Cosmic ray energy spectrum (>1017 eV) of the Yakutsk EAS array

被引：1

作者：

Pravdin M.I. ^{[1
]}

Glushkov A.V. ^{[1
]}

Djachkovski N.A. ^{[1
]}

Egorov Yu.A. ^{[1
]}

Ivanov A.A. ^{[1
]}

Kolosov V.A. ^{[1
]}

Krasilnikov A.D. ^{[1
]}

Knurenko S.P. ^{[1
]}

Makarov I.T. ^{[1
]}

Mikhailov A.A. ^{[1
]}

Petrov Z.E. ^{[1
]}

Prokhorova V.P. ^{[1
]}

Sabourov A.V. ^{[1
]}

Sleptsov I.E. ^{[1
]}

Struchkov G.G. ^{[1
]}

机构：

[1] Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Division, Russian Academy of Sciences

来源：

Bulletin of the Russian Academy of Sciences: Physics | 2009年 / 73卷 / 5期

基金：

俄罗斯基础研究基金会;

关键词：

Energy Spectrum; Auger; Zenith Angle; Cherenkov Light; Muon Component;

D O I：

10.3103/S1062873809050013

中图分类号：

学科分类号：

摘要：

The energy spectrum obtained on the Yakutsk array for the parameter S600 is compared with the results obtained on the AGASA and HiRes arrays and the latest Pierre Auger Observatory data. The discrepancy in the intensity of the energy spectra obtained in different experiments can be explained by the presence of systematic errors in shower energy estimations. © Allerton Press, Inc. 2009.

引用

页码：541 / 543

页数：2

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Cosmic ray energy spectrum (&gt;1017 eV) of the Yakutsk EAS array

Cosmic ray energy spectrum (>1017 eV) of the Yakutsk EAS array