Signal Fluctuations in the Auger Surface Detector
Astrophysics
2019-08-14 v1
Abstract
We measured the Cerenkov signal fluctuations in the water tanks of the Pierre Auger Observatory. Two stations located near the center of the 32-tank Engineering Array separated by 11 m were used for the purpose. At this separation the stations sample nearly the same region of the air shower. Sources of the signal fluctuations are discussed.
Cite
@article{arxiv.astro-ph/0309491,
title = {Signal Fluctuations in the Auger Surface Detector},
author = {T. Yamamoto},
journal= {arXiv preprint arXiv:astro-ph/0309491},
year = {2019}
}
Comments
Submitted to 28th International Cosmic Ray Conferences (ICRC 2003), Tsukuba, Japan, 31 Jul - 7 Aug 2003