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E 0       − jβ + z  − jβ − z       − jβ + z  − jβ − z
                                           =      ˆ x e  + e     + j ˆ y −e   + e
                                              2
                                                          
     1                1
                                                   1
                                           = E 0 e − j (β + +β − )z  ˆ x cos (β + − β − )z + ˆ y sin (β + − β − )z
                                                   2
                                                                2                2
                        or
                                                      1
                                             ˜
                                            E = E 0 e − j (β + +β − )z  [ˆ x cos θ(z) + ˆ y sin θ(z)]
                                                      2
                        where θ(z) = (β + − β − )z/2. Because β +  = β − , the velocities of the two circularly
                        polarized waves differ and the waves superpose to form a linearlypolarized wave with a
                        polarization that depends on the observation plane z-value. We maythink of the wave
                        as undergoing a phase shift of (β + + β − )z/2 radians as it propagates, while the direction
                          ˜
                        of E rotates to an angle θ(z) = (β + − β − )z/2 as the wave propagates. Faraday rotation
                        can onlyoccur at frequencies where both the LHCP and RHCP waves propagate, and
                        therefore not within the stopband ω 0 <ω <ω 0 + ω M .
                          Faradayrotation is non-reciprocal. That is, if a wave that has undergone a rotation of
                        θ 0 radians bypropagating through a distance z 0 is made to propagate an equal distance
                        back in the direction from whence it came, the polarization does not return to its initial
                        state but rather incurs an additional rotation of θ 0 . Thus, the polarization angle of the
                        wave when it returns to the starting point is not zero, but 2θ 0 . This effect is employed
                        in a number of microwave devices including gyrators, isolators, and circulators. The
                        interested reader should see Collin [40], Elliott [67], or Liao [111] for details. We note
                        that for ω   ω M we can approximate the rotation angle as
                                               1  √    
       ω M           ω M       1    √
                          θ(z) = (β + − β − )z/2 =  ωz  µ 0  1 +    −   1 +        ≈− zω M  µ 0 ,
                                               2              ω 0 − ω       ω 0 + ω    2
                        which is independent of frequency. So it is possible to construct Faraday rotation-based
                        ferrite devices that maintain their properties over wide bandwidths.
                          It is straightforward to extend the above analysis to the case of a lossy ferrite. We
                        find that for typical ferrites the attenuation constant associated with µ − is small for all
                        frequencies, but the attenuation constant associated with µ + is large near the resonant
                        frequency(ω ≈ ω 0 ) [40]. See Problem  4.16.

                        4.11.7   Propagation of cylindrical waves

                          Bystudying plane waves we have gained insight into the basic behavior of frequency-
                        domain and time-harmonic waves. However, these solutions do not displaythe funda-
                        mental propertythat waves in space must diverge from their sources. To understand this
                        behavior we shall treat waves having cylindrical and spherical symmetries.


                        Uniform cylindrical waves. In § 2.10.7 we studied the temporal behavior of cylin-
                        drical waves in a homogeneous, lossless medium and found that theydiverge from a line
                        source located along the z-axis. Here we shall extend the analysis to lossy media and
                        investigate the behavior of the waves in the frequencydomain.
                          Consider a homogeneous region of space described bythe permittivity ˜ (ω), permeabil-
                        ity ˜µ(ω), and conductivity ˜σ(ω). We seek solutions that are invariant over a cylindrical
                                                ˜
                                ˜
                                        ˜
                                                         ˜
                        surface: E(r,ω) = E(ρ, ω), H(r,ω) = H(ρ, ω). Such waves are called uniform cylindrical
                        waves. Since the fields are z-independent we maydecompose them into TE and TM sets
                        as described in § 4.11.2. For TM polarization we mayinsert (4.211) into (4.212) to find
                                                                    ˜
                                                              1   ∂E z (ρ, ω)
                                                 ˜
                                                 H φ (ρ, ω) =              .                  (4.327)
                                                            jω ˜µ(ω)  ∂ρ
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