Sun's shadow by 10 TeV cosmic rays under the influence of solar activity

M. Amenomori; S. Ayabe; P. Y. Cao; B. Z. Dai; 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; S. M. Liu; H. Lu; S. L. Lu; G. X. Luo; D. M. Mei; X. R. Meng; K. Mizutani; J. Mu; H. Nanjo; M. Nishizawa; M. Ohnishi; I. Ohta; T. Ouchi; J. R. Ren; To Saito; M. Sakata; T. Sasaki; C. Shi; Z. Z. Shi; M. Shibata; A. Shiomi; T. Shirai; H. Sugimoto; K. Taira; Y. H. Tan; N. Tateyama; Shoji Torii; T. Utsugi; C. R. Wang; H. Wang; P. X. Wang; W. Xie; 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; Zhaxisangzhu; Zhaxiciren; S. J. Zhou; W. D. Zhou

Sun's shadow by 10 TeV cosmic rays under the influence of solar activity

M. Amenomori^*, S. Ayabe, P. Y. Cao, B. Z. Dai, 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. LiS. M. Liu, H. Lu, S. L. Lu, G. X. Luo, D. M. Mei, X. R. Meng, K. Mizutani, J. Mu, H. Nanjo, M. Nishizawa, M. Ohnishi, I. Ohta, T. Ouchi, J. R. Ren, To Saito, M. Sakata, T. Sasaki, C. Shi, Z. Z. Shi, M. Shibata, A. Shiomi, T. Shirai, H. Sugimoto, K. Taira, Y. H. Tan, N. Tateyama, Shoji Torii, T. Utsugi, C. R. Wang, H. Wang, P. X. Wang, W. Xie, 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, Zhaxisangzhu, Zhaxiciren, S. J. Zhou, W. D. Zhou

^*この研究の対応する著者

研究成果: Article › 査読

2 被引用数 (Scopus)

抄録

We examined the Sun's shadow by 10 TeV cosmic rays observed with the Tibet air shower array during the period from 1991 through 1997. The results suggest that there is a causal relation between the shadow's movement and the changing inclination of the heliospheric current sheet of the large-scale solar magnetic field. Thus, further observations with higher statistics may provide direct information on the relation between a time variation of the large-scale structure of the solar and interplanetary magnetic fields and the phase of solar activity cycle.

本文言語	English
ページ（範囲）	611-615
ページ数	5
ジャーナル	Advances in Space Research
巻	23
号	3
出版ステータス	Published - 1999
外部発表	はい

ASJC Scopus subject areas

宇宙惑星科学
天文学と天体物理学

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引用スタイル

Amenomori, M, Ayabe, S, Cao, PY, Dai, BZ, Ding, LK, Feng, ZY, Fu, Y, Guo, HW, He, M, Hibino, K, Hotta, N, Huang, Q, Huo, AX, Izu, K, Jia, HY, Kajino, F, Kasahara, K, Katayose, Y, Labaciren, Li, JY, Liu, SM, Lu, H, Lu, SL, Luo, GX, Mei, DM, Meng, XR, Mizutani, K, Mu, J, Nanjo, H, Nishizawa, M, Ohnishi, M, Ohta, I, Ouchi, T, Ren, JR, Saito, T, Sakata, M, Sasaki, T, Shi, C, Shi, ZZ, Shibata, M, Shiomi, A, Shirai, T, Sugimoto, H, Taira, K, Tan, YH, Tateyama, N, Torii, S, Utsugi, T, Wang, CR, Wang, H, Wang, PX, Xie, W, Xu, XW, Yamamoto, Y, Yu, GC, Yuan, AF, Yuda, T, Zhang, CS, Zhang, HM, Zhang, JL, Zhang, NJ, Zhang, XY, Zhaxisangzhu, Zhaxiciren, Zhou, SJ & Zhou, WD 1999, 'Sun's shadow by 10 TeV cosmic rays under the influence of solar activity', Advances in Space Research, vol. 23, no. 3, pp. 611-615.

@article{aced2674e56f4ea5a01331c9dcd6a357,

title = "Sun's shadow by 10 TeV cosmic rays under the influence of solar activity",

abstract = "We examined the Sun's shadow by 10 TeV cosmic rays observed with the Tibet air shower array during the period from 1991 through 1997. The results suggest that there is a causal relation between the shadow's movement and the changing inclination of the heliospheric current sheet of the large-scale solar magnetic field. Thus, further observations with higher statistics may provide direct information on the relation between a time variation of the large-scale structure of the solar and interplanetary magnetic fields and the phase of solar activity cycle.",

author = "M. Amenomori and S. Ayabe and Cao, {P. Y.} and Dai, {B. Z.} and Ding, {L. K.} and Feng, {Z. Y.} and Y. Fu and Guo, {H. W.} and M. He and K. Hibino and N. Hotta and Q. Huang and Huo, {A. X.} and K. Izu and Jia, {H. Y.} and F. Kajino and K. Kasahara and Y. Katayose and Labaciren and Li, {J. Y.} and Liu, {S. M.} and H. Lu and Lu, {S. L.} and Luo, {G. X.} and Mei, {D. M.} and Meng, {X. R.} and K. Mizutani and J. Mu and H. Nanjo and M. Nishizawa and M. Ohnishi and I. Ohta and T. Ouchi and Ren, {J. R.} and To Saito and M. Sakata and T. Sasaki and C. Shi and Shi, {Z. Z.} and M. Shibata and A. Shiomi and T. Shirai and H. Sugimoto and K. Taira and Tan, {Y. H.} and N. Tateyama and Shoji Torii and T. Utsugi and Wang, {C. R.} and H. Wang and Wang, {P. X.} and W. Xie and Xu, {X. W.} and Y. Yamamoto and Yu, {G. C.} and Yuan, {A. F.} and T. Yuda and Zhang, {C. S.} and Zhang, {H. M.} and Zhang, {J. L.} and Zhang, {N. J.} and Zhang, {X. Y.} and Zhaxisangzhu and Zhaxiciren and Zhou, {S. J.} and Zhou, {W. D.}",

year = "1999",

language = "English",

volume = "23",

pages = "611--615",

journal = "Advances in Space Research",

issn = "0273-1177",

publisher = "Elsevier Limited",

number = "3",

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TY - JOUR

T1 - Sun's shadow by 10 TeV cosmic rays under the influence of solar activity

AU - Amenomori, M.

AU - Ayabe, S.

AU - Cao, P. Y.

AU - Dai, B. Z.

AU - Ding, L. K.

AU - Feng, Z. Y.

AU - Fu, Y.

AU - Guo, H. W.

AU - He, M.

AU - Hibino, K.

AU - Hotta, N.

AU - Huang, Q.

AU - Huo, A. X.

AU - Izu, K.

AU - Jia, H. Y.

AU - Kajino, F.

AU - Kasahara, K.

AU - Katayose, Y.

AU - Labaciren,

AU - Li, J. Y.

AU - Liu, S. M.

AU - Lu, H.

AU - Lu, S. L.

AU - Luo, G. X.

AU - Mei, D. M.

AU - Meng, X. R.

AU - Mizutani, K.

AU - Mu, J.

AU - Nanjo, H.

AU - Nishizawa, M.

AU - Ohnishi, M.

AU - Ohta, I.

AU - Ouchi, T.

AU - Ren, J. R.

AU - Saito, To

AU - Sakata, M.

AU - Sasaki, T.

AU - Shi, C.

AU - Shi, Z. Z.

AU - Shibata, M.

AU - Shiomi, A.

AU - Shirai, T.

AU - Sugimoto, H.

AU - Taira, K.

AU - Tan, Y. H.

AU - Tateyama, N.

AU - Torii, Shoji

AU - Utsugi, T.

AU - Wang, C. R.

AU - Wang, H.

AU - Wang, P. X.

AU - Xie, W.

AU - Xu, X. W.

AU - Yamamoto, Y.

AU - Yu, G. C.

AU - Yuan, A. F.

AU - Yuda, T.

AU - Zhang, C. S.

AU - Zhang, H. M.

AU - Zhang, J. L.

AU - Zhang, N. J.

AU - Zhang, X. Y.

AU - Zhaxisangzhu,

AU - Zhaxiciren,

AU - Zhou, S. J.

AU - Zhou, W. D.

PY - 1999

Y1 - 1999

N2 - We examined the Sun's shadow by 10 TeV cosmic rays observed with the Tibet air shower array during the period from 1991 through 1997. The results suggest that there is a causal relation between the shadow's movement and the changing inclination of the heliospheric current sheet of the large-scale solar magnetic field. Thus, further observations with higher statistics may provide direct information on the relation between a time variation of the large-scale structure of the solar and interplanetary magnetic fields and the phase of solar activity cycle.

AB - We examined the Sun's shadow by 10 TeV cosmic rays observed with the Tibet air shower array during the period from 1991 through 1997. The results suggest that there is a causal relation between the shadow's movement and the changing inclination of the heliospheric current sheet of the large-scale solar magnetic field. Thus, further observations with higher statistics may provide direct information on the relation between a time variation of the large-scale structure of the solar and interplanetary magnetic fields and the phase of solar activity cycle.

UR - http://www.scopus.com/inward/record.url?scp=0039254590&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0039254590&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:0039254590

SN - 0273-1177

VL - 23

SP - 611

EP - 615

JO - Advances in Space Research

JF - Advances in Space Research

IS - 3

ER -

Sun's shadow by 10 TeV cosmic rays under the influence of solar activity

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