Development of Cosmic Rays Shower Based on Monte Carlo Simulation;
基于Monte Carlo模拟的宇宙线簇射发展研究
The Shape of Cerenkov Light Front Wave on the Ground About Cosmic Gamma Ray Air Shower
宇宙γ射线大气簇射切仑科夫光波阵面的形状
cosmic-ray neutron monitor
宇宙射线中子监测仪
cosmic-ray high energy physics
宇宙射线高能物理学
cosmic-ray intensity recorder
宇宙射线强度记录仪
cosmic radiation measuring or detecting instrument
宇宙射线测量或探测仪
cosmic-ray space physics
宇宙射线空间物理学
cosmic-ray muon spectrometer
宇宙射线μ介子能谱仪
fermi theory of cosmic ray acceleration
费米宇宙射线加速理论
The properties of the EAS are hidden as the peak is sharp around zero.
由于两组探测器相隔太近，空气簇射引发的峰值只出现于零附近，不利于分析宇宙射线的特性。
The number of cascade particles changes according to the incident cosmic ray energy, observation height, etc.
到达地面的簇射粒子数目会随不同因素而改变，包括原初宇宙射线的能量、观测高度等。
Effect of the cosmic microwave background Radiation to the flux of the Superhigh Energetic Cosmic Ray
宇宙微波背景辐射对超高能宇宙线流强的影响
A study of relation between Cherenkov light distribution and character of cosmic rays by Monte Carlo method
用蒙特卡洛方法研究大气簇射契仑柯夫光与初级宇宙线特性之间的关系
cosmic-ray transition radiation detector
宇宙射线跃迁辐射探测器
cosmic-ray charge composition detector
宇宙射线电荷组成探测器
cosmic-ray neutron and muon monitor
宇宙射线中子与μ介子监测仪
nuclides generated by cosmic ray irradiation
宇宙射线辐照生成的核素
VERY HIGH-ENERGY PARTICLE EMISSION FROM THE SOLAR COSMIC RAY FLARES
太阳宇宙线耀斑中的甚高能粒子发射