Page 385 - Electromagnetics
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where ˜ p is the dipole moment defined by
                                                                  ˜
                                                                 Il
                                                           ˜
                                                       ˜ p = Ql ˆ p =  ˆ p.
                                                                 jω
                        That is, we consider a Hertzian dipole to be a “point source” of electromagnetic radiation.
                        With this notation we have

                                     ˜


                                    A e = ˜µ     jω˜ pδ(r − r p ) G(r|r ; ω) dV = jω ˜µ˜ pG(r|r p ; ω),


                                            V
                        which is identical to (5.87). The electromagnetic fields are then
                                               ˜
                                               H(r,ω) = jω∇× [˜ pG(r|r p ; ω)],                (5.88)
                                                        1
                                               ˜
                                               E(r,ω) =  c  ∇× ∇× [˜ pG(r|r p ; ω)].           (5.89)
                                                        ˜
                                             ˜
                                                    ˜
                        Here we have obtained E from H outside the source region by applying Ampere’s law.
                        By duality we may obtain the fields produced by a magnetic Hertzian dipole of moment
                                                               ˜ I m l
                                                          ˜ p m =  ˆ p
                                                               jω
                        located at r = r p as
                                               ˜
                                              E(r,ω) =− jω∇× [˜ p m G(r|r p ; ω)],
                                                        1
                                               ˜
                                              H(r,ω) =   ∇× ∇× [˜ p m G(r|r p ; ω)].
                                                        ˜ µ
                          We can learn much about the fields produced by localized sources by considering the
                        simple case of a Hertzian dipole aligned along the z-axis and centered at the origin. Using
                        ˆ p = ˆ z and r p = 0 in (5.88) we find that
                                                      ˜ I  e       1    1     k
                                                         − jkr
                                    ˜
                                                                     ˜
                                                                 ˆ
                                   H(r,ω) = jω∇× ˆ z   l      = φ    Il    + j  sin θe − jkr .  (5.90)
                                                     jω 4πr       4π    r 2   r
                        By Ampere’s law
                                       1
                            ˜                 ˜
                            E(r,ω) =      ∇× H(r,ω)
                                      jω˜  c
                                       η      2    2       − jkr   η      k   1     1       − jkr
                                         ˜
                                   = ˆ r  Il   − j    cos θe   + θ ˆ  ˜ Il j  +  − j   sin θe  .
                                      4π    r 2   kr 3            4π     r   r 2   kr 3
                                                                                               (5.91)
                                                                                    3
                        The fields involve various inverse powers of r, with the 1/r and 1/r terms 90 out-of-
                                                                                             ◦
                                        2
                        phase from the 1/r term. Some terms dominate the field close to the source, while others
                                                                              1
                        dominate far away. The terms that dominate near the source are called the near-zone
                        or induction-zone fields:
                                                        ˜ Il e − jkr
                                                      ˆ
                                           ˜ NZ
                                          H   (r,ω) = φ        sin θ,
                                                       4π r 2
                                                          ˜ Il e  − jkr
                                           ˜ NZ
                                                                           ˆ
                                          E   (r,ω) =− jη         2ˆ r cos θ + θ sin θ .
                                                          4π kr 3
                        1 Note that we still require r   l.
                        © 2001 by CRC Press LLC
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