Elemental Mercury Concentrations and Fluxes in the Tropical Atmosphere and Ocean

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Elemental Mercury Concentrations and Fluxes in the Tropical Atmosphere and Ocean

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Title: Elemental Mercury Concentrations and Fluxes in the Tropical Atmosphere and Ocean
Author: Soerensen, Anne Laerke; Mason, Robert P.; Balcom, Prentiss H.; Jacob, Daniel James; Zhang, Yanxu; Kuss, Joachim; Sunderland, Elynor M

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Citation: Soerensen, Anne L., Robert P. Mason, Prentiss H. Balcom, Daniel J. Jacob, Yanxu Zhang, Joachim Kuss, and Elsie M. Sunderland. 2014. “Elemental Mercury Concentrations and Fluxes in the Tropical Atmosphere and Ocean.” Environ. Sci. Technol. 48 (19) (October 7): 11312–11319. doi:10.1021/es503109p.
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Abstract: Air–sea exchange of elemental mercury (Hg0) is a critical component of the global biogeochemical Hg cycle. To better understand variability in atmospheric and oceanic Hg0, we collected high-resolution measurements across large gradients in seawater temperature, salinity, and productivity in the Pacific Ocean (20°N-15°S). We modeled surface ocean Hg inputs and losses using an ocean general circulation model (MITgcm) and an atmospheric chemical transport model (GEOS-Chem). Observed surface seawater Hg0 was much more variable than atmospheric concentrations. Peak seawater Hg0 concentrations (∼130 fM) observed in the Pacific intertropical convergence zone (ITCZ) were ∼3-fold greater than surrounding areas (∼50 fM). This is similar to observations from the Atlantic Ocean. Peak evasion in the northern Pacific ITCZ was four times higher than surrounding regions and located at the intersection of high wind speeds and elevated seawater Hg0. Modeling results show that high Hg inputs from enhanced precipitation in the ITCZ combined with the shallow ocean mixed layer in this region drive elevated seawater Hg0 concentrations. Modeled seawater Hg0 concentrations reproduce observed peaks in the ITCZ of both the Atlantic and Pacific Oceans but underestimate its magnitude, likely due to insufficient deep convective scavenging of oxidized Hg from the upper troposphere. Our results demonstrate the importance of scavenging of reactive mercury in the upper atmosphere driving variability in seawater Hg0 and net Hg inputs to biologically productive regions of the tropical ocean.
Published Version: doi:10.1021/es503109p
Other Sources: http://acmg.seas.harvard.edu/publications/2014/Soerensent2014_Manuscript.pdf
Terms of Use: This article is made available under the terms and conditions applicable to Open Access Policy Articles, as set forth at http://nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of-use#OAP
Citable link to this page: http://nrs.harvard.edu/urn-3:HUL.InstRepos:34306002
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