Energy spectrum and anisotropy of cosmic rays with E0 ≥ 1017 eV from Yakutsk EAS array data

被引：14

作者：

Glushkov, AV ^{[1
]}

Pravdin, MI ^{[1
]}

机构：

[1] Russian Acad Sci, Shafer Inst Space Phys & Aeron, Yakutsk 677891, Russia

来源：

JOURNAL OF EXPERIMENTAL AND THEORETICAL PHYSICS | 2005年 / 101卷 / 01期

基金：

俄罗斯基础研究基金会;

关键词：

D O I：

10.1134/1.2010665

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Data from the Yakutsk extensive air shower array for the period 1974-2004 are used to analyze the energy spectrum and anisotropy of primary cosmic rays (PCRs) with energy E-0 >= 10(17) eV. The spectra from different regions of the sky are shown to differ in shape. Enhanced and reduced particle fluxes come from the disks of the Galaxy and the Supergalaxy (the Local Supercluster of galaxies) at E-0 >= 5 x 10(18) eV and E-0 <= (2-3) x 10(18) eV, respectively. This is interpreted as a manifestation of the possible interaction between extragalactic PCRs and the matter of these spatial structures. (c) 2005 Pleiades Publishing, Inc.

引用

页码：88 / 97

页数：10

共 50 条

[31] On the origin of E0≥1017eV cosmic rays according to data from the Yakutsk array for studying extensive air showers
Glushkov, A. V.
PHYSICS OF ATOMIC NUCLEI, 2007, 70 (02) : 326 - 341
[32] Small-scale Anisotropy and composition of E0 ≈ 1017 eV cosmic rays according to data from the Yakutsk array for studying extensive air showers
Glushkov, AV
PHYSICS OF ATOMIC NUCLEI, 2003, 66 (07) : 1252 - 1259
[33] Small-scale anisotropy and composition of E0 ≈ 1017 eV cosmic rays according to data from the Yakutsk array for studying extensive air showers
A. V. Glushkov
Physics of Atomic Nuclei, 2003, 66 : 1252 - 1259
[34] Spectra of above 1017 eV cosmic rays from the different sky regions by Yakutsk EAS array data
Glushkov, A. V.
Pravdin, M. I.
PROCEEDINGS OF THE 29TH INTERNATIONAL COSMIC RAY CONFERENCE VOL 7: HE 1.4, 2005, : 251 - 254
[35] 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
[36] Quasars as probable sources of E0 greater than or equal 5 · 1018 eV cosmic rays by Yakutsk EAS array data
Glushkov, A.V.
Izvestiya Akademii Nauk. Ser. Fizicheskaya, 2002, 66 (11): : 1599 - 1603
[37] 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
[38] Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array
Glushkov, A. V.
Saburov, A. V.
JETP LETTERS, 2019, 109 (09) : 559 - 563
[39] Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array
A. V. Glushkov
A. V. Saburov
JETP Letters, 2019, 109 : 559 - 563
[40] 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

← 1 2 3 4 5 →