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Here the results of calculations of pulses in Cherenkov light detectors forthe Yakutsk array are presented. As long as the Vavilov-Cherenkov light is usedto calibrate signals in scintillation detectors at the Yakutsk array it isvital for these measurements to be precise. The validity of measurements of thesignal Q(400) used as the estimation parameter at the Yakutsk array has beenconfirmed. Our calculations show that the width of time pulses increases fromnearly 50 ns at a distance of 100 m from the shower axis up to 700 ns at 1000m.

The time-space structure of pulses in Cherenkov light detectors