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

Research output: Contribution to journalArticle

2 Citations (Scopus)

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.

Original languageEnglish
Pages (from-to)611-615
Number of pages5
JournalAdvances in Space Research
Volume23
Issue number3
Publication statusPublished - 1999
Externally publishedYes

Fingerprint

solar magnetic field
Cosmic rays
solar activity
Sun
cosmic ray
cosmic rays
sun
Magnetic fields
magnetic field
Tibet
cosmic ray showers
interplanetary magnetic fields
current sheets
solar cycles
inclination
Statistics
statistics
air
Air

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Amenomori, M., Ayabe, S., Cao, P. Y., Dai, B. Z., Ding, L. K., Feng, Z. Y., ... Zhou, W. D. (1999). Sun's shadow by 10 TeV cosmic rays under the influence of solar activity. Advances in Space Research, 23(3), 611-615.

Sun's shadow by 10 TeV cosmic rays under the influence of solar activity. / Amenomori, M.; Ayabe, S.; Cao, P. Y.; Dai, B. Z.; Ding, L. K.; Feng, Z. Y.; Fu, Y.; Guo, H. W.; He, M.; Hibino, K.; Hotta, N.; Huang, Q.; Huo, A. X.; Izu, K.; Jia, H. Y.; Kajino, F.; Kasahara, K.; Katayose, Y.; Labaciren; Li, J. Y.; Liu, S. M.; Lu, H.; Lu, S. L.; Luo, G. X.; Mei, D. M.; Meng, X. R.; Mizutani, K.; Mu, J.; Nanjo, H.; Nishizawa, M.; Ohnishi, M.; Ohta, I.; Ouchi, T.; Ren, J. R.; Saito, To; Sakata, M.; Sasaki, T.; Shi, C.; Shi, Z. Z.; Shibata, M.; Shiomi, A.; Shirai, T.; Sugimoto, H.; Taira, K.; Tan, Y. H.; Tateyama, N.; Torii, Shoji; Utsugi, T.; Wang, C. R.; Wang, H.; Wang, P. X.; Xie, W.; Xu, X. W.; Yamamoto, Y.; Yu, G. C.; Yuan, A. F.; Yuda, T.; Zhang, C. S.; Zhang, H. M.; Zhang, J. L.; Zhang, N. J.; Zhang, X. Y.; Zhaxisangzhu; Zhaxiciren; Zhou, S. J.; Zhou, W. D.

In: Advances in Space Research, Vol. 23, No. 3, 1999, p. 611-615.

Research output: Contribution to journalArticle

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.
Amenomori M, Ayabe S, Cao PY, Dai BZ, Ding LK, Feng ZY et al. Sun's shadow by 10 TeV cosmic rays under the influence of solar activity. Advances in Space Research. 1999;23(3):611-615.
Amenomori, M. ; Ayabe, S. ; Cao, P. Y. ; Dai, B. Z. ; Ding, L. K. ; Feng, Z. Y. ; Fu, Y. ; Guo, H. W. ; He, M. ; Hibino, K. ; Hotta, N. ; Huang, Q. ; Huo, A. X. ; Izu, K. ; Jia, H. Y. ; Kajino, F. ; Kasahara, K. ; Katayose, Y. ; Labaciren ; Li, J. Y. ; Liu, S. M. ; Lu, H. ; Lu, S. L. ; Luo, G. X. ; Mei, D. M. ; Meng, X. R. ; Mizutani, K. ; Mu, J. ; Nanjo, H. ; Nishizawa, M. ; Ohnishi, M. ; Ohta, I. ; Ouchi, T. ; Ren, J. R. ; Saito, To ; Sakata, M. ; Sasaki, T. ; Shi, C. ; Shi, Z. Z. ; Shibata, M. ; Shiomi, A. ; Shirai, T. ; Sugimoto, H. ; Taira, K. ; Tan, Y. H. ; Tateyama, N. ; Torii, Shoji ; Utsugi, T. ; Wang, C. R. ; Wang, H. ; Wang, P. X. ; Xie, W. ; Xu, X. W. ; Yamamoto, Y. ; Yu, G. C. ; Yuan, A. F. ; Yuda, T. ; Zhang, C. S. ; Zhang, H. M. ; Zhang, J. L. ; Zhang, N. J. ; Zhang, X. Y. ; Zhaxisangzhu ; Zhaxiciren ; Zhou, S. J. ; Zhou, W. D. / Sun's shadow by 10 TeV cosmic rays under the influence of solar activity. In: Advances in Space Research. 1999 ; Vol. 23, No. 3. pp. 611-615.
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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.",
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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.

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M3 - Article

AN - SCOPUS:0039254590

VL - 23

SP - 611

EP - 615

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 3

ER -