CORC  > 国家天文台  > 中国科学院国家天文台  > 应用天文研究部
Performance of new 8-inch photomultiplier tube used for the Tibet muon-detector array
Zhang, Y.1,2; Huang, J.1; Chen, D.3; Zhai, L. -M.3; Chen, X.1,2; Hu, X. -B.1,4; Lin, Y. -H.1,2; Jin, H. -B.3; Zhang, X. -Y.; Feng, C. -F.4
刊名JOURNAL OF INSTRUMENTATION
2016-06-01
卷号11
关键词Cherenkov detectors Photon detectors for UV, visible and IR photons (vacuum) (photomultipliers, HPDs, others)
英文摘要Since 2014, a new hybrid experiment consisting of a high-energy air-shower-core array (YAC-II), a high-density air-shower array (Tibet-III) and a large underground water-Cherenkov muon-detector array (MD) has been continued by the Tibet AS gamma collaboration to measure the chemical composition of cosmic rays in the wide energy range including the "knee". In this experiment, YAC-II is used to select high energy core events induced by cosmic rays in the above energy region, while MD is used to estimate the type of nucleus of primary particles by measuring the number of muons contained in the air showers. However, the dynamic range of each MD cell is only 5 to 2000 photoelectrons (PEs) which is mainly designed for observation of high-energy celestial gamma rays. In order to obtain the primary proton, helium and iron spectra and their "knee" positions with energy up to 1016 eV, each of PMTs equipped to the MD cell is required to measure the number of photons capable of covering a wide dynamic range of 100-106 PEs according to Monte Carlo simulations. In this paper, we firstly compare the characteristic features between R5912-PMT made by Japan Hamamatsu and CR365-PMT made by Beijing Hamamatsu. If there exists no serious difference, we will then add two 8-inch-in-diameter PMTs to meet our requirements in each MD cell, which are responsible for the range of 100-10000 PEs and 2000-1000000 PEs, respectively. That is, MD cell is expected to be able to measure the number of muons over 6 orders of magnitudes.
收录类别SCI
语种英语
WOS记录号WOS:000379239700028
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/5300]  
专题国家天文台_应用天文研究部
作者单位1.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
4.Shandong Univ, Dept Phys, Jinan 250100, Peoples R China
5.Southwest Jiaotong Univ, Inst Modern Phys, Chengdu 610031, Peoples R China
6.Tibet Univ, Dept Phys, Sch Sci, Lhasa 850000, Peoples R China
推荐引用方式
GB/T 7714
Zhang, Y.,Huang, J.,Chen, D.,et al. Performance of new 8-inch photomultiplier tube used for the Tibet muon-detector array[J]. JOURNAL OF INSTRUMENTATION,2016,11.
APA Zhang, Y..,Huang, J..,Chen, D..,Zhai, L. -M..,Chen, X..,...&Zhaxiciren.(2016).Performance of new 8-inch photomultiplier tube used for the Tibet muon-detector array.JOURNAL OF INSTRUMENTATION,11.
MLA Zhang, Y.,et al."Performance of new 8-inch photomultiplier tube used for the Tibet muon-detector array".JOURNAL OF INSTRUMENTATION 11(2016).
个性服务
查看访问统计
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。


©版权所有 ©2017 CSpace - Powered by CSpace