Use of ecosystem-level flux measurements to improve atmosphere-surface exchange parameterization of elemental mercury in chemical transport models

Tanvir Khan1, Daniel Obrist2, Yannick Agnan3, Noelle E. Selin4 and Judith A. Perlinger5

To simulate global mercury (Hg) dynamics in chemical transport models (CTMs), surface-atmosphere exchange of gaseous elemental mercury, Hg0, is often parameterized based on a resistance-based dry deposition scheme coupled with a re-emission function from soils. Despite extensive use of this approach, direct evaluations of this implementation against field observations of net Hg0 exchange flux are lacking. In this study, we evaluate an existing net exchange parameterization (referred to here as the base model) by comparing modeled fluxes of Hg0 to fluxes measured in the field using micrometeorological techniques. Comparisons were performed in two terrestrial ecosystems: a grassland site in Switzerland and an Arctic tundra site in Alaska, U.S. in summer and winter. The base model included the dry deposition and soil re-emission parameterizations from Zhang et al. (2003) and the global CTM GEOS-Chem, respectively. Comparisons of modeled and measured Hg0 fluxes showed large discrepancies, particularly in the summer months when the base model overestimated daytime net deposition by approximately 9 and 2 ng m-2 h-1 at the grassland and tundra sites, respectively. In addition, the base model was unable to capture a measured nighttime net Hg0 deposition and wintertime deposition. We conducted a series of sensitivity analyses and recommend that Hg simulations using CTMs: (i) reduce stomatal uptake of Hg0 over grassland and tundra in models by a factor from 5-7; (ii) increase nighttime net Hg0 deposition, e.g., by increasing ground and cuticular uptake by reducing the respective resistance terms by factors of 3-4 and 2-4, respectively; and (iii) implement a new soil re-emission parameterization to produce larger daytime emissions and lower nighttime emissions. We conclude that the resistance-based model combined with the new soil re-emission flux parameterization is able to reproduce observed diel and seasonal patterns of Hg0 exchange in these ecosystems. This approach can be used to improve model parameterizations for other ecosystems in which flux measurements are available.

 

1Florida Solar Energy Center, a research institute of the University of Central Florida, tkhan@fsec.ucf.edu
2Department of Environmental, Earth and Atmospheric Sciences, University of Massachusetts Lowell, MA , Daniel_Obrist@uml.edu
3Earth and Life Institute, Université catholique de Louvain, 1348 Louvain-la-Neuve, Belgium, yannick.agnan@gmail.com
4Institute for Data, Systems, and Society, and Department of Earth, Atmospheric, and Planetary Scienc, selin@mit.edu
5Department of Civil and Environmental Engineering, Michigan Technological University, Houghton, MI 4, jperl@mtu.edu