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Variation of Sun shadow in the Solar Cycle 23 observed with the Tibet air shower array
Amenomori, M.; Ayabe, S.; Cui, S. W.; Danzengluobu,; Ding, L. K.; Ding, X. H.; Feng, C. F.; Feng, Z. Y.; Gao, X. Y.; Geng, Q. X.; Guo, H. W.; He, H. H.; He, M.; Hibino, K.; Hotta, N.; Hu, H. B.; Huang, J.; Huang, Q.; Izumi, M.; Jia, H. Y.; Kajino, F.; Kasahara, K.; Katayose, Y.; Kato, C.; Kawata, K.; Labaciren,; Le, G. M.; Li, J. Y.; Lu, H.; Lu, S. L.; Meng, X. R.; Mizutani, K.; Mu, J.; Munakata, K.; Nagai, A.; Nanjo, H.; Nishizawa, M.; Ohnishi, M.; Ohta, I.; Onuma, H.; Ouchi, T.; Ozawa, S.; Ren, J. R.; Saito, T.; Sakata, M.; Sasaki, T.; Shibata, M.; Shiomi, A.; Shirai, T.; Sugimoto, H.; Takita, M.; Tan, Y. H.; Tateyama, N.; Torii, S.; Tsuchiya, H.; Udo, S.; Utsugi, T.; Wang, B. S.; Wang, H.; Wang, X.; Wang, Y. G.; Wu, H. R.; Xue, L.; Yamamoto, Y.; Yan, C. T.; Yang, X. C.; Yasue, S.; Ye, Z. H.; Yu, G. C.; Yuan, A. F.; Yuda, T.; Zhang, H. M.; Zhang, J. L.; Zhang, N. J.; Zhang, X. Y.; Zhang, Y.; Zhaxisangzhu,; Zhou, X. X.; Tibet AsGamma, Collaboration; 北京8701信箱
Department其他
Source PublicationAdvances in Space Research
2006
Volume38Issue:5Pages:936-941
ISSN0273-1177
Language英语
KeywordTev Cosmic Rays Sun Shadow Gnevyshev Gap Tibet As Gamma Experiment Cosmic-rays Phase Maximum Features
AbstractAccording 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.
Indexed BySCI
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/1705
Collection其他部室
Corresponding Author北京8701信箱
Recommended Citation
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(5):936-941.
APA Amenomori, M..,Ayabe, S..,Cui, S. W..,Danzengluobu,.,Ding, L. K..,...&北京8701信箱.(2006).Variation of Sun shadow in the Solar Cycle 23 observed with the Tibet air shower array.Advances in Space Research,38(5),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 38.5(2006):936-941.
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