Abstract
We analyze the solar cycle variation of the Sun's shadow in 10 TeV cosmic ray intensity observed with the Tibet air shower array over an entire period of the Solar Cycle 23 between 1996 and 2008. The amplitude of the variation is as large as one half of the deficit intensity expected when all cosmic rays arriving from the direction of the optical Sun disk are excluded from the observation. The correlations between the deficit intensity in the Sun's shadow and cosmic-ray modulation parameters are overall significant. Among those parameters, we find the highest correlation with the Heliospheric Current Sheet tilt-angle.
| Original language | English |
|---|---|
| Title of host publication | Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011 |
| Publisher | Institute of High Energy Physics |
| Pages | 239-242 |
| Number of pages | 4 |
| Volume | 11 |
| DOIs | |
| Publication status | Published - 2011 |
| Event | 32nd International Cosmic Ray Conference, ICRC 2011 - Beijing Duration: 2011 Aug 11 → 2011 Aug 18 |
Other
| Other | 32nd International Cosmic Ray Conference, ICRC 2011 |
|---|---|
| City | Beijing |
| Period | 11/8/11 → 11/8/18 |
Fingerprint
Keywords
- Cosmic rays
- Solar magnetic field
- Solar modulation
- Sun's shadow
- Tibet
ASJC Scopus subject areas
- Nuclear and High Energy Physics
Cite this
Correlation between solar activity and the sun's shadow observed by the tibet air shower array. / Amenomori, M.; Bi, X. J.; Chen, D.; Chen, W. Y.; Cui, S. W.; Danzengluobu; Ding, L. K.; Ding, X. H.; Feng, C. F.; Feng, Zhaoyang; Feng, Z. Y.; Gou, Q. B.; Guo, H. W.; Guo, Y. Q.; He, H. H.; He, Z. T.; Hibino, K.; Hotta, N.; Hu, Haibing; Hu, H. B.; Huang, J.; Li, W. J.; Jia, H. Y.; Jiang, L.; Kajino, F.; Kasahara, K.; Katayose, Y.; Kato, C.; Kawata, K.; Labaciren; Le, G. M.; Li, A. F.; Liu, C.; Liu, J. S.; Lu, H.; Meng, X. R.; Mizutani, K.; Munakata, K.; Nanjo, H.; Nishizawa, M.; Ohnishi, M.; Ohta, I.; Ozawa, Shunsuke; Qian, X. L.; Qu, X. B.; Saito, T.; Saito, T. Y.; Sakata, M.; Sako, T. K.; Shao, J.; Shibata, M.; Shiomi, A.; Shirai, T.; Sugimoto, H.; Takita, M.; Tan, Y. H.; Tateyama, N.; Torii, Shoji; Tsuchiya, H.; Udo, S.; Wang, H.; Wu, H. R.; Xue, L.; Yamamoto, Y.; Yang, Z.; Yasue, S.; Yuan, A. F.; Yuda, T.; Zhai, L. M.; Zhang, H. M.; Zhang, J. L.; Zhang, X. Y.; Zhang, Y.; Zhang, Yi; Zhang, Ying; Zhaxisangzhu; Zhou, X. X.
Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011. Vol. 11 Institute of High Energy Physics, 2011. p. 239-242.Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
}
TY - GEN
T1 - Correlation between solar activity and the sun's shadow observed by the tibet air shower array
AU - Amenomori, M.
AU - Bi, X. J.
AU - Chen, D.
AU - Chen, W. Y.
AU - Cui, S. W.
AU - Danzengluobu,
AU - Ding, L. K.
AU - Ding, X. H.
AU - Feng, C. F.
AU - Feng, Zhaoyang
AU - Feng, Z. Y.
AU - Gou, Q. B.
AU - Guo, H. W.
AU - Guo, Y. Q.
AU - He, H. H.
AU - He, Z. T.
AU - Hibino, K.
AU - Hotta, N.
AU - Hu, Haibing
AU - Hu, H. B.
AU - Huang, J.
AU - Li, W. J.
AU - Jia, H. Y.
AU - Jiang, L.
AU - Kajino, F.
AU - Kasahara, K.
AU - Katayose, Y.
AU - Kato, C.
AU - Kawata, K.
AU - Labaciren,
AU - Le, G. M.
AU - Li, A. F.
AU - Liu, C.
AU - Liu, J. S.
AU - Lu, H.
AU - Meng, X. R.
AU - Mizutani, K.
AU - Munakata, K.
AU - Nanjo, H.
AU - Nishizawa, M.
AU - Ohnishi, M.
AU - Ohta, I.
AU - Ozawa, Shunsuke
AU - Qian, X. L.
AU - Qu, X. B.
AU - Saito, T.
AU - Saito, T. Y.
AU - Sakata, M.
AU - Sako, T. K.
AU - Shao, J.
AU - Shibata, M.
AU - Shiomi, A.
AU - Shirai, T.
AU - Sugimoto, H.
AU - Takita, M.
AU - Tan, Y. H.
AU - Tateyama, N.
AU - Torii, Shoji
AU - Tsuchiya, H.
AU - Udo, S.
AU - Wang, H.
AU - Wu, H. R.
AU - Xue, L.
AU - Yamamoto, Y.
AU - Yang, Z.
AU - Yasue, S.
AU - Yuan, A. F.
AU - Yuda, T.
AU - Zhai, L. M.
AU - Zhang, H. M.
AU - Zhang, J. L.
AU - Zhang, X. Y.
AU - Zhang, Y.
AU - Zhang, Yi
AU - Zhang, Ying
AU - Zhaxisangzhu,
AU - Zhou, X. X.
PY - 2011
Y1 - 2011
N2 - We analyze the solar cycle variation of the Sun's shadow in 10 TeV cosmic ray intensity observed with the Tibet air shower array over an entire period of the Solar Cycle 23 between 1996 and 2008. The amplitude of the variation is as large as one half of the deficit intensity expected when all cosmic rays arriving from the direction of the optical Sun disk are excluded from the observation. The correlations between the deficit intensity in the Sun's shadow and cosmic-ray modulation parameters are overall significant. Among those parameters, we find the highest correlation with the Heliospheric Current Sheet tilt-angle.
AB - We analyze the solar cycle variation of the Sun's shadow in 10 TeV cosmic ray intensity observed with the Tibet air shower array over an entire period of the Solar Cycle 23 between 1996 and 2008. The amplitude of the variation is as large as one half of the deficit intensity expected when all cosmic rays arriving from the direction of the optical Sun disk are excluded from the observation. The correlations between the deficit intensity in the Sun's shadow and cosmic-ray modulation parameters are overall significant. Among those parameters, we find the highest correlation with the Heliospheric Current Sheet tilt-angle.
KW - Cosmic rays
KW - Solar magnetic field
KW - Solar modulation
KW - Sun's shadow
KW - Tibet
UR - http://www.scopus.com/inward/record.url?scp=84899520148&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84899520148&partnerID=8YFLogxK
U2 - 10.7529/ICRC2011/V02/0352
DO - 10.7529/ICRC2011/V02/0352
M3 - Conference contribution
AN - SCOPUS:84899520148
VL - 11
SP - 239
EP - 242
BT - Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011
PB - Institute of High Energy Physics
ER -