Long-term monitoring of changes in the concentration of radionuclides in the atmosphere can provide valuable information for studying atmospheric dynamics (Yamagata et al., 2019;Zhang et al., 2021). Radionuclides 7 Be (T 1/2 = 53.29 d) and 10 Be (T 1/2 = 1.36 Ma) (Nishiizumi et al., 2007) are produced by the collision of high-energy cosmic ray flux with nitrogen atoms and oxygen atoms in the atmosphere. After generation, 7 Be and 10 Be are adsorbed on submicron aerosols, and their lifetimes are determined by the residence time of the aerosols (Lal et al., 1958). Since the sources of 7 Be and 10 Be are controlled only by cosmic rays, and mainly produced at the lower of the stratosphere and the top of the troposphere (Brown et al., 1989), the variation of 7 Be concentration in the near-surface air is generally observed to trace atmospheric mass transport processes (Bhandari et al., 1966). However, in addition to stratosphere-troposphere exchange variability, local effects (such as local