Multicore Shower of Large Zenith Angle

Ren Jingru; Lu Suiling; Xie Wei; He Mao; Zhang Naijian; Wang Shizhi; Bai Guangzhi

Chinese Physics C> 1997, Vol. 21> Issue(2) : 116-120

Multicore Shower of Large Zenith Angle

Institute of High Energy Physics,The Chinses Academy of Sciences,Beijing 1000392 Department of Physics,Shandong University,Jinan 2501003 Department of Physics,Zhengzhou University,Zhengzhou 4500524 Physics Group,Chongqing University of Architecture,Chongqing 630045

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Abstract：
The events of multicore shower with zenith angle tgθ>4 are found in the emulsion chamber at Mt.Kanbala.Possible mechanisms leading to these,which may predict a new phenomenon in cosmic ray experiments,are discussed.

References

[1]

J. R. Ren et al., IL Nuov Cim., 10C(1987)43.[2] K. Mizutani et al., IL Nuou Cim., 48A(1978)429.[3] N. Hotta et al., ICR Report 97一8l一13(1981).[4] I. Ohta et al., Proc. Int. Coanic Ray Symp. on High Energy TOKYO (1974)34.[5] 张乃健等, 高能物理与核物理, 13(1989)961.[6] X. Hayakawa, Cosmic Ray Physic (John Wiley Sons Inc.) p299.

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Ren Jingru, Lu Suiling, Xie Wei, He Mao, Zhang Naijian, Wang Shizhi and Bai Guangzhi. Multicore Shower of Large Zenith Angle[J]. Chinese Physics C, 1997, 21(2): 116-120.

Ren Jingru, Lu Suiling, Xie Wei, He Mao, Zhang Naijian, Wang Shizhi and Bai Guangzhi. Multicore Shower of Large Zenith Angle[J]. Chinese Physics C, 1997, 21(2): 116-120. shu

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Received: 1900-01-01
Revised: 1900-01-01

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沈阳化工大学材料科学与工程学院沈阳 110142

Multicore Shower of Large Zenith Angle

Corresponding author: Ren Jingru,

Institute of High Energy Physics,The Chinses Academy of Sciences,Beijing 1000392 Department of Physics,Shandong University,Jinan 2501003 Department of Physics,Zhengzhou University,Zhengzhou 4500524 Physics Group,Chongqing University of Architecture,Chongqing 630045

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1997-02-05

Abstract: The events of multicore shower with zenith angle tgθ>4 are found in the emulsion chamber at Mt.Kanbala.Possible mechanisms leading to these,which may predict a new phenomenon in cosmic ray experiments,are discussed.