156
in the air and water. Strictly speaking, the air–water CO 2 flux should be calculated
from the fugacity of CO 2 (fCO 2 ), which is the partial pressure of an ideal gas with
the same chemical potential as the real gas. However, for the sake of simplicity no
distinction between pCO 2 and fCO 2 has been made in this chapter. The difference in
the estimated CO 2 fluxes would be very small (Weiss 1974).
The following assumptions are made in the thin-film model (Fig. 6.2): (1) pCO 2
at the top of the film is the same as atmospheric pCO 2 , (2) pCO 2 at the bottom of the
film is the same as that in water, and (3) the concentration gradient within the film
is linear. Using these assumptions, the air–water CO 2 flux can be determined from
the thickness of the film and the difference in pCO 2 between the air and water.
If the CO 2 concentrations at the top and bottom of the film are C top and C bottom ,
respectively, assumptions (1) and (2) lead to Eqs. 6.1 and 6.2.
C
pCO
S pCO
S
top
t op
air
=
´ =
´
2
2
(6.1)
C
pCO
S pCO
S
bottom
bottom
w ater
=
´ =
´
2
2
(6.2)
In these equations, pCO 2top and pCO 2bottom are the pCO 2 at the top and bottom of the
film, respectively, and pCO 2air and pCO 2water are the pCO 2 in the atmosphere and in
water deeper than the film, respectively. S is the CO 2 solubility in the water.
Under assumption (3), introduction of Fick’s law and Eqs. 6.1 and 6.2 into the
thin-film model gives the following equation.
C
z
C top = pCO 2air . S
C top
C bottom
δ
C bottom = pCO 2water . S
0
Fig. 6.2 Schematic diagram of the thin-film model. The horizontal axis shows the CO 2 concentration (C), and the vertical axis shows the vertical depth (z = 0 at water surface). This figure illustrates the case where the CO 2 concentration in water is lower than that in the atmosphere. In the
thin-film model, the air–water CO 2 flux (F) is determined by multiplying the molecular diffusion
coefficient of CO 2 (D) by the concentration gradient (∂C water /∂z) in the boundary layer just below
the water surface (Fick’s law). This gradient is calculated from both the thickness (δ) of the boundary layer and the difference between C at the top of the layer (C top ) and C at the bottom of the layer
(C bottom ). This model assumes that the top and bottom of the layer are in equilibrium with the partial
pressure of CO 2 (pCO 2 ) in the atmosphere and water, respectively (C top  = pCO 2air · S, C bottom  = pCO 2water · S; where S is the solubility of CO 2 ). Whether the atmospheric CO 2 concentration and C top are
equal depends on the water temperature and salinity. This figure illustrates the case where their
concentrations are equal
T. Tokoro et al.
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