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publications > 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

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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:

equation 1 D

equation 2 D

equation 3 D

equation 4 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], rho is water density [ML-3], R is the bottom-stress coefficient [T-1], Cd is the windstress coefficient [L0], rhoa is air density [ML-3], W is wind speed [LT-1], psi 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:

equation 5 D

where rhof is the reference fluid density (that is, the density of freshwater) [ML-3], and deltarho /deltaC is the slope of a linear relation between fluid density and salinity [L0]. For salinities ranging between freshwater and typical seawater, deltarho /deltaC 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, rho, vx, and vy.

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