On the origin of the pion-decay radiation in the 1982 June 3 solar flare
On the origin of the pion-decay radiation in the 1982 June 3 solar flare
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关于 1982 年 6 月 3 日太阳耀斑中π介子衰变辐射的起源
DOI：
10.1086/184888
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发表时间：
1987
期刊：
影响因子：
--
通讯作者：
C. Dermer
中科院分区：
文献类型：
--
作者：
R. Ramaty;R. Murphy;C. Dermer
1982年6月3日的耀斑产生了大量观测到的伽马射线、高能粒子和中子辐射。结果表明，Murphy，Dermer和Ramty(1987)为6月3日耀斑建立的相互作用模型的预测结果与有关该耀斑的随时间变化的π衰变辐射通量的新数据相吻合。结论是，产生大部分介子的粒子可能与6月3日耀斑时在星际空间观察到的粒子具有相同的来源。参考文献23篇。
The June 3, 1982 flare produced a wealth of observed gamma-ray, energetic particle, and neutron emissions. It is shown that the predictions of an interaction model developed for the June 3 flare by Murphy, Dermer, and Ramaty (1987) compare favorably with new data on the time-dependent flux on pion-decay emission from this flare. It is concluded that the particles which produced the bulk of the pions could have the same origin as the particle observed in interplanetary space from the June 3 flare. 23 references.