Abstract
The operation of a wide field-of-view Cherenkov telescope is described. The detection of extensive air showers (EAS) of cosmic rays (CR) is based upon the coincidence with signals from the Yakutsk array. The data acquisition system of the telescope yields signals connected with EAS development parameters: presumably, shower age and position of shower maximum in the atmosphere. Here we describe the application of digital signal processing in order to reconstruct Cherenkov radiation signals induced by CR showers.
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