Page 192 - Satellite Communications, Fourth Edition
P. 192

172  Chapter Six

                              an example of the improvements obtained, the conventional approach
                              to producing a CONUS beam requires 56 feed horns, and the feed
                              weighs 84 pounds and has a 1-dB loss. With a shaped reflector, a
                              single-feed horn is used, and it weighs 14 pounds and has 0.3-dB loss
                              (see Vectors, 1993).
                                Shaped reflectors also have been used to compensate for rainfall atten-
                              uation, and this has particular application in direct broadcast satellite
                              (DBS) systems (see Chap. 16). In this case, the reflector design is based
                              on a map similar to that shown in Fig. 16.8, which gives the rainfall
                              intensity as a function of latitude and longitude. The attenuation result-
                              ing from the rainfall is calculated as shown in Sec. 4.4, and the reflec-
                              tor is shaped to redistribute the radiated power to match, within
                              practical limits, the attenuation.


                              6.17 Arrays

                              Beam shaping can be achieved by using an array of basic elements. The
                              elements are arranged so that their radiation patterns provide mutual
                              reinforcement in certain directions and cancellation in others. Although
                              most arrays used in satellite communications are two-dimensional horn
                              arrays, the principle is most easily explained with reference to an in-line
                              array of dipoles (Fig. 6.26a and b). As shown previously (Fig. 6.8), the
                              radiation pattern for a single dipole in the xy plane is circular, and it is this
                              aspect of the radiation pattern that is altered by the array configuration.
                              Two factors contribute to this: the difference in distance from each element
                              to some point in the far field and the difference in the current feed to each
                              element. For the coordinate system shown in Fig. 6.26b, the xy plane, the
                              difference in distance is given by s cos   . Although this distance is small
                              compared with the range between the array and point P, it plays a cru-
                              cial role in determining the phase relationships between the radiation
                              from each element. It should be kept in mind that at any point in the far
                              field the array appears as a point source, the situation being as sketched
                              in Fig. 6.26c. For this analysis, the point P is taken to lie in the xy plane.
                              Since a distance of one wavelength corresponds to a phase difference of 2 ,
                              the phase lead of element n relative to n   1 resulting from the difference
                              in distance is (2 /l)scos . To illustrate the array principles, it will be
                              assumed that each element is fed by currents of equal magnitude but dif-
                              fering in phase progressively by some angle  . Positive values of   mean
                              a phase lead and negative values a phase lag. The total phase lead of
                              element n relative to n   1 is therefore

                                                               2
                                                                 s cos                   (6.36)
                                                               l
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