论文部分内容阅读
The "knee" of the cosmic ray Spectrum ·Spectra contain very rich information (e.g.,Blackbody spectrum, beta decay electron spectrum).
On the PeV knee of cosmic ray spectrum and TeV cutoff of electron spectrum
【摘 要】
：
The "knee" of the cosmic ray Spectrum ·Spectra contain very rich information (e.g.,Blackbody spectrum, beta decay electron spectrum).
【机 构】
：
InstituteofHighEnergyPhysics
【出 处】
：
第8届高海拔宇宙线探测国际研讨会(The 8th International Workshop on Air Showe
【发表日期】
：
2017年12期
其他文献
介绍了CEI测量系统结构、分析了测量结果以及CEI技术在GEO卫星轨道监测中的应用。增加实时标校后，改善了观测的数据质量；尤其对于白天的数据；气温变化引起电缆温度变化对观测相
LHAASO could provide useful data on solar diurnal anisotropy～100 GeV LHAASO may reconstruct shower events for cosmic rays down to about～100 GeV.
会议
Summary ·Background and Motivation ·3-D Forbush Decrease Numerical Model · Simulation Results ·Conclusion
会议
24 Medium Size Telescopes 12m diameter Mirror 200 GeV-10 TeV 70 Small Size Telescopes 4m diameter mirror 1 TeV-200 TeV 4 Large Size Telescopes 24m Diameter Mirr
会议
Spectrum of CRs ·Above ‘ankle’:extragalactic ·Below ‘knee’:galactic origin(Gal.E.den.＞ SMC E.den) Two great ideas in a single short paper
会议
Taken from Ana Franckowiaks talk Why multimessenger? How? Reveal the existence of hidden sources opaque to hadrons and photons Escaping gravitational wave and n
会议
Outline · Introduction · Science case for AugerPrime · AugerPrime design · Results from engineering array · Conclusions
会议
Outline:·Introduction ·Site properties ·Brief History ·Baikal-GVD ·Perspectives ·Conclusion
会议
Why study old SNRs?·Study of gamma ray emission from old SNRs Can help us understand SNRs contribution to the Galactic CRs.
会议
Outline Energy threshold Cosmic Ray Energy Spectrum Cosmic Ray Anisotropy The minimun detectable flux Sensitivity in 1 year.
会议