Signal Fluctuations in the Auger Surface Detector
arXiv:astro-ph/0309491
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.
Submitted to 28th International Cosmic Ray Conferences (ICRC 2003), Tsukuba, Japan, 31 Jul - 7 Aug 2003