Abstract
Gaseous elemental mercury (Hg0) is a prolific and persistent contaminant in the atmosphere. Atmospheric concentrations of Hg0 were determined from 17 September to 7 October 2015 in the northwest Sea of Japan aboard the Russian research vessel Professor Gagarinsky. Simultaneous measurements of Hg0 concentrations were performed 2m and 20m above the sea surface using automatic Hg0 analysers RA-915M and RA-915+, respectively. Concentrations ranged from 0.3 to 25.9ng/m3 (n=5207) and from 0.3 to 27.8ng/m3 (n=4415), with medians of 1.7 and 1.6ng/m3, respectively. Elevated Hg0 was observed during three episodes from 19 to 22 September, likely caused by one or more of the following factors: 1) atmospheric transport of Hg0 from the west and south-west (from N. Korea, China, and the Yellow Sea region); 2) Hg0 emission from the sea due to pollution by water from the Tumannaya River; or 3) underwater geological activities. Increased Hg0 concentration was observed during periods when air masses flowed from the south, and low concentrations were observed when air masses came from the north. A daytime increase of Hg0 concentrations at a height of 2m occurred simultaneously with decreasing Hg0 at a height of 20m. These diurnal variations suggest that two contrasting processes occur during the daytime in the marine boundary layer (MBL): Hg0 emission from the sea surface and Hg0 oxidation in the MBL by active halogens formed by photolysis.
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