MERCURY SPECIATION ADSORPTION (MESA) METHOD FOR COMBUSTION FLUE-GAS - METHODOLOGY, ARTIFACTS, INTERCOMPARISON, AND ATMOSPHERIC IMPLICATIONS

Chemical speciation of mercury (Hg) in a wide variety of combustion flue gas matrices has been determined using the mercury speciation adsorption (MESA) method. The MESA sampling system for gas phase Hg species employs a series of heated solid phase adsorbent traps. Flue gas oxidized Hg species (Hg(II) and MMHg) are adsorbed by a potassium chloride (KCl) impregnated soda lime sorbent. Elemental Hg (Hg-o) is collected by an iodated carbon sorbent after passing through the KCl/soda lime sorbent. Total Hg (Hg-t) is determined by summation of species. In the laboratory, cold vapor atomic fluorescence spectroscopy (CVAFS) is used for detection of Hg collected on the solid sorbents, after appropriate sample digestion and preparation. The MESA method has been evaluated for species stability, matrix effects, breakthrough, artifacts and precision. Based on eight duplicate samples a mean precision of 6.8% 11% and 4.5% (relative percent difference) has been calculated for Hg-o, Hg(II) and Hg-t respectively. Intercomparison of the MESA method with other methods shows very good agreement for Hg-t. Mass balance calculations at 5 sites range from 75 to 140%, with a mean of 97 +/- 25%. Overall mean speciation results from 19 separate determinations suggest that Hg(II) has a 1 sigma range of 40 to 94% in coal combustion flue gas at, the inlet to pollution control devices.