“…There is a need for deposition flux observations to improve the wet scavenging routines of the models. A number of 7 Be deposition observations exist [e.g., Baskaran et al , 1993; Bleichrodt , 1978; Brown et al , 1988; Crecelius , 1981; Dibb , 1989; Graham et al , 2003; Hasebe et al , 1981; Huh et al , 2006; Ishikawa et al , 1995; Olsen et al , 1985; Papastefanou et al , 1995; Todd et al , 1989; Turekian et al , 1983; Uematsu et al , 1994; Young and Silker , 1980], but many of them cover only a period of less than 5 years, and they are not evenly distributed over the globe. The year‐to‐year variation of deposition is large due to production changes as well as changes in the local precipitation rate.…”