The rapid atmospheric monitoring system of the Pierre Auger Observatory

0388012 - FZÚ 2013 RIV GB eng J - Článek v odborném periodiku
Abreu, P. - Aglietta, M. - Ahlers, M. - Boháčová, Martina - Chudoba, Jiří - Ebr, Jan - Mandát, Dušan - Nečesal, Petr - Nožka, Libor - Palatka, Miroslav - Pech, Miroslav - Prouza, Michael - Řídký, Jan - Schovancová, Jaroslava - Schovánek, Petr - Šmída, Radomír - Trávníček, Petr - Vícha, Jakub … celkem 510 autorů
The rapid atmospheric monitoring system of the Pierre Auger Observatory.
Journal of Instrumentation. Roč. 7, č. 9 (2012), s. 1-40. ISSN 1748-0221. E-ISSN 1748-0221
Grant CEP: GA TA ČR TA01010517; GA MŠMT(CZ) MEB111003; GA AV ČR KJB100100904; GA MŠMT LA08015; GA MŠMT(CZ) LA08016
Výzkumný záměr: CEZ:AV0Z10100502; CEZ:AV0Z10100522
Klíčová slova: large detector systems for particle and astroparticle physics * real-time monitoring * control and monitor systems online
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 1.656, rok: 2012

The Pierre Auger Observatory is a facility built to detect air showers produced by cosmic rays above 10(17) eV. During clear nights with a low illuminated moon fraction, the UV fluorescence light produced by air showers is recorded by optical telescopes at the Observatory. To correct the observations for variations in atmospheric conditions, atmospheric monitoring is performed at regular intervals ranging from several minutes (for cloud identification) to several hours (for aerosol conditions) to several days (for vertical profiles of temperature, pressure, and humidity). In 2009, the monitoring program was upgraded to allow for additional targeted measurements of atmospheric conditions shortly after the detection of air showers of special interest, e. g., showers produced by very high-energy cosmic rays or showers with atypical longitudinal profiles.
Trvalý link: http://hdl.handle.net/11104/0216848