【作者】M. Amenomori，S. Ayabe，Caidong，Danzengluobu，L. K. Ding，Z. Y. Feng，Y. Fu，H. W. Guo，M. He，K. Hibino，N. Hotta，Q. Huang，A. X. Huo，K. Izu，H. Y. Jia，F. Kajino，K. Kasahara，Y. Katayose，Labaciren，J. Y. Li，H. Lu，S. L. Lu，G. X. Luo，X. R. Meng，K. Mizutani，J. Mu，H. Nanjo，M. Nishizawa，M. Ohnishi，I. Ohta，T. Ouchi，Z. R. Peng，J. R. Ren，T. Saito，M. Sakata，T. Sasaki，Z. Z. Shi，M. Shibata，A. Shiomi，T. Shirai，Y. Suga，H. Sugimoto，K. Taira，Y. H. Tan，N. Tateyama，S. Torii，T. Utsugi，C. R. Wang，H. Wang，X. W. Xu，Y. Yamamoto，G. C. Yu，A. F. Yuan，T. Yuda，C. S. Zhang，H. M. Zhang，J. L. Zhang，N. J. Zhang，X. Y. Zhang，Zhaxiciren，Zhaxisangzhu，
【DOI】10.1086/309479
【作者单位】Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan;Department of Physics, Saitama University, Urawa 338-8570, Japan;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Department of Physics, South West Jiaotong University, Chengdu 610031, China;Department of Physics, Shangdong University, Jinan 250100, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Department of Physics, Shangdong University, Jinan 250100, China;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan;Department of Physics, South West Jiaotong University, Chengdu 610031, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Department of Physics, South West Jiaotong University, Chengdu 610031, China;Department of Physics, Konan University, Kobe 658-8501, Japan;Faculty of Systems Engineering, Shibaura Institute of Technology, Omiya 330-8570, Japan;Faculty of Engineering, Yokohama National University, Yokohama 240-0067, Japan;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Department of Physics, Shangdong University, Jinan 250100, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Department of Physics, Saitama University, Urawa 338-8570, Japan;Department of Physics, Yunnan University, Kunming 650091, China;Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan;National Institute of Informatics, Tokyo 101-8430, Japan;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Tokyo Metropolitan College of Aeronautical Engineering, Tokyo 116-0003, Japan;Department of Physics, Konan University, Kobe 658-8501, Japan;Department of Physics, Konan University, Kobe 658-8501, Japan;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Faculty of Engineering, Yokohama National University, Yokohama 240-0067, Japan;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Department of Physics, Konan University, Kobe 658-8501, Japan;Shonan Institute of Technology, Fujisawa 251-8511, Japan;Shonan Institute of Technology, Fujisawa 251-8511, Japan;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Department of Physics, Saitama University, Urawa 338-8570, Japan;Department of Physics, Shangdong University, Jinan 250100, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Department of Physics, Konan University, Kobe 658-8501, Japan;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya 464-8601, Japan;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Academia Sinica, Beijing 100039, China;Department of Physics, Shangdong University, Jinan 250100, China;Department of Physics, Shangdong University, Jinan 250100, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China
【年份】2000
【卷号】Vol.541 No.2
【页码】1051-1058
【ISSN】0004-637X
【关键词】cosmic rays, interplanetary medium, magnetic fields, solar-terrestrial relations, solar wind
【摘要】 We have shown that the Sun's shadow by high-energy cosmic rays moves year by year and its behavior is correlated with a time variation of the large-scale structure of the solar and interplanetary magnetic fields. The solar activity was near minimum i...
