A Very High Energy GLE Event Possibly Associated With the X Solar Flare of 15th June 1991

Peng Zhaoran; Li Jing; Ma Xinhua; Wang Wei; Zhu Qingqi; Shen Changquan; Jing Cailiu; Deng Yuju; Yuan Yukui; Huo Anxiang

Chinese Physics C> 1999, Vol. 23> Issue(11) : 1033-1038

A Very High Energy GLE Event Possibly Associated With the X Solar Flare of 15th June 1991

The Key Lab. of Cosmic Ray and High Energy Astrophisics, Institute of High Energy Physics, The Chinese Academy of Sciences, Beijing 100039

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Abstract：
Analysing the changes of cosmic ray counting rates obtained by the Hial-Rou EAS array in June of 1991, we find a very high energy GLE event after the X solar flare of 15 June 1991. The event started at 1100 UT of the day and lasted about 25 minutes. The counting rate in the 25 minutes for the event exceeds the monthly mean value with about 4σ.

References

[1]

Filippov A T et al. Proc. of 22nd ICRC, Dublin, 1991, 3: 1132 Huo Anxiang, Dai Yifang, Yuan Yukui. High Energy Physics and Nuclear Physics (in Chinese), 1990, 14(9):862–864(霍安祥、戴义方、袁余奎.高能物理与核物理,1990,14(9):862—864)3 Webber W K Rapporteur Paper on Outer Heliosphere Regions, Rapporteur Paper on 16th ICRC, Kyoto,1979, 14:2534 Srivastave N B. Basic Nuclear Physics Cosmic Rays, 1979 5 Zhang Li et al. Proc. of 23rd ICRC, Calgary, 1993, 3:33–376 Akimov V V et al. Proc. of 22rd ICRC, Calgary, 1993, 3:737 Kudela K et al. Proc. of 23rd ICRC, Calgary, 1993, 3:718 Solar–Terrestrial Environment Laboratory et al. Cosmic–Ray Intensity 37, Graphs of Hourly Neutron Intensities 1990–1991(1996) 9 Chinese Solar–Geophysical Data (in Chinese), 1991, 216(太阳地球物理资料,1991,216) 10 Karpov S N et al. Proc. of 25th ICRC, Durban, 1997, 1: 157

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Peng Zhaoran, Li Jing, Ma Xinhua, Wang Wei, Zhu Qingqi, Shen Changquan, Jing Cailiu, Deng Yuju, Yuan Yukui and Huo Anxiang. A Very High Energy GLE Event Possibly Associated With the X Solar Flare of 15th June 1991[J]. Chinese Physics C, 1999, 23(11): 1033-1038.

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Received: 1998-12-15
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

A Very High Energy GLE Event Possibly Associated With the X Solar Flare of 15th June 1991

Corresponding author: Peng Zhaoran,

The Key Lab. of Cosmic Ray and High Energy Astrophisics, Institute of High Energy Physics, The Chinese Academy of Sciences, Beijing 100039

Received Date: 1998-12-15
Accepted Date: 1900-01-01
Available Online: 1999-11-05

Abstract: Analysing the changes of cosmic ray counting rates obtained by the Hial-Rou EAS array in June of 1991, we find a very high energy GLE event after the X solar flare of 15 June 1991. The event started at 1100 UT of the day and lasted about 25 minutes. The counting rate in the 25 minutes for the event exceeds the monthly mean value with about 4σ.