S
S. L. Lu
Researcher at Chinese Academy of Sciences
Publications - 55
Citations - 1343
S. L. Lu 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 15, co-authored 54 publications receiving 1237 citations. Previous affiliations of S. L. Lu include Tsinghua University.
Papers
More filters
Journal ArticleDOI
Multi-TeV Gamma-Ray Flares from Markarian 421 in 2000 and 2001 Observed with 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,K. Kawata,Labaciren,G. M. Le,J. Y. Li,Hong-peng Lu,S. L. Lu,X. R. Meng,K. Mizutani,J. Mu,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,T. Ouchi,Shunsuke Ozawa,Jieru Ren,To. Saito,M. Sakata,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,K. Taira,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,T. Utsugi,B. S. Wang,Huanyu Wang,X. Wang,Y. G. Wang,L. Xue,Y. Yamamoto,X. C. Yang,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,T. Yuda,HongMei Zhang,J. L. Zhang,N. J. Zhang,X. Y. Zhang,Y. Zhang,Zhaxisangzhu,X. X. Zhou +72 more
TL;DR: In this paper, a power-law energy spectrum for γ-rays from this source is assumed, the spectral index is calculated to be -3.24 ± 0.69 at the most active phase in 2001.
Journal ArticleDOI
Primary proton spectrum between 200-TeV and 1000-TeV observed with the Tibet burst detector and air shower array
M. Amenomori,S. Ayabe,Caidong,Danzengluobu,L. K. Ding,Z. Y. Feng,Y. Fu,H. W. Guo,M. He,K. Hibino,N. Hotta,Q. Huang,A. X. Huo,K. Izu,H. Y. Jia,F. Kajino,Katsuaki Kasahara,Y. Katayose,Labaciren,J. Y. Li,Hsiao-Chi Lu,S. L. Lu,G. X. Luo,X. R. Meng,K.Mizutani K.Mizutani,J. Mu,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,T. Ouchi,Z. R. Peng,Jieru Ren,Takeshi Saito,M. Sakata,T. Sasaki,Z. Z. Shi,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,K. Taira,Y. H. Tan,N. Tateyama,S. Torii,T. Utsugi,C. R. Wang,Huaguang Wang,X. W. Xu,Y. Yamamoto,G. C. Yu,A. F. Yuan,T. Yuda,T. Yuda,C. S. Zhang,H. M. Zhang,Jia Zhang,N. J. Zhang,X. Y. Zhang,Zhaxiciren,Zhaxisangzhu +60 more
TL;DR: In this paper, a hybrid experiment consisting of the emulsion chamber and burst detector array and the Tibet-II air-shower array has been operated at Yangbajing (4300 m above sea level, 606 $\mathrm{g}/{\mathm{cm}}^{2})$ in Tibet.
Journal ArticleDOI
Multi-Tev Gamma-Ray Observation from the Crab Nebula Using the Tibet-III Air Shower Array Finely Tuned by the Cosmic-Ray Moon's Shadow
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,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,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,T. K. 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,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 article, the authors estimate the systematic error in determining the primary energy from its shower size, which is estimated to be less than ±12% in their experiment. But this error is consistent with other independent γ-ray observations by imaging air Cherenkov telescopes.
Journal ArticleDOI
Cosmic-ray energy spectrum around the knee obtained by the Tibet experiment and future prospects
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,Kazumasa Kawata,Labaciren,G. M. Le,A. F. Li,J. Y. Li,Y. Q. Lou,Hsiao-Chi 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,Takeshi 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. S. Wang,Huaguang Wang,X. 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,Yizhang,Zhaxisangzhu,X. X. Zhou +84 more
TL;DR: In this paper, the authors used a low threshold air-shower core detector named YAC to measure the heavy elements around the knee, which indicated the dominance of nuclei heavier than helium.
Journal ArticleDOI
Observation by an air-shower array in Tibet of the multi-TeV cosmic-ray anisotropy due to terrestrial orbital motion around the Sun.
M. Amenomori,S. Ayabe,S. W. Cui,Danzengluobu,L. K. Ding,X. H. Ding,Cunfeng 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,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,G. M. Le,J. Y. Li,Hsiao-Chi Lu,S. L. Lu,X. R. Meng,K. Mizutani,S. Mori,J. Mu,Kazuoki Munakata,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,Shunsuke Ozawa,Jieru Ren,Takeshi Saito,M. Sakata,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. E. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,T. Utsugi,B. S. Wang,Huaguang Wang,X. Wang,Yu 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,N. J. Zhang,Xuan Zhang,Y. Zhang,Zhaxisangzhu,X. X. Zhou +77 more
TL;DR: The solar diurnal variation of the galactic cosmic-ray intensity observed by the Tibet III air shower array during the period from 1999 to 2003 is reported, suggesting an additional anisotropy superposed at the multi-TeV energies, e.g., the solar modulation effect.