Study of Variations of Muon Flux According to Muon Hodoscope Uragan Data at Different Phases of Solar Activity

Abstract

The paper presents the results of the analysis of data of the muon hodoscope URAGAN over the period from 2007 to 2017, which covers both the minimum and maximum of solar activity. The OMNI2 database was used for selection geomagnetic disturbance intervals. The correlation dependences between the parameters of perturbations of the heliosphere and the magnetosphere with the characteristics of the local anisotropy of the muon flux at different phases of solar activity are given.