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

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estimating for Alert an average springtime dry-deposition flux for mercury of 2.5 ± 0.5 ng m -2 h -1<br />

based on their measurements of TGM. Comparing the flux with the average meteorological<br />

conditions in Table 2., gives no direct correlations. One would expect that emissions would increase<br />

as a function of the rising temperatures, but this can not said to be readily apparent. What seems to<br />

be apparent is that following a large depositional event; there is a small re-emission. This is<br />

probably the snow pack regaining equilibrium with the atmosphere.<br />

As seen in Fig. 1., the depositional velocities noted for depositional events are fast, around 2<br />

cm s -1 this is what would be expected for a very reactive gaseous species such as HNO3. On<br />

average, the depositional velocity is approximately 1 cm s -1 . Comparing with measured dry<br />

deposition velocities over snow for HNO3, reviewed in Karlson and Nyholm, 1998, show that the<br />

measured dry depositional velocities for RGM may be an order of magnitude higher than that for<br />

HNO3, given the snow surface temperature of < 2 0 C.<br />

3.2 Comparison of RGM flux with RGM ambient concentrations<br />

Fig. 2, are the monitored results RGM concentrations during the Barrow 2001flux measurement<br />

campaign. Comparing with Fig. 1., show that when there is a deposition recorded by the REA<br />

machine, there are correspondingly low RGM ambient values. The air has been apparently depleted<br />

of RGM due to deposition. Trends of RGM rising in the air on the 8 th , 9 th and 12 th of April are<br />

recorded by the REA system as reemission, perhaps indicating that RGM can be re-volatized from<br />

the snow surface.<br />

3.3 Drawbacks and other possible accumulators<br />

Stable weather conditions are the greatest drawback to deploying the RGM system in the Arctic<br />

for investigating mercury depletion events. Lu et al., 2001, summarize that the environmental<br />

conditions favouring mercury depletion events at high latitudes are: 1, marine/maritime location; 2,<br />

calm weather, low wind speeds, non-turbulent air flow; 3, the existence of a temperature inversion;<br />

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