【作者单位】1 Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan ; 2 Department of Physics, Saitama University, Saitama 338-8570, Japan ; 3 Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100039, China ; 4 Department of Mathematics and Physics, Tibet University, Lhasa 850000, China ; 5 Department of Physics, Shangdong University, Jinan 250100, China ; 6 Institute of Modern Physics, South West Jiaotong University, Chengdu 610031, China ; 7 Department of Physics, Yunnan University, Kunming 650091, China ; 8 Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan ; 9 Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan ; 10 Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan ; 11 Department of Physics, Konan University, Kobe 658-8501, Japan ; 12 Faculty of Systems Engineering, Shibaura Institute of Technology, Saitama 330-8570, Japan ; 13 Faculty of Engineering, Yokohama National University, Yokohama 240-0067, Japan ; 14 Center of Space Science and Application Research, Chinese Academy of Sciences, Beijing 100080, China ; 15 National Institute for Informatics, Tokyo 112-8640, Japan ; 16 Tokyo Metropolitan College of Aeronautical Engineering, Tokyo 116-0003, Japan ; 17 Shonan Institute of Technology, Fujisawa 251-8511, Japan ; 18 Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya 464-8601, Japan ;
【年份】2002
【卷号】Vol.580 No.2
【页码】887-895
【ISSN】0004-637X
【关键词】acceleration of particles, cosmic rays, Galaxy disk, ISM general
【摘要】 Data from the Tibet III air shower array (with energies around 3 TeV) and from the Tibet II array (with energies around 10 TeV) have been searched for diffuse gamma rays from the Galactic plane. These arrays have an angular resolution of about 0 \doc...
