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Northern sky galactic cosmic ray anisotropy between 10 and 1000 tev with the tibet air shower array

文献类型:期刊论文

作者Amenomori,M.1; Bi,X. J.2; Chen,D.3; Chen,T. L.4; Chen,W. Y.2; Cui,S. W.5; Danzengluobu,4; Ding,L. K.2; Feng,C. F.6; Feng,Zhaoyang2
刊名The astrophysical journal
出版日期2017-02-16
卷号836期号:2
ISSN号0004-637X
关键词Astroparticle physics Cosmic rays
DOI10.3847/1538-4357/836/2/153
英文摘要Abstract 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°. 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 ~100 tev. the spatial distribution of the gcr intensity with an excess (7.2σ pre-trial, 5.2σ post-trial) and a deficit (?5.8σ 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 ~100 tev, indicating a new component of the anisotropy. all these results may shed new light on understanding the origin and propagation of gcrs.
语种英语
出版者The American Astronomical Society
WOS记录号IOP:0004-637X-836-2-153
URI标识http://www.irgrid.ac.cn/handle/1471x/2175674
专题高能物理研究所
作者单位1.Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan
2.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
3.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
4.Department of Mathematics and Physics, Tibet University, Lhasa 850000, China
5.Department of Physics, Hebei Normal University, Shijiazhuang 050016, China
6.Department of Physics, Shandong University, Jinan 250100, China
7.Institute of Modern Physics, Southwest Jiaotong University, Chengdu 610031, China
8.Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan
9.Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan
10.Department of Physics, Konan University, Kobe 658-8501, Japan
推荐引用方式
GB/T 7714
Amenomori,M.,Bi,X. J.,Chen,D.,et al. Northern sky galactic cosmic ray anisotropy between 10 and 1000 tev with the tibet air shower array[J]. The astrophysical journal,2017,836(2).
APA Amenomori,M..,Bi,X. J..,Chen,D..,Chen,T. L..,Chen,W. Y..,...&Zhou,X. X..(2017).Northern sky galactic cosmic ray anisotropy between 10 and 1000 tev with the tibet air shower array.The astrophysical journal,836(2).
MLA Amenomori,M.,et al."Northern sky galactic cosmic ray anisotropy between 10 and 1000 tev with the tibet air shower array".The astrophysical journal 836.2(2017).

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来源:高能物理研究所

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