Page 534 - Engineering Electromagnetics, 8th Edition
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516                ENGINEERING ELECTROMAGNETICS

                                     simplifies to

                                                          1       2πr     2πr       2πr
                                                    H φ =    cos        +     sin                    (21)
                                                          r 2      λ       λ        λ
                                        Afew important points emerge when studying Eq. (21). First, at distances r that
                                     are on the order of a wavelength, the expression consists of two sinusoidal functions
                                     having the same period but in which the amplitude of the second one increases with
                                     increasing r. This leads to significant nonsinusoidal behavior, in that the field as a
                                     function of r/λ will oscillate, but with nonuniform periodicity, and with positive and
                                     negative amplitudes that differ in each cycle. Second, at distances r that are much
                                     greater than a wavelength, the second term in (21) dominates, and the field variation
                                     with r approaches that of a pure sinusoid. We may therefore say that, for all practical
                                     purposes, the wave at large distances, wherer >> λ,isa uniform plane wave having a
                                     sinusoidal variation with distance (and time, of course) and a well-defined wavelength.
                                     This wave evidently carries power away from the differential antenna.
                                        We should now take a more careful look at the expressions containing terms
                                                 3
                                                      2
                                     varying as 1/r ,1/r , and 1/r in Eqs. (10), (13a), and (13b). At points very close
                                                              3
                                     to the current element, the 1/r term must be dominant. In the numerical example
                                                                                 3    2
                                     we have used, the relative values of the terms in 1/r ,1/r , and 1/r in the E θs
                                     expression are about 250, 16, and 1, respectively, when r is 1 cm. The variation
                                                          3
                                     of an electric field as 1/r should remind us of the electrostatic field of the dipole
                                     (Chapter 4). The development of this concept is the subject of Problem 14.4. The
                                     near-field terms represent energy stored in a reactive (capacitive) field, and they do
                                     not contribute to the radiated power. The inverse-square term in the H φs expression
                                     is similarly important only in the region very near to the current element. It corre-
                                     sponds to the induction field of the dc element, as found through the Biot-Savart law
                                     (Problem 14.5).
                                        At distances corresponding to, say, 10 or more wavelengths from the current
                                     element, the product kr = 2πr/λ > 20π, and the fields dramatically simplify.
                                                                                       2
                                                                                                 4
                                     In Eqs. (14)–(16), the terms within brackets involving 1/(kr) and 1/(kr) can be
                                     considered much less than unity, and can be neglected. In addition, the phases (Eqs.
                                     (17) and (18)) all approach π/2. The effect is also seen in Eqs. (10), (13a), and (13b),
                                     in which all terms except the inverse-distance (1/r) term may be neglected. At such
                                     distances, at which kr >> 1 (equivalently r >> λ), we are said to be in the far-field
                                     or far-zone. The remaining field terms that have the 1/r dependence are the radiation
                                     fields. This produces an approximately zero E rs field, leaving only E θs and H φs . Thus,
                                     in the far zone:
                                                                .
                                                            E rs = 0
                                                                   I 0 kd
                                                            E θs = j    η sin θ e − jkr              (22)
                                                                   4πr
                                                                    I 0 kd
                                                            H φs = j    sin θ e − jkr                (23)
                                                                    4πr
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