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By the end of 2014, a cosmic ray muon telescope was installed at ZhongshanStation in Antarctic and has been continuously collecting data since then. Itis the first surface muon telescope to be built in Antarctic. In June 2015,five CMEs were ejected towards the Earth initiating a big large Forbushdecrease (FD) event. We conduct a comprehensive study of the galactic cosmicray intensity fluctuations during the FD using the data from cosmic raydetectors of multiple stations (Zhongshan, McMurdo, South Polar and Nagoya) andhe solar wind measurements from ACE and WIND. A pre-increase before the shockarrival was observed. Distinct differences exist in the timelines of thegalactic cosmic ray recorded by the neutron monitors and the muon telescopes.FD onset for Zhongshan muon telescope is delayed (2.5h) with respect to SSConset. This FD had a profile of four-step decrease. The traditional one- ortwo-step classification of FDs was inadequate to explain this FD.

Study on 2015 June 22 Forbush decrease with the muon telescope in Antarctic