【作者】Amenomori, M,Bi, X. J,Chen, D,Chen, T. L,Chen, W. Y,Cui, S. W,Danzengluobu,Ding, L. K,Feng, C. F,Feng, Zhaoyang,Feng, Z. Y,Gou, Q. B,Guo, Y. Q,He, H. H,He, Z. T,Hibino, K,Hotta, N,Hu, Haibing,Hu, H. B,Huang, J
【作者单位】1 Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan 2 Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China 3 National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China 4 Department of Mathematics and Physics, Tibet University, Lhasa 850000, China 5 Department of Physics, Hebei Normal University, Shijiazhuang 050016, China 6 Department of Physics, Shandong University, Jinan 250100, China 7 Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China 8 Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan 9 Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan
【年份】2019
【卷号】Vol.208
【ISSN】2100-014X
【摘要】 We analyze the temporal variation of the solar diurnal anisotropy of the multi-TeV cosmic-ray intensity observed with the Tibet air shower array from 2000 to 2009, covering the maximum and minimum of the 23rd solar cycle. We comfirm that a remarkable...