The pierre auger observatory scaler mode for the study of solar activity modulation of galactic cosmic rays

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 cosm...

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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17480221_v6_n1_p_Multitudinario
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spelling todo:paper_17480221_v6_n1_p_Multitudinario2023-10-03T16:32:11Z The pierre auger observatory scaler mode for the study of solar activity modulation of galactic cosmic rays Multitudinario:485 Cherenkov detectors Large detector systems for particle and astroparticle physics Particle detectors 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. © 2011 IOP Publishing Ltd and SISSA. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17480221_v6_n1_p_Multitudinario
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Cherenkov detectors
Large detector systems for particle and astroparticle physics
Particle detectors
spellingShingle Cherenkov detectors
Large detector systems for particle and astroparticle physics
Particle detectors
Multitudinario:485
The pierre auger observatory scaler mode for the study of solar activity modulation of galactic cosmic rays
topic_facet Cherenkov detectors
Large detector systems for particle and astroparticle physics
Particle detectors
description 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. © 2011 IOP Publishing Ltd and SISSA.
format JOUR
author Multitudinario:485
author_facet Multitudinario:485
author_sort Multitudinario:485
title The pierre auger observatory scaler mode for the study of solar activity modulation of galactic cosmic rays
title_short The pierre auger observatory scaler mode for the study of solar activity modulation of galactic cosmic rays
title_full The pierre auger observatory scaler mode for the study of solar activity modulation of galactic cosmic rays
title_fullStr The pierre auger observatory scaler mode for the study of solar activity modulation of galactic cosmic rays
title_full_unstemmed The pierre auger observatory scaler mode for the study of solar activity modulation of galactic cosmic rays
title_sort pierre auger observatory scaler mode for the study of solar activity modulation of galactic cosmic rays
url http://hdl.handle.net/20.500.12110/paper_17480221_v6_n1_p_Multitudinario
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AT multitudinario485 pierreaugerobservatoryscalermodeforthestudyofsolaractivitymodulationofgalacticcosmicrays
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