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

• Main Authors: Huang, De-Hong, Hu, Hong-Qiao, Zhang, Ji-Long, Lu, Hong, Zhang, Da-Li, Xue, Bin-Shen, Lu, Jing-Tian
• Format: Report
• Language: unknown
• Published: arXiv 2017
• Subjects: High Energy Astrophysical Phenomena astro-ph.HE; Space Physics physics.space-ph; FOS Physical sciences; Antarctic; Zhongshan; Zhongshan Station; Antarc*
• Online Access: https://dx.doi.org/10.48550/arxiv.1710.00945; https://arxiv.org/abs/1710.00945

By the end of 2014, a cosmic ray muon telescope was installed at Zhongshan Station in Antarctic and has been continuously collecting data since then. It is the first surface muon telescope to be built in Antarctic. In June 2015, five CMEs were ejected towards the Earth initiating a big large Forbush decrease (FD) event. We conduct a comprehensive study of the galactic cosmic ray intensity fluctuations during the FD using the data from cosmic ray detectors of multiple stations (Zhongshan, McMurdo, South Polar and Nagoya) and he solar wind measurements from ACE and WIND. A pre-increase before the shock arrival was observed. Distinct differences exist in the timelines of the galactic cosmic ray recorded by the neutron monitors and the muon telescopes. FD onset for Zhongshan muon telescope is delayed (2.5h) with respect to SSC onset. This FD had a profile of four-step decrease. The traditional one- or two-step classification of FDs was inadequate to explain this FD. : 10 pages,6 figures