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242  5. Some worked examples arising from physical problems



          and thus (5.108a) gives directly




          and then  (5.108b) becomes




          The appropriate solution of this equation, which satisfies both the matching condition
          and (5.106d), is





          Higher-order terms, in  both the  outer  and boundary-layer solutions,  can be  found
          altogether routinely (although the calculations are rather tedious).



          This completes our few examples in this group; we now turn to one of the areas where
          singular perturbation theory has played a very significant rôle.


          5.5 FLUID MECHANICS
          The study of fluid mechanics is broad and deep  and it often has far-reaching conse-
          quences. Many  of the  classical  techniques of singular perturbation  theory were  first
          developed in order to tackle particular difficulties that were encountered in this field.
          Examples that are available are numerous, and any number could have been selected for
          discussion here (and some have already appeared as examples in earlier chapters). We
          will content ourselves with just four more very different problems that give a flavour
          of what is possible, but these are all fairly classical examples of their type. Many others
          can be found in most of the texts already cited earlier. We will discuss: E5.19 Viscous
          boundary layer on a flat plate; E5.20 Very viscous flow past a sphere; E5.21 A piston
          problem; E5.22 A variable-depth Korteweg-de Vries equation for water waves.

          E5.19  Viscous boundary layer on a flat plate
          The solution of this problem (about 1905), with Poincaré’s work on celestial mechanics,
          together laid the  foundations for  singular perturbation  theory. In  this  example,  we
          consider an incompressible,  viscous fluid (in y >  0)  flowing  over a flat plate,
          the flow direction at infinity being parallel to the plate. The governing equations are the
          Navier-Stokes equation (in the absence of gravity) and the equation of mass conservation:
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