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第三回 空気シャワー観測による宇宙線の起源探索勉強会

25 March 2019
宇宙線研
Asia/Tokyo timezone

Contribution List

11 out of 11 displayed
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  1. 25. SIBYLL 2.3c
    felix riehn (LIP Lisbon)
    25/03/2019, 10:00
  2. 34. Recent result of Telescope Array Experiment, and the current status of TA x 4
    Dr Yuichiro Tameda (Facility of Engineering, Kanagawa University)
    25/03/2019, 10:30
  3. 26. Report on the UHECR2018 hadronic interaction WG results
    Ryuji Takeishi (ICRR Univ. Tokyo)
    25/03/2019, 11:00
  4. 27. Results and prospects of LHCf/RHICf
    Hiroaki Menjo (Nagoya University (JP))
    25/03/2019, 11:30
  5. 28. Measure the light-component spectrum of primary cosmic rays at the ‘knee’ energies with the Tibet YAC-II experiment
    Yusaku Katayose (Yokohama National University (JP))
    25/03/2019, 13:00
  6. 29. Cosmic-ray Monte Carlo simulation studies in IACT experiments
    Michiko Ohishi
    25/03/2019, 13:30
  7. 31. Shower Structure Analysis using Telescope Array data SD
    Rosa Mayta Palacios (Osaka City University)
    25/03/2019, 14:00
  8. 30. Hadronic interaction and air shower development
    Nobuyki Sakurai
    25/03/2019, 14:40
  9. 32. Impact of diffractive collisions on air shower development
    Ken Ohashi (Nagoya University (JP))
    25/03/2019, 15:10
  10. 33. Discussion
    25/03/2019, 15:30
  11. 24. Interactions of ultra-high energy cosmic rays
    felix riehn (LIP Lisbon)
    25/03/2019, 16:30

    Ultra-high energy cosmic rays are the most energetic particles observed in nature. As such they provide a unique view to the universe at its most extreme. In this presentation I will focus on the interactions of UHECR in the atmosphere. I will summarize the current observations and discuss what these observations imply about the nature of particle interactions at the highest energies and what...

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