Elsevier, Astroparticle Physics, (84), p. 29-35
DOI: 10.1016/j.astropartphys.2016.08.002
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The Gerda experiment at Lngs of INFN is equipped with an active muon veto. The main part of the system is a water Cherenkov veto with 66 PMTs in the water tank surrounding the Gerda cryostat. The muon flux recorded by this veto shows a seasonal modulation. Two causes have been identified: ( i ) sec- ondary muons from the Cngs neutrino beam (2.2%) and ( ii ) a temperature modulation of the atmosphere (1.4%). A mean cosmic muon rate of I 0 μ= (3 . 477 ±0 . 002 stat ±0 . 067 sys ) ×10 −4 /(s ·m 2 ) was found in good agreement with other experiments at Lngs . Combining the present result with those from previous ex- periments at Lngs the effective temperature coefficient αT, Lngs is determined to 0.93 ±0.03. A fit of the temperature coefficients measured at various underground sites yields a kaon to pion ratio r K / πof 0.10 ±0.03. ; JRC.G.2-Standards for Nuclear Safety, Security and Safeguard