This letter investigates the use of a backing cavity composed of a frequency selective surface (FSS) above a metal plate as a means to supress the backlobe radiation and increase the gain of an Archimedean spiral antenna which operates from 3 to 10 GHz. The FSS is designed to reflect signals in the upper band (7 -10 GHz) with a loss <0.25 dB, and allow transmission in the lower band (3 -6 GHz). Good impedance match and bidirectional to unidirectional beam transformation is obtained when the FSS and metal plate are inserted a distance /4 below the spiral at the centre of the upper and lower bands respectively. Simulated and measured radiation patterns are employed to show the performance enhancement which is attributed to the FSS reflector.
Introduction:The Archimedean spiral is a class of frequency independent antennas which generate circularly polarised bidirectional radiation with equal power in the upper and lower hemisphere [1]. Significant pattern distortion is often observed when low gain antennas strongly illuminate the platform on which they are mounted [2], therefore suppression of backlobe energy is desirable for applications that require unidirectional coverage. For planar spirals this is normally obtained by backing the antenna with a cavity containing an electromagnetic absorber. However a major disadvantage of this classical arrangement is that 50% of the radiated energy is dissipated in the load. A more efficient method, which can increase the antenna gain by 3 dB, is to insert a flat metal plate /4 distance below the radiating aperture. However this technique is only suitable for narrow band operation, therefore a wideband spiral would require the deployment of a more advanced ground plane architecture to reduce performance degradation in terms of impedance mismatch and high crosspolarisation [3] at low frequencies, and beam distortion at high frequencies [4]. In [5] the authors reported on a structure composed of eight unequal size metal rings placed one quarter wavelength below the corresponding active regions of an Archimedean spiral. Although the antenna was shown to work from 3 to 10 GHz, the 3D metal step arrangement used to suppress the backlobe radiation was complicated to manufacture and difficult to position precisely below the discrete active regions.In this paper we report on a much simpler cavity design which consists of a FSS that reflects strongly between 7 -10 GHz (upper band) and simultaneously allows transmission between 3 -6 GHz (lower band). The FSS and metal plate are inserted λ/4 (at 8.5 GHz and 4.5 GHz respectively) distance below the antenna, thus forming a cavity which effectively presents two stacked ground planes, one for each band. Unidirectional operation of the new configuration is demonstrated by comparing the predicted VSWR, gain, front-to-back (F/B) ratio, axial ratio and measured radiation patterns at the edges of the two bands, to the performance obtained from an identical unbacked spiral antenna.