| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1770831 | Astroparticle Physics | 2009 | 8 Pages |
Abstract
Azimuthal asymmetries in signals of non-vertical showers have been observed in ground arrays of water Cherenkov detectors, like Haverah Park and the Pierre Auger Observatory. The asymmetry in time distributions of arriving particles offers a new possibility for the determination of the mass composition. The dependence of this asymmetry on atmospheric depth shows a clear maximum at a position that is correlated with the primary species. In this work a novel method to determine mass composition based on these features of the ground signals is presented and a Monte Carlo study of its sensitivity is carried out.
Related Topics
Physical Sciences and Engineering
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Astronomy and Astrophysics
Authors
M.T. Dova, M.E. Manceñido, A.G. Mariazzi, H. Wahlberg, F. Arqueros, D. GarcÃa-Pinto,