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

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Fate of Mercury in the Arctic 23<br />

The tropospheric depletion of ozone in the Arctic has been observed to be depleted during<br />

spring since, at least, 1966 (Tarasick and Bottenheim, 2002). It is generally accepted that the<br />

destruction of ozone is caused by catalytic reactions involving halogens, especially bromine, which<br />

originate from the polar oceans (Barrie et al., 1988 and Barrie and Platt, 1997). Our measurements<br />

suggest that the solar activity and present ice crystals influence the atmospheric transformation of<br />

elemental gaseous mercury to divalent mercury, which is more rapidly deposited (Lindberg et al.<br />

2002, paper 2, Appendix C). Satellite observations of BrO (as discussed in paper 2) suggest a<br />

correlation between mercury depletion and the total amount of BrO in the atmosphere, though later<br />

work shows the previously suggested mechanism to be more plausible, with the mechanisms<br />

presented in Lindberg et al., 2002 being thermodynamically unfavourable i.e. it is not likely that<br />

BrO/ClO + Hg 0 → HgO + Br/Cl radicals. Or that Hg 0 + 2Br/Cl radicals → HgBr2 or HgCl2.<br />

The most likely source of the halogens is the sea ice. Mercury depletion events therefore appear<br />

correlated with the presence of sea ice and are therefore probably found wherever there is sea ice<br />

and the potential for open leads. Today, typical levels of gaseous elemental mercury in the remote<br />

Northern hemisphere atmosphere and Arctic are about 1.5 ng m -3 (see paper 2). This level is a little<br />

bit less in the Southern Hemisphere, since most of the anthropogenic sources of gaseous mercury,<br />

are found in the Northern Hemisphere, and there is a lag time in transequatorial mixing.<br />

How long have mercury depletion events been occurring? Tarasick and Bottenheim (2002)<br />

have looked at surface ozone depletion events in the Arctic and Antarctic from historical ozone<br />

sonde records, and have noted ozone depletions since 1966, with an increasing frequency through<br />

2000 “explaining the apparent increase of Hg in Arctic biota in recent times”. They further note that<br />

“If the key to GEM depletion is the presence of reactive bromine, which can only be sustained via<br />

BrO recycling and hence ozone depletion, the increase of mercury in Arctic biota is a direct result<br />

of the increase in occurrence of ozone depletion episodes. “ Work accomplished by the present

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