Analysis of Background Cosmic Ray Rate in the 2010-2012 Period from the LAGO-Chacaltaya Detectors

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dc.contributor.authorC. Sarmiento‐Cano
dc.contributor.authorLuis Arturo Nuñez-Castiñeyra
dc.contributor.authorH. Asorey
dc.contributor.authorLuis A. Núñez
dc.contributor.authorPedro Miranda
dc.contributor.authorC. J. Solano Salinas
dc.contributor.authorR. Ticona
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T15:24:45Z
dc.date.available2026-03-22T15:24:45Z
dc.date.issued2016
dc.descriptionCitaciones: 5
dc.description.abstractThe Latin American Giant Observatory (LAGO) is an extended Cosmic Rays observatory composed by a network of Cherenkov Detectors (WCDs) spread over Latin America. This work will report the analysis of three years of data from three LAGO WCD located in Cerro Chacaltaya, Bolivia, at 5200 m a.s.l. Background cosmic ray rate from these detectors is checked for DAQ issues and inconsistencies, and corrected for atmospheric effects. An analysis for short transients up to the minute timescale is performed, in search for coincidence with transients observed by satellites. Sidereal and solar long term epoch data analysis are also presented.
dc.identifier.doi10.22323/1.236.0414
dc.identifier.urihttps://doi.org/10.22323/1.236.0414
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/52217
dc.language.isoen
dc.relation.ispartofProceedings of The 34th International Cosmic Ray Conference — PoS(ICRC2015)
dc.sourceIndustrial University of Santander
dc.subjectCosmic ray
dc.subjectDetector
dc.subjectPeriod (music)
dc.subjectCOSMIC cancer database
dc.subjectPhysics
dc.subjectAstronomy
dc.titleAnalysis of Background Cosmic Ray Rate in the 2010-2012 Period from the LAGO-Chacaltaya Detectors
dc.typearticle

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