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Proceedings Paper

The Pierre Auger Observatory surface detector array
Author(s): James J. Beatty
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Paper 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.

Paper Details

Date Published: 3 March 2003
PDF: 6 pages
Proc. SPIE 4858, Particle Astrophysics Instrumentation, (3 March 2003); doi: 10.1117/12.458541
Show Author Affiliations
James J. Beatty, The Pennsylvania State Univ. (United States)


Published in SPIE Proceedings Vol. 4858:
Particle Astrophysics Instrumentation
Peter W. Gorham, Editor(s)

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