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In Low Background Laboratory at Institute of Physics Belgrade, plasticscintillators are used to continuously monitor flux of the muon component ofsecondary cosmic rays. Measurements are performed on the surface as well asunderground (25 m.w.e depth). Temperature effect on muon component of secondarycosmic rays is well known and several methods to correct for it are alreadydeveloped and widely used. Here, we apply integral method to calculatecorrection coefficients and use GFS (Global Forecast System) model to obtainatmospheric temperature profiles. Atmospheric corrections reduce variance ofmuon flux and lead to improved sensitivity to transient cosmic ray variations.Influence of corrections on correlation with neutron monitor data is discussed.

Effect of pressure and temperature corrections on muon flux variability at ground level and underground