Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory
To interpret the mean depth of cosmic ray air shower maximum and its dispersion, we parametrize those two observables as functions of the first two moments of the ln A distribution. We examine the goodness of this simple method through simulations of test mass distributions. The application of the p...
Guardado en:
| Publicado: |
2013
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14757516_v2013_n2_p_Multitudinario http://hdl.handle.net/20.500.12110/paper_14757516_v2013_n2_p_Multitudinario |
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