Publication:
Galactic Cosmic-Ray Anisotropy in the Northern Hemisphere from the ARGO-YBJ Experiment during 2008-2012

Submitted Date
Received Date
Accepted Date
Issued Date
2018-07-10
Copyright Date
Announcement No.
Application No.
Patent No.
Valid Date
Resource Type
Article
Edition
Resource Version
Language
File Type
No. of Pages/File Size
ISBN
ISSN
15384357
0004637X
eISSN
DOI
10.3847/1538-4357/aac6cc
Scopus ID
WOS ID
Pubmed ID
arXiv ID
Call No.
Other identifier(s)
2-s2.0-85050652783
Journal Title
Volume
Issue
item.page.oaire.edition
Start Page
End Page
Access Rights
Access Status
Rights
Mahidol University
Rights Holder(s)
SCOPUS
Physical Location
Bibliographic Citation
Astrophysical Journal. Vol.861, No.2 (2018)
Citation
B. Bartoli, P. Bernardini, X. J. Bi, Z. Cao, S. Catalanotti, S. Z. Chen, T. L. Chen, S. W. Cui, B. Z. Dai, A. D'Amone, Danzengluobu, I. De Mitri, B. D.Ettorre Piazzoli, T. Di Girolamo, G. Di Sciascio, C. F. Feng, Z. Y. Feng, W. Gao, Q. B. Gou, Y. Q. Guo, H. H. He, Haibing Hu, Hongbo Hu, M. Iacovacci, R. Iuppa, H. Y. Jia, Labaciren, H. J. Li, C. Liu, J. Liu, M. Y. Liu, H. Lu, L. L. Ma, X. H. Ma, G. Mancarella, S. M. Mari, G. Marsella, S. Mastroianni, P. Montini, C. C. Ning, L. Perrone, P. Pistilli, D. Ruffolo, P. Salvini, R. Santonico, P. R. Shen, X. D. Sheng, F. Shi, A. Surdo, Y. H. Tan, P. Vallania, S. Vernetto, C. Vigorito, H. Wang, C. Y. Wu, H. R. Wu, L. Xue, Q. Y. Yang, X. C. Yang, Z. G. Yao, A. F. Yuan, M. Zha, H. M. Zhang, L. Zhang, X. Y. Zhang, Y. Zhang, J. Zhao, Zhaxiciren, Zhaxisangzhu, X. X. Zhou, F. R. Zhu, Q. Q. Zhu (2018). Galactic Cosmic-Ray Anisotropy in the Northern Hemisphere from the ARGO-YBJ Experiment during 2008-2012. Retrieved from: https://repository.li.mahidol.ac.th/handle/123456789/45736.
Research Projects
Organizational Units
Authors
Journal Issue
Thesis
Title
Galactic Cosmic-Ray Anisotropy in the Northern Hemisphere from the ARGO-YBJ Experiment during 2008-2012
Alternative Title(s)
Author(s)
B. Bartoli
 P. Bernardini
 X. J. Bi
 Z. Cao
 S. Catalanotti
 S. Z. Chen
 T. L. Chen
 S. W. Cui
 B. Z. Dai
 A. D'Amone
 Danzengluobu
 I. De Mitri
 B. D.Ettorre Piazzoli
 T. Di Girolamo
 G. Di Sciascio
 C. F. Feng
 Z. Y. Feng
 W. Gao
 Q. B. Gou
 Y. Q. Guo
 H. H. He
 Haibing Hu
 Hongbo Hu
 M. Iacovacci
 R. Iuppa
 H. Y. Jia
 Labaciren
 H. J. Li
 C. Liu
 J. Liu
 M. Y. Liu
 H. Lu
 L. L. Ma
 X. H. Ma
 G. Mancarella
 S. M. Mari
 G. Marsella
 S. Mastroianni
 P. Montini
 C. C. Ning
 L. Perrone
 P. Pistilli
 D. Ruffolo
 P. Salvini
 R. Santonico
 P. R. Shen
 X. D. Sheng
 F. Shi
 A. Surdo
 Y. H. Tan
 P. Vallania
 S. Vernetto
 C. Vigorito
 H. Wang
 C. Y. Wu
 H. R. Wu
 L. Xue
 Q. Y. Yang
 X. C. Yang
 Z. G. Yao
 A. F. Yuan
 M. Zha
 H. M. Zhang
 L. Zhang
 X. Y. Zhang
 Y. Zhang
 J. Zhao
 Zhaxiciren
 Zhaxisangzhu
 X. X. Zhou
 F. R. Zhu
 Q. Q. Zhu
Author's Affiliation
Author's E-mail
Editor(s)
Editor's Affiliation
Corresponding Author(s)
Creator(s)
Compiler
Advisor(s)
Illustrator(s)
Applicant(s)
Inventor(s)
Issuer
Assignee
Other Contributor(s)
Trento Institute for Fundamental Physics and Applications
 Istituto Nazionale di Fisica Nucleare, Sezione di Lecce
 Istituto Nazionale di Fisica Nucleare, Sezione di Torino
 Istituto Nazionale di Fisica Nucleare, Sezione di Pavia
 Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
 Università degli Studi di Roma La Sapienza
 Shandong University
 Istituto Nazionale Di Astrofisica, Rome
 Yunnan University
 Institute of High Energy Physics Chinese Academy of Science
 Università degli Studi di Roma Tor Vergata
 University of Chinese Academy of Sciences
 Istituto Nazionale di Fisica Nucleare - INFN
 Università degli Studi di Napoli Federico II
 Mahidol University
 Università degli Studi Roma Tre
 Università degli Studi di Torino
 Southwest Jiaotong University
 Hebei Normal University
 Tibet University
 Dipartimento di Fisica
 Gran Sasso Science Institute
 Dipartimento di Matematica Ennio de Giorgi
Series
Has Part
Abstract
© 2018. The American Astronomical Society. All rights reserved. This paper reports on the observation of the sidereal large-scale anisotropy of cosmic rays using data collected by the ARGO-YBJ experiment over 5 years (2008-2012). This analysis extends previous work limited to the period from 2008 January to 2009 December, near the minimum of solar activity between cycles 23 and 24. With the new data sample, the period of solar cycle 24 from near minimum to maximum is investigated. A new method is used to improve the energy reconstruction, allowing us to cover a much wider energy range, from 4 to 520 TeV. Below 100 TeV, the anisotropy is dominated by two wide regions, the so-called "tail-in" and "loss-cone" features. At higher energies, a dramatic change of the morphology is confirmed. The yearly time dependence of the anisotropy is investigated. Finally, no noticeable variation of cosmic-ray anisotropy with solar activity is observed for a median energy of 7 TeV.
Table of contents
Description
Sponsorship
Degree Name
Degree Level
Degree Department
Degree Discipline
Degree Grantor(s)
Classification
DDC
MESH
Subject(s)
Keyword(s)
Earth and Planetary Sciences
 Physics and Astronomy
View online Resources
URI
https://repository.li.mahidol.ac.th/handle/123456789/45736
Collections
Scopus 2018