Abstract. The spillover noise of a reflector antenna can be reduced by attaching a shroud extending forward from the edge of the reflector; the shroud prevents ground radiation from entering the feed. Symmetrical paraboloidal antennas of diameter 40 wavelengths, equipped with cylindrical and conical shrouds, are analyzed using the method of moments. A cylindrical shroud, parallel to the reflector axis, may reduce antenna noise, but it raises the sidelobe level in the front hemisphere substantially and can also reduce antenna gain. These drawbacks can be overcome by using a conical shroud, flared outward. Such a shroud reduces the spillover lobes in the back hemisphere, thus lowering the antenna noise temperature, but generates a conical sidelobe in the front hemisphere. The peak level of this sidelobe can be reduced by building the shroud using two cones of different flare angles or by curving its cross section. The decrease in noise temperature, as well as the location and level of the conical sidelobes in the front hemisphere, can be predicted to useful accuracy using geometrical optics. The addition of a shroud increases the level of cross polarization near the main beam. However, this effect is reduced if the sharp corner where the shroud joins the reflector rim is replaced by a smooth transition. The level of cross polarization is then at a level comparable to that produced by scattering from feedsupport struts.
IntroductionThermal radiation from the ground is one of the principal sources of noise in microwave systems using reflector antennas. Receiver noise can be reduced to 10 K or less using modern receiver technology, and ground noise can easily become the dominant contributor to system noise. In this paper we investigate the use of a cylindrical or conical shroud or fence, attached at the reflector rim, to reduce ground noise in paraboloidal antennas. The antennas we consider are symmetrical reflectors, fed at the prime focus, but our methods are applicable to many types of reflector antennas, and we reach quite general conclusions.The antennas which we discuss are paraboloids of diameter 8. MHz. This paper is the third in a series concerning the noise performance of these antennas at 1420 MHz. In the first paper, Anderson et al. [1991] analyzed the various contributions to the total antenna noise and showed that the most significant sources of noise are ground radiation reaching the feed directly over the edge of the reflector (spillover) and ground radiation scattered from the feed-support struts into the aperture; these two contributions are approximately equal. In the second paper, Landecker et al. [1991] analyzed scattering of ground radiation from the feed-support struts and showed how this source of noise could be reduced. In this paper we study methods for reducing spillover noise.Our study began experimentally. A cylindrical shroud of length I = 0.91 m was attached to the rim of one of the 8.53-m antennas, parallel to the antenna axis. Antenna temperature at 1420 MHz was reduced substantial...