Ep. Achterberg et Cmg. Vandenberg, CHEMICAL SPECIATION OF CHROMIUM AND NICKEL IN THE WESTERN MEDITERRANEAN, Deep-sea research. Part 2. Topical studies in oceanography, 44(3-4), 1997, pp. 693-720
The chemical speciation of dissolved Cr and Ni was measured onboard sh
ip in the western Mediterranean Sea using cathodic stripping voltammet
ry (CSV) during the winter of 1992 and summer of 1993. Vertical profil
es for dissolved Cr(III) in the water column showed concentrations bet
ween 0 and 1.4 nM, with highest concentrations in the surface layer, p
ossibly caused by photochemical conversion of Cr(VI) to Cr(III) during
summer periods and by atmospheric inputs during winter periods. Enhan
ced Cr(III) levels also were encountered in the deeper Mediterranean w
aters and were attributed to mineralisation of sinking biological mate
rial and diffusion from sediments. Dissolved Cr(VI) concentrations ran
ged between 2 and 3 nM, and total dissolved Cr concentrations between
2 and 3.5 nM. Lowest concentrations of total Cr and Cr(VI) occurred in
the surface Atlantic waters and highest levels in the deeper Mediterr
anean waters. Total dissolved Ni concentrations ranged between 1.5 and
5 nM. Between 10 and 20% of the total dissolved Ni in the western Med
iterranean appeared to be strongly organically complexed. Both labile
and total dissolved Ni concentrations were lower in the surface Atlant
ic waters than in the Mediterranean deeper waters. Little difference w
as observed between the data sets for winter and summer, indicating th
at the influence of seasonal changes on the speciation of Ni was small
. A clear nutrient-like behaviour was not apparent for Ni and Cr, and
their vertical and horizontal distributions were mainly determined by
physical processes. Dissolved budget results for Cr and Ni for the Val
divia and Disco very (data in parentheses) cruises of -572 (55) and -4
39 (369) t yr(-1) were calculated, indicating that the dissolved budge
ts for these elements were well balanced. The budget deficits and surp
luses for dissolved Cr and Ni were small compared to the mass fluxes i
nvolved in the calculation of the mass balances. (C) 1997 Elsevier Sci
ence Ltd.