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

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Fate of Mercury in the Arctic 109<br />

REA measurements rely on the transport of mass near the surface of the Earth where<br />

turbulence in the air is the main transport and mixing mechanism that eventually causes deposition.<br />

Fluid dynamics show that at any rough boundary, the friction causes velocity of a fluid (e.g. air) to<br />

go to zero. As this occurs, the air velocity vectors straighten out and are laminar in a plane a few<br />

millimeters thick over the Earth. Once gas molecules get into this plane they will either diffuse<br />

towards the surface, or evade towards the atmosphere, depending on the concentration gradient<br />

between this layer, known as the quasi-laminar boundary layer. Under higher turbulent conditions,<br />

the amount of mass transported greatly exceeds the amount of mass diffused, and generally<br />

turbulent transport is the most important physical method for deposition. A REA system samples<br />

this mass, as it is transported up from emission, or deposited. A valid flux determination relies on<br />

the principle that the mass of the trace gas measured, in this case RGM, is unique to that air mass.<br />

This means that it wasn’t produced or destroyed in the air mass.<br />

From the GEM concentration results from the Station Nord campaign, it can however be seen<br />

in the high Arctic, that under stable weather conditions that gaseous diffusion may be important.<br />

This is an area requiring further investigation in the future.<br />

Shear stress from surface friction is one of the main driving forces of turbulence; the other<br />

driving force is the change in buoyancy with the change in air temperature and thus density with<br />

height. This force may be important over the Arctic snow surface, however the cold surface cause<br />

stable cold air, that is difficult to move, and results in calm conditions, with wind speed under 2 m<br />

per second, as witnessed at Station Nord in 2002.<br />

These stable weather conditions are the greatest draw back to deploying the RGM system in the<br />

Arctic 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;

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