Abstract

Understanding atmospheric mercury chemistry is the key for explaining the biogeochemical cycle of mercury and for improving the predictive capability of computational models. Increased efforts are being made to ensure comparable Hg speciation measurements in the air through establishing metrological traceability. While traceability for elemental mercury has been recently set, this is by no means the case for gaseous oxidized mercury (GOM). Since a calibration unit suitable for traceable GOM calibrations based on evaporation of HgCl2 solution was recently developed, the purpose of our work was to extensively evaluate its performance. A highly specific and sensitive 197Hg radiotracer was used for validation over a wide range of concentrations. By comparing experimental and calculated values, we obtained recoveries for the calibration unit. The average recoveries ranged from 88.5% for 1178 ng m−3 HgCl2 gas concentration to 39.4% for 5.90 ng m−3 HgCl2 gas concentration. The losses were due to the adsorption of oxidized Hg on the inner walls of the calibrator and tubing. An adsorption isotherm was applied to estimate adsorption enthalpy (ΔHads); a ΔHads value of −12.33 kJ mol−1 was obtained, suggesting exothermal adsorption. The results of the calibrator performance evaluation suggest that a newly developed calibration unit is only suitable for concentrations of HgCl2 higher than 1 µg m−3. The concentration dependence of recoveries prevents the system from being used for calibration of instruments for ambient GOM measurements. Moreover, the previously assessed uncertainty of this unit at µg m−3 level (2.0%, k = 2) was re-evaluated by including uncertainty related to recovery and was found to be 4.1%, k = 2. Calibrator performance was also evaluated for HgBr2 gas calibration; the recoveries were much lower for HgBr2 gas than for HgCl2 gas even at a high HgBr2 gas concentration (>1 µg m−3). As HgBr2 is often used as a proxy for various atmospheric HgBr species, the suitability of the unit for such calibration must be further developed.

Highlights

  • Mercury is present in the atmosphere in different forms as a result of anthropogenic activities and natural processes

  • Atmospheric Hg fractions are operationally defined as gaseous elemental mercury (GEM, Hg0 ), gaseous oxidized mercury (GOM, Hg2+ ), particulate-bound mercury (PBM, Hg-p), and total gaseous mercury (TGM)

  • The 197 Hg radiotracer has proven to be suitable for studying the characteristics of calibrators because it enabled us to closely follow the processes that limit the use of calibrators based on evaporation, especially for low GOM concentrations

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Summary

Introduction

Mercury is present in the atmosphere in different forms as a result of anthropogenic activities and natural processes. Mercury can be carried long distances across the hemisphere and deposited into terrestrial and aquatic environments, where it is taken into the food web or re-emitted into air [1]. Atmospheric Hg fractions are operationally defined as gaseous elemental mercury (GEM, Hg0 ), gaseous oxidized mercury (GOM, Hg2+ ), particulate-bound mercury (PBM, Hg-p), and total gaseous mercury (TGM). Since the atmosphere is the major pathway for global Hg transport, understanding the atmospheric Hg cycle is of great importance. A critical parameter of understanding the Hg atmospheric cycle [2]. Even though GEM is the most abundant atmospheric Hg form, PBM and especially

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