Observation of the 2005 January 20 GLE Event Using Yangbajing Solar Neutron Telescope &amp; Neutron Monitor

ZHU Feng-Rong; WANG Rui-Guang; TANG Yun-Qiu; LU Hong; CHEN Song-Zhan; CHENG Ning; FENG Zhao-Yang; GUO Yi-Qing; SHI Feng; WANG Yun-Gang; WANG Yue; TAN You-Heng; ZHANG Hu

Chinese Physics C> 2007, Vol. 31> Issue(4) : 341-344

Observation of the 2005 January 20 GLE Event Using Yangbajing Solar Neutron Telescope & Neutron Monitor

Key Lab. of Particle Astrophysics, Institute of High Energy Physics, CAS, Beijing 100049, China2 National Center for Space Weather, National Satellite Meteorological Center, Beijing 100081, China

Abstract
HTML
Reference
Related

PDF

Abstract：
A solar cosmic rays Ground Level Enhancement(GLE) event associated with a X7.1/2b solar flare in 2005 January 20 was observed by the Yangbajing solar neutron telescope(SNT) and neutron monitor(NM), located at Yangbajing Tibet(90.53°E, 30.11°N, 4310m a.s.l) with the highest vertical geomagnetic cut-off rigidity of 14.1GV in NM network. The statistical significance of the counting rate enhancement recorded by solar neutron telescope in >40MeV channel was 3.7σ in the time window of 07:00—07:05UT and 6.0σ in the time window of 07:00—07:20UT, respectively. The onset time of 06:51—06:52UT for this GLE event was clearly observed by the Yangbajing NM. Our observation indicates that solar protons have been accelerated up to energies of >10GeV during this solar event.

References

[1]

. Forbush S E. Phys. Rev., 1946, 70: 7712. WANG R G, WANG J X. Adv. Space Res., 2006, 38: 4893. WANG R G, WANG J X. Proc. of IAU Symposium 2005,226: 3794. Storini M et al. Memorie della Societ Astronomica Italiana, 2001, 72(3): 6205. Chiba N et al. Astroparticle Physics, 1992, 1(1): 276. Karpov S N et al. 25th ICRC, 1997,1: 2057. Lovell J L et al. Journal of Geophysics Research, 1998,103(A10): 237338. Brueckner G E, Howard R A, Koomen et al. Sol. Phys.,1995, 162: 3579. Kuznetsov S N et al. 29th ICRC, 2005, 1: 4910. Kohno T et al. 26th ICRC, 1999, 6: 6211. Katayose Y et al. 26th ICRC, 1999,1.6: 5812. Tsuchiya H et al. Nucl. Instrum. Methods, 2001, A463:18313. ZHANG Ji-Long et al. HEP NP, 2000, 24(12): 1081(in Chinese)(张吉龙等.高能物理与核物理,2000, 24(12): 1081)14. Smart D F et al. 24th ICRC, 1995, 4: 17115. Valdc-Galicia J F et al. Solar Phys., 2000, 191(2): 40916. JIA H Y et al. 29th ICRC, 2005, 1: 13717. Flueckiger E O et al. 29th ICRC, 2005, 1: 22518. Tsuchiya H et al. 27th ICRC, 2001, 1.2: 305619. WANG R G, WANG J X. Astroparticle Physics, 2006, 25:4120. Achard P et al. L3 Collaboration Astronomy Astro-physics, 2006, 456: 35121. WANG R G, WANG J X. Proc. of IAU Symposium, 2005,226: 38122. WANG R G. Astroparticle Physics, 2006, 26: 202

[1]	WANG Rui-Guang . Proton spectrum of the 2005 January 20 solar flare. Chinese Physics C, 2008, 32(2): 104-107. doi: 10.1088/1674-1137/32/2/006
[2]	WANG Min-Jie , JIA Huan-Yu . Cosmic Ray Flux Variation due to Solar Flares during January 16—20, 2005 with YBJ-ARGO Experiment. Chinese Physics C, 2007, 31(1): 34-37.
[3]	LI Hua . Statistic Analysis of the Deposited Energy in Single Event Upset Induced by 10—20MeV Neutrons. Chinese Physics C, 2006, 30(12): 1238-1241.
[4]	ZHOU Yuan , HE Hui-Hai , MU Jun . Monte Carlo Study of Methods for Off-Line Calibration of ARGO-YBJ Experiment. Chinese Physics C, 2005, 29(8): 787-792.
[5]	LIU Kun , HE Hui-Hai , CHEN Xin , LU Hong , MU Jun , SHEN Pei-Ruo , TAN You-Heng , WU Chao-Yong , YANG Qun-Yu , ZHANG Hui-Min , ZHANG Yong . Study on the Performance of YBJ Preliminary Carpet. Chinese Physics C, 2004, 28(9): 914-917.
[6]	YANG Qun-Yu , HE Hui-Hai , CHEN Xin , LIU Kun , LU Hong , MU Jun , SHEN Pei-Ruo , TAN You-Heng , WU Chao-Yong , ZHANG Hui-Min , ZHANG Yong . Study on the Analog Read-Out of the YBJ-ARGO RPC. Chinese Physics C, 2004, 28(8): 866-869.
[7]	HE Hui-Hai , LIU Kun , LU Hong , SHEN Pei-Ruo , TAN You-Heng , WU Chao-Yong , YANG Qun-Yu , ZHANG Hui-Min , ZHANG Yong . Study on the Performance of the YBJ-ARGO RPC. Chinese Physics C, 2004, 28(4): 422-425.
[8]	HE Hui-Hai , ZHANG Yong . Data Acquisition System of the YBJ-ARGO Experiment. Chinese Physics C, 2003, 27(12): 1106-1108.
[9]	QU Ruo-Fei , HE Hui-Hai , ZHU Qing-Qi , CHA Min , LU Hong , JING Cai-Liu , WANG Huan-Yu . Monte Carlo Simulation of 50m² RPC Carpet at Yang Ba Jing. Chinese Physics C, 2001, 25(5): 371-376.
[10]	ZHANG JiLong , BAO KeZhi , DING LinKai , Cai Dong , DAI BenZhong , FENG ZhenYong , FU Yu , GUO HongWei , HE Mao , HUANG Qing , HUO AnXiang , JIA HuanYu , , , , , . An Observation of Solar Flare Neutrons Using Yangbajing Solar Cosmic Ray Detector. Chinese Physics C, 2000, 24(12): 1081-1087.
[11]	Peng Zhaoran , Li Jing , Ma Xinhua , Wang Wei , Zhu Qingqi , Shen Changquan , Jing Cailiu , Deng Yuju , Yuan Yukui , Huo Anxiang . A Very High Energy GLE Event Possibly Associated With the X Solar Flare of 15th June 1991. Chinese Physics C, 1999, 23(11): 1033-1038.
[12]	Jiang Yinlin , Chen Yongzhong , Xu Chunxian , He Huilin , He Huihai , Li Huidong , Huo Anxiang . Atmospheric Cherenkov Telescope. Chinese Physics C, 1997, 21(7): 583-590.
[13]	Qi Zhong , Guo Zhongyan , Zhan Wenlong , Zhou Jianqun , Liu Guanhua , Zhang Wansheng , Wang Jinchuan , Lin Yungen , Zhu Yongtai , Xu Hushan , Xie Yuanxiang . A NE102A+CsI(T1)+PMT Detector Telescope for Intermediate Energy Heavy Ion Reactions. Chinese Physics C, 1997, 21(6): 481-485.
[14]	Ye Banjiao , Fan Yangmei , Wang Zhongmin , Han Rongdian , Mei Wen , Yu Xiaoqi , Yang Yanming , Han Renyu , Du Huaijiang , Xiao Zhenxi . A Multitelescope System for the Measurement of Differential (n,Charged Particle)Reaction Cross-sections. Chinese Physics C, 1994, 18(S1): 13-19.
[15]	ZHOU Jian-Qun , ZHAN Wen-Long , XI Hong-Fei , ZHU Yong-Tai , GUO Zhong-Yan , HU Xiao-Qing , LIU Guan-Hua , ZHAO You-Xiong . A High Mass Resolution Telescope for Heavy-Ion Reaction Research at Intermediate Energies. Chinese Physics C, 1992, 16(10): 933-937.
[16]	NI Hui-Ling , ZHOU Hua-Shi , JIANG Chun-Hua , GUO Hong-Fei , XU Jian-Guo , ZHU Qi-Ming , WANG Fang , LIU Wei , LI Jia-Hua . THE LUMINOSITY MONITOR OF BES. Chinese Physics C, 1990, 14(6): 490-499.
[17]	XU Shu-Wei , LIU Man-Qing . ENERGY CALIBRATION FOR A PLASTIC SCINTILLATOR BETA-DETECTOR TELESCOPE. Chinese Physics C, 1990, 14(2): 181-183.
[18]	NI Hui-Ling , JIANG Chun-Hua , ZHOU Hua-Shi , GUO Hong-Fei , XU Jian-Guo , ZHU Qi-Ming , WANG Fang , LUI Wei , LI Jia-Hua . TEST AND CALIBRATION OF THE DETECTORS OF THE BES LUMINOSITY MONITOR. Chinese Physics C, 1989, 13(10): 870-878.
[19]	LI Song-Lin , HU Xiao-Qing , ZHU Yong-Tai , WANG Xiao-Ming , WANG Gao-Sheng , XIE Yuan-Xiang , SHEN Wen-Qing . A NEW TYPE OF IONIZATION CHAMBER TELESCOPE. Chinese Physics C, 1988, 12(4): 529-533.
[20]	LEI Chuan-Heng . A NEW KIND OF POCKET GAMMA-NEUTRON DOSERATE CHIRPER. Chinese Physics C, 1987, 11(5): 609-613.

Access

Get Citation

ZHU Feng-Rong, WANG Rui-Guang, TANG Yun-Qiu, LU Hong, CHEN Song-Zhan, CHENG Ning, FENG Zhao-Yang, GUO Yi-Qing, SHI Feng, WANG Yun-Gang, WANG Yue, TAN You-Heng, ZHANG Hu, Observation of the 2005 January 20 GLE Event Using Yangbajing Solar Neutron Telescope & Neutron Monitor[J]. Chinese Physics C, 2007, 31(4): 341-344.

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2006-07-24
Revised: 2006-11-15

Article Metric

Article Views(3335)
PDF Downloads(824)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

Observation of the 2005 January 20 GLE Event Using Yangbajing Solar Neutron Telescope & Neutron Monitor

Corresponding author: ZHU Feng-Rong,

Key Lab. of Particle Astrophysics, Institute of High Energy Physics, CAS, Beijing 100049, China2 National Center for Space Weather, National Satellite Meteorological Center, Beijing 100081, China

Received Date: 2006-07-24

Accepted Date: 2006-11-15

Available Online: 2007-04-05

Abstract: A solar cosmic rays Ground Level Enhancement(GLE) event associated with a X7.1/2b solar flare in 2005 January 20 was observed by the Yangbajing solar neutron telescope(SNT) and neutron monitor(NM), located at Yangbajing Tibet(90.53°E, 30.11°N, 4310m a.s.l) with the highest vertical geomagnetic cut-off rigidity of 14.1GV in NM network. The statistical significance of the counting rate enhancement recorded by solar neutron telescope in >40MeV channel was 3.7σ in the time window of 07:00—07:05UT and 6.0σ in the time window of 07:00—07:20UT, respectively. The onset time of 06:51—06:52UT for this GLE event was clearly observed by the Yangbajing NM. Our observation indicates that solar protons have been accelerated up to energies of >10GeV during this solar event.

HTML

Reference (1)

Observation of the 2005 January 20 GLE Event Using Yangbajing Solar Neutron Telescope & Neutron Monitor

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Observation of the 2005 January 20 GLE Event Using Yangbajing Solar Neutron Telescope & Neutron Monitor

Corresponding author: ZHU Feng-Rong,

HTML

目录