Very heavy' (iron-like) and 'light' (proton-like) cosmic ray primaries are identified at primary energies Ee x 1015 eV by means of simultaneous measurements of shower size Ne, N,, GeV (= N,,(E, > 1 GeV)) at the surface, and N Tev (= N,(E, > 1.3 TeV)) and AE,,/AL (i.e. muon energy losses per unit of
✦ LIBER ✦
EAS Cherenkov at Gran Sasso: correlated observations at the surface and with deep underground events
✍ Scribed by M. Aglietta; B. Alessandro; P. Antonioli; F. Arneodo; L. Bergamasco; A. Campos Fauth; C. Castagnoli; A. Castellina; C. Cattadori; A. Chiavassa; G. Cini; B. D’Ettorre Piazzoli; G. Di Sciascio; W. Fulgione; P. Galeotti; P. L. Ghia; M. Iacovacci; G. Mannocchi; C. Morello; G. Navarra; L. Riccati; O. Saavedra; G. C. Trinchero; P. Vallania; S. Vernetto; EAS-TOP Collaboration
- Book ID
- 112841674
- Publisher
- Springer-Verlag
- Year
- 1992
- Weight
- 349 KB
- Volume
- 105
- Category
- Article
- ISSN
- 0369-3546
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Identification of light and very heavy c
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G. Navarra
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1999
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English
⚖ 301 KB