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dc.contributorElsevieres_CL
dc.contributor.authorCordaro, EG [Universidad de Chile. Observatorios de Radiación Cósmica]es_CL
dc.contributor.authorOlivares, E. [Chile. Universidad Mayor. Escuela de Ingeniería Electrónica]es_CL
dc.contributor.authorGálvez, D. [Universidad de Chile. Observatorios de Radiación Cósmica]es_CL
dc.contributor.authorSalazar-Aravena, D. [Universidad de Santiago de Chile]es_CL
dc.contributor.authorLaroze, D. [Alemania. Max Planck Institute for Polymer Research]es_CL
dc.date.accessioned2018-08-23T00:21:05Z
dc.date.available2018-08-23T00:21:05Z
dc.date.issued2012es_CL
dc.identifier.citationCordaro, Enrique & Olivares,, E & Galvez,, D & Salazar-Aravena, Diego & Laroze, David. (2012). New 3He neutron monitor for Chilean Cosmic-Ray Observatories from the Altiplanic zone to the Antarctic zone. Advances in Space Research. 49. 1670-1683. 10.1016/j.asr.2012.03.015.es_CL
dc.identifier.issnISSN: 0273-1177es_CL
dc.identifier.issnESSN 1879-1948es_CL
dc.identifier.urihttp://repositorio.umayor.cl/xmlui/handle/sibum/2571
dc.identifier.urihttps://ac.els-cdn.com/S0273117712001810/1-s2.0-S0273117712001810-main.pdf?_tid=a413735a-b972-41f2-af18-3fc4bf9be398&acdnat=1534450583_bf2669dcc8d5d063efa52c5710bd8250es_CL
dc.identifier.urihttps://doi.org/10.1016/j.asr.2012.03.015es_CL
dc.description.abstractWe present the results of three years of continuous operations and the principal characteristics of our new 3He neutron monitors installed in the Chilean Network of Cosmic-Ray Observatories. During the years 2004 and 2005, we began the construction of this International Geophysical Year (IGY)-type 3He neutron monitor, with the intention of replacing the older proportional tubes of the BF3. These new monitors are installed in stations at locations ranging from the near-equatorial zone to the Antarctic zone. As a reference system, we used our own BF3 neutron monitors and previously complemented the collected data with a Monte Carlo simulation for the proton-yield function response of the Putre neutron monitor. Herein, we present for the first time the data obtained from our new high-mountain observatory located in the Altiplanic zone.es_CL
dc.description.sponsorshipEste trabajo fue financiado parcialmente por: Fondecyt 11080229 and Fondecyt 1120764, the Millennium Scientific Initiative, P10 061 F , the Basal Program Center for the Development of Nanoscience and Nanotechnology (CEDENNA) and Performance Agreement Project UTA/ Mineduc UTA-Project 8750-12. D.S.A acknowledges CONICYT PhD program fellowship.es_CL
dc.format.extentARTÍCULO ORIGINALes_CL
dc.language.isoenes_CL
dc.publisherFacultad de Cienciases_CL
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chilees_CL
dc.subjectCIENCIAS BÁSICASes_CL
dc.titleNew 3He neutron monitor for Chilean Cosmic-Ray Observatories from the Altiplanic zone to the Antarctic zonees_CL
dc.typeArtículo o Paperes_CL
umayor.indizadorCOTes_CL
umayor.politicas.sherpa/romeoLicencia color: VERDE C/RSe puede archivar el pre-print y el post-print o versión de editor/PDF, el autor no puede archivar la versión del editor/PDF) --Authors pre-print on any website, including arXiv and RePEC Author's post-print on author's personal website immediately Author's post-print on open access repository after an embargo period of between 12 months and 48 months Permitted deposit due to Funding Body, Institutional and Governmental policy or mandate, may be required to comply with embargo periods of 12 months to 48 months Author's post-print may be used to update arXiv and RepEC La versión de editor/PDF no puede utilizarse Debe enlazar a la versión de editor con DOI Author's post-print must be released with a Creative Commons Attribution Non-Commercial No Derivatives Licensees_CL
umayor.indexadoSCOPUSes_CL
dc.identifier.doi10.1016/j.asr.2012.03.015es_CL]


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