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dc.date.accessioned 2019-07-15T18:42:36Z
dc.date.available 2019-07-15T18:42:36Z
dc.date.issued 2003-07
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/78179
dc.description.abstract One of the foremost issues in astrophysics today is that of the origin of the ultra high energy cosmic rays. The Pierre Auger Observatory (PAO), currently under construction in the Province of Mendoza, Argentina, is a broadly based international effort to make a high statistic study of the upper-end of the cosmic ray spectrum. The PAO is the first experiment designed to work in a hybrid detection mode. It consists of an array of 1600 particle detectors spread over 3000 km2 and four fluorescence telescopes placed on the boundaries of the surface array. The concept of the experiment as well as the current status and future prospects are presented. en
dc.format.extent 170-178 es
dc.language en es
dc.subject Pierre Auger Observatory en
dc.subject Física es
dc.subject astrophysics en
dc.subject cosmic rays spectrum en
dc.title The Pierre Auger Observatory en
dc.type Articulo es
sedici.identifier.other https://doi.org/10.1016/S0920-5632(03)80373-0
sedici.identifier.issn 0550-3213 es
sedici.creator.person Dova, María Teresa es
sedici.subject.materias Ciencias Exactas 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 es
sedici.relation.journalVolumeAndIssue vol. 122 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)