The present invention relates generally to satellites, and more particularly, to electrically large, circularly symmetric, stepped-wall and smooth-wall, direct-radiating horn antennas for use in satellite spot beam applications.
Electrically-small smooth-wall horns have been used as feeds for reflector antennas. In particular, smooth-wall horns have been used as feed elements in satellite-based, multi-beam systems that employ array-fed, single offset reflectors. Advantages of smooth-wall horns include their compact size, low mass, high aperture efficiency, and ease of manufacture. The horn aperture for such multibeam applications typically measures less than about 6.5 wavelengths in diameter over the operating band, with maximum peak horn directivity less than 26 dBi.
A number of patents and open literature papers describe the use of profiled, smooth-wall horns for low-gain applications as feeds for reflector systems. However, it is believed that no spline-profiled, smooth-wall nor spline-profiled stepped-wall horn has heretofore been used to generate direct-radiating high-gain spot beams.
Exemplary patents and papers relating to profiled, smooth-wall horns for low-gain applications include U.S. Pat. No. 6,396,453 issued May 28, 2002, to Amyotte et al., U.S. Pat. No. 6,384,795 issued May 7, 2002 to Bhattacharyya et al., U.S. Pat. No. 7,183,991 issued Feb. 27, 2007 to Bhattacharyya et al., U.S. Pat. No. 7,463,207 issued Dec. 9, 2008 to Rao et al., along with papers entitled “A Smooth-Walled Spline-Profile Horn as an Alternative to the Corrugated Horn for Wide Band Millimeter-Wave Applications” by Christophe Granet, et al., IEEE Transactions on Antennas and Propagation, Vol. 52, No. 3, March 2004, “Optimized Spline-Profile Smooth-Walled Tri-Band 20/30/44-GHz Horns” by Christophe Granet, et al., IEEE Transactions on Antennas and Propagation, Vol. 6, 2007, “A Novel Horn Radiator With High Aperture Efficiency and Low Cross-Polarization and Applications in Arrays and Multibeam Reflector Antennas” by Arun K. Bhattacharyya, IEEE Transactions on Antennas and Propagation, Vol. 52, No. 11, November 2004, “Comments and Replies” by Arun K. Bhattacharyya et al. and Kwok Kee Chan, et al., IEEE Transactions on Antennas and Propagation, Vol. 56, No. 8, August 2007, “Design of High Efficiency Circular Horn Feeds for Multibeam Reflector Applications” by Kwok Kee Chan, et al., IEEE Transactions on Antennas and Propagation, Vol. 56, No. 1, January 2008. Other papers include “A Compact Multi-Flare Born Design for Spacecraft Reflector Antenna,” by C. H. Chen et al., Antennas and Propagation Society International Symposium, 1986, Vol. 24, pages 907-910, “A Square Multiflare Horn with 1-megawatt CW Power-Handling Capability,” by Dan Hoppe, Microwave and Optical Technology Letters, Vol. 2 No. 11, November 1989, “Antenna System Supporting Multiple Frequency Bands and Multiple Beams,” by Sudhakar K. Rao, et al. IEEE Transactions on Antennas and Propagation, Vol. 56, No. 10, October 2008, “Smooth-Walled Spline-Profile Ka-Band Horn covering both the full commercial and Military Bands,” by Christophe Granet, et al., Microwave and Optical Technology Letters, Vol. 50 No. 8, November 2008, and “The Electrical Characteristics of the Conical Horn-Reflector Antenna,” by J. N. Hines, et al., available from the NASA Astrophysics Data System. Another paper relevant to this invention is “Monotone Piecewise Cubic Interpolation” by F. N. Fritsch et al, published in Siam J. Numer. Anal., Vol. 17, No. 2, April 1980.
The problem addressed by the present invention is the generation of high-gain spot beams with linear or circular polarization using an antenna having low mass, small volume, simple construction, high reliability. Prior art solutions have used empty conical or pyramidal tapered horns, conical or pyramidal horns with a larger flare angle and with a dielectric lens inserted in the aperture for phase correction, small reflector/feed combinations, or waveguide slot arrays.
In view of the above, it would be desirable to have electrically large, circularly symmetric, stepped-wall and smooth-wall, direct-radiating horn antennas for use in satellite spot beam applications.
The various features and advantages of the present invention may be more readily understood with reference to the following detailed description taken in conjunction with the accompanying drawing figures, wherein like reference numerals designate like structural element, and in which:
a illustrates another view of the stepped-wall horn antenna shown in
b illustrates a side view of the stepped-wall horn antenna shown in
c illustrates a partially cutaway view of the stepped-wall horn antenna shown in
d illustrates an enlarged portion of a stepped wall tapered section of the stepped-wall horn antenna shown in
a is a graph that illustrates monotonicity properties of PCHIP spline versus a standard cubic spline;
As was mentioned above, electrically small smooth-wall horns are commonly used as feeds for reflector antennas. Disclosed herein are improvements over such electrically small smooth-wall horns in the form of electrically large, profiled, high directivity, stepped-wall and smooth-wall horn antennas that may be used onboard satellites as direct radiators for generating spot beams. Such electrically large, profiled, high directivity, stepped-wall and smooth-wall horn antennas may be used in single-band and multiple-band applications, such as antennas employed on satellites, for example. For the purposes of the present invention, the electrically large aperture diameters of the electrically large stepped-wall or smooth-wall horns are greater than 10 free space wavelengths.
More particularly, discussed below is another useful application for spline-profile, stepped-wall and smooth-wall horns as direct radiating antennas for generating high-directivity spot beams. Such applications can require horn apertures as large as 24 or more wavelengths with peak directivities exceeding 36 dBi.
Referring to the drawing figures,
The exemplary electrically large stepped-wall horn 10, or horn antenna 10, shown in
The stepped-wall or smooth-wall tapered section 13 has a predetermined profile that is designed to achieve an electrically large, high directivity horn 11. In particular, the stepped-wall or smooth-wall tapered section 13 of the electrically large smooth-wall horn antenna 10 preferably has a spline-shaped profile.
The spline-shaped profile is monotonic in the sense that the radius (or equivalently, the diameter) of the horn never decreases as one traverses the profile from input port 11 to output port 14. Maintaining a monotonically nondecreasing horn profile is useful for the following reason: If the diameter were not constrained to be nondecreasing, one could encounter a situation where a large diameter region is located between two small diameter regions. Such a region could support one or more propagating modes that can not propagate in the surrounding regions—a form of resonant cavity. Trapped modes in such regions can give rise to very undesirable “spikes” and “glitches” in horn performance.
A spline profile is fully characterized by a set of discrete knot z locations (where z is the axial distance measured along the horn profile) and corresponding radii at the knot locations, as shown by the black dots in
The horn profile is optimized so as to meet total length, return loss, and radiation pattern goals. The radiation pattern goals include edge of coverage directivity, cross-polarization suppression, pattern taper and other desired pattern properties of interest.
The basic parameterization of the horn 10 is smooth (a PCHIP spline). When the horn 10 is manufactured, sometimes the horn inner surface is preferably fabricated as a smooth surface of revolution using the smooth spline as the generating curve, but sometimes using a stepped approximation to the underlying smooth parameterization. Typically the steps are small, approximately 1/30 of a wavelength at the highest operating frequency, although that is not required.
For spot beam applications, horns 10 having size ranging from about 11 wavelengths in diameter at the lowest frequency for one application, to as large as 24 wavelengths in diameter at the highest frequency for another, different application have been developed by the assignee of the present invention. It is believed that the use of spline-profile, stepped-wall and smooth-wall horns 10 with apertures this large has heretofore not been used in the satellite communication art.
The design methodology for generating the horn profile is discussed below.
Horn Parameterization.
The horns 10 under consideration are bodies of revolution about the z-axis. The interior surface of the horn 10 is therefore completely characterized by the generating function, or horn profile function ρ=f(z), where ρ is the radius of the inner surface of the horn wall, and z is distance measured along the axis of the horn. The z=0 plane is chosen to coincide with the horn aperture plane, and the positive z direction is taken to be out of the horn, so that the body of the horn 10 lies in the z<0 half-space. The horn radius profile is represented as a PCHIP spline consisting of N spline sections (or horn sections) bounded by N+1 knots. For example, in
Horn Optimization.
The particular values for the horn parameters are determined by numerical optimization of an objective function similar to that described by K. K. Chan and S. K. Rao, “Design of high efficiency circular horn feeds for multibeam reflector applications,” IEEE Trans. Antennas Propagation, vol. 56, no. 1, pp. 253-258, January 2008, where departures from various performance goals (return loss, directivity, cross-polarization depth, etc.) evaluated at discrete optimization frequencies are squared, weighted, and added together to form the objective or cost function. To analyze the performance of a candidate horn 10, various techniques are available, such as mode matching, method of moments, finite difference time domain (FDTD), finite elements, as described in the previously cited references, and in the open literature.
The performance goals for this single-band design are shown in Table I. This horn 10 was optimized at 3 discrete frequencies using 22 horn sections. The profile of the 22-section horn 10 designed for this application is shown in
The length and aperture inner diameter of the horn 10 are 25.46 inch and 9.4 inch, respectively, or approximately 65λmin and 24λmin (λmin being the wavelength at the highest frequency, 30 GHz). The inner surface of the horn 10 was manufactured as a stepped structure with constant steps in radius of approximately 0.01 in or λmin/40.
Table II below shows knot coordinates for the exemplary single-band horn 10 whose profile is illustrated in
A comparison of the measured and predicted return loss is presented in
Peak directivity of the horn was estimated from the measured pattern cuts via numerical integration. The results are compared to predictions in
Dual-Band Design.
The performance goals for the design of this dual-band horn 10 are shown in Table III.
The profile of the 20-section horn 10 designed for this application is shown in
Table IV below shows knot coordinates for the exemplary dual-band horn 10 illustrated in
As was mentioned above, the disclosed horns 10 generate high-gain spot beams.
Reduced-to-practice profiled horns 10 are much shorter (and therefore have lower mass and volume) compared with prior art (empty) conical or pyramidal horns. The horn 10 is much simpler, less massive and less expensive than a conventional horn with a dielectric lens, and is much simpler and less expensive than a horn/reflector combination. Compared to a waveguide slot array, the horn 10 is much simpler, and can support multiple frequency bands, dual simultaneous polarization, of either linear or circular polarization. Waveguide slot arrays are very narrow band, single-band, single-polarization antennas.
In summary, compared to conical horns, the electrically large smooth-wall horn 10 has a spline-profile shape. A novel parameterization of the horn profile is used that guarantees monotonicity of the profile radius versus axial length of the horn 10 during the numerical optimization process used to arrive at the horn profile. This monotonicity property is desirable since it precludes the existence of any regions of the horn 10 that could support trapped modes, which can cause undesirable return loss and directivity spikes. The other novel feature is the large electrical size of the horn aperture 14, particularly one used in a spot beam application. For example, aperture diameters exceeding 24 wavelengths have been successfully designed, built, and tested by the assignee of the present invention.
The disclosed horns 10 are direct radiating horn antennas 10 that produce high gain spot beams having linear or circular polarization. The horns 10 have stepped- or smooth-wall spline profiles generated using an algorithm and optimization procedure that ensures monotonicity to avoid trapped modes. The horns 10 preferably have electrically-large aperture with diameters typically a 10 free space wavelengths to provide for high gain. The horns 10 have a much shorter physical length compared with conventional horns (conical/multi-flare/multi-step) of the same aperture size and are thus more desirable for use on a satellite 20. The horns 10 have a lighter weight and ease of manufacturing (compared with conventional corrugated horns and horn reflector antennas). The horns 10 have high aperture efficiency. Reduced-to-practice horns 10 exhibit low cross-polarization in the intended coverage area hence high copolarization to cross-polarization ratio. The horns 10 may be single-band or multiple-band.
Thus, electrically large stepped-wall and smooth-wall horns for use in satellite spot beam applications have been disclosed. It is to be understood that the above-described embodiments are merely illustrative of some of the many specific embodiments that represent applications of the principles of the present invention. Clearly, numerous and other arrangements can be readily devised by those skilled in the art without departing from the scope of the invention.