652
R. Feistel et al.: Oceanographic application and numerical implementation of TEOS-IO: Part 1
Ocean Sci., 6, 633-677, 2010
www.ocean-sci.net/6/633/2010/
Temperature T / K
800
700
600
500
400
300
200
Fig. 7. Temperature-pressure phase diagram of seawater in the
vicinity of the triple point. At different salinities, the triple point
(TP), i.e. the equilibrium between liquid seawater, ice and vapour
is displaced along the sublimation line (in bold) of the ice-vapour
equilibrium. Note that the triple-point pressure can change by a fac
tor of 2 while the vapour-pressure lowering at constant temperature
is only of order 10% or less.
P = (p W ) 2 / p W (5-47)
Equations (5.44)-(5.47) provide four conditions for the five
unknowns Sa, T, P, p v and p w . Any one of the five parame
ters may be specified to complete the system which may then
be solved as discussed in Appendix A9.
If any one of the three variables Sa, T, P is specified, the
other two are determined by the above conditions. Figure 7
shows the displacement of the triple point along the sublima
tion line as a function of salinity.
In the library, the equilibrium properties P, T and Sa of
sea-ice vapour are available from the functions
sea.ice.vap.pressure.si,
sea_ice_vap_temperature_si and
sea_ice_vap_salinity_si. Note that the equilibrium
conditions are actually determined by calling one of
set_sea_ice_vap_eq_at-p,
set_sea_ice_vap_eq_at_t or
set_sea_ice_vap_eq_at_s, depending on which of
pressure, temperature or salinity is specified. Thus, one of
these ’’set-’’-routines must be called before accessing P,
T or Sa using the above function calls, but all three equi
librium properties corresponding to the specified parameter
choice are available once the appropriate ’’set-’’-routine is
executed.
5.8 Equilibrium humid air - liquid water
The state in which humid air is in equilibrium with liquid wa
ter is commonly referred to as “saturated air”, the “dewpoint”
or the “condensation point”. The condition for this equilib
rium is equal chemical potentials of liquid water, Eq. (4.2),
and of water in humid air, Eq. (S12.15),
S AV -A
dA ) T p 6
(5.48)
In terms of the Primary Standard functions and their inde
pendent variables (Sect. 2), Eq. (5.48) is expressed using the
relations
g w (T,P) = / F (r,p w ) + P/p w (5.49)
(5.50)
g AV = / AV (A,r,p AV ) +P/p AV
(5.51)
The independent variables in this scheme are the total pres
sure, P, the liquid density, p w , the humid-air density, p AV ,
the temperature, T, and the air fraction, A. Using Eqs. (5.49)
and (5.51) to eliminate the Gibbs potential in favour of the
Helmholtz potentials results in three equations for these five
unknowns.
For the numerical solution, two of the five unknowns as
well as starting values for the remaining unknowns must be
specified. Four important cases are considered in detail in
Appendix A10.
No matter which of the four cases considered in the ap
pendix is applied to compute the equilibrium between liquid
water and humid air, the numerical solution of Eqs. (5.48)-
(5.52) provides a consistent set of equilibrium values for A,
T,P, p w and p AV which is then available for the computa
tion of any other property of either saturated humid air or
liquid water in this state.
For example, at given temperature T and total pressure P,
the partial vapour pressure of saturated air is available in the
form
Psat, calc =x AV p (5.53)
from the solution obtained for A (T, P), using
library function liq_air_massf raction_air_si
and then converting to the mole fraction of vapour,
x AV =l — x^ v (A), Eq. (SI.5), using the library function
air_molf raction_vap-si. The comparison with ex
perimental data for the saturated vapour pressure (Feistel et
al., 2010a), Fig. 8, permits an estimate of the effect of the
cross-virial coefficients Baw(T), Caaw(T) and Caww(T’)