Lateral Distribution Functions of Signals in Surface Scintillation Detectors of the Yakutsk Array, New Energy Estimates of Extensive Air Showers and the Energy Spectrum of the Primary Cosmic Radiation at Energies ∼1017–1019 eV


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Fluctuations of lateral distributions of signals in the surface scintillation detectors of the Yakutsk array are found to be large. New estimates of the inclined shower energy had been suggested. In view of these estimates the Yakutsk energy spectrum becomes quite comparable with the spectra observed at the Pierre Auger Observatory and the Telescope Array. The shower energy calculated using the data of only one detector may be overestimated if fluctuations are neglected.

作者简介

L. Dedenko

Moscow State University, Faculty of Physics; Skobeltsyn Institute of Nuclear Physics

编辑信件的主要联系方式.
Email: ddn@dec1.sinp.msu.ru
俄罗斯联邦, Moscow; Moscow

A. Lukyashin

NRC “Kurchatov Institute”-ITEP; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: ddn@dec1.sinp.msu.ru
俄罗斯联邦, Moscow; Moscow

T. Roganova

Skobeltsyn Institute of Nuclear Physics

Email: ddn@dec1.sinp.msu.ru
俄罗斯联邦, Moscow

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