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IDENTIFICATION OF THE ORIGINS OF ELEVATED ATMOSPHERIC MERCURY EPISODES USING A LAGRANGIAN MODELLING SYSTEM
Deyong Wen
; Waterloo Centre for Atmospheric Sciences, Department of Earth and Environmental Sciences, University of Waterloo, Waterloo, Ontario, N2L 3G1 Canada
John C. Lin
; Waterloo Centre for Atmospheric Sciences, Department of Earth and Environmental Sciences, University of Waterloo, Waterloo, Ontario, N2L 3G1 Canada
Fan Meng
; Waterloo Centre for Atmospheric Sciences, Department of Earth and Environmental Sciences, University of Waterloo, Waterloo, Ontario, N2L 3G1 Canada
James J. Sloan
; Waterloo Centre for Atmospheric Sciences, Department of Earth and Environmental Sciences, University of Waterloo, Waterloo, Ontario, N2L 3G1 Canada
Sažetak
We report the application of a receptor-oriented transport model, the Stochastic Time-Inverted Lagrangian Transport
(STILT) model, to the interpretation of hourly total gaseous mercury (TGM) concentrations at three monitoring sites in Southern
Ontario during four episodes of high TGM. STILT is a Lagrangian modelling system (Lin, J.C. et al. 2003) that simulates the
transport of ensembles of air parcels backward in time from an observation point to upstream locations where surface inputs of
target species occurred. A complete inventory of anthropogenic and natural mercury sources were used to compute the emissions.
The study was initiated by simulating the mercury concentrations in a North American domain using CMAQ-Hg, a regional
Eulerian chemical transport model (CTM). The STILT model was applied to several short episodes (usually lasting for 1-4 days) in
which the TGM measurements at four air quality measurement stations in Southern Ontario significantly exceeded the predictions of
the CTM. The STILT analysis compared the origins of air parcels arriving during the elevated TGM episodes with those of air
parcels arriving at proximal times when the measurements and the CTM predictions were both low.
The results consist of the STILT–predicted hourly concentrations at the measurement site as well as the surface footprint where the
mercury responsible for the episode was emitted. The temporal STILT prediction is in better agreement with the measured time
series than that of CMAQ-Hg. We believe this is partly due to the superior ability of STILT to capture near-field influences and
partly due to the spatial averaging inherent in Eulerian modelling. Also, the predicted footprint locations were reasonable,
coinciding with known locations of large mercury sources during the high episodes and with cleaner areas otherwise.
Ključne riječi
Hrčak ID:
64254
URI
Datum izdavanja:
12.12.2008.
Posjeta: 871 *