M
M. Shibata
Researcher at Yokohama National University
Publications - 123
Citations - 2089
M. Shibata is an academic researcher from Yokohama National University. The author has contributed to research in topics: Air shower & Cosmic ray. The author has an hindex of 21, co-authored 123 publications receiving 1861 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
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.
Posted Content
High-energy electron observations by PPB-BETS flight in Antarctica
Shoji Torii,K. Mizutani,T. Tamura,Hisao Yamagishi,Shigeo Ohta,Michiyoshi Namiki,Hiroshi Murakami,Y. Katayose,Yukihiko Matsuzaka,T. Yamashita,Yoshihiko Saito,Yoshiko Komori,Issei Iijima,M. Shibata,Kenji Yoshida,Tadashi Kobayashi,N. Tateyama,Jin Chang,Masaki Ejiri,Jun Nishimura,Akira Kadokura,Kazuaki Anraku,Hisashi Kitamura,T. Yuda,K. Kasahara,Takamasa Yamagami +25 more
TL;DR: In this article, a long duration balloon flight using Polar Patrol Balloon (PPB) in Antarctica was used to observe cosmic-ray electrons from 10 GeV to 800 GeV.
Journal ArticleDOI
Are protons still dominant at the knee of the cosmic-ray energy spectrum?
M. Amenomori,S. Ayabe,D. Chen,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,J. Mu,Kazuoki Munakata,A. Nagai,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. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,X. 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,N. J. Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou +77 more
TL;DR: In this article, a hybrid experiment consisting of emulsion chambers, burst detectors and the Tibet-II air-shower array was carried out at Yangbajing (4300 m a.s.l., 606 g / cm 2 ) in Tibet to obtain the energy spectra of primary protons and heliums.
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.