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Astroparticle Physics 33 (2010) 221-247
Full Simulation of Space-Based Extensive Air Showers Detectors with ESAF
C. Berat1, S. Bottai, D. De Marco, S. Moreggia1, D. Naumov, M. Pallavicini, R. Pesce, A. Petrolini, A. Stutz1, E. Taddei, A. Thea

Future detection of Extensive Air Showers (EAS) produced by Ultra High Energy Cosmic Particles (UHECP) by means of space based fluorescence telescopes will open a new window on the universe and allow cosmic ray and neutrino astronomy at a level that is virtually impossible for ground based detectors. In this paper we summarize the results obtained in the context of the EUSO project by means of a detailed Monte Carlo simulation of all the physical processes involved in the fluorescence technique, from the Extensive Air Shower development to the instrument response. Particular emphasis is given to modeling the light propagation in the atmosphere and the effect of clouds. Main results on energy threshold and resolution, direction resolution and Xmax determination are reported. Results are based on EUSO telescope design, but are also extended to larger and more sensitive detectors.
1 :  LPSC - Laboratoire de Physique Subatomique et de Cosmologie
Physique/Astrophysique/Instrumentation et méthodes pour l'astrophysique

Planète et Univers/Astrophysique/Instrumentation et méthodes pour l'astrophysique

Physique/Astrophysique/Phénomènes cosmiques de haute energie

Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie
cosmic rays – space detectors – extensive air showers – atmosphere models
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