Comparison of atmospheric mercury speciation and deposition at nine sites across central and eastern North America

dc.contributor.author Engle, Mark A.
dc.contributor.author Tate, Michael T.
dc.contributor.author Krabbenhoft, David P.
dc.contributor.author Schauer, James J.
dc.contributor.author Kolker, Allan
dc.contributor.author Shanley, James B.
dc.contributor.author Bothner, Michael H.
dc.date.accessioned 2010-10-18T15:53:01Z
dc.date.available 2011-03-22T08:23:45Z
dc.date.issued 2010-09-22
dc.description Author Posting. © American Geophysical Union, 2010. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research 115 (2010): D18306, doi:10.1029/2010JD014064. en_US
dc.description.abstract This study presents >5 cumulative years of tropospheric mercury (Hg) speciation measurements, over the period of 2003–2009, for eight sites in the central and eastern United States and one site in coastal Puerto Rico. The purpose of this research was to identify local and regional processes that impact Hg speciation and deposition (wet + dry) across a large swath of North America. Sites sampled were selected to represent both a wide range of mercury exposure and environmental conditions. Seasonal mean concentrations of elemental Hg (1.27 ± 0.31 to 2.94 ± 1.57 ng m−3; inline equation ± σ), reactive gaseous mercury (RGM; 1.5 ± 1.6 to 63.3 ± 529 pg m−3), and fine particulate Hg (1.2 ± 1.4 to 37.9 ± 492 pg m−3) were greatest at sites impacted by Hg point sources. Diel bin plots of Hgo and RGM suggest control by a variety of local/regional processes including impacts from Hg point sources and boundary layer/free tropospheric interactions as well as from larger-scale processes affecting Hg speciation (i.e., input of the global Hg pool, RGM formed from oxidation of Hgo by photochemical compounds at coastal sites, and elemental Hg depletion during periods of dew formation). Comparison of wet Hg deposition (measured), RGM and fine particulate Hg dry deposition (calculated using a multiple resistance model), and anthropogenic point source emissions varied significantly between sites. Significant correlation between emission sources and dry deposition was observed but was highly dependant upon inclusion of data from two sites with exceptionally high deposition. Findings from this study highlight the importance of environmental setting on atmospheric Hg cycling and deposition rates. en_US
dc.description.sponsorship Funding for this research was provided by the USGS Toxic Substances Hydrology Program, U.S. Department of Interior Landscapes Program, the USGS Mendenhall Postdoctoral Program, the USGS Energy Program, and by U.S. EPA STAR grant R829798. en_US
dc.format.mimetype application/pdf
dc.format.mimetype text/plain
dc.format.mimetype application/postscript
dc.identifier.citation Journal of Geophysical Research 115 (2010): D18306 en_US
dc.identifier.doi 10.1029/2010JD014064
dc.identifier.uri https://hdl.handle.net/1912/3949
dc.language.iso en_US en_US
dc.publisher American Geophysical Union en_US
dc.relation.uri https://doi.org/10.1029/2010JD014064
dc.subject Atmospheric mercury en_US
dc.subject Wet deposition en_US
dc.subject Dry deposition en_US
dc.subject Diel patterns en_US
dc.title Comparison of atmospheric mercury speciation and deposition at nine sites across central and eastern North America en_US
dc.type Article en_US
dspace.entity.type Publication
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Figure S1: Diel bin plots showing mean ± standard deviation of NOx concentrations at the C-AL, C-SC, and C-MA sites.
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Figure S2: Diel bin plots showing mean ± standard deviation of SO2 concentrations at the C-AL, C-SC, and C-MA sites.
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Figure S3: Diel bin plots showing mean ± standard deviation of O3 concentrations at the C-AL, C-SC, and C-MA sites.
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Figure S4: Diel bin plots showing mean ± standard deviation of CO concentrations at the C-SC site.
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