The sorption of mercury from simulated coal combustion hue gases on coal-de
rived chars, activated carbons, and zeolites has been examined using mercur
y L-III XAFS spectroscopy. The energy difference between the two inflection
points (IPD) in the mercury XANES spectra has been shown to be a sensitive
indicator of the local structure around the mercury adsorbed on the sorben
t The value of the IPD appears to reflect the form of mercury added to the
flue gas and to be sensitive to acidic gaseous species such as HCI and H2SO
4 that may be present in the flue gas, whether from addition to the flue ga
s or from the sulfur and chlorine in the coal. The data suggest that well-d
efined mercury species are not formed on carbon-based sorbents, but rather
the structure and chemistry of the sorbed mercury species reflect the diffe
rent anionic species present in the flue gas, as well as any activating ele
ment on the sorbent itself.