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SOLUTION OF BASIC EQUATIONS OF ELECTRODYNAMICS                          167


                                                                                  (, )
            However, in general, it is known and defined by the given sources of electric current 
                                                                                 
            only. Finally, the vector equation (4.6) can be written as
                                           2           (,)
                                         1  (,)
                                2
                                ∇ (, ) −  −    = (, )                   (4.11)
                                                   0 
                                         2    2  
            In a similar manner, we obtain applying the ( x) operation to both parts of the second equation
            in (4.1)
                                       2
                                    1  (,)  (,)
                           2                                     (, )                   (4.12)
                          ∇ (, ) −  −    = − ×  
                                               0 
                                      2   2  
            The vector equations (4.11) and (4.12) are customarily called the wave equations. Note that
            each of them is equivalent to three (not six) scalar equations.
            4.1.2   Wave Equation in Space-Frequency Domain. Wavenumber.
            In Chapter 1 we showed that the time-frequency conversion comes to the replacement of the
            differentiation operator with the factor . Therefore, the second derivative in time domain
            must be equivalent to the  factor  ∙  = − .  Therefore, the  wave equations (4.11)  and
                                                   2
            (4.12) can be written as

                                          2
                               2
                             ∇ (, ) + ( −  )(, ) = (, )  �       (4.13)
                                                0 
                                       2
                           2
                          ∇ (, ) + ( −  )(, ) = − ×   (, )
                                            0 
                                                                
            Here  =   [(rad/s) ∙ (s/m) = rad/m] is called the wavenumber or propagation number and
                      ⁄
            one of the fundamental physical parameters characterizing the energy of EM waves. Indeed, let
            us recall the EM wave duality discussed shortly in Chapter 1 and 3. According to this principle,
            EM  wave can be considered as a flow of  N  photons  each carrying  the discrete portion of
                                                  ⁄
            energy    =  = ℎ. In the vacuum   =   = 2/  or  = /2. Then the single
                                  ℎ
            photon energy is    = � �  =  3.1615∙ 10 −26   [Joule]. Thereby, the energy carried by
                            
                                  2
            whole EM wave is equal to    = 3.1615 ∙ 10 −26 () and proportional to its wavenumber
            k. If so, the EM energy can  be directly  measured in  wavelengths at any  frequency as it is
            customary in the optical band.
            A quick look at (4.13) reveals that the  complex  number called the  complex propagation
            constant and denoted by symbol
                                       = � −   =  −         (4.14)
                                      �
                                            2
                                                          1
                                                  0 
                                                               2
            can be interpreted as the complex  wavenumber in the lossy medium ( ≠ 0). Since   is a
                                                                                   �
            complex number, EM waves should experience loss when they propagate. The loss level is
            defined by the attenuation coefficient  . Evidently, in (4.14)
                                           2
                                                         2
                                                              2
                                              4
                                   √2 = �� + (  ) +  ⎫
                                      1
                                                    0 
                                                               ⎪
                                                                                    (4.15)
                                                               ⎬
                                              4
                                                         2
                                   √2 = �� + (  ) −  2⎪
                                                    0 
                                      2
                                                               ⎭
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