Abstract

Abstract. Dry deposition of speciated mercury, i.e., gaseous oxidized mercury (GOM), particulate-bound mercury (PBM), and gaseous elemental mercury (GEM), was estimated for the year 2008–2009 at 19 monitoring locations in eastern and central North America. Dry deposition estimates were obtained by combining monitored two- to four-hourly speciated ambient concentrations with modeled hourly dry deposition velocities (Vd) calculated using forecasted meteorology. Annual dry deposition of GOM+PBM was estimated to be in the range of 0.4 to 8.1 μg m−2 at these locations with GOM deposition being mostly five to ten times higher than PBM deposition, due to their different modeled Vd values. Net annual GEM dry deposition was estimated to be in the range of 5 to 26 μg m−2 at 18 sites and 33 μg m−2 at one site. The estimated dry deposition agrees very well with limited surrogate-surface dry deposition measurements of GOM and PBM, and also agrees with litterfall mercury measurements conducted at multiple locations in eastern and central North America. This study suggests that GEM contributes much more than GOM+PBM to the total dry deposition at the majority of the sites considered here; the only exception is at locations close to significant point sources where GEM and GOM+PBM contribute equally to the total dry deposition. The relative magnitude of the speciated dry deposition and their good comparisons with litterfall deposition suggest that mercury in litterfall originates primarily from GEM, which is consistent with the limited number of previous field studies. The study also supports previous analyses suggesting that total dry deposition of mercury is equal to, if not more important than, wet deposition of mercury on a regional scale in eastern North America.

Highlights

  • Atmospheric mercury (Hg) dry and wet deposition need to be quantified to reduce large gaps existing in global Hg mass balance estimates, assess Hg effects on various ecosystems, and attribute sources of deposited Hg for Hg emission controls (Mason and Sheu, 2002; Mason et al, 2005; Lindberg et al, 2007; Selin et al, 2007)

  • The Mercury Deposition Network (MDN) of the National Atmospheric Deposition Program (NADP) in the USA and Canada was established more than a decade ago to measure the wet deposition of Hg in Published by Copernicus Publications on behalf of the European Geosciences Union

  • Despite the potentially large uncertainties in the concentration measurements and in the calculated deposition velocities, the estimated dry deposition of gaseous oxidized mercury (GOM)+particulate-bound mercury (PBM) agrees with the limited surrogate-surface dry deposition measurements and the estimated annual total dry deposition (GOM+PBM+net gaseous elemental mercury (GEM)) is in the same range as the annual litterfall Hg measurements

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Summary

Introduction

Atmospheric mercury (Hg) dry and wet deposition need to be quantified to reduce large gaps existing in global Hg mass balance estimates, assess Hg effects on various ecosystems, and attribute sources of deposited Hg for Hg emission controls (Mason and Sheu, 2002; Mason et al, 2005; Lindberg et al, 2007; Selin et al, 2007). L. Zhang et al.: Estimation of speciated and total mercury dry deposition precipitation (Vanarsdale et al, 2005; Prestbo and Gay, 2009; Risch et al, 2012b). The Atmospheric Mercury Network (AMNet) of NADP was established to monitor speciated concentrations of atmospheric Hg for subsequent dry deposition estimation (NADP, 2011a, b, c, d, e). Mercury monitoring networks and/or monitoring sites exist in many other parts of the world (Sakata and Asakura, 2008; Sprovieri et al, 2010)

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