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we can envision a uniform plane wave as being created by a uniform surface source of
                        doubly-infinite extent, plane waves are also useful as models for spherical waves over
                        localized regions of the wavefront.
                          We choose the plane of field invariance to be the xy-plane and later generalize the
                        resulting solution to any planar surface by a simple rotation of the coordinate axes. Since
                        the fields vary with z only we choose to write the wave equation (2.325) in rectangular
                        coordinates, giving for a source-free region of space 4
                              2
                                          2
                                                      2
                                                                                2
                             ∂ E x (z, t)  ∂ E y (z, t)  ∂ E z (z, t)  ∂E(z, t)  ∂ E(z, t)
                            ˆ x       + ˆ y       + ˆ z       − µσ        − µ
         = 0.   (2.328)
                                ∂z 2        ∂z 2        ∂z 2         ∂t          ∂t 2
                          If we return to Maxwell’s equations, we soon find that not all components of E are
                        present in the plane-wave solution. Faraday’s law states that
                                           ∂E y (z, t)  ∂E x (z, t)  ∂E(z, t)    ∂H(z, t)
                             ∇× E(z, t) =−ˆ x       + ˆ y      = ˆ z ×      =−µ         .     (2.329)
                                              ∂z          ∂z           ∂z           ∂t
                        We see that ∂ H z /∂t = 0, hence H z must be constant with respect to time. Because
                        a nonzero constant field component would not exhibit wave-like behavior, we can only
                        have H z = 0 in our wave solution. Similarly, Ampere’s law in a homogeneous conducting
                        region free from impressed sources states that
                                                         ∂D(z, t)            ∂E(z, t)
                                         ∇× H(z, t) = J +       = σE(z, t) +
                                                           ∂t                  ∂t
                        or
                                  ∂ H y (z, t)  ∂ H x (z, t)  ∂H(z, t)          ∂E(z, t)
                               − ˆ x       + ˆ y      = ˆ z ×       = σE(z, t) + 
     .      (2.330)
                                     ∂z          ∂z           ∂z                  ∂t
                        This implies that
                                                              ∂E z (z, t)
                                                  σ E z (z, t) + 
    = 0,
                                                                 ∂t
                        which is a differential equation for E z with solution
                                                                     σ
                                                                     
 .
                                                     E z (z, t) = E 0 (z) e − t
                        Since we are interested only in wave-type solutions, we choose E z = 0.
                          Hence E z = H z = 0, and thus both E and H are perpendicular to the z-direction.
                        Using (2.329) and (2.330), we also see that
                                    ∂             ∂H      ∂E
                                      (E · H) = E ·  + H ·
                                    ∂t            ∂t      ∂t
                                                 1        ∂E         σ     1        ∂H
                                            =− E · ˆ z ×      − H ·   E + H · ˆ z ×
                                                µ         ∂z         
     
         ∂z
                        or
                                        ∂   σ           1        ∂E     1        ∂H

                                                                         ˆ
                                          +    (E · H) =  ˆ z · E ×   − z · H ×       .
                                       ∂t   
           µ         ∂z    
         ∂z
                        We seek solutions of the type E(z, t) = ˆ pE(z, t) and H(z, t) = ˆ qH(z, t), where ˆ p and ˆ q are
                        constant unit vectors. Under this condition we have E × ∂E/∂z = 0 and H × ∂H/∂z = 0,
                        giving
                                                      ∂    σ

                                                        +     (E · H) = 0.
                                                      ∂t
                        4 The term “source free” applied to a conducting region implies that the region is devoid of impressed
                        sources and, because of the relaxation effect, has no free charge. See the discussion in Jones [97].


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