The energy spectrum of the primary cosmic rays is obtained by conversion from the truncated muon size spectrum of EAS studied with the GAMMA array. The previously observed dependence of E0 on N tr ยต at various zenith angles is used. It is shown that the present spectrum has the same structure ("bump
Uncertanties of atmospheric high-energy muon fluxes and spectrum of primary cosmic rays
โ Scribed by A. A. Kochanov; T. S. Sinegovskaya; S. I. Sinegovskii
- Publisher
- Springer
- Year
- 2007
- Tongue
- English
- Weight
- 266 KB
- Volume
- 50
- Category
- Article
- ISSN
- 1573-9228
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