2018
DOI: 10.1016/j.dsr2.2018.05.012
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The distribution and speciation of mercury in the California current: Implications for mercury transport via fog to land

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Cited by 22 publications
(42 citation statements)
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“…As the advective marine fogs that comprised our sample set typically form under dark conditions, the Hg species entrained within them would be less susceptible to photoreduction processes and the corresponding shifts in odd-MIF signatures after entrainment within the cloud, suggesting most of this photoreduction process occurred in the marine environment prior to aerosol incorporation within the air masses. 3 Coastal California fogwater exhibits even-MIF signatures generally consistent with previous observations of precipitation samples, with positive Δ 200 Hg and negative Δ 204 Hg signatures [Δ 200 Hg = −0.16‰ to 0.24‰, average of 0.08 ± 0.10‰ (1SD); Δ 204 Hg = −0.31‰ to 0.32‰, average of −0.07 ± 0.19‰ (1SD)] (Figure S1). However, one sample (FRF_2014_1) exhibited even-MIF values (Δ 200 Hg = −0.16‰, and Δ 204 Hg = 0.32‰) that were greater than values typically observed in measurements of total gaseous Hg (TGM) but exhibited positive odd-MIF signatures that are inconsistent with previous observations of TGM.…”
Section: Resultssupporting
confidence: 87%
“…As the advective marine fogs that comprised our sample set typically form under dark conditions, the Hg species entrained within them would be less susceptible to photoreduction processes and the corresponding shifts in odd-MIF signatures after entrainment within the cloud, suggesting most of this photoreduction process occurred in the marine environment prior to aerosol incorporation within the air masses. 3 Coastal California fogwater exhibits even-MIF signatures generally consistent with previous observations of precipitation samples, with positive Δ 200 Hg and negative Δ 204 Hg signatures [Δ 200 Hg = −0.16‰ to 0.24‰, average of 0.08 ± 0.10‰ (1SD); Δ 204 Hg = −0.31‰ to 0.32‰, average of −0.07 ± 0.19‰ (1SD)] (Figure S1). However, one sample (FRF_2014_1) exhibited even-MIF values (Δ 200 Hg = −0.16‰, and Δ 204 Hg = 0.32‰) that were greater than values typically observed in measurements of total gaseous Hg (TGM) but exhibited positive odd-MIF signatures that are inconsistent with previous observations of TGM.…”
Section: Resultssupporting
confidence: 87%
“… Hemispheric mercury gradients in different Pacific Ocean reservoirs. The boxplots illustrate the hemispheric gradient of ( A ) atmospheric Hg 0 model estimates (nanograms ⋅ meters −3 ) extracted at tuna sampling locations (see Materials and Methods ), ( B ) observed total Hg concentrations (picomolar) in seawater ( 12 , 34 , 38 , 53 , 54 , 56 ), ( C ) observed MeHg concentrations at peak (picomolar) in seawater ( 12 , 34 , 53 57 ), ( D ) standardized total Hg concentrations (micrograms ⋅ grams −1 , dw) in skipjack tuna (this study), and ( E ) observed total Hg concentrations (nanograms ⋅ grams −1 , dw) in marine sediments ( 2 , 73 78 ). ** indicates significant differences between the northern and southern hemispheres (Kruskal–Wallis test; P < 0.01).…”
Section: Resultsmentioning
confidence: 99%
“…Measured Seawater Methylmercury Concentrations in the Pacific Ocean. Seawater MeHg data from the Pacific Ocean were compiled from the literature from both filtered and unfiltered samples (12,34,38,(53)(54)(55)(56)(57). In particular, we used the maximum total Hg and MeHg concentrations observed in the water column (picomolar) and the depth of maximum MeHg concentrations (meters).…”
Section: Methodsmentioning
confidence: 99%
“…On the central coast of California, USA, coastal marine fog varies seasonally, partially overlapping in time with coastal upwelling in the California Current. Upwelling brings elevated concentrations of methylated Hg compounds to the surface waters from deeper, low-oxygen waters and/or sediments (where anaerobic microbes are active), whereby sea-air exchange of methylated Hg compounds can be source of gaseous dimethylmercury (DMHg) and/or gaseous and particulate MMHg to the atmosphere 24,25 . Dimethyl Hg in the atmosphere is unstable and will break down into MMHg in the gas phase 26 or the aqueous phase at low pH 27 , followed by rapid adsorption onto aerosols and cloud droplets in the marine boundary layer 28 .…”
Section: Introductionmentioning
confidence: 99%