Page 340 - Electromagnetics
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erroneously chosen  < k i we would not have properly enclosed the pole and would have
                        obtained an incorrect inverse transform.
                          Now that we know how to represent the Fourier transform pair, let us apply the
                                                                                ˜
                        transform to solve (4.394). Our hope is that by representing ψ in terms of a spatial
                        Fourier integral we will make the equation easier to solve. We have
                                                      ∞+ j
                                                   1         x        − jk x x
                                                            ˜
                                            2
                                                 2
                                          (∇ + k )         ψ (k x , y,ω)e  dk x = 0.
                                            t
                                                   2π
                                                     −∞+ j
                        Differentiation under the integral sign with subsequent application of the Fourier integral
                                           ˜
                        theorem implies that ψ must obey the second-order harmonic differential equation
                                                     2
                                                    d     2   x
                                                             ˜
                                                       + k y  ψ (k x , y,ω) = 0
                                                   dy 2
                                                                                                   2
                                                                                          2
                                                                                              2
                        where we have defined the dependent parameter k y = k yr + jk yi through k + k = k .
                                                                                          x   y
                        Two independent solutions to the differential equation are e ∓ jk y y  and thus
                                                  ˜
                                                  ψ(k x , y,ω) = A(k x ,ω)e ∓ jk y y .
                        Substituting this into the inversion integral, we have the solution to the Helmholtz equa-
                        tion:
                                                         ∞+ j
                                                      1
                                          ˜                           − jk x x ∓ jk y y
                                          ψ(x, y,ω) =         A(k x ,ω)e  e    dk x .         (4.400)
                                                     2π
                                                        −∞+ j
                        If we define the wave vector k = ˆ xk x ± ˆ yk y , we can also write the solution in the form
                                                            ∞+ j
                                                         1
                                             ˜                           − jk·ρ
                                            ψ(x, y,ω) =          A(k x ,ω)e  dk x             (4.401)
                                                        2π
                                                          −∞+ j
                        where ρ = ˆ xx + ˆ yy is the two-dimensional position vector.
                          The solution (4.401) has an important physical interpretation. The exponential term
                        looks exactly like a plane wave with its wave vector lying in the xy-plane. For lossy media
                        the plane wave is nonuniform, and the surfaces of constant phase may not be aligned
                        with the surfaces of constant amplitude (see § 4.11.4). For the special case of a lossless
                        medium we have k i → 0 and can let   → 0 as long as  > k i . As we perform the inverse
                                                                                               2
                        transform integral over k x from −∞ to ∞ we will encounter both the condition k > k 2
                                                                                               x
                             2
                                        2
                                            2
                                 2
                        and k ≤ k .For k ≤ k we have
                             x          x
                                                                     √
                                                                       2
                                                                          2
                                                  − jk x x ∓ jk y y  − jk x x ∓ j  k −k x y
                                                 e    e    = e    e
                        where we choose the upper sign for y > 0 and the lower sign for y < 0 to ensure that the
                        waves propagate in the ±y-direction, respectively. Thus, in this regime the exponential
                        represents a propagating wave that travels into the half-plane y > 0 along a direction
                        which depends on k x , making an angle ξ with the x-axis as shown in Figure 4.28. For k x  in
                        [−k, k], every possible wave direction is covered, and thus we may think of the inversion
                        integral as constructing the solution to the two-dimensional Helmholtz equation from a
                        continuous superposition of plane waves. The amplitude of each plane wave component
                        is given by A(k x ,ω), which is often called the angular spectrum of the plane waves and
                        © 2001 by CRC Press LLC
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