Page 41 - Radar Technology Encyclopedia
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antenna gain                                                                        antenna, horn   31



                              G  =20logF                        bandwidth can be increased by 10 to 1 if the helix is wound
                                dB
           SAL                                                  on the surface of a cone with spacing between the turns
           Ref.: Johnson (1984), p. 1.5; Skolnik (1990), p. 7.2; Barton (1988), p. 166.  increased logarithmically with the turn diameter. Beamwidths
                                                                up  to 90°  are typically obtained. Helices have  higher gain
           A Gregorian (reflector) antenna is a reflector antenna with
                                                                than spiral antennas, relatively lower dissipation losses, but
           two concave mirrors (Fig. A57). The main mirror is of para-
                                                                their structure is larger than spiral antennas. SAL
           bolic  shape, and  subreflector has elliptic  shape. One of the
                                                                Ref.: Saad (1971), vol, 2, p. 48; Johnson (1984), p. 13.1; Schleher (1986), p.
           foci, F , of the subreflector is located at the focus of the main  480.
                1
           mirror. The phase center of the feed is placed in the second
                                                                A high-gain antenna is one with relatively high gain (tens of
                                                                decibels) in the main lobe. These are necessarily directional
                        Paraboloidal
                        main                                    antennas, which can be of the array or aperture type.
                         reflector                              Ref.: Johnson (1993), p. 1.15.
                                                                A “honey” antenna is a broad-beam biconical horn antenna
                    Other focus                   Ellipsoidal
                    of ellipsoid, F                subreflector  that provides an omnidirectional pattern in the azimuth plane.
                          2
                                                                It is formed by a biconical horn. Outputs with amplitudes pro-
                                                                portional to the sine or cosine of the signal’s angle-of-arrival
                                                                over the 360° azimuth coverage are formed by specially com-
                                                                bining four probes at the bottom of the feed. The main range
                                                  Plane
                     Focus of                     wavefront     of application is direction-finding and electronic warfare sys-
                      paraboloid F
                           ,
                             1                                  tems. SAL
                                                                Ref.: Johnson (1993), p. 40.2; Schleher (1986), p. 479.
                                                                A horn antenna is a directional antenna made as an exten-
                                                                sion of the waveguide feeding the horn, in a manner similar to
             Figure A57 Dual-reflector Gregorian antenna.       the wire antenna. Antenna directivity increases as horn aper-
                                                                ture increases and as the angle of the horn decreases (e.g., the
                                                                length of the horn increases). The most popular types of horns
           focus, F , of the ellipse. The waves going from the feed illu-
                  2
           minate the subreflector, are focused in the point F  and travel  are pyramidal, diagonal,  conical, and corrugated conical
                                                   1
           to the main reflector, creating an in-phase front in its aperture.  (Fig. A59).
           Typically, this  type of antenna is used in electrically large
           reflector antennas, as used in tracking radars and radar astron-
           omy. AIL
           Ref.: Johnson (1993), pp. 17.33–17.46; Sazonov (1988), p. 387.
           A helical antenna is a broad-beam antenna typically consist-
                                                                                 (a)                (b)
           ing of  a helix radiator  that resembles an uncoiled watch
           spring (Fig. A58). The polarization of radiated waves is circu-
           lar, and the direction of radiation is along the axis of the helix
           when the circumference of the helix is nominally one wave-
           length. For a typical helix with constant diameter, the band-
           width ratio is about 1.5 to 1, the gain is the function of the
           number of turns and is about 10 dB for a 6-turn helix. The
                                                                               (c)                  (d)


                                                                  Figure A59 Common types of horn antennas: (a) pyramidal
                                                                  horn; (b) diagonal horn; (c) conical horn; (d) corrugated horn
                                                                  (after Currie, 1987, Fig. 12.12, p. 539).

                                                                    The pyramidal  horn is  one of the most  common struc-
                                                                tures, as it can be made cheaply from the flat pieces of metal
                                                                that are cut along the straight lines. Its gain G  is equal to
                                                                                                    p
                                                                               [
                                                                        G   =  10 1.008 +  log ( a × b )] L +–  (  L  )
                                                                          P               l  l     E   H
                                                                where a  and b  are the aperture dimensions in wavelengths
                                                                             l
                                                                       l
              Figure A58 Helix antenna (after Macnamara, 1995, Fig. 5.18,   l , and L and L  are the losses in decibels due to phase error
                                                                       E
                                                                             H
              p. 161).
                                                                in the E and H planes as given in Fig. A60.
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