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Northern Sky Galactic Cosmic Ray Anisotropy between 10 and 1000TeV with the Tibet Air Shower Array

文献类型:期刊论文

作者Wang, H.24; Tibet AS Colloboration; Zhou, X. X.5; Zhaxisangzhu25; Zhang, Ying24; Zhang, Yi24; Zhang, Y.24; Zhang, X. Y.4; Zhang, J. L.24; Zhang, H. M.24
刊名ASTROPHYSICAL JOURNAL
出版日期2017-02-20
卷号836期号:2
关键词Astroparticle Physics Cosmic Rays
DOI10.3847/1538-4357/836/2/153
文献子类Article
英文摘要We report on the analysis of the 10-1000 TeV large-scale sidereal anisotropy of Galactic cosmic rays (GCRs) with the data collected by the Tibet Air Shower Array from 1995 October to 2010 February. In this analysis, we improve the energy estimate and extend the decl. range down to -30 degrees. We find that the anisotropy maps above 100 TeV are distinct from that at a multi-TeV band. The so-called tail-in and loss-cone features identified at low energies get less significant, and a new component appears at similar to 100TeV. The spatial distribution of the GCR intensity with an excess (7.2 sigma pre-trial, 5.2 sigma post-trial) and a deficit (-5.8 sigma pre-trial) are observed in the 300 TeV anisotropy map, in close agreement with IceCube's results at 400 TeV. Combining the Tibet results in the northern sky with IceCube's results in the southern sky, we establish a full-sky picture of the anisotropy in hundreds of TeV band. We further find that the amplitude of the first order anisotropy increases sharply above similar to 100 TeV, indicating a new component of the anisotropy. All these results may shed new light on understanding the origin and propagation of GCRs.
WOS关键词SIDEREAL ANISOTROPY ; ARRIVAL DIRECTIONS ; TEV ; PROPAGATION ; INTENSITY ; SPECTRUM ; ICECUBE ; SOLAR
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000395866500001
资助机构Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Natural Sciences Foundation of China(11405182 ; Natural Sciences Foundation of China(11405182 ; 1135010 ; 1135010 ; 11405180) ; 11405180) ; Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Natural Sciences Foundation of China(11405182 ; Natural Sciences Foundation of China(11405182 ; 1135010 ; 1135010 ; 11405180) ; 11405180)
源URL[http://ir.bao.ac.cn/handle/114a11/8886]  
专题国家天文台_射电天文研究部
作者单位1.Shonan Inst Technol, Fujisawa, Kanagawa 2518511, Japan
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
3.Hebei Normal Univ, Dept Phys, Shijiazhuang 050016, Peoples R China
4.Shandong Univ, Dept Phys, Jinan 250100, Peoples R China
5.Southwest Jiaotong Univ, Inst Modern Phys, Chengdu 610031, Peoples R China
6.Kanagawa Univ, Fac Engn, Yokohama, Kanagawa 2218686, Japan
7.Utsunomiya Univ, Fac Educ, Utsunomiya, Tochigi 3218505, Japan
8.Konan Univ, Dept Phys, Kobe, Hyogo 6588501, Japan
9.Waseda Univ, Res Inst Sci & Engn, Tokyo 1698555, Japan
10.Yokohama Natl Univ, Fac Engn, Yokohama, Kanagawa 2408501, Japan
推荐引用方式
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Wang, H.,Tibet AS Colloboration,Zhou, X. X.,et al. Northern Sky Galactic Cosmic Ray Anisotropy between 10 and 1000TeV with the Tibet Air Shower Array[J]. ASTROPHYSICAL JOURNAL,2017,836(2).
APA Wang, H..,Tibet AS Colloboration.,Zhou, X. X..,Zhaxisangzhu.,Zhang, Ying.,...&Sako, T. K..(2017).Northern Sky Galactic Cosmic Ray Anisotropy between 10 and 1000TeV with the Tibet Air Shower Array.ASTROPHYSICAL JOURNAL,836(2).
MLA Wang, H.,et al."Northern Sky Galactic Cosmic Ray Anisotropy between 10 and 1000TeV with the Tibet Air Shower Array".ASTROPHYSICAL JOURNAL 836.2(2017).

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来源:国家天文台

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