Maqola

Analysis of the method for studying the zenith-angle EAS distribution

P. F. Beil’Lebedev Institute of Physics, Russian Academy of Sciences, Moscow, 119991, RussiaR. U. BeisembaevLebedev Institute of Physics, Russian Academy of Sciences, Moscow, 119991, RussiaN. G. VildanovLebedev Institute of Physics, Russian Academy of Sciences, Moscow, RussiaM. I. VildanovaLebedev Institute of Physics, Russian Academy of Sciences, Moscow, RussiaV. V. ZhukovLebedev Institute of Physics, Russian Academy of Sciences, Moscow, 119991, RussiaA. V. StepanovLebedev Institute of Physics, Russian Academy of Sciences, Moscow, 119991, RussiaT. Kh. SadykovPhysicotechnical Institute, Kazakhstan Academy of Sciences, Alma-Ata, 480082, KazakhstanV. I. YakovlevLebedev Institute of Physics, Russian Academy of Sciences, Moscow, 119991, Russia

Bulletin of the Russian Academy of Sciences Physicsjournal2007en

Ochiq kirish: yoʻq

ABI

Annotatsiya

The methodical problems related to analysis of the zenith-angle distribution of extensive air showers with N e > 107 particles are discussed. The effect of the array geometry on the angle measurement error is considered. Possible distortions of angular distribution due to errors have been calculated. The presence of excess showers detected at large zenith angles is shown.

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Mavzular

Astrophysics and Cosmic Phenomena Dark Matter and Cosmic Phenomena Atmospheric aerosols and clouds

Identifikatorlar

DOI: 10.3103/s1062873807040284

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