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The detector DANSS is located under n industrial nuclear reactor atKalininskaya Nuclear Power Plant. This location provides ~ 50 m.w.e. reductionof the cosmic muon flux in the vertical direction, which places the experimentin an intermediate position between ground and underground experiments in termsof shielding from the cosmic rays. The detector DANSS is located under anindustrial nuclear reactor at Kalininskaya Nuclear Power Plant. This locationprovides ~50 m.w.e. reduction of the cosmic muon flux in the verticaldirection, which places the experiment in an intermediate position betweenground and underground experiments in terms of shielding from the cosmic rays.The detector's sensitive area consists of 2500 plastic scintillator counters,each 100x4x1 cm$^3$ in size, making in total a 1 m$^3$ volume, which issurrounded by a muon veto system and multiple layers of passive shielding. Themain goal of the DANSS experiment is to study the antineutrino spectra atdifferent distances from the source. For this purpose the detector is placed ona lifting platform, and the data is collected at three positions: 10.9 m, 11.9m and 12.9 m from the center of the reactor core. The detector is capable ofreconstructing muon tracks passing though the sensitive volume. In this workthe barometric, height and temperature correlation coefficients are calculatedin three areas of the zenith angle $\theta$ using the Duperier approach. Theseresults are based on the muon data collected during four years.

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Application of the Duperier method to the analysis of the cosmic muon  flux dependence on the meteorological parameters, based on the DANSS detector  data