【作者】Zhang Ji Long*，Bao Ke Zhi，Ding Lin Kai，Cai Dong，Danzengluobu，Dai Ben Zhong，Feng Zhen Yong，Fu Yu，Guo Hong Wei，He Mao，Huang Qing，Huo An Xiang，Jia Huan Yu，Lu Hong，Lu Sui Ling，Luo Guang Xuan，Meng Xian Ru，Mu Jun，Peng Zhao Ran，Ren Jing Ru，Shi Zhi Zheng，Tan You Heng，Wang Cheng Rui，Wang Hui，Xu Xian Wu，Yu Guang Ce，Yuan Ai Fang，Zhang Chun Sheng，Zhang HuiMin，Zhang NaiJai，Zhang XueYao，Zhaxisangzhu，Zhaxiciren
【作者单位】[ 1 ] CAS, Inst High Energy Phys, Lab Cosm Ray & High Energy Astrophys, Beijing 100039, Peoples R China [ 2 ] Shandong Univ, Dept Phys, Jinan 250100, Peoples R China [ 3 ] Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China [ 4 ] SW Jiaotong Univ, Dept Phys, Chengdu 610031, Peoples R China [ 5 ] Tibet Univ, Dept Math & Phys, Lhasa 850000, Peoples R China [ 6 ] Zhengzhou Univ, Dept Phys, Kunming 650091, Peoples R China
【摘要】 The Geographical location of Yangbajing is suitable for the direct detection of the solar flare neutron events. The Yangbajing neutron telescope (NT) and Neutron Monitor (NM) were established in 1998 October to provide the observation of solar neutro...
