PAIR ANGULAR CORRELATION OF SECONDARY PARTICLES IN COSMIC RAY SHOWERS WITH ENERGIES E0]1011EV

被引：0

|

作者：

MISHAKOV.AP

NIKOLSKI.BA

机构：

来源：

SOVIET PHYSICS JETP-USSR | 1965年 / 20卷 / 04期

关键词：

D O I：

暂无

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

引用

收藏

页码：820 / &

相关论文

共 26 条

[21] Mass Composition of Cosmic Rays with Energies E0 ≥ 1017 eV According to the Data from the Ground-Based Detectors of the Yakutsk EAS Array
Glushkov, A. V.
Saburov, A. V.
JETP LETTERS, 2015, 100 (11) : 695 - 698
[22] Mass composition of cosmic rays with energies E0 ≥ 1017 eV according to the data from the ground-based detectors of the Yakutsk EAS array
A. V. Glushkov
A. V. Saburov
JETP Letters, 2015, 100 : 695 - 698
[23] Ordered structure of the directions of arrival of E0 ≈ 5 x 1017 eV cosmic rays according to data from the Yakutsk array for recording extensive air showers
Glushkov, AV
Pravdin, MI
PHYSICS OF ATOMIC NUCLEI, 2003, 66 (05) : 854 - 863
[24] Investigation of Gamma-Ray Families Originating from Nucleus-Nucleus Interactions at Ultrahigh Energies E0 in Excess of 1016 eV
Yuldashbaev, T. S.
Nuritdinov, Kh.
PHYSICS OF ATOMIC NUCLEI, 2013, 76 (12) : 1434 - 1436
[25] Investigation of gamma-ray families originating from nucleus-nucleus interactions at ultrahigh energies E0 in excess of 1016 eV
T. S. Yuldashbaev
Kh. Nuritdinov
Physics of Atomic Nuclei, 2013, 76 : 1434 - 1436
[26] Identification of light and very heavy cosmic ray primaries at E0 ≈ 1015 eV from surface and deep underground measurements at the Gran Sasso Laboratories
Navarra, G
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 1999, 70 : 512 - 514