Volume 301 -
35th International Cosmic Ray Conference (ICRC2017) -
Session Cosmic-Ray Indirect. CRI-properties of CRs at high energies (anisotropy, energy, mass)
Zenith angle distribution of cosmic ray showers measured with the Yakutsk array
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Pre-published on:
August 16, 2017
Published on:
August 03, 2018
Abstract
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.
DOI: https://doi.org/10.22323/1.301.0550
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.