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dc.date.accessioned 2019-11-22T13:00:48Z
dc.date.available 2019-11-22T13:00:48Z
dc.date.issued 2015
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/85936
dc.description.abstract To understand the origin and nature of Ultra High Energy Cosmic Rays their mass composition must be known. The Pierre Auger Observatory is an instrument which provides valuable information for the determination of the primary mass. Different parameters that describe various characteristics of the shower development and at the same time are sensitive to the primary mass are discussed. Their energy dependence and a comparison with predictions from different models are also presented. en
dc.format.extent 399-402 es
dc.language en es
dc.subject Composition es
dc.subject Pierre Auger Observatory es
dc.subject UHECR es
dc.title Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory en
dc.type Articulo es
sedici.identifier.other doi:10.1016/j.nuclphysbps.2015.10.136 es
sedici.identifier.other eid:2-s2.0-84983171185 es
sedici.identifier.issn 2405-6014 es
sedici.creator.person Jarne, Cecilia Gisele 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-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-nd/4.0/
sedici.relation.event X Latin American Symposium of High Energy Physics (Colombia, 24 al 28 de noviembre de 2014) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Nuclear and Particle Physics Proceedings es
sedici.relation.journalVolumeAndIssue vol. 267-269 es
sedici.rights.sherpa * Link a Sherpa: http://sherpa.ac.uk/romeo/issn/2405-6014/es/


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