The Pierre Auger Observatory scaler mode for the study of solar activity modulation of galactic cosmic rays

0372029 - FZÚ 2013 RIV GB eng J - Článek v odborném periodiku
Abreu, P. - Aglietta, M. - Ahn, E.J. - Boháčová, Martina - Chudoba, Jiří - Ebr, Jan - Mandát, Dušan - Nečesal, Petr - Nožka, Libor - Nyklíček, Michal - Palatka, Miroslav - Pech, Miroslav - Prouza, Michael - Řídký, Jan - Schovancová, Jaroslava - Schovánek, Petr - Šmída, Radomír - Trávníček, Petr … celkem 485 autorů
The Pierre Auger Observatory scaler mode for the study of solar activity modulation of galactic cosmic rays.
Journal of Instrumentation. Roč. 6, č. 1 (2011), 1-15. ISSN 1748-0221. E-ISSN 1748-0221
Grant CEP: GA MŠMT LC527; GA MŠMT(CZ) 1M06002; GA AV ČR KJB100100904; GA MŠMT(CZ) LA08016
Výzkumný záměr: CEZ:AV0Z10100502; CEZ:AV0Z10100522
Klíčová slova: Cherenkov detectors * large detector systems for particle and astroparticle physics * particle detectors
Kód oboru RIV: BF - Elementární částice a fyzika vys. energií
Impakt faktor: 1.869, rok: 2011
http://iopscience.iop.org/1748-0221/6/01/P01003/pdf/1748-0221_6_01_P01003.pdf

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.
Trvalý link: http://hdl.handle.net/11104/0205424