超高能宇宙线

  • 网络super-high energy cosmic ray
超高能宇宙线超高能宇宙线
  1. 超高能宇宙线电子在星际介质中的传播

    The propagation of EXTRA-RELATIVISTIC cosmic ray electron in the interstellar medium

  2. 超高能宇宙线的研究

    The study of super high energy component of cosmic rays

  3. 超高能宇宙线与核的相互作用。

    Properties of super high energy cosmic rays-nucleus interactions .

  4. 文章还评述了超高能宇宙线的几点倾向性结论。

    Some trends in very high energy studies are also reviewed in this paper .

  5. 强子-强子核相互作用参数化模型在超高能宇宙线研究中的应用

    Application of Hadron-Hadron Nuclear Interaction Parametrization Model in the Study of Superhigh Energy Cosmic Rays

  6. 极端超高能宇宙线的天体起源含磁单极的活动星系核模型

    Where Do the Extra High Energy Cosmic Rays Come From A Model of Active Galactic Nuclei With Magnetic Monopoles

  7. 宇宙微波背景辐射对超高能宇宙线流强的影响

    Cosmic-ray high energy physics Effect of the cosmic microwave background Radiation to the flux of the Superhigh Energetic Cosmic Ray

  8. 大天顶角超高能宇宙线μ子能谱甚高能宇宙线与太阳活动

    ENERGY SPECTRUM OF SUPER HIGH ENERGY COSMIC RAY MUON SHOWERS OF LARGE ZENITH ANGLES Very High Energy Cosmic Rays and Solar Activity

  9. 分析了超高能宇宙线的核子-空气核和核-空气核作用的非弹性度,并讨论了核碰撞几何对它的影响。

    The inelasticity of p-air and A-air interactions of superhigh energy cosmic rays is analysed and the influence of the nuclear collision geometry is investigated .

  10. 入射光复用滤波和光辐射强度估计的改进宇宙微波背景辐射对超高能宇宙线流强的影响

    Incident Radiance Reuse Filter and Improvement of Radiance Estimation ; Effect of the cosmic microwave background Radiation to the flux of the Superhigh Energetic Cosmic Ray

  11. 本文根据原子核物理学,粒子物理学和大爆炸宇宙论研究超高能宇宙线质子在宇宙空间中的平均自由程和宇宙线从产生处到达地球经历的平均温度。

    This paper researches the mean free path of the superhigh energetic cosmic ray proton in cosmic space and the mean temperature of the cosmic ray from the produced place to our Earth on the basis of Nuclear physics , Particle physics and Big-bang cosmology .

  12. 超高能原初宇宙线成分分辨

    Identification of primary cosmic - ray component at the ultrahigh energy region

  13. 在对超高能区宇宙线产生的广延大气簇射的模拟计算中注意到,质子&空气核碰撞中的受伤核子数分布和非弹性截面对于簇射的纵向发展有着重要的影响。

    The inelastic cross-section and the distribution of the number of wounded nucleons in proton-Air collision have significant influence on the development of EAS caused by superhigh energy cosmic rays .