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Probe of the Solar Magnetic Field Using the "Cosmic-Ray Shadow" of the Sun
Amenomori, M; Bi, XJ; Chen, D; Chen, TL; Chen, WY; Cui, SW; Danzengluobu; Ding, LK; Feng, CF; Feng, ZY; Feng, ZY; Gou, QB; Guo, YQ; Hakamada, K; He, HH; He, ZT; Hibino, K; Hotta, N; Hu, HB; Hu, HB; Huang, J; Jia, HY; Jiang, L; Kajino, F; Kasahara, K; Katayose, Y; Kato, C; Kawata, K; Labaciren; Le, GM; Li, AF; Li, HJ; Li, WJ; Liu, C; Liu, JS; Liu, MY; Lu, H; Meng, XR; Mizutani, K; Munakata, K; Nanjo, H; Nishizawa, M; Ohnishi, M; Ohta, I; Onuma, H; Ozawa, S; Qian, XL; Qu, XB; Saito, T; Saito, TY; Sakata, M; Sako, TK; Shao, J; Shibata, M; Shiomi, A; Shirai, T; Sugimoto, H; Takita, M; Tan, YH; Tateyama, N; Torii, S; Tsuchiya, H; Udo, S; Wang, H; Wu, HR; Xue, L; Yamamoto, Y; Yang, Z; Yasue, S; Yuan, AF; Yuda, T; Zhai, LM; Zhang, HM; Zhang, JL; Zhang, XY; Zhang, Y; Zhang, Y; Zhang, Y; Zhaxisangzhu; Zhou, XX; Bi XJ(毕效军); Chen WY(陈文益); Ding LK(丁林凯); Feng CY(冯朝阳); Gou QB(苟全补); Guo YQ(郭义庆); He HH(何会海); Hu HB(胡红波); Huang J(黄晶); Li WJ(李万杰); Jiang L(姜龙); Kang MM(康明铭); Le GM(乐贵明); Liu C(刘成); Liu JS(刘金胜); Lu H(卢红); Qu XB(曲晓波); Tan YH(谭有恒); Wang H(王辉); Wu HR(吴含荣); Shen ZQ(沈长铨); Shen PR(沈培若); Yang Z(杨振); Zhai LM(翟留名); Zhang HM(张慧敏); Zhang JL(张吉龙); Zhang Y(张勇); Zhang Y(张毅); Zhang Y(张颖)
2013
发表期刊PHYSICAL REVIEW LETTERS
卷号111期号:1页码:11101
摘要We report on a clear solar-cycle variation of the Sun's shadow in the 10 TeV cosmic-ray flux observed by the Tibet air shower array during a full solar cycle from 1996 to 2009. In order to clarify the physical implications of the observed solar cycle variation, we develop numerical simulations of the Sun's shadow, using the potential field source surface model and the current sheet source surface (CSSS) model for the coronal magnetic field. We find that the intensity deficit in the simulated Sun's shadow is very sensitive to the coronal magnetic field structure, and the observed variation of the Sun's shadow is better reproduced by the CSSS model. This is the first successful attempt to evaluate the coronal magnetic field models by using the Sun's shadow observed in the TeV cosmic-ray flux.
学科领域Physics
DOI10.1103/PhysRevLett.111.011101
收录类别SCI
WOS记录号WOS:000321126500003
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被引频次:10[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/224471
专题粒子天体物理中心
中国科学院高能物理研究所_中国散裂中子源
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Amenomori, M,Bi, XJ,Chen, D,et al. Probe of the Solar Magnetic Field Using the "Cosmic-Ray Shadow" of the Sun[J]. PHYSICAL REVIEW LETTERS,2013,111(1):11101.
APA Amenomori, M.,Bi, XJ.,Chen, D.,Chen, TL.,Chen, WY.,...&张颖.(2013).Probe of the Solar Magnetic Field Using the "Cosmic-Ray Shadow" of the Sun.PHYSICAL REVIEW LETTERS,111(1),11101.
MLA Amenomori, M,et al."Probe of the Solar Magnetic Field Using the "Cosmic-Ray Shadow" of the Sun".PHYSICAL REVIEW LETTERS 111.1(2013):11101.
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