【作者单位】Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences；Department of Physics,Hirosaki University,Hirosaki 036-8561,Japan；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 Particle A；Faculty of Engineering,Kanagawa University,Yokohama 221-8686,Japan；Faculty of Education,Utsunomiya University,Utsunomiya 321-8505,Japan；Institute for Cosmic Ray Research,University of Tokyo,Kashiwa 277-8582,Japan；Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences；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；School of Information Science and Engineering,Shandong Agriculture University,Taian 271018,China Dep；Research Institute for Science and Engineering,Waseda University,Tokyo 169-8555,Japan Saitama Univer；National Institute of Informatics,Tokyo 101-8430,Japan；Department of Physics,Hebei Normal University,Shijiazhuang 050016,China；Sakushin Gakuin University,Utsunomiya 321-3295,Japan；Department of Physics,Shandong University,Jinan 250100,China Key Laboratory of Particle Astrophysics；Tokyo Metropolitan College of Industrial Technology,Tokyo 116-8523,Japan；Max-Planck-Institut f ur Physik,M unchen D-80805,Deutschland；Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences；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 sidereal anisotropy TeV energies Loss Cone
【摘要】 The galactic cosmic-ray anisotropy at TeV energies has a large-scale de cit region distributed around 150 to240 degrees in right ascension,which is called 'Loss-Cone '.The Milagro experiment in the U.S.detected a signi cantincrease in the Loss-Cone a...
