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We analyze temporal characteristics of signals from the wide field-of-view(WFOV) Cherenkov telescope (CT) detecting extensive air showers (EAS) of cosmicrays (CR) in coincidence with surface detectors of the Yakutsk array. Our aimis to reveal causal relationships between measured characteristics and physicalproperties of EAS.

Temporal signatures of the Cherenkov light induced by extensive air showers of cosmic rays detected with the Yakutsk array