Behaviour of Cosmic Rays in the Atmosphere at Super High Energy Region : Particles and Fields

スポンサーリンク

概要

• 論文の詳細を見る

• Propagation of high energy cosmic rays in the atmosphere is calculated analytically relative to their longitudinal as well as lateral aspects, based on a model using the accelerator results on multiple meson production. Main concern is the energy spectrum I(>E), and the lateral energy spread, <E^2r^2>, of particles of various components in each resultant atmospheric cosmic-ray phenomenon, called "family" in emulsion chamber experiments. Discussions are made on how each constituent assumption in the model affect the above-mentioned quantities.

• 理論物理学刊行会の論文
• 1987-06-25

著者

• Ohsawa Akinori

  Institute For Cosmic Ray Research University Of Tokyo

• OHSAWA Akinori

  Institute for Cosmic Ray Research, University of Tokyo

• Yamashita Seibun

  Science and Engineering Research Laboratory Waseda University

関連論文

• Wavelet Spectra of JACEE Events : Nuclear Physics
• Nuclear Interactions in Super High Energy Region : Nuclear Physics
• Scaling Breaking-Down in Multiple Pion Production at High Energy
• Violation of the Feynman Scaling Law in the Forward Region : Particles and Fields
• Behaviour of Cosmic Rays in the Atmosphere at Super High Energy Region : Particles and Fields
• The Highest Energy Events Observed by Chacaltaya Emulsion Chambers

スポンサーリンク