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Review of Hydrodynamic Theory Chapter | 2 37


             equations are the basis of linear wave theory and potential flow theory. Linear
             wave theory will be presented briefly in Chapter 5 that discusses wave energy.


             2.3.2 Viscous and Turbulent Flows

             The shear stresses in Eq. (2.29) are associated with the fluid viscosity and
             turbulence. For the case of laminar flow, where the shear stresses are caused
             by the viscosity, Newton’s shear-stress relationship can help to evaluate the
             stresses. Newton’s viscosity law in a simple form (horizontal flow) can be
             written as
                                              ∂u
                                         τ = μ                         (2.35)
                                              ∂z
             where μ is dynamic viscosity and is the property of a fluid. In general, Newton’s
             law expresses the relationship between the stress field and the deformations in a
             fluid, and is called the constitutive relation. The simplest case of the constitutive
             relation is the linear one (e.g. Newton’s viscosity law), in which the stress is a
             linear function of the strain rate. Newton’s viscosity law, for incompressible 3D
             flow, can be generalized as

                                            ∂u i  ∂u j
                                    τ ij = μ   +                       (2.36)
                                            ∂x j  ∂x i
                Replacing the shear stresses by the previous equation, the momentum
             equation (2.26) becomes
                                                         2
                             ∂u i   ∂u i      1 ∂p   μ ∂ u i
                                + u j  = B i −     +                   (2.37)
                             ∂t     ∂x j      ρ ∂x i  ρ ∂x k ∂x k
                    2
             where  ∂ u i  , as mentioned before, is the Laplacian of u i and in the expanded
                   ∂x k ∂x k
                     2     2      2
             form is  ∂ u i  +  ∂ u i  +  ∂ u i  . Eqs 2.37 and 2.19 (continuity) are called the
                     ∂x  2  ∂y 2  ∂z 2
             incompressible Navier Stokes Equations.
                For turbulent flows, the shear stresses would be dependent on the turbulency
             in the flow field. One approach is replacing the dynamic viscosity with an ‘eddy
             viscosity’ or ‘turbulent viscosity’. However, unlike dynamic viscosity, which is
             constant and a property of fluid, the eddy viscosity is highly variable in a flow
             field, depending on the level of turbulency. Some turbulence models introduce
             additional equations to estimate the distribution of eddy viscosity in a domain.
             More details are provided in Chapter 8.

             2.3.3 Shallow Water Equations

             The Navier-Stokes equations, which were discussed in the previous section, can-
             not be directly solved by any mathematical method, unless many assumptions/
             simplifications are made. Numerical methods have been developed to solve
             the 3D form of the Navier-Stokes equations, for small-scale problems (e.g.
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