摘要
分析影响高山乳胶室γ族强度的种种因素,比较强度的实验数据和模拟计算值。结果表明超高能区(～10^(15)eV)初级宇宙线化学成分中质子占～30%的推断是可以接受的。
Through the analysis of the various factors which affect the intensity of γ-families ob- served by mountain emulsion chamber and the comparison of the experimetal data with the results from Monte-Carlo simulation,the inference that the proton fraction in primary chem- ical composition at UHE region,say 10^(15)eV,is about 30% is proved to be acceptable.
出处
《高能物理与核物理》
CSCD
北大核心
1990年第4期296-302,共7页
High Energy Physics and Nuclear Physics
基金
世界实验室资助
