【作者】M. AMENOMORI，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，X. J. BI，H. B. HU，J. HUANG，W. J. LI，H. Y. JIA，L. JIANG，F. KAJINO，K. KASAHARA，Y. KATAYOSE，C. KATO，K. KAWATA，D. CHEN，LABACIREN，G. M. LE，A. F. LI，C. LIU，J. S. LIU，H. LU，X. R. MENG，K. MIZUTANI，K. MUNAKATA，H. NANJO，W. Y. CHEN，M. NISHIZAWA，M. OHNISHI，I. OHTA，S. OZAWA，X. L. QIAN，X. B. QU，T. SAITO，T. Y. SAITO，M. SAKATA，T. K. SAKO，S. W. CUI，J. SHAO，M. SHIBATA，A. SHIOMI，T. SHIRAI，H. SUGIMOTO，M. TAKITA，Y. H. TAN，N. TATEYAMA，S. TORII，H. TSUCHIYA，DANZENGLUOBU，S. UDO，H. WANG，H. R. WU，L. XUE，Y. YAMAMOTO，Z. YANG，S. YASUE，A. F. YUAN，T. YUDA，L. M. ZHAI，L. K. DING，H. M. ZHANG，J. L. ZHANG，X. Y. ZHANG，Y. ZHANG，YI ZHANG，YING ZHANG，ZHAXISANGZHU，X. X. ZHOU，X. H. DING，C. F. FENG
【作者单位】Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan；Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Scienc；Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China；Department of Mathematics and Physics, Tibet University, Lhasa 850000, China；Department of Physics, Hebei Normal University, Shijiazhuang 050016, China Key Laboratory of Particl；Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan；Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan；Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Scienc；Department of Physics, Konan University, Kobe 658-8501, Japan；Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan；Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan；Department of Physics, Shinshu University, Matsumoto 390-8621, Japan；Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan；School of Information Science and Engineering, Shandong Agriculture University, Taian 271018, China；11Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan Saitama U；National Institute of Informatics, Tokyo 101-8430, Japan；Sakushin Gakuin University, Utsunomiya 321-3295, Japan；Department of Physics, Shandong University, Jinan 250100, China Key Laboratory of Particle Astrophys；Tokyo Metropolitan College of Industrial Technology, Tokyo 116-8523, Japan；Max-Planck-Institut fur Physik, Munchen D-80805, Deutschland；Department of Physics, Hebei Normal University, Shijiazhuang 050016, China；Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Scienc；College of Industrial Technology, Nihon University, Narashino 275-8576, Japan；Shonan Institute of Technology, Fujisawa 251-8511, Japan；RIKEN, Wako 351-0198, Japan；Department of Physics, Shandong University, Jinan 250100, China；School of General Education, Shinshu University, Matsumoto 390-8621, Japan
【召开年】2011
【会议地点】北京
【会议录】第32届国际宇宙线大会论文集
【关键词】Tibet galactic cosmic rays anisotropy TeV energies
【摘要】 A possible origin of the large-scale anisotropy of TeV galactic cosmic rays is discussed. It can be well modeled by a superposition of the Global Anisotropy and the Midscale Anisotropy. The Global Anisotropy would be generated by galactic cosmic rays...
