Seasonal variation of the underground cosmic muon flux observed at Daya Bay

FP An, AB Balantekin, HR Band, M Bishai… - … of Cosmology and …, 2018 - iopscience.iop.org
FP An, AB Balantekin, HR Band, M Bishai, S Blyth, D Cao, GF Cao, J Cao, YL Chan
Journal of Cosmology and Astroparticle Physics, 2018iopscience.iop.org
Abstract The Daya Bay Experiment consists of eight identically designed detectors located in
three underground experimental halls named as EH1, EH2, EH3, with 250, 265 and 860
meters of water equivalent vertical overburden, respectively. Cosmic muon events have
been recorded over a two-year period. The underground muon rate is observed to be
positively correlated with the effective atmospheric temperature and to follow a seasonal
modulation pattern. The correlation coefficient α, describing how a variation in the muon rate …
Abstract
The Daya Bay Experiment consists of eight identically designed detectors located in three underground experimental halls named as EH1, EH2, EH3, with 250, 265 and 860 meters of water equivalent vertical overburden, respectively. Cosmic muon events have been recorded over a two-year period. The underground muon rate is observed to be positively correlated with the effective atmospheric temperature and to follow a seasonal modulation pattern. The correlation coefficient α, describing how a variation in the muon rate relates to a variation in the effective atmospheric temperature, is found to be α EH1= 0.362±0.031, α EH2= 0.433±0.038 and α EH3= 0.641±0.057 for each experimental hall.
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