Zenith angle distribution of cosmic ray showers measured with the Yakutsk array
August 16, 2017
August 03, 2018
The Yakutsk array dataset in the energy interval (3✕1016;1019) eV is re-visited in order to interpret the zenith angle distribution of extensive air shower event rate. The close relation of the distribution to the attenuation of the main measurable parameter of showers, S600, is examined. Knowledge of the threshold effect on fluctuations of the parameter is essential in order to calculate surface array exposure.
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