main staps required for the semiautomatic analysis of light curves