1.
Adjustment of Parameters of Primary Cosmic Ray Energy Spectrum with Recent Direct Measurments
利用宇宙线直接测量结果对初级宇宙线能谱参数的调整
2.
latitude effect of primary cosmic rays
初级宇宙线纬度效应
3.
charge composition of primary cosmic rays
初级宇宙线电荷成分
4.
cosmic-ray muon spectrometer
宇宙射线μ介子能谱仪
5.
THE ENERGY SPECTRA OF COSMIC RAY HADRONS AT MT.KAMBALA 5500m ABOVE SE LEVEL
高山5500米超高能宇宙线强子的能谱
6.
cosmic-ray high energy physics
宇宙射线高能物理学
7.
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
8.
Space exploration is still in its infancy.
宇宙探索仍处于初级阶段
9.
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
10.
Cosmic rays test and calibration in BESIII EMC
BESIII电磁量能器宇宙线测试与刻度
11.
SIMULATION CALCULATION FOR DETECTION EFFICIENCY IN THE MEASUREMENT OF COSMIC RAY HADRON SPECTRA
宇宙线强子谱测量中探测效率的模拟计算
12.
MEASUREMENT OF INTENSITY AND MOMENTUM SPECTRUM OF HORIZONTAL COSMIC RAY MUON AT 3220m ABOVE SEA LEVEL
海拔3220米水平宇宙线μ子强度和动量谱测量
13.
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
14.
The Method of Discriminating Primary Cosmic Ray at the "Knee" in ARGO Experiment;
ARGO实验中“膝”区原初宇宙线成分分辨方法研究
15.
Cosmic rays and X-rays produce energetic electrons by ionization.
宇宙射线和X射线因其电离作用产生高能电子。
16.
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。
17.
Hence the properties, such as energy and incident direction, of the incident cosmic ray can be calculated according to data from stations.
因此，透过比较不同观测站的数据，可以推算原初宇宙射线的能量、入射方向等资料。
18.
One Huge Diamond That Even Beckham Can't Buy
宇宙中的"超级大钻石"