0387239 - 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 515 autorů
Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Obervatory.
Journal of Instrumentation. Roč. 7, Oct (2012), s. 1-42. ISSN 1748-0221. E-ISSN 1748-0221
Grant CEP: GA MŠMT LC527; GA MŠMT(CZ) 1M06002; GA MŠMT(CZ) MEB111003; GA AV ČR KJB100100904; GA MŠMT(CZ) LA08016
Výzkumný záměr: CEZ:AV0Z10100502; CEZ:AV0Z10100522
Klíčová slova: large detector systems for particle and astroparticle physics * antennas
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 1.656, rok: 2012 ; AIS: 0.805, rok: 2012
DOI: https://doi.org/10.1088/1748-0221/7/10/P10011

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineering Radio Array (AERA) addresses both technological and scientific aspects of the radio technique. A first phase of AERA has been operating since September 2010 with detector stations observing radio signals at frequencies between 30 and 80 MHz. In this paper we present comparative studies to identify and optimize the antenna design for the final configuration of AERA consisting of 160 individual radio detector stations. The transient nature of the air shower signal requires a detailed description of the antenna sensor.
Trvalý link: http://hdl.handle.net/11104/0216378