The Pierre Auger Observatory surface detector array

James J. Beatty

doi:10.1117/12.458541

3 March 2003 The Pierre Auger Observatory surface detector array

James J. Beatty

Proceedings Volume 4858, Particle Astrophysics Instrumentation; (2003) https://doi.org/10.1117/12.458541
Event: Astronomical Telescopes and Instrumentation, 2002, Waikoloa, Hawai'i, United States

Abstract

The Auger Observatory southern site's surface detector will consist of 1600 water Cerenkov detectors spaced 1.5 km apart on a 3000 km² site in Mendoza, Argentina. A discussion of the design and results from deployment of an engineering array are presented.

Citation Download Citation

James J. Beatty "The Pierre Auger Observatory surface detector array", Proc. SPIE 4858, Particle Astrophysics Instrumentation, (3 March 2003); https://doi.org/10.1117/12.458541

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