中文核心期刊
CNKI期刊全文数据库
中国科学引文数据库(CSCD)源期刊
中国科技论文统计源期刊
万方数据知识服务平台
英国《科学文摘》(SA)
美国化学文摘(CA)
俄罗斯《文摘杂志》(AJ)
德国《天文学与天体物理学文摘》(AAA)
英国《中国天文学和天体物理学》(SCI收录)全文摘译期刊之一
《中国学术期刊文摘》
《中国物理文摘》
《中国天文学文摘》

Chinese Journal of Space Science ›› 2016, Vol. 36 ›› Issue (6): 897-903.doi: 10.11728/cjss2016.06.897

Previous Articles     Next Articles

Cosmic Ray Observation at Antarctic Zhongshan Station

HUANG Dehong1, HU Hongqiao1, LIU Yang1,2, LU Hong3, ZHANG Dali3,4, ZHANG Jilong3   

  1. 1. SOA Key Laboratory for Polar Science, Polar Research Institute of China, Shanghai 200136;
    2. School of Electronic Information, Wuhan University, Wuhan 430072;
    3. Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Beijing 100049;
    4. Chinese Academy of Sciences University, Beijing 100049
  • Received:2015-07-09 Revised:2016-03-21 Online:2016-11-15 Published:2016-11-23

Abstract:

By the end of 2014, a cosmic ray muon telescope consisting of two detectors which has 0.5m×0.5m area scintillator was installed at Antarctic Zhongshan Station. The observation data is sent to China by satellite link and is released through network, which can be used to monitor and forecast space environment disasters, and provides support for China operational monitoring of space environment and multidisciplinary research of Polar Regions. The Zhongshan Station muon telescope data shows that there is a significant effect of pressure change with negative correlations. The vertical cutoff rigidity of cosmic ray protons at Zhongshan Station is 0.076GV, compared with those observations from Yangbajing and Beijing in China, Zhongshan Station is very conducive to the observation of the solar proton events.

Key words: Cosmic rays, Solar proton, cutoff rigidity, Zhongshan Station

CLC Number: