Document Type
Article
Publication Date
10-21-2015
Department
Department of Physics
Abstract
The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world's largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2, 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory.
Publication Title
Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Recommended Citation
Aab, A.,
Abreu, P.,
Aglietta, M.,
Ahn, E.,
Al Samarai, I.,
Albert, J.,
Dhital, N.,
Diaz, J. C.,
Fick, B.,
Kieckhafer, R. M.,
Nitz, D.,
&
Yapici, T.
(2015).
The Pierre Auger Cosmic Ray Observatory.
Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment,
798, 172-213.
http://doi.org/10.1016/j.nima.2015.06.058
Retrieved from: https://digitalcommons.mtu.edu/michigantech-p/6948
Creative Commons License
This work is licensed under a Creative Commons Attribution-NonCommercial-No Derivative Works 4.0 International License.
Version
Publisher's PDF
Publisher's Statement
© 2015 The Author. Published by Elsevier B.V. Publisher’s version of record: https://doi.org/10.1016/j.nima.2015.06.058