Page 234 - Maxwell House
P. 234

214                                                       ANTENNA BASICS


                                                                          3
        Here the binomial expansion was truncated since the terms proportional to � ⁄ �  and all the
                                                                        
                                                                        0
        followings quickly converge toward zero. Therefore, a good approximation for ∆  can be
                                                                             
        written as
                                                             2
                                                              2
                                ∆ = ( −  ) ≅  cos −  cos                    (5.26)
                                         0
                                                    
                                   
                                             1
                                                            2 0
        The presence of the quadratic term in (5.26) incredibly complicates the far field theoretical
        analysis as well the interpretation of far field graphs and measurements. So a compromise was
        made to start counting the far field zone or Fraunhofer’s region from the point where
                                              2     2
                                                 
                                         ≫  =
                                         0          �                        (5.27)
                                              2
                                        ∆ ≅  cos
                                                
                                          
        Note that in this zone
                     1   1      1       1                   1      1
                                                  
                       ≅              ≅  �1 − � ⁄ �cos� =  −  cos ≅        (5.28)
                                                   0
                                                
                               ⁄
                      1   0 1−�   0 �cos   0   0    2   0
                                                                 0
        Here in Taylor’s expansion (1 + ) −1  ≅ 1 −  we kept the zeroth- and first-order terms only.
        On the other hand, the emitting elements can be arranged not only along y-axis but be shifted
        also in the direction of x- or z-axis that creates additional phase shifts between the fields in far
        field zone. Using the same approach we obtain
                                                 2
                                               
                                           ≫             ⎫
                                           0
                                                2            ⎪
                                     ∆ ≅  cos =  sin  ∙ cos   (5.29)
                                                  
                                        
                                  
                               ∆ ≅  cos =  sin  ∙ sin⎬
                                                  
                                  
                                        
                                                             ⎪
                               ∆ ≅  cos  =  cos            ⎭
                                  
                                                  
                                        
                      2
                               2
                           2
        In (5.29)  = � +  +    while the total phase shift can be found as ∆ = ∆ + ∆ +
                                                                           
                               
                      
                                                                                 
                           
        ∆ . For example, one of the biggest steering radio telescope in the world built in Spain and
           
        has a parabolic dish of a 30-meter diameter. According to (5.29) the radiation pattern of such
        an antenna is fully formed at a distance beyond 27 km (!) at  = 10.5 cm.
        5.2.6   Radiation Pattern. Main Beam, Beamwidth, and Sidelobes
        An antenna can be isotropic or directional as shown in 5.2.6a and 5.2.6b, respectively. The
        isotropic  antenna as it follows  from its name radiates or receives EM waves of the same
        intensity in or from any direction of 3D-space. A good example of the isotropic radiator is the
        sun shining almost uniformly in all direction (horizontally and vertically). An ideal isotropic
        antenna is  an imaginative  fiction useful only as a reference radiation source in  antenna
        parameter definitions such as directivity and gain (see later). As it radiates uniformly in all
        directions, it is also called omnidirectional radiator and has a directivity of 1 (see definition of
        directivity later).
   229   230   231   232   233   234   235   236   237   238   239