Z
Zhaoyang Feng
Researcher at Chinese Academy of Sciences
Publications - 10
Citations - 292
Zhaoyang Feng is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Air shower & Cosmic ray. The author has an hindex of 3, co-authored 10 publications receiving 281 citations.
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Journal ArticleDOI
Anisotropy and corotation of galactic cosmic rays.
M. Amenomori,S. Ayabe,X. J. Bi,D. Chen,Shuwang Cui,Danzengluobu,Liming Ding,X. H. Ding,Cunfeng Feng,Zhaoyang Feng,Zhenyong Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,Hailan Hu,Jing Huang,Q. Huang,H. Y. Jia,F. Kajino,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,G. M. Le,A. F. Li,J. Y. Li,Y. Q. Lou,Hong-peng Lu,S. L. Lu,X. R. Meng,K. Mizutani,K. Mizutani,J. Mu,Kazuoki Munakata,A. Nagai,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,Shunsuke Ozawa,Jieru Ren,To. Saito,Takashi Saito,M. Sakata,Takashi Sako,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,B. Wang,H. Wang,X. Wang,Y. G. Wang,Hong Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yang,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,H. M. Zhang,J. L. Zhang,Ning Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou +85 more
TL;DR: Two-dimensional high-precision anisotropy measurement for energies from a few to several hundred teraelectronvolts (TeV) is presented, using the large data sample of the Tibet Air Shower Arrays, revealing finer details of the known anisotropies.
Journal ArticleDOI
Underground water Cherenkov muon detector array with the Tibet air shower array for gamma-ray astronomy in the 100 TeV region
M. Amenomori,S. Ayabe,X. J. Bi,D. Chen,Shuwang Cui,Danzengluobu,Liming Ding,X. H. Ding,Cunfeng Feng,Zhaoyang Feng,Z. Y. Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,Hailan Hu,Jing Huang,Q. Huang,H. Y. Jia,F. Kajino,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,G. M. Le,A. F. Li,J. Y. Li,Hong-peng Lu,S. L. Lu,X. R. Meng,K. Mizutani,K. Mizutani,J. Mu,Kazuoki Munakata,A. Nagai,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,Shunsuke Ozawa,Jieru Ren,To. Saito,Takashi Saito,M. Sakata,Takashi Sako,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,B. Wang,H. Wang,X. Wang,Y. G. Wang,Hong Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yang,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,H. M. Zhang,J. L. Zhang,Ning Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou +84 more
TL;DR: In this article, a water-Cherenkov-type muon-detector array (Tibet MD array) was built around the 37 000 m2 Tibet air shower array, which is already constructed at 4300 m above sea level in Tibet, China.
Journal ArticleDOI
Tibet air shower array: results and future plan
M. Amenomori,X. J. Bi,D. Chen,S. W. Cui,Danzengluobu,L. K. Ding,X. H. Ding,C. Fan,C. F. Feng,Zhaoyang Feng,Z. Y. Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jing Huang,Q. Huang,H. Y. Jia,F. Kajino,K. Kasahara,Y. Katayose,Chihiro Kato,K. Kawata,Labaciren,G. M. Le,A. F. Li,J. Y. Li,Y. Q. Lou,Hong-peng Lu,S. L. Lu,X. R. Meng,K. Mizutani,J. Mu,Kazuoki Munakata,A. Nagai,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,Shunsuke Ozawa,Jieru Ren,To. Saito,Takashi Saito,M. Sakata,Takashi Sako,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,B. Wang,Huaguang Wang,Xiaoqun Wang,Yu-Sa Wang,Y. G. Wang,H. R. Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yang,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,H. M. Zhang,Jia Zhang,Ning Zhang,X. Y. Zhang,Y. Zhang,Zhaxisangzhu,X. X. Zhou +83 more
TL;DR: In this article, the authors introduce the recent gamma-ray observation with the present Tibet air shower array and their future plan which is called the Tibet muon detector (MD) project.
Test of the hadronic interaction models at around *10 TeV with Tibet EAS core data
M. Amenomori,X. J. Bi,D. Chen,W. Y. Chen,S. W. Cui,Danzeng Luobu,L. K. Ding,X. H. Ding,C. F. Feng,Zhaoyang Feng,Z. Y. Feng,Q. B. Gou,H. W. Guo,Y. Q. Guo,H. H. He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jian Huang,W. J. Li,H. Y. Jia,L. L. Jiang,F. Kajino,K. Kasahara,Y. Katayose,Chihiro Kato,K. Kawata,Laba Ciren,Gui-Ming Le,A. F. Li,A. F. Li,C. X. Liu,J. S. Liu,Hsiao-Chi Lu,X. R. Meng,K. Mizutani,Kazuoki Munakata,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,Shunsuke Ozawa,X. L. Qian,X. B. Qu,Takeshi Saito,Takashi Saito,M. Sakata,T. K. Sako,J. Shao,J. Shao,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,H. R. Wu,L. Xue,Y. Yamamoto,Zicai Yang,S. Yasue,A. F. Yuan,T. Yuda,L. M. Zhai,H. M. Zhang,Jia Zhang,X. Y. Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Zhaxisa Ngzhu,X. X. Zhou +78 more
TL;DR: In this article, a burstdetector-grid (YAC-I) is used to check hadronic interaction models currently used for air-shower simulations such as QGSJET, SIBYLL, EPOS etc.
Observation of the temporal variation of the sidereal anisotropy by Tibet III array
M. Amenomori,X. J. Bi,D. Chen,S. W. Cui,Danzengluobu,L. K. Ding,X. H. Ding,C. Fan,C. F. Feng,Zhaoyang Feng,Z. Y. Feng,X. Y. Gao,Q. X. Geng,Q. B. Gou,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jian Huang,Q. Huang,H. Y. Jia,L. Jiang,F. Kajino,K. Kasahara,Y. Katayose,Chihiro Kato,K. Kawata,Labaciren,Gui-Ming Le,A. F. Li,H. C. Li,J. Y. Li,C. X. Liu,Y. Q. Lou,Hsiao-Chi Lu,X. R. Meng,K. Mizutani,J. Mu,K. Munakata,K. Munakata,A. Nagai,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,Shunsuke Ozawa,Takeshi Saito,T. Y. Saito,M. Sakata,Takashi Sako,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,B. S. Wang,Huaguang Wang,Yu-Sa Wang,Y. G. Wang,H. R. Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yan,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,H. M. Zhang,Jia Zhang,Ning Zhang,X. Y. Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Zhaxisangzhu,X. X. Zhou +85 more
Abstract: We have analyzed the large scale sidereal anisotropy of multi-TeV Galactic cosmic rays by Tibet Air Shower Array, with the data taken from Nov. 1999 to Nov. 2005. To study the temporal variation of the anisotropy, the data set is divided into 6 samples, each in a time scale of one year.It is shown that the sidereal anisotropy with the magnitude about 0.1% is fairly stable from year to year over the entire observation period. This indicates that the anisotropy of TeV galactic cosmic rays is insensitive to solar activities.