Abstract
The solar activity is gradually changing from the Solar Cycle 23 to 24. Sun's shadow generated by multi-TeV cosmic-ray particles has been continuously observed with the Tibet-II and Tibet- III air shower array in 1996 through 2008. We have shown that the Sun's shadow is strongly affected by the solar and interplanetary magnetic fields changing with the solar activity in the previous papers. In this paper, we present yearly variation of the Sun's shadow in the changing phase to the Solar Cycle 24. Additionally, we discuss comparison between our observation and simulation of the Sun's shadow.
Original language | English |
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Title of host publication | 31st International Cosmic Ray Conference, ICRC 2009 |
Publisher | University of Lodz |
Publication status | Published - 2009 |
Event | 31st International Cosmic Ray Conference, ICRC 2009 - Lodz Duration: 2009 Jul 7 → 2009 Jul 15 |
Other
Other | 31st International Cosmic Ray Conference, ICRC 2009 |
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City | Lodz |
Period | 09/7/7 → 09/7/15 |
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Keywords
- Solar cycle 24
- Sun's shadow
- Tibet air sower array
ASJC Scopus subject areas
- Nuclear and High Energy Physics
Cite this
Sun's shadow in changing phase from the solar cycle 23 to 24 observed with the Tibet Air sower array. / Amenomori, M.; Bi, X. J.; Chen, D.; Cui, S. W.; Danzengluobu; Ding, L. K.; Ding, X. H.; Fan, C.; Feng, C. F.; Feng, Zhaoyang; Feng, Z. Y.; Gao, X. Y.; Geng, Q. X.; Gou, Q. B.; Guo, H. W.; He, H. H.; He, M.; Hibino, K.; Hotta, N.; Hu, Haibing; Hu, H. B.; Huang, J.; Huang, Q.; Jia, H. Y.; Jiang, L.; Kajino, F.; Kasahara, K.; Katayose, Y.; Kato, C.; Kawata, K.; Labaciren; Le, G. M.; Li, A. F.; Li, H. C.; Li, J. Y.; Liu, C.; Lou, Y. Q.; Lu, H.; Meng, X. R.; Mizutani, K.; Mu, J.; Munakata, K.; Nagai, A.; Nanjo, H.; Nishizawa, M.; Ohnishi, M.; Ohta, I.; Ozawa, Shunsuke; Saito, T.; Saito, T. Y.; Sakata, M.; Sako, T. K.; Shibata, M.; Shiomi, A.; Shirai, T.; Sugimoto, H.; Takita, M.; Tan, Y. H.; Tateyama, N.; Torii, Shoji; Tsuchiya, H.; Udo, S.; Wang, B.; Wang, H.; Wang, Y.; Wang, Y. G.; Wu, H. R.; Xue, L.; Yamamoto, Y.; Yan, C. T.; Yan, 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.; Zhang, Yi; Zhang, Ying; Zhaxisangzhu; Zhou, X. X.
31st International Cosmic Ray Conference, ICRC 2009. University of Lodz, 2009.Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
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TY - GEN
T1 - Sun's shadow in changing phase from the solar cycle 23 to 24 observed with the Tibet Air sower array
AU - Amenomori, M.
AU - Bi, X. J.
AU - Chen, D.
AU - Cui, S. W.
AU - Danzengluobu,
AU - Ding, L. K.
AU - Ding, X. H.
AU - Fan, C.
AU - Feng, C. F.
AU - Feng, Zhaoyang
AU - Feng, Z. Y.
AU - Gao, X. Y.
AU - Geng, Q. X.
AU - Gou, Q. B.
AU - Guo, H. W.
AU - He, H. H.
AU - He, M.
AU - Hibino, K.
AU - Hotta, N.
AU - Hu, Haibing
AU - Hu, H. B.
AU - Huang, J.
AU - Huang, Q.
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 - Li, H. C.
AU - Li, J. Y.
AU - Liu, C.
AU - Lou, Y. Q.
AU - Lu, H.
AU - Meng, X. R.
AU - Mizutani, K.
AU - Mu, J.
AU - Munakata, K.
AU - Nagai, A.
AU - Nanjo, H.
AU - Nishizawa, M.
AU - Ohnishi, M.
AU - Ohta, I.
AU - Ozawa, Shunsuke
AU - Saito, T.
AU - Saito, T. Y.
AU - Sakata, M.
AU - Sako, T. K.
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, B.
AU - Wang, H.
AU - Wang, Y.
AU - Wang, Y. G.
AU - Wu, H. R.
AU - Xue, L.
AU - Yamamoto, Y.
AU - Yan, C. T.
AU - Yan, X. C.
AU - Yasue, S.
AU - Ye, Z. H.
AU - Yu, G. C.
AU - Yuan, A. F.
AU - Yuda, T.
AU - Zhang, H. M.
AU - Zhang, J. L.
AU - Zhang, N. J.
AU - Zhang, X. Y.
AU - Zhang, Y.
AU - Zhang, Yi
AU - Zhang, Ying
AU - Zhaxisangzhu,
AU - Zhou, X. X.
PY - 2009
Y1 - 2009
N2 - The solar activity is gradually changing from the Solar Cycle 23 to 24. Sun's shadow generated by multi-TeV cosmic-ray particles has been continuously observed with the Tibet-II and Tibet- III air shower array in 1996 through 2008. We have shown that the Sun's shadow is strongly affected by the solar and interplanetary magnetic fields changing with the solar activity in the previous papers. In this paper, we present yearly variation of the Sun's shadow in the changing phase to the Solar Cycle 24. Additionally, we discuss comparison between our observation and simulation of the Sun's shadow.
AB - The solar activity is gradually changing from the Solar Cycle 23 to 24. Sun's shadow generated by multi-TeV cosmic-ray particles has been continuously observed with the Tibet-II and Tibet- III air shower array in 1996 through 2008. We have shown that the Sun's shadow is strongly affected by the solar and interplanetary magnetic fields changing with the solar activity in the previous papers. In this paper, we present yearly variation of the Sun's shadow in the changing phase to the Solar Cycle 24. Additionally, we discuss comparison between our observation and simulation of the Sun's shadow.
KW - Solar cycle 24
KW - Sun's shadow
KW - Tibet air sower array
UR - http://www.scopus.com/inward/record.url?scp=84899055640&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84899055640&partnerID=8YFLogxK
M3 - Conference contribution
AN - SCOPUS:84899055640
BT - 31st International Cosmic Ray Conference, ICRC 2009
PB - University of Lodz
ER -