Page 95 - Introduction to Computational Fluid Dynamics
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                            and where ψ is the stream function defined by       2D BOUNDARY LAYERS
                                                          ∂ψ
                                                             =−ρv r,                            (4.3)
                                                          ∂x
                                                          ∂ψ
                                                             = ρ ur.                            (4.4)
                                                          ∂y
                            Thus, at any x

                                                      ψ =     ρ ur dy + C,                      (4.5)
                            where C is a constant. The y coordinate is thus related to ψ and the latter, in turn, is
                            related to ω via Equation 4.2. Suffixes I and E, of course, refer to inner and external
                            boundaries.



                            4.3 Transformation to (x, ω) Coordinates
                            Our task now is to transform Equation 4.1 from the (x, y) coordinate system to
                            the (x, ω) coordinate syatem. To do this, we shall follow the sequence (x, y) →
                            (x,ψ) → (x,ω). Making use of the mass conservation equation (  = 1), we can
                            write Equation 4.1 in nonconservative form as

                                                 ∂       ∂       1 ∂      ∂
                                            ρ u      + v      =        r 
      + S.            (4.6)
                                                  ∂x     ∂y      r ∂y      ∂y
                               Now, the transformation (x, y) → (x,ψ) implies that



                                                         ∂ψ ∂         ∂
                                                 ∂
                                                      =            +       ,                    (4.7)
                                                         ∂x ∂ψ       ∂x
                                                ∂x   y           x       ψ

                                                 ∂       ∂ψ ∂              ∂
                                                       =           = ρ ru       .               (4.8)
                                                ∂y    x  ∂y ∂ψ    y       ∂ψ    y
                            Substituting these equations in Equation 4.6, we can show that

                                                          ∂          ∂        S
                                                ∂                2
                                                      =       ρ r u 
     +     .               (4.9)

                                                ∂x       ∂ψ          ∂ψ      ρ u
                                                    ψ
                            Further, the (x,ψ) → (x,ω) transformation implies that

                                                 ∂        ∂        ∂ω    ∂
                                                        =        +              ,              (4.10)
                                                  ∂x    ψ  ∂x    ω  ∂x    ψ  ∂ω    x
                            but, from Equation 4.2,

                                                            ∂ψ

                                              ∂ω        −1        ∂ψ I     ∂ψ EI
                                                    = ψ EI      −     − ω
                                              ∂x            ∂x     ∂x       ∂x
                                                  ψ                              ψ

                                                    =−ψ   −1  ∂ψ I  + ω  ∂ψ EI  ,              (4.11)
                                                         EI
                                                              ∂x        ∂x
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