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paper > simulation of integrated surface-water/ground-water flow and salinity... > governing equations > sw flow & solute transport
Simulation of integrated surface-water/ground-water flow and salinity for a coastal wetland and adjacent estuary
2. Governing equations
The subsequent governing equations are well described in the literature, and have been selected
to represent hydrologic processes in coastal wetlands
and adjacent estuaries. The two-dimensional vertically
averaged flow equations are used for the surface
flow as a compromise that allows better horizontal
resolution at the cost of vertical resolution. This is
justified by the observation that in coastal wetlands,
it is important to accurately represent topographic
relief, because variations in ground-surface
elevations are of the same order as water depths,
while the shallow depths make baroclinic driving-a
main cause of third-dimension flow-highly ineffectual.
The equations used to couple the surface-water
model with the ground-water model assume that
unsaturated zones are thin to absent, and leakage to
the water table can, therefore, be treated as
instantaneous. This assumption may limit the
approach to areas with shallow water tables and
highly porous materials.
2.1. Surface-water flow and solute transport
The governing equations for a shallow surfacewater
system consist of conservation of mass, volume,
and momentum. Leendertse and Gritton (1971) and
Leendertse (1987) present the following governing
equations, which were modified by Swain et al. (2004)
to include aerially distributed sources and sinks,
describing the (1) conservation of water volume, (2)
conservation of momentum in the x-direction, (3)
conservation of momentum in the y-direction, and (4)
solute mass transport:
D
D
D
D
where h is water stage [L], d is water depth [L], vx and vy are vertically averaged velocities in the x- and y- directions
[LT-1], qsg is a source/sink term representing
the volumetric exchange between surface water and ground water per unit area [LT-1], qr is a rainfall source term representing the volumetric rate per unit area [LT-1], qet is an evapotranspiration sink term representing the volumetric rate per unit area [LT-1],
f is the Coriolis parameter [T-1], g is gravitational acceleration [LT-2], is water density [ML-3], R is the bottom-stress coefficient [T-1], Cd is the windstress coefficient [L0], a is air density [ML-3], W is wind speed [LT-1], is the angle between wind direction and the positive y-axis [degrees], k is the horizontal momentum-exchange coefficient [L2T-1], C is solute concentration for a conservative nonreactive constituent [ML-3], Dx and Dy are the dispersion coefficients in the x- and y-directions [L2T-1], Csg is the leakage concentration between surface water and ground water [ML-3], and Cr is the solute concentration of rainfall. In this paper, the source concentration for rainfall and the sink concentration for evapotranspiration are both assumed to be zero, because C represents salinity concentration, which is considered conservative and non-reacting. The transport equation (Eq. (4)) can
easily be extended to represent reactive and decaying
constituents. Fluid density is related to salinity, in practical salinity units (psu), using the following
equation of state:
D
where f is the reference fluid density (that is, the
density of freshwater) [ML-3], and  / C is the slope of a linear relation between fluid density and salinity [L0]. For salinities ranging between freshwater and typical seawater,  / C has an approximate value of 0.7. The effect of temperature on fluid density is not considered here, although it could be important for some applications. For the Everglades application, seasonal temperature variations can be substantial, but spatial variations are assumed to have a negligible effect on flow. Simultaneous solutions to Eq. (1), (2), (3), (4), (5)
result in spatial distributions for h, C, , vx, and vy.
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