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To calculate a(x, y, t) and b(x, y, t), we must use the boundary conditions (A.17) and
                        (A.18). To apply (A.17), we put z = 0 into (A.28) to give

                                                a(x, y, t) + b(x, y, t) = f (x, y, t).         (A.29)
                        Using (A.18) is a bit more complicated since we must compute ∂ψ/∂z, and z is a pa-
                        rameter in the limits of the integral describing ψ. To compute the derivative we apply
                        Leibnitz’ rule for differentiation:
                           d     θ(α)           dθ                dφ                θ(α)  ∂ f
                                   f (x,α) dx =     f (θ(α), α) −     f (φ(α), α) +      dx.   (A.30)
                           dα  φ(α)             dα               dα               φ(α) ∂α
                        Using this on the integral term in (A.28) we have

                                    z       z−ζ                      z       z−ζ
                            ∂  c       t+  c                     c    ∂    t+  c
                                            S(x, y,ζ,τ) dτ  dζ  =               S(x, y,ζ,τ) dτ  dζ,
                           ∂z  2  0     z−ζ                      2  0 ∂z    z−ζ
                                      t−
                                         c                                t−  c
                        which is zero at z = 0.Thus
                                                              1           1



                                                = g(x, y, t) =− a (x, y, t) + b (x, y, t)
                                         ∂ψ

                                          ∂z z=0              c           c


                        where a = ∂a/∂t and b = ∂b/∂t. Integration gives
                                                                      t
                                           − a(x, y, t) + b(x, y, t) = c  g(x, y,τ) dτ.        (A.31)
                                                                    −∞
                        Equations (A.29) and (A.31) represent two algebraic equations in the two unknown
                        functions a and b. The solutions are
                                                                     t
                                           2a(x, y, t) = f (x, y, t) − c  g(x, y,τ) dτ,
                                                                   −∞
                                                                    t

                                           2b(x, y, t) = f (x, y, t) + c  g(x, y,τ) dτ.
                                                                   −∞
                        Finally, substitution of these into (A.28) gives us the solution to the inhomogeneous wave
                        equation
                                         z
                                     c       t+  z−ζ              1            z              z
                                              c
                        ψ(x, y, z, t) =         S(x, y,ζ,τ) dτ dζ +  f x, y, t −  + f x, y, t +   +
                                     2  0    z−ζ                  2            c              c
                                           t−
                                             c
                                           z
                                     c   t+  c

                                   +        g(x, y,τ) dτ.                                      (A.32)
                                     2    z
                                        t−
                                          c
                        This is known as the D’Alembert solution. The terms f (x, y, t ∓ z/c) contribute to ψ
                        as waves propagating away from the plane z = 0 in the ±z-directions, respectively. The
                        integral over the forcing term S is seen to accumulate values of S over a time interval
                        determined by z − ζ.
                          The boundary conditions could have been applied while still in the temporal frequency
                        domain (but not the spatial frequency domain, since the spatial position z is lost). But to
                        do this, we would need the boundary conditions to be in the temporal frequency domain.
                        This is easily accomplished by transforming them to give

                                                   ˜             = f (x, y,ω),
                                                                   ˜
                                                  ψ(x, y, z,ω)
                                                              z=0
                                                 ∂
                                                   ˜             = ˜ g(x, y,ω).
                                                ∂z  ψ(x, y, z,ω)  z=0
                        © 2001 by CRC Press LLC
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