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

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8<br />

F = βσv(C1-C3) (1),<br />

where β is an empirical coefficient, the “proportionality constant”, dependent on wind speed and<br />

turbulence, generally 0.6 for a fixed deadband and approximately 0.3 for a dynamic deadband, and<br />

calculated via the heat flux with the Metsupport system. σv is the standard deviation of the vertical<br />

wind velocity: both values are obtained directly as output from the REA system; C1 and C3 are the<br />

concentrations of RGM in upward and downward air masses, respectively.<br />

From the flux measurements the depositional velocity of RGM can be calculated if the ambient<br />

concentration for RGM is known:<br />

vd = F/C (2),<br />

where C is the concentration of RGM, and F is from 1.<br />

Due to the uncertainty of the concentration measurements in Barrow: 10 % and of the<br />

meteorological measurements, 10 % for β, σw for the Metsupport system (Christensen et al., 2000)<br />

the uncertainty on the flux measurements using the Landis et al. 2002, KCl coated annular denuder<br />

sampling end, heating caps and Metsupport REA system are estimated to be within 40% on a 95%<br />

confidence interval, though 20% would be a more conservative estimate of denuder precision, given<br />

the fact that flow at 10 lpm is not instantaneously developed, so there is necessarily some flow and<br />

turbulence information lost when switching at 1 Hz. This gives a conservative sampling error for<br />

flux as 50 % for the above system in Barrow.<br />

As a quality assurance check for the REA flux measurements, the total concentration of the<br />

three annular denuders for each run was compared with ambient concentration from a CMDL<br />

collocated automated RGM monitoring system described in Lindberg et al., 2002. Results were<br />

favourable, within 25% of each other on average.<br />

3. Results and Discussion

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