“…The fluxes obtained in the two cruises were comparable to open regions of many other marine systems, such as the Pacific Ocean ($3 ng m À2 h À1 , Kim and Fitzgerald, 1986;Mason and Fitzgerald, 1993), the Mediterranean Sea (1.52-4.92 ng m À2 h À1 , Andersson et al, 2007;4.2-7.9 ng m À2 h À1 , Gårdfeldt et al, 2003; 2.2 ± 1.5 ng m À2 h À1 , Fantozzi et al, 2013), the Arctic Ocean (2.4 ng m À2 h À1 , Andersson et al, 2008b), the North Sea ($2-6 ng m À2 h À1 , Baeyens and Leermakers, 1998) and the SCS (4.5-3.4 ng m À2 h À1 , Fu et al, 2010), but significantly lower than those Hg-polluted region, such as the Adriatic Sea (10.0-165.5 ng m À2 h À1 , Andersson et al, 2007), the Augusta Basin (72 ng m À2 h À1 , Bagnato et al, 2013). The fluxes were also comparable to the corresponding seasons in CST with similar S a and wind speed but significantly lower ($5-10 times) than the summer cruise (Table 1) because the high S a and great wind speed in the summer cruise substantially promoted the Hg(0) emission (Ci et al, 2011d).…”