Abstract
The vertical underground muon intensity has been measured in the slant depth range 3200-7000 hg cm-2 (standard rock) with the completed lower part of the MACRO detector at the Gran Sasso laboratory, using a large sample of data. These observations are used to compute the surface muon flux and the primary ''all-nucleon'' spectrum. An analysis of systematic uncertainties introduced by the interaction models in the atmosphere and the underground propagation of muons is presented. A comparison of our results with published data is also presented.
Lingua originale | Inglese |
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pagine (da-a) | 3793-3802 |
Numero di pagine | 10 |
Rivista | Physical Review D |
Volume | 52 |
Numero di pubblicazione | 7 |
DOI | |
Stato di pubblicazione | Pubblicato - 1995 |