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

共 50 条

[11] Observation of "the knee" in cosmic ray energy spectrum with underground muons and primary mass composition in the range 1015-1017 eV
Bakatanov, VN
Novosel'tsev, YF
Novosel'tseva, RV
ASTROPARTICLE PHYSICS, 1999, 12 (1-2) : 19 - 24
[12] Extensive Air Showers and Cosmic Ray Physics above 1017 eV
Bertaina, Mario
XLV INTERNATIONAL SYMPOSIUM ON MULTIPARTICLE DYNAMICS (ISMD 2015), 2016, 120
[13] Measurement of the cosmic-ray energy spectrum above 1016 eV with the LOFAR Radboud Air Shower Array
Thoudam, S.
Buitink, S.
Corstanje, A.
Enriquez, J. E.
Falcke, H.
Horandel, J. R.
Nelles, A.
Rachen, J. P.
Rossetto, L.
Schellart, P.
Scholten, O.
ter Veen, S.
Trinh, T. N. G.
van Kessel, L.
ASTROPARTICLE PHYSICS, 2016, 73 : 34 - 43
[14] Estimation of the PCR mass composition in the energy range 1017–1019 eV on the basis of multicomponent analysis of the characteristics of EASs detected at the Yakutsk array
A. A. Ivanov
S. P. Knurenko
A. A. Lagutin
M. I. Pravdin
A. V. Saburov
I. E. Sleptsov
Bulletin of the Russian Academy of Sciences: Physics, 2007, 71 (4) : 448 - 450
[15] Estimate of the mass composition of cosmic rays with E0 ≤ 1018 eV according to the data from a new muon detector at the Yakutsk EAS array
A. V. Glushkov
A. V. Saburov
JETP Letters, 2013, 97 : 444 - 446
[16] About the character of the “Knee” at E⋍3×1015 eV in the energy spectrum and the mass composition of primary cosmic rays in the energy range 1015–1017 eV
Yu. F. Novosel’tsev
Physics of Atomic Nuclei, 2000, 63 : 1053 - 1057
[17] The Light Nuclei Energy Spectrum of Primary Cosmic Rays using EAS MSU Array Data
Kalmykov, N. N.
Kalmykov, V. N.
Kulikov, G. V.
Sulakov, P. V.
Fomin, Yu. A.
MOSCOW UNIVERSITY PHYSICS BULLETIN, 2008, 63 (06) : 425 - 427
[18] The light nuclei energy spectrum of primary cosmic rays using EAS MSU array data
N. N. Kalmykov
V. N. Kalmykov
G. V. Kulikov
P. V. Sulakov
Yu. A. Fomin
Moscow University Physics Bulletin, 2008, 63 : 425 - 427
[19] Estimates of the energy of the most intense extensive air shower observed at the Yakutsk EAS array
L. G. Dedenko
A. V. Glushkov
S. P. Knurenko
I. T. Makarov
M. I. Pravdin
D. A. Podgrudkov
I. E. Sleptsov
T. M. Roganova
G. F. Fedorova
JETP Letters, 2010, 90 : 691 - 696
[20] Ordered structure of the directions of arrival of E0∼5×1017 eV cosmic rays according to data from the Yakutsk array for recording extensive air showers
A. V. Glushkov
M. I. Pravdin
Physics of Atomic Nuclei, 2003, 66 : 854 - 863

← 1 2 3 4 5 →