An observation of solar flare neutrons using yangbajing solar cosmic ray detector

张吉龙,丁林恺,霍安祥,卢红,陆穗苓,罗光宣,彭朝然, 任敬儒,施志政,谭有恒, 王辉,许贤武,张春生,张慧敏,Jl Zhang,Kz Bao,Lk Ding,CaiDong,Danzengluobu,Bz Dai,Zy Feng,Y Fu,Hw Guo,M He,Q Huang,Ax Huo, Hy Jian,Jy Li,H Lu,Sl Lu,Gx Luo,Xr Meng,J Mu,Zr Peng, Ren,Zz Shi,Yh Tan,Cr Wang, H Wang,Xw Xu,Gc Yu,Af Yuan,Cs Zhang,Hm Zhang,Nj Zhang,Xy Zhang, Zhaxisangzhu, Zhaxiciren

Kao Neng Wu Li Yu Ho Wu Li/High Energy Physics and Nuclear Physics（2000）

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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 neutrons during the 23rd solar cycle. An unusual large enhancement of the NT and NM count rates over background was observed from 05:38 UT to 05:40 UT at Yangbajing on 1998 November 28.

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关键词

Cosmic ray,Neutron monitor,Neutron telescope,Solar flare,Solar neutron

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