Auger: What, Why and How?

Details Auger: What, Why and How? Auger: What, Why and How?

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..433..312p&link_type=abstract

Workshop on observing giant cosmic ray air showers from >1020 eV particles from space. AIP Conference Proceedings, Volume 433, p

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

Scientific paper

The Pierre Auger Observatories for the highest energy cosmic rays will be hybrid systems, employing water Čerenkov ground arrays over-looked by atmospheric fluorescence detectors. This will allow accurate reconstruction of primary cosmic ray energy and arrival direction in a cost effective manner, and without dependence on uncertain models. In this paper the design of the proposed instrument is reviewed, together with the simulations on which it is based, and the resulting performance predictions.

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