The Chemical Composition and the Energy Spectrum of Heavy Nuclei in the Cosmic Radiation above 10 GeV/nucleon
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- Saito Takeshi
- Department of Physics, University of Tokyo
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A total of 7695 heavy nuclei were located in the Brawley emulsion stack. The error in energy estimation was about 30% and that in charge estimation was 0.25 units of charge for nuclei with z≤9 and 0.5 for the iron group. The flux values for respective charge groups at the top of the atmosphere at energies above 10 GeV/nucleon are JM0=0.686±0.117, JH0=0.241±0.032, JLH0=0.166±0.022, JMH0=0.015±0.004 and JVH0=0.060±0.012, particles/m2·sec·sterad. The integral energy spectra of the individual charge groups have the same exponent of γ=1.60 up to several hundreds of GeV/nucleon. On the basis of the experimental results in the present investigation, the mechanisms of cosmic ray acceleration and the amount of matter traversed by the cosmic rays are discussed.
収録刊行物
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- Journal of the Physical Society of Japan
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Journal of the Physical Society of Japan 30 (6), 1535-1545, 1971
一般社団法人 日本物理学会
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詳細情報 詳細情報について
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- CRID
- 1390282679172068224
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- NII論文ID
- 110001958272
- 130003893128
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- NII書誌ID
- AA00704814
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- BIBCODE
- 1971JPSJ...30.1535S
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- COI
- 1:CAS:528:DyaE3MXkt1yrs7s%3D
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- ISSN
- 13474073
- 00319015
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- NDL書誌ID
- 8502833
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- NDL
- Crossref
- CiNii Articles
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- 抄録ライセンスフラグ
- 使用不可