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Abstract The operation of a wide field-of-view (WFOV) Cherenkov telescope is described. Detection of extensive air showers (EAS) of cosmic rays (CR) is based on the coincidence with signals from… Click to show full abstract
Abstract The operation of a wide field-of-view (WFOV) Cherenkov telescope is described. Detection of extensive air showers (EAS) of cosmic rays (CR) is based on the coincidence with signals from the Yakutsk array. The data acquisition system (DAQ) of the telescope yields signals connected with EAS development parameters: shower age and position of shower maximum in the atmosphere. Here we describe the application of digital signal processing for reconstruction of Cherenkov radiation signals induced by air showers.
Keywords:
convolution wide;
fov cherenkov;
wide fov;
cherenkov telescope;
signal convolution;
cherenkov
Journal Title: Physics of Atomic Nuclei
Year Published: 2020
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Journal Title: Physics of Atomic Nuclei
Year Published: 2020
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!