H
Hong-peng Lu
Researcher at Guizhou University
Publications - 118
Citations - 3257
Hong-peng Lu is an academic researcher from Guizhou University. The author has contributed to research in topics: Cosmic ray & Air shower. The author has an hindex of 32, co-authored 113 publications receiving 2852 citations. Previous affiliations of Hong-peng Lu include Chinese Academy of Sciences & South China Normal University.
Papers
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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
The All-Particle Spectrum of Primary Cosmic Rays in the Wide Energy Range from 1014 to 1017 eV Observed with the Tibet-III Air-Shower Array
M. Amenomori,X. J. Bi,D. Chen,Shuwang Cui,Danzengluobu,Liming Ding,X. H. Ding,C. Fan,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,K. 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,M. Shibata,A. Shiomi,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,Yu-Sa 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,Jia Zhang,Ning Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou +86 more
TL;DR: In this paper, the authors presented an updated all-particle energy spectrum of primary cosmic rays in a wide range from 10 14 to 10 17 eVusing 5:5 ; 10 7 events collected from 2000 November through 2004 October by the Tibet-III air-shower array located 4300 m in altitude.
Journal ArticleDOI
Large-Scale Sidereal Anisotropy of Galactic Cosmic-Ray Intensity Observed by the Tibet Air Shower Array
M. Amenomori,S. Ayabe,S. W. Cui,Danzengluobu,L. K. Ding,X. H. Ding,Cunfeng Feng,Zhenyong Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,Hongbo Hu,Jing Huang,Q. Huang,H. Y. Jia,F. Kajino,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,G. M. Le,J. Y. Li,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,M. Sakata,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,T. Utsugi,B. S. Wang,Huanyu Wang,X. Wang,Yu 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,HongMei Zhang,J. L. Zhang,N. J. Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou +78 more
TL;DR: In this paper, the sidereal anisotropy of cosmic ray intensity in the multi-TeV region observed with the Tibet-III air shower array during the period from 1999 through 2003 was analyzed.
Journal ArticleDOI
Knee of the cosmic hydrogen and helium spectrum below 1 PeV measured by ARGO-YBJ and a Cherenkov telescope of LHAASO
B. Bartoli,P. Bernardini,X. J. Bi,Zihuang Cao,S. Catalanotti,S. Z. Chen,T. L. Chen,S. W. Cui,B. Z. Dai,A. D'Amone,Null Danzengluobu,I. De Mitri,B. D'Ettorre Piazzoli,T. Di Girolamo,G. Di Sciascio,C. F. Feng,Zhaoyang Feng,Zhenyong Feng,Q. b. Guo,Y. Q. Guo,H. H. He,Haibing Hu,Hongbo Hu,M. Iacovacci,R. Iuppa,H. Y. Jia,Null Labaciren,H. J. Li,C. Liu,J. Liu,M. Y. Liu,Hong-peng Lu,L. L. Ma,X. H. Ma,Giovanni Mancarella,S. M. Mari,G. Marsella,S. Mastroianni,Paolo Montini,Chang-Chun Ning,L. Perrone,P. Pistilli,P. Salvini,R. Santonico,P. R. Shen,X. D. Sheng,Fudong Shi,A. Surdo,Y. H. Tan,P. Vallania,S. Vernetto,Carlo Vigorito,Huaguang 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. B. Zhao,Null Zhaxiciren,Null Zhaxisangzhu,X. X. Zhou,F. R. Zhu,Q. Q. Zhu,Bai Yibing,M. J. Chen,S. H. Feng,Bingshui Gao,M. H. Gu,C. Hou,Jinyao Liu,Xuelong Wang,Gary Guishan Xiao,B. k. Zhang,Shengxue Zhang,Bin Zhou,X. Zuo +83 more
TL;DR: In this paper, a measurement of the mixed proton and helium energy spectrum, obtained with the combined data of the ARGO-YBJ experiment and a wide field of view Cherenkov telescope, a prototype of the future LHAASO experiment, is reported.
Journal ArticleDOI
First Detection of sub-PeV Diffuse Gamma Rays from the Galactic Disk: Evidence for Ubiquitous Galactic Cosmic Rays beyond PeV Energies.
M. Amenomori,Yongjun Bao,X. J. Bi,Donghong Chen,T. L. Chen,W. Y. Chen,Xu Chen,Yu-Lei Chen,Cirennima,S. W. Cui,Danzengluobu,L. K. Ding,J. Fang,K. Fang,C. F. Feng,Zhaoyang Feng,Z. Y. Feng,Qi Gao,Q. B. Gou,Y. Q. Guo,Yang Guo,H. H. He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jian Huang,H. Y. Jia,L. L. Jiang,H. B. Jin,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Shigeaki Kato,K. Kawata,W. Kihara,Y. Ko,Masayoshi Kozai,Labaciren,Gui-Ming Le,Ang Li,Ang Li,H. J. Li,W. J. Li,W. J. Li,Y. H. Lin,B. Liu,C. X. Liu,J. S. Liu,Minghui Liu,Wenwei Liu,Y. Q. Lou,Hong-peng Lu,X. R. Meng,Kazuoki Munakata,H. Nakada,Y. Nakamura,H. Nanjo,Masaki Nishizawa,M. Ohnishi,T. Ohura,S. Ozawa,X. L. Qian,X. B. Qu,To. Saito,M. Sakata,Takashi Sako,J. Shao,J. Shao,M. Shibata,A. Shiomi,H. Sugimoto,W. Takano,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,H. R. Wu,L. Xue,Y. Yamamoto,Zicai Yang,Y. Yokoe,A. F. Yuan,L. M. Zhai,H. M. Zhang,Jia Zhang,Xiang Zhang,X. Y. Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Shi-Ping Zhao,Zhaxisangzhu,X. X. Zhou,mrow> γ<,mrow,msub +100 more
TL;DR: For the first time, the long-awaited detection of diffuse gamma rays with energies between 100 TeV and 1 PeV in the Galactic disk was reported in this paper, which is consistent with expectations from the hadronic emission scenario in which gamma rays originate from the decay of π 0's produced through the interaction of protons with the interstellar medium.