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              To validate our approach, various types of ship geometry, such as  the DTMB 5415 model, the KCS
              model, the HTC model and the tanker model, are used as the test cases with two turbulence models,
              the  Baldwin-Lomax  model  and  the  Chien's  low  Reynolds  number  k-E  model.  The  convergence
              performance and the effect of the grid density on the free-surface waves are investigated. The results
              obtained  are compared  well  with the experimental  data provided by the KRISO, the MSEAN, the
              shipyard and the HSVA. For the former two test cases, an improvement for the free-surface waves has
              been achieved  as compared  with  our latest work  (Li et al., 2000), which has been  presented  in  the
              workshop held  recently  at Gothenburg (Larsson, et al.,  2000). Without doubt, the studies from CFD
              groups of various countries represent the major advances in this area, although just a few CFD groups
              completed these two cases in this workshop.


              2  NUMERICAL  METHODS

              2. I  Mathematical Models
              On the Cartesian co-ordinate (x, y, z, t) system, where the origin is fixed at the intersection of the bow
              with the still free surface, x is positive in the at? direction, y is positive towards the starboard and the z-
              direction is positive upwards, the RANS equations can be written in the compact form, namely
                     - d(F -Fv) + a(G- G,)   + d(H - H,)
                     dU
                        +
                     at     h        ay       az    =Q
                                                '.
              where  the variable U=(p, pu, pv, pw, pk, p~) The inviscid fluxes (F,  G, H), the viscous fluxes (Fv,
              G,, Hv) and the source term Q are e   respectively


                     F=              G=             H=








                      Q=  the 9-L mod el;   Q=                                       (3)
                          0
                          OI


                              rv  1
                              0

                and           r=
                                                                                    (4)





              p is the density of the fluid, the mean-velocity components in the x-, y- and z-directions are denoted by
              u, v and w, and \v is the so-called piezometric pressure. For the k-E  model, k and E are the turbulent
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