The forward particle production in the energy range of 1 PeV as seen with the Tibet hybrid Experiment

M. Amenomori, X. J. Bi, D. Chen, W. Y. Chen, S. W. Cui, Danzeng Luobu, L. K. Ding, X. H. Ding, C. F. Feng, Zhaoyang Feng, Z. Y. Feng, Q. B. Gou, H. W. Guo, Y. Q. Guo, H. H. He, Z. T. He, K. Hibino, N. Hotta, Haibing Hu, H. B. HuJ. Huang, W. J. Li, H. Y. Jia, L. Jiang, F. Kajino, K. Kasahara, Y. Katayose, C. Kato, K. Kawata, Laba Ciren, G. M. Le, A. F. Li, C. Liu, J. S. Liu, H. Lu, X. R. Meng, K. Mizutani, K. Munakata, H. Nanjo, M. Nishizawa, M. Ohnishi, I. Ohta, Shunsuke Ozawa, X. L. Qian, X. B. Qu, T. Saito, T. Y. Saito, M. Sakata, T. K. Sako, J. Shao, M. Shibata, A. Shiomi, T. Shirai, H. Sugimoto, M. Takita, Y. H. Tan, N. Tateyama, Shoji Torii, H. Tsuchiya, S. Udo, H. Wang, H. R. Wu, L. Xue, Y. Yamamoto, Z. Yang, S. Yasue, A. F. Yuan, T. Yuda, L. M. Zhai, H. M. Zhang, J. L. Zhang, X. Y. Zhang, Y. Zhang, Y. I. Zhang, Ying Zhang, Zhaxisa Ngzhu, X. X. Zhou

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

We are now operating the 500 m2 Yangbajing air-shower core (YAC-II) array near the center of the Tibet air-shower array ( Tibet-III ) to observe cosmic-ray chemical composition at the knee energy region since February 2011. The first step of YAC, called YAC-I, containing 16 detector units, was operated from May, 2009 to February, 2010. In this paper, we used the YAC-I and Tibet-III coincident data set obtained from May, 2009 through January, 2010 to present the electromagnetic spectrum of air shower cores at around 10 15 eV energy region. The effective live time is calculated as 100.5 days. We would like to report the comparison of our experimental data with MC model prediction in this paper.

Original languageEnglish
Title of host publicationProceedings of the 32nd International Cosmic Ray Conference, ICRC 2011
PublisherInstitute of High Energy Physics
Pages157-160
Number of pages4
Volume1
DOIs
Publication statusPublished - 2011
Event32nd International Cosmic Ray Conference, ICRC 2011 - Beijing
Duration: 2011 Aug 112011 Aug 18

Other

Other32nd International Cosmic Ray Conference, ICRC 2011
CityBeijing
Period11/8/1111/8/18

Fingerprint

Tibet
cosmic ray showers
particle production
electromagnetic spectra
energy
cosmic rays
chemical composition
detectors
predictions

Keywords

  • Air shower
  • Cosmic ray
  • Hadronic interaction

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

Amenomori, M., Bi, X. J., Chen, D., Chen, W. Y., Cui, S. W., Luobu, D., ... Zhou, X. X. (2011). The forward particle production in the energy range of 1 PeV as seen with the Tibet hybrid Experiment. In Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011 (Vol. 1, pp. 157-160). Institute of High Energy Physics. https://doi.org/10.7529/ICRC2011/V01/1251

The forward particle production in the energy range of 1 PeV as seen with the Tibet hybrid Experiment. / Amenomori, M.; Bi, X. J.; Chen, D.; Chen, W. Y.; Cui, S. W.; Luobu, Danzeng; 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.; Ciren, Laba; 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, Y. I.; Zhang, Ying; Ngzhu, Zhaxisa; Zhou, X. X.

Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011. Vol. 1 Institute of High Energy Physics, 2011. p. 157-160.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Amenomori, M, Bi, XJ, Chen, D, Chen, WY, Cui, SW, Luobu, D, Ding, LK, Ding, XH, Feng, CF, Feng, Z, Feng, ZY, Gou, QB, Guo, HW, Guo, YQ, He, HH, He, ZT, Hibino, K, Hotta, N, Hu, H, Hu, HB, Huang, J, Li, WJ, Jia, HY, Jiang, L, Kajino, F, Kasahara, K, Katayose, Y, Kato, C, Kawata, K, Ciren, L, Le, GM, Li, AF, Liu, C, Liu, JS, Lu, H, Meng, XR, Mizutani, K, Munakata, K, Nanjo, H, Nishizawa, M, Ohnishi, M, Ohta, I, 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, YI, Zhang, Y, Ngzhu, Z & Zhou, XX 2011, The forward particle production in the energy range of 1 PeV as seen with the Tibet hybrid Experiment. in Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011. vol. 1, Institute of High Energy Physics, pp. 157-160, 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, 11/8/11. https://doi.org/10.7529/ICRC2011/V01/1251
Amenomori M, Bi XJ, Chen D, Chen WY, Cui SW, Luobu D et al. The forward particle production in the energy range of 1 PeV as seen with the Tibet hybrid Experiment. In Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011. Vol. 1. Institute of High Energy Physics. 2011. p. 157-160 https://doi.org/10.7529/ICRC2011/V01/1251
Amenomori, M. ; Bi, X. J. ; Chen, D. ; Chen, W. Y. ; Cui, S. W. ; Luobu, Danzeng ; 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. ; Ciren, Laba ; 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, Y. I. ; Zhang, Ying ; Ngzhu, Zhaxisa ; Zhou, X. X. / The forward particle production in the energy range of 1 PeV as seen with the Tibet hybrid Experiment. Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011. Vol. 1 Institute of High Energy Physics, 2011. pp. 157-160
@inproceedings{8bbfc84765934b46be0833d98316fe1a,
title = "The forward particle production in the energy range of 1 PeV as seen with the Tibet hybrid Experiment",
abstract = "We are now operating the 500 m2 Yangbajing air-shower core (YAC-II) array near the center of the Tibet air-shower array ( Tibet-III ) to observe cosmic-ray chemical composition at the knee energy region since February 2011. The first step of YAC, called YAC-I, containing 16 detector units, was operated from May, 2009 to February, 2010. In this paper, we used the YAC-I and Tibet-III coincident data set obtained from May, 2009 through January, 2010 to present the electromagnetic spectrum of air shower cores at around 10 15 eV energy region. The effective live time is calculated as 100.5 days. We would like to report the comparison of our experimental data with MC model prediction in this paper.",
keywords = "Air shower, Cosmic ray, Hadronic interaction",
author = "M. Amenomori and Bi, {X. J.} and D. Chen and Chen, {W. Y.} and Cui, {S. W.} and Danzeng Luobu and Ding, {L. K.} and Ding, {X. H.} and Feng, {C. F.} and Zhaoyang Feng and Feng, {Z. Y.} and Gou, {Q. B.} and Guo, {H. W.} and Guo, {Y. Q.} and He, {H. H.} and He, {Z. T.} and K. Hibino and N. Hotta and Haibing Hu and Hu, {H. B.} and J. Huang and Li, {W. J.} and Jia, {H. Y.} and L. Jiang and F. Kajino and K. Kasahara and Y. Katayose and C. Kato and K. Kawata and Laba Ciren and Le, {G. M.} and Li, {A. F.} and C. Liu and Liu, {J. S.} and H. Lu and Meng, {X. R.} and K. Mizutani and K. Munakata and H. Nanjo and M. Nishizawa and M. Ohnishi and I. Ohta and Shunsuke Ozawa and Qian, {X. L.} and Qu, {X. B.} and T. Saito and Saito, {T. Y.} and M. Sakata and Sako, {T. K.} and J. Shao and M. Shibata and A. Shiomi and T. Shirai and H. Sugimoto and M. Takita and Tan, {Y. H.} and N. Tateyama and Shoji Torii and H. Tsuchiya and S. Udo and H. Wang and Wu, {H. R.} and L. Xue and Y. Yamamoto and Z. Yang and S. Yasue and Yuan, {A. F.} and T. Yuda and Zhai, {L. M.} and Zhang, {H. M.} and Zhang, {J. L.} and Zhang, {X. Y.} and Y. Zhang and Zhang, {Y. I.} and Ying Zhang and Zhaxisa Ngzhu and Zhou, {X. X.}",
year = "2011",
doi = "10.7529/ICRC2011/V01/1251",
language = "English",
volume = "1",
pages = "157--160",
booktitle = "Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011",
publisher = "Institute of High Energy Physics",

}

TY - GEN

T1 - The forward particle production in the energy range of 1 PeV as seen with the Tibet hybrid Experiment

AU - Amenomori, M.

AU - Bi, X. J.

AU - Chen, D.

AU - Chen, W. Y.

AU - Cui, S. W.

AU - Luobu, Danzeng

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 - Ciren, Laba

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, Y. I.

AU - Zhang, Ying

AU - Ngzhu, Zhaxisa

AU - Zhou, X. X.

PY - 2011

Y1 - 2011

N2 - We are now operating the 500 m2 Yangbajing air-shower core (YAC-II) array near the center of the Tibet air-shower array ( Tibet-III ) to observe cosmic-ray chemical composition at the knee energy region since February 2011. The first step of YAC, called YAC-I, containing 16 detector units, was operated from May, 2009 to February, 2010. In this paper, we used the YAC-I and Tibet-III coincident data set obtained from May, 2009 through January, 2010 to present the electromagnetic spectrum of air shower cores at around 10 15 eV energy region. The effective live time is calculated as 100.5 days. We would like to report the comparison of our experimental data with MC model prediction in this paper.

AB - We are now operating the 500 m2 Yangbajing air-shower core (YAC-II) array near the center of the Tibet air-shower array ( Tibet-III ) to observe cosmic-ray chemical composition at the knee energy region since February 2011. The first step of YAC, called YAC-I, containing 16 detector units, was operated from May, 2009 to February, 2010. In this paper, we used the YAC-I and Tibet-III coincident data set obtained from May, 2009 through January, 2010 to present the electromagnetic spectrum of air shower cores at around 10 15 eV energy region. The effective live time is calculated as 100.5 days. We would like to report the comparison of our experimental data with MC model prediction in this paper.

KW - Air shower

KW - Cosmic ray

KW - Hadronic interaction

UR - http://www.scopus.com/inward/record.url?scp=84899519670&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84899519670&partnerID=8YFLogxK

U2 - 10.7529/ICRC2011/V01/1251

DO - 10.7529/ICRC2011/V01/1251

M3 - Conference contribution

AN - SCOPUS:84899519670

VL - 1

SP - 157

EP - 160

BT - Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011

PB - Institute of High Energy Physics

ER -