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             72 in Dahlquist( 1974)). In order to study the wave systems behind the source, we study the change of
             the phase of the integrand in expression (4). Due to symmetry only positive  y - v  needs to be studied.
             The phase function  k(lx - 41 cos0,  + (y - v) sin 0,) increases monotonically with increasing  k  and will
             give no wave  contribution  far away. If  a = arctan((y - v)/~x - 51)  is larger than some value  p , the
             phase function  k(lx -<lcosO0 - (y- q)sine0) will decrease monotonically with increasing  k  and will
             not give any wave contribution. If a  is less than B, this phase function will have one local maximum
             and/or minimum. Thus p  determines the wave angle behind the source. For subcritical case, the phase
             function  will  have  both  local  minimum  and  maximum,  which  corresponds  to  respectively  the
             transverse and divergent wave systems. For supercritical case, it has only one local maximum which
             corresponds to the divergent wave systems. Fig 1 shows the relationship between wave angle and  Fh .
             If  Fh <-  0.6, the wave angle is almost the same as in deep water (19'28'),  and approaches  90'  when
             reaching the critical speed. It then decreases with increasing speed.
                   Michell's  thin  ship theory is used to determine the densities of the source distribution on the
                                                              U
             centreplane  So of the  ship. This gives the velocity  potential  4 = - jjdtd< -
                                                                          ')  G(x, y. r; 6.0, <)
                                                              2x so     at
             due to the presence of the ship. Here y  = f(x, z) descirbes the hull surface for  y > 0 . By expressing
             the  hydrodynamic  pressure  as  p  = PUI$~ , the  corresponding  longitudinal  force  5, vertical  force
              4 and pitch moment 4 about the y - axis  are:













             Here  S,  is  the  mean  wetted  ship  hull  surface,  p  is  the  mass  density  of  water  and  n3  is  the  z-
             component of the normal vector to the body surface. Positive normal direction is into the body. We can
             use the pressure at the centreplane in the integration of  4 and  F5, but must integrate over s,  in order
             to properly account for area. By decomposing the Green's  function into an odd and even function in
              x - 6 , we can see that the only non-vanishing contribution to  F;  is coming from the odd term. This
             gives:



             where  P + iQ = jjdxd&(x,z)cosh(k(l+  z))exp(ikxcose). This is a well known result (Lunde (1951)).
                         S,,
              We then have two equations to calculate the wave resistance, either Eq. (5) or Eq. (8). This can be used
             to check the accuracy of the results.


             3  RESULTS FOR WIGLEY HULL
              Wigley's  (1 942) parabolic hull is used in the case studies. The hull surface for y > 0 is given by:
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