Page 196 - Basic Structured Grid Generation
P. 196

Moving grids and time-dependent co-ordinate systems  185

                           7.4 Transformation of continuity
                                 and momentum equations


                        In this section we show the transformation of both the continuity and momentum
                        equations of continuum mechanics to a general time-dependent curvilinear co-ordinate
                        system. As indicated in the above sections, an important role is played by the grid-
                        point velocity vector W, and both the cartesian and the contravariant components of
                        W will be required at the grid nodes at any instant. With a differential model of
                        grid generation, a partial differential equation will have to be solved at each time-step
                        (a Dirichlet boundary-value problem) to obtain the new grid.


                        7.4.1 Continuity equation


                        The continuity equation of Continuum Mechanics can be written in terms of the density
                        function ρ(y i ,t) as
                                                    ∂ρ

                                                         +∇ · (vρ) = 0.                    (7.29)
                                                    ∂t
                                                        y i
                        This can be written with respect to a moving grid, using eqn (7.22), as
                                            ∂ρ

                                                  + ρ∇· W +∇ ·[(v − W)ρ]= 0,               (7.30)
                                            ∂t
                                                x  i
                        or, by (7.27), as
                                                                 	             i
                           ∂ √        ∂  √    i    ∂ √        ∂   √      i   ∂x
                            ( gρ) +     ( gρU ) =    ( gρ) +        gρ v +            = 0, (7.31)
                          ∂t         ∂x i          ∂t        ∂x i             ∂t
                                                                                 y j
                        using eqn (7.18).

                        7.4.2 Momentum equations


                        We start with the standard (non-conservative) cartesian form of the Momentum Equa-
                        tions for a viscous fluid with viscosity µ:

                                                   ∂v i        ∂v i  ∂σ ij
                                                ρ        + ρv j   =     ,                  (7.32)
                                                   ∂t         ∂y j   ∂y j
                                                       y i
                        with the stress tensor σ ij given in terms of pressure p and viscous stress T ij by
                                                    σ ij =−pδ ij + T ij ,
                        where T ij is related to the strain-rate ε ij through the equations

                                                               1 ∂v k
                                                 T ij = 2µ ε ij −   δ ij
                                                               3 ∂y k
                        and ε ij = 1/2(∂v i /∂y j + ∂v j /∂y i ).
   191   192   193   194   195   196   197   198   199   200   201