Atmospheric mercury dispersion over the South African Highveld

Coal combustion in coal-fired power plants is the dominant source of mercury (Hg) emissions in South Africa. The majority of these plants are located in the South African Highveld, an area that experiences poor air quality. Despite this, the specifics of Hg emissions – such as the amounts emitted, mercury species emitted and their spatial variability – from these plants remain unclear. This study presents the first dispersion modelling of Hg concentrations and wet and dry deposition in the Highveld using CALPUFF. It focuses on inorganic gaseous elemental (Hg0), inorganic reactive gaseous (Hg2+) and inorganic particle-bound Hg (HgP) emissions from 12 coal-fired power plants from 2011 to 2014. Results show that Hg concentrations are highest near the central cluster of power plants, with levels ranging from 0.0028 to 0.0631 ng/m3 for Hg0, 0.0028 to 0.0497 ng/m3 for Hg2+ and 0.0008 to 0.0137 ng/m3 for HgP. Significant wet and dry deposition, measured at 0.07–7.46 and 0.03–3.33 (g/ha)/year, respectively, also occurs in these areas, indicating that proximity to power plants leads to higher deposition. A health risk assessment suggests that nearby populations may be at risk of acute health impacts from Hg0 inhalation. However, the accuracy of this assessment is limited by the overestimation of Hg0 concentrations in dry deposition modelling. The findings highlight the need for further studies to characterise and quantify methylmercury, the most toxic form of Hg, in the environment. This study also potentially shows important locations where new Hg monitoring stations should be placed.