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dc.date.accessioned 2019-10-31T13:59:37Z
dc.date.available 2019-10-31T13:59:37Z
dc.date.issued 2011
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/84497
dc.description.abstract Since data-taking began in January 2004, the Pierre Auger Observatory has been recording the count rates of low energy secondary cosmic ray particles for the self-calibration of the ground detectors of its surface detector array. After correcting for atmospheric effects, modulations of galactic cosmic rays due to solar activity and transient events are observed. Temporal variations related with the activity of the heliosphere can be determined with high accuracy due to the high total count rates. In this study, the available data are presented together with an analysis focused on the observation of Forbush decreases, where a strong correlation with neutron monitor data is found. en
dc.language en es
dc.subject Cherenkov detectors es
dc.subject Large detector systems for particle and astroparticle physics es
dc.subject Particle detectors es
dc.title The Pierre Auger Observatory scaler mode for the study of solar activity modulation of galactic cosmic rays en
dc.type Articulo es
sedici.identifier.other doi:10.1088/1748-0221/6/01/P01003 es
sedici.identifier.other eid:2-s2.0-79952673362 es
sedici.identifier.issn 1748-0221 es
sedici.creator.person Badagnani, Daniel Omar es
sedici.creator.person Dova, María Teresa es
sedici.creator.person Gómez Albarracín, Flavia Alejandra es
sedici.creator.person Hansen, Patricia María es
sedici.creator.person Mariazzi, Analisa Gabriela es
sedici.creator.person Moreno, Juan Cruz es
sedici.creator.person Sciutto, Sergio Juan es
sedici.creator.person Tarutina, Tatiana es
sedici.creator.person Tueros, Matías Jorge es
sedici.creator.person Wahlberg, Hernán Pablo es
sedici.creator.person The 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-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 Journal of Instrumentation es
sedici.relation.journalVolumeAndIssue vol. 6, no. 1 es
sedici.rights.sherpa * Color: verde* Pre-print del autor: si* Post-print del autor: si* Versión de editor/PDF:no* Condiciones:>>Pre-print on author's personal website, repository, non-commercial scientific social network, arXiv or non-commercial website>>Pre-print si not be updated after submission>>Post-print on author's personal website or Arxiv immediately>>Post-print on institutional website, institutional repository, subject-based repository, bioRxiv, PubMed Central, non-commercial scientific social network or third party eprint servers after 12 months embargo>>La versión de editor/PDF no puede utilizarse>>La fuente publicada debe reconocerse con la cita>>Debe enlazar a la versión de editor con DOI>>Set statements to accompany different versions (see policy)>>Post-print is not permitted on commercial scientific social networks e.g. ResearchGate, Mendely and Academia.edu>>Articles si not be deposited under an open access license or creative commons license>>Authors may make a closed deposit of post-print on a non-commercial repository within three months of date of acceptance.* Link a Sherpa: http://sherpa.ac.uk/romeo/issn/1748-0221/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)