T. Bergan et H. Rodhe, Oxidation of elemental mercury in the atmosphere; Constraints imposed by global scale modelling, J ATMOS CH, 40(2), 2001, pp. 191-212
We use the global mercury model published by Bergan et al. (1999) to evalua
te the potential role of ozone and the hydroxyl radical as gas phase oxidan
ts for the oxidation of elemental mercury in the atmosphere. The magnitude
of natural and man-made mercury emissions are taken from recent literature
estimates. We consider only two mercury reservoirs, elemental mercury, Hg-0
, and the more soluble divalent form, HgII. Wet and dry deposition of HgII
is explicitly treated.
Applying monthly mean fields of ozone for the oxidation of gas phase Hg-0 a
nd using the reaction rate by Hall (1995) yields a global transformation of
Hg-0 to HgII which is too slow to keep the simulated concentration of Hg-0
near observed values. This shows that there must be additional important r
emoval processes for Hg-0 or that the reaction rate proposed by Hall (1995)
is too slow. A simulation in which the oxidation rate was artificially inc
reased, so that the global turn-over time of Hg-0 is one year and the simul
ated average concentration of Hg-0 realistic, produces latitudinal and seas
onal variations in Hg-0 that do not support the hypothesis that gas phase r
eaction with O-3 is the major oxidation process for Hg-0.
Recent studies indicate that OH may be an important gas phase oxidant for H
g-0 (Sommar et al., 2001). Using OH as the sole oxidant and applying the ox
idation rate by Sommar et al., we calculate a concentration of Hg-0 well be
low (about a factor of three) the observations. By prescribing a slower rat
e, corresponding to a turn-over time of Hg-0 of one year, we calculate conc
entrations of both Hg-0 in surface air and HgII in precipitation which corr
espond reasonably well, both in magnitude and temporal variation, with seas
onal observations in Europe and North America. This result supports the sug
gestion that the oxidation by OH is an important pathway for the removal of
Hg-0. In view of the uncertainties associated with our calculations, this
conclusion should still be regarded as tentative.