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dc.date.accessioned 2021-11-18T18:21:55Z
dc.date.available 2021-11-18T18:21:55Z
dc.date.issued 2009
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/128395
dc.description.abstract The mass composition of ultra-high energy cosmic rays is a critical issue to understand their origin and nature. The Pierre Auger Observatory is a hybrid instrument which provides a powerful environment for the determination of the primary mass. The Surface Detector of the Pierre Auger Observatory alone allows the study of several shower parameters with high discriminating power between primary elements. Novel analysis techniques using different features of signals in the Cherenkov stations are discussed. These are the signal risetime, the azimuthal time asymmetry and the muon density of the showers. en
dc.format.extent 195-198 es
dc.language en es
dc.subject Mass composition es
dc.subject Ultra-high energy cosmic rays es
dc.title Mass composition studies using the surface detector of the Pierre Auger Observatory en
dc.type Articulo es
sedici.identifier.other doi:10.1016/j.nuclphysbps.2009.09.036 es
sedici.identifier.issn 0920-5632 es
sedici.creator.person Wahlberg, Hernán Pablo es
sedici.creator.corporate Pierre Auger Collaboration es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Exactas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Nuclear Physics B - Proceedings Supplements es
sedici.relation.journalVolumeAndIssue vol. 196 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)