Part III Composition of Primary Cosmic Rays
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概要
- 論文の詳細を見る
Experimental results on the composition of the primary cosmic rays are reviewed and their implications discussed. A special emphasis was placed on the isotopic abundances and the type of information obtainable therefrom was exploited in some detail.
- 理論物理学刊行会の論文
著者
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Ito Kensai
Department Of Physics Rikkyo University
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Koshiba Masatoshi
Department Of Physcis Tokyo University
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AIZU Hideko
Department of Physics, University of Tokyo
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Aizu Hideko
Department Of Physics University Of Tokyo
関連論文
- Atmospheric Neutrino Background and Pion Nuclear Effect for KAMIOKA Nucleon Decay Experiment
- Search for Nucleon Decays into Anti-Neutrino+Mesons
- Search for Nucleon Decays Catalyzed by Magnetic Monopoles
- Search for Nucleon Decay into Charged Lepton+Mesons
- Observations of Ultraheavy Cosmic Ray Particles with Z>45 at 10 GV Geomagnetic Cutoff Rigidity
- Inclusive Production of π^0 and η^0 in 12 GeV p-Be Collisions
- Observation of Parallel Muons 1350 hg/cm^2 Underground
- Isotopic Abundance of Carbon in Primary Cosmic Rays
- Analysis of Muon Bundles Underground
- Systematic Investigation of Ultra High Energy Interactions. II
- Positive Temperature Effect of Cosmic Rays
- Nuclear Interaction of μ-Meson
- Search for Slow Monopoles and Quarks
- Very High Energy Nuclear Reactions and Alpha-Particle Model
- Part III Composition of Primary Cosmic Rays
- On Fissionability of Heavy Nuclei
- A Consistent Interpretation of Ultra High Energy Phenomena
- Stellar Synthesis of the Proton-Rich Heavy Elements