“…We simply average over whatever period the observations cover and compare them with the modelled 5-yr mean fluxes. There are 7 Be observations from 37 stations (Baskaran et al, 1993;Bleichrodt, 1978;Brown et al, 1988;Crecelius, 1981;Hasebe et al, 1981;Heikkilä et al, 2008a;Hirose et al, 2004;Huh et al, 2006;Igarashi et al, 1998;Knies, 1994;McNeary and Baskaran, 2003;Olsen et al, 1985;Todd et al, 1989;Turekian et al, 1983;Uematsu et al, 1994;Young and Silker, 1980), 210 Pb from 71 stations (Baskaran et al, 1993;Graustein and Turekian, 1986;Huh et al, 2006;Hirose et al, 2004;McNeary and Baskaran, 2003;Nijampurkar and Clausen, 1990;Todd et al, 1989;Turekian et al, 1977Turekian et al, , 1983 and 10 Be from 21 stations (Chengde et al, 1992;Graham et al, 2003;Heikkilä et al, 2008a;Monaghan et al, 1986;Somayulu et al, 1984). The modelled 5-yr mean deposition fluxes of 7 Be, 10 Be and 210 Pb are shown in Figures 4, 5 and 6, together with the location and measured flux of the observations.…”