dc.creatorSato R.
dc.creatorEscobar C.O.
dc.date2005
dc.date2015-06-26T14:10:14Z
dc.date2015-11-26T14:10:13Z
dc.date2015-06-26T14:10:14Z
dc.date2015-11-26T14:10:13Z
dc.date.accessioned2018-03-28T21:10:53Z
dc.date.available2018-03-28T21:10:53Z
dc.identifier
dc.identifier29th International Cosmic Ray Conference, Icrc 2005. Tata Institute Of Fundamental Research, v. 8, n. , p. 13 - 16, 2005.
dc.identifier
dc.identifier
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-84899029380&partnerID=40&md5=0ff6ee145331312bf5158a6f8deaf55b
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/94000
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/94000
dc.identifier2-s2.0-84899029380
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1241456
dc.descriptionWe present an analysis of the effect that the corrector lenses (Schmidt Optics) have on the overall performance of the Auger Fluorescence Detector. The analysis uses real data from the telescopes. Figures of merit for the corrector lenses performance include shower trigger rate and the distribution of the distance of closest approach to the shower axis. As a result of this analysis we may say that the effective light collection area of a telescope nearly doubles with the use of a corrector lens at its aperture.
dc.description8
dc.description
dc.description13
dc.description16
dc.descriptionMatthiae, G., Optics and mechanics of the auger fluorescence detector (2001) Proceedings of the ICRC, , for the Auger Observatory Collaboration Hamburg
dc.descriptionDe Oliveira, M.A.L., Manufacturing the schmidt corrector lenses for the pierre auger observatory (2004) Nucl. Instr.and Meth. A, 522, pp. 360-370
dc.languageen
dc.publisherTata Institute of Fundamental Research
dc.relation29th International Cosmic Ray Conference, ICRC 2005
dc.rightsfechado
dc.sourceScopus
dc.titleThe Performance Of The Corrector Lenses For The Auger Fluorescence Detector
dc.typeActas de congresos


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