【作者】Amenomori, M.，Bi, X. J.，Chen, D.，Cui, S. W.，Danzengluobu，Ding, L. K.，Ding, X. H.，Fan, C.，Feng, C. F.，Feng, Zhaoyang，Feng, Z. Y.，Gao, X. Y.，Geng, Q. X.，Gou, Q. B.，Guo, H. W.，He, H. H.，He, M.，Hibino, K.，Hotta, N.，Hu, Haibing
【DOI】10.1063/1.3529985
【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 Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan 4 Department of Physics, Hebei Normal University, Shijiazhuang 050016, China 5 Department of Mathematics and Physics, Tibet University, Lhasa 850000, China 6 Department of Physics, Shandong University, Jinan 250100, China 7 Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China 8 Department of Physics, Yunnan University, Kunming 650091, China 9 Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan 10 Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan
【年份】2010
【卷号】Vol.1302 No.1
【页码】285-290
【ISSN】0094-243X
【摘要】 Mapping the global heliosphere by detecting energetic neutral atoms (ENAs), IBEX derived the semi-direct information on the structure of the large-scale magnetic field surrounding the heliosphere. Multi-TeV galactic cosmic rays (GCRs) also sense the ...
