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南极中山站宇宙线观测

黄德宏 胡红桥 刘杨 卢红 张大力 张吉龙

黄德宏, 胡红桥, 刘杨, 卢红, 张大力, 张吉龙. 南极中山站宇宙线观测[J]. 空间科学学报, 2016, 36(6): 897-903. doi: 10.11728/cjss2016.06.897
引用本文: 黄德宏, 胡红桥, 刘杨, 卢红, 张大力, 张吉龙. 南极中山站宇宙线观测[J]. 空间科学学报, 2016, 36(6): 897-903. doi: 10.11728/cjss2016.06.897
HUANG Dehong, HU Hongqiao, LIU Yang, LU Hong, ZHANG Dali, ZHANG Jilong. Cosmic Ray Observation at Antarctic Zhongshan Station[J]. Journal of Space Science, 2016, 36(6): 897-903. doi: 10.11728/cjss2016.06.897
Citation: HUANG Dehong, HU Hongqiao, LIU Yang, LU Hong, ZHANG Dali, ZHANG Jilong. Cosmic Ray Observation at Antarctic Zhongshan Station[J]. Journal of Space Science, 2016, 36(6): 897-903. doi: 10.11728/cjss2016.06.897

南极中山站宇宙线观测

doi: 10.11728/cjss2016.06.897
基金项目: 

国家自然科学基金项目(41431072,11575204)和极地专项项目(CHINARE2016-02-03)共同资助

详细信息
    通讯作者:

    黄德宏,E-mail:huangdehong@pric.org.cn

  • 中图分类号: P353.5

Cosmic Ray Observation at Antarctic Zhongshan Station

  • 摘要: 2014年由两个具有0.5m×0.5m闪烁体面积的探测器组成的宇宙线μ子望远镜在南极中山站建成,观测数据通过卫星链路传回并发布.通过对中山站μ子望远镜数据的气象效应分析,发现中山站的气压变化对宇宙线计数率影响显著并呈负相关.计算得到宇宙线高能质子在中山站的垂直截止刚度RC为0.076GV,对比中国西藏羊八井和北京高能质子的垂直截止刚度,中山站非常有利于对太阳高能质子事件的观测.

     

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出版历程
  • 收稿日期:  2015-07-09
  • 修回日期:  2016-03-21
  • 刊出日期:  2016-11-15

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