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Variation of Sun shadow in the Solar Cycle 23 observed with the Tibet air shower array
Amenomori, M.2; Ayabe, S.3; Cui, S. W.4; Danzengluobu5; Ding, L. K.4; Ding, X. H.5; Feng, C. F.6; Feng, Z. Y.7; Gao, X. Y.8; Geng, Q. X.8
刊名ADVANCES IN SPACE RESEARCH
2006
卷号38页码:936-941
关键词TeV cosmic rays Sun shadow Gnevyshev gap Tibet AS gamma experiment
ISSN号0273-1177
DOI10.1016/j.asr.2006.04.023
英文摘要According to many solar observations, the solar activity, during the Solar Cycle 23, is gradually declining to the quiet phase from the high state in 2000-2004. The Tibet air shower array has been continuing the observation of the shadow that cosmic rays make in the direction of the sun or the moon since 1991. We have shown the influence of the magnetic field around the sun, the interplanetary and the geomagnetic fields for the sun shadow at the multi-TeV region. We discuss the variation of the Sun's shadow with the Gnevyshev gap (GG) in the maximum phase of the Solar Cycle 23. Unfortunately, the bottom in GG corresponds to off-observation period. Nonetheless, we found the anti-correlation between the significance of the Sun's shadow and the variation of the magnetic field intensity around GG, although the statistical significance is not so high. It is expected that a detailed analysis of the Sun's shadow will reveal interesting features of the anti-correlation. (c) 2006 COSPAR. Published by Elsevier Ltd. All rights reserved.
WOS关键词COSMIC-RAYS ; PHASE ; MAXIMUM ; FEATURES
WOS研究方向Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences
语种英语
出版者ELSEVIER SCI LTD
WOS记录号WOS:000202988200017
内容类型期刊论文
源URL[http://119.78.100.186/handle/113462/26889]  
专题中国科学院近代物理研究所
通讯作者Nishizawa, M.
作者单位1.Natl Inst Informat, Tokyo 1018430, Japan
2.Hirosaki Univ, Dept Phys, Hirosaki, Aomori 0368561, Japan
3.Saitama Univ, Dept Phys, Saitama City, Saitama 3388570, Japan
4.Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China
5.Tibet Univ, Dept Math & Phys, Lhasa 850000, Peoples R China
6.Shandong Univ, Dept Phys, Jinan 250100, Peoples R China
7.S W Jiaotong Univ, Inst Modern Phys, Chengdu 610031, Peoples R China
8.Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China
9.Kanagawa Univ, Fac Engn, Yokohama, Kanagawa 2218686, Japan
10.Utsunomiya Univ, Fac Educ, Utsunomiya, Tochigi 3218505, Japan
推荐引用方式
GB/T 7714
Amenomori, M.,Ayabe, S.,Cui, S. W.,et al. Variation of Sun shadow in the Solar Cycle 23 observed with the Tibet air shower array[J]. ADVANCES IN SPACE RESEARCH,2006,38:936-941.
APA Amenomori, M..,Ayabe, S..,Cui, S. W..,Danzengluobu.,Ding, L. K..,...&Zhou, X. X..(2006).Variation of Sun shadow in the Solar Cycle 23 observed with the Tibet air shower array.ADVANCES IN SPACE RESEARCH,38,936-941.
MLA Amenomori, M.,et al."Variation of Sun shadow in the Solar Cycle 23 observed with the Tibet air shower array".ADVANCES IN SPACE RESEARCH 38(2006):936-941.
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