Multiscale modeling of the atmospheric fate and transport of mercury
Multiscale modeling of the atmospheric fate and transport of mercury
复制标题
DOI:
10.1029/2000jd000273
复制
发表时间:
2001-11
影响因子:
--
通讯作者:
C. Seigneur;P. Karamchandani;K. Lohman;K. Vijayaraghavan;R. Shia
中科院分区:
文献类型:
--
作者:
C. Seigneur;P. Karamchandani;K. Lohman;K. Vijayaraghavan;R. Shia
A numerical simulation of the atmospheric fate and transport of mercury (Hg) was conducted using a multiscale approach. Two different spatial scales were used to simulate (1) the global cycling of atmospheric Hg and (2) the atmospheric deposition of Hg in potentially sensitive areas. The global simulation was conducted using an updated version of our global Hg chemical transport model (CTM). The imbedded continental simulation was conducted using an updated version of the regional/continental CTM, TEAM. Simulations were conducted using 1998 meteorology and 1998/1999 emission inventories. Model simulation results show improved performance compared to earlier simulations. For example, the global simulation shows background concentrations of Hg species, interhemispheric gradients, and vertical gradients that are consistent with available measurements. The comparison of simulated Hg wet deposition fluxes with data from the Mercury Deposition Network in the United States shows a coefficient of determination (r2) of 0.75, little bias (−3%), and an average gross error of 21%. The major remaining sources of uncertainties, which include speciation of Hg emissions, Hg atmospheric chemistry, and dry and wet deposition processes for Hg species, are discussed.