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FATE OF MERCURY IN THE ARCTIC Michael Evan ... - COGCI

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Fate of Mercury in the Arctic 14<br />

After polar sunrise, in Barrow, Alaska, KCl coated manual RGM denuders were used as the<br />

accumulator with the REA system. At 3 m above the snow pack significant RGM fluxes measured<br />

during March 29 th – April 12 th 2000 were directed toward the snow surface. Overall mean<br />

deposition was found to be - 0.4 +/- 0.2 pg m -2 s -1 ; N=9, +/1 SE and re-evasion was also observed.<br />

Using measured total RGM concentrations; depositional velocities were then computed and found<br />

to be on the order of 1 cm s -1 . Upon closer examination of field data, a relative rate study (paper 3,<br />

Skov et al., submitted) and utilizing knowledge from recently published reaction kinetics (Ariya et<br />

al., 2002), an updated mechanism is suggested (paper 4, Goodsite et al., submitted).<br />

The proposed reaction mechanism is that gaseous elemental mercury, Hg (0) combines with Br<br />

atoms, called X, coming from the polar sunrise destruction of ozone, in a reversible reaction,<br />

forming the energised HgBr*. Through a third body reaction, M, where M is N2 or O2, the HgBr<br />

radical is formed. The HgBr radical can live long enough at the low temperatures of the Arctic to<br />

combine with O2 forming the HgBrOO peroxy radical or can combine with Br forming HgBr2. It is<br />

not likely to react with Cl, since this reaction would be endothermic. Similarly, the product cannot<br />

be Hg2Br2 since this would imply a tri molecular reaction, which is highly unlikely to occur in the<br />

atmosphere given the very low concentrations of the reactants. Nor would the end product be HgO,<br />

since this formation is similarly thermodynamically not favourable. The final product is the divalent<br />

gaseous mercury unknown, HgXY. By modelling the reaction of Hg and Br in the atmosphere, with<br />

current reaction constant data, and BrO and Br measurements, we find that assuming 20 ppt BrO<br />

and 2 ppt in the atmosphere during a depletion event that the lifetime of Hg is 4.6 hrs against<br />

forming HgBr, The lifetime of HgBr is 0.35 hrs. against forming HgBr2; comparing with the<br />

lifetime of HgBr of 0.75 hrs means that 68% of the time HgBr will form HgBr2. Thus the overall<br />

lifetime of removal of Hg to HgBr2 is 4.6 hrs. / .68 = 6.7 hrs. This is in good agreement with the<br />

observed 10 hr lifetime of Hg under depletion.

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