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

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In the model the removal of GEM leads to build-up of RGM as observed in the field (6). The<br />

calculated concentrations of RGM have been compared with measured integrated surface column of<br />

BrO as obtained from the GOME satellite (36). In Fig. 6 the mean BrO column near the surface (in<br />

the boundary layer) and RGM concentrations for each month are shown for the period of January to<br />

June 2000. The figures show clearly that BrO and RGM have the same general temporal and<br />

geographical variability and reach their maximum level and extension in April to May. This finding<br />

supports that the conversion of GEM in fact is connected to sea-ice with temperatures below –4 o C<br />

and to the chemistry of Br. Notwithstanding there is general good agreement between RGM and<br />

BrO, some clear discrepancies can be observed. In May the largest BrO concentrations are found<br />

along the coast of the Beaufort Sea (North of Canada and Alaska), whereas maximum RGM<br />

concentrations are predicted North of Greenland. At present there is no explanation for this<br />

observation but most probably it reflects the rough assumption that RGM is produced ubiquitously<br />

above surfaces with temperatures below –4 o C. Bromine is most probably formed on the surface of<br />

re-freezing leads (6). These leads form and disappear again more or less randomly around the Arctic<br />

Ocean depending on the oceanic currents, wind, temperature and solar flux. Therefore large<br />

variation in the concentrations of bromine is expected during spring and thus also in the removal of<br />

GEM and build up of RGM concentration. This feature is in fact clearly seen in the measurements<br />

of GEM, Fig. 2 and 5; and it explains the discrepancy between the model results giving a smooth<br />

depletion event extending for the whole depletion period, whereas measurements show a long series<br />

of shorter depletion episodes during the depletion period.<br />

The deposition of atmospheric mercury calculated with DEHM is shown in Fig. 7 for some selected<br />

locations in the Arctic: Station Nord (Greenland), Barrow (Alaska), Alert (Canada), Thule<br />

(Greenland), Spitzbergen (Norway), in the sub-Arctic, Nuuk area (south Greenland), and on Faeroe<br />

Islands and Denmark. The total deposition is divided into three components: the contribution from<br />

deposition of; RGM, photo-chemically formed TPM, and directly emitted TPM. It is clearly seen<br />

how important the depletion phenomenon is for the deposition of mercury in the high Arctic,<br />

whereas it has practically no importance in the Faroe Islands. However, the Nuuk area appears to be<br />

influenced by AMDEs and there are on going field activities to confirm experimentally if AMDEs<br />

extends to this sub-arctic area. The importance of AMDE for the mercury load is seen for example<br />

for the Thule area, where the total deposition of mercury is increased by a factor 3, while for the<br />

Faeroe Islands the depletion phenomena only lead to a 10% increase of the mercury deposition. The<br />

contribution from directly emitted particulate mercury is very small in the high Arctic. It is mainly<br />

the large atmospheric reservoir of elemental mercury, which contributes through its chemical<br />

conversion to RGM followed by fast deposition of RGM. For all places close to the sea the total<br />

deposition is at the same levels. However, the large contribution of RGM deposition in the Arctic<br />

occurs only over a 4 month period from March to June where the algae bloom occurs (9). This fact<br />

might lead to a higher uptake of mercury in the food chain than would be expected if one simply<br />

extrapolated data from mid latitudes to the Arctic.<br />

The deposition of mercury for 1999 and 2000 is shown in Fig. 8 for the Northern Hemisphere with<br />

and without AMDE’s. The largest depositions are found close to the sources in Asia, Europe and<br />

North America mainly due to the deposition of primarily emitted RGM and TPM that is removed<br />

fast mainly due to dry deposition and washout by rain. The calculations with and without AMDE’s<br />

show again the importance of AMDE in the Arctic for the total deposition of mercury. Here the<br />

photochemically formed RGM is removed mainly by dry deposition as the Arctic is characterized<br />

by its very dry climate. The total annual deposition increases in the whole Arctic, and for the area<br />

north of the Polar Circle the total deposition of mercury increases from 89 to 208 tons/year due to<br />

the depletion.<br />

7

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