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We propose an improved method for the atmospheric extinction reduction withinoptical photometry. Our method is based on the simultaneous multicolorobservations of photometric standards. Such data are now available within themodern wide-field sky surveys and contain a large amount of information aboutinstant atmospheric conditions. So, it became possible to estimate theextinction parameters on the basis of a quite short observational dataset and,hence, to trace the rapid stars twinkling accurately. Having been developed fora new MiniMegaTORTORA observational system, the proposed method can be adoptedfor a wide range of modern observational programs.

On the Atmospheric Extinction Reduction Procedure in Multiband Wide-Field Photometric Surveys