An Observation of Solar Flare Neutrons Using Yangbajing Solar Cosmic Ray Detector

ZHANG JiLong; BAO KeZhi; DING LinKai; Cai Dong; DAI BenZhong; FENG ZhenYong; FU Yu; GUO HongWei; HE Mao; HUANG Qing; HUO AnXiang; JIA HuanYu

Chinese Physics C> 2000, Vol. 24> Issue(12) : 1081-1087

An Observation of Solar Flare Neutrons Using Yangbajing Solar Cosmic Ray Detector

The Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, CAS, Beijing 100039, China2 Department of Physics, Shangdong University,Ji'nan 250100, China3 Department of Physics, Yunnan University, Kunming 650091, China4 Department of physics, South West Jiaotong University, Chengdu 610031, China5 Department of Mathematics and Physics, Tibet University , Lhasa 850000, China6 Department of Physics, Zhengzhou University, Zhengzhou 650091, China

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Abstract：
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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ZHANG JiLong, BAO KeZhi, DING LinKai, Cai Dong, DAI BenZhong, FENG ZhenYong, FU Yu, GUO HongWei, HE Mao, HUANG Qing, HUO AnXiang, JIA HuanYu, An Observation of Solar Flare Neutrons Using Yangbajing Solar Cosmic Ray Detector[J]. Chinese Physics C, 2000, 24(12): 1081-1087.

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Received: 2000-01-19
Revised: 1900-01-01

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