Simulations of the surface detector of the Pierre Auger Observatory-Calibration and Monitoring-

Details Simulations of the surface detector of the Pierre Auger Observatory-Calibration and Monitoring- Simulations of the surface detector of the Pierre Auger Observatory-Calibration and Monitoring-

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..490..388m&link_type=abstract

The eighth mexican school on particles and fields. AIP Conference Proceedings, Volume 490, pp. 388-392 (1999).

Other

Cherenkov Detectors, Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors

Scientific paper

Once completed, the Pierre Auger Observatory will be the cosmic ray detector with the largest aperture (2×7000 km2 sr). The design of this observatory and, in the future, the data analysis depend, at least partially, on simulations of the response of the detector to an extended air shower. In the following, we present briefly the Pierre Auger Observatory and discuss simulations of the surface detector. As a concrete example we discuss the simulation of calibration and monitoring methods.

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