1. Field of the Invention
This invention relates generally to large aperture lightweight antennas. Such antennas are especially suited for use on lighter than air platforms. More particularly, this invention is especially well suited to provide inflatable and collapsible transreflector antennas.
2. Related Art
Lighter-than-air (LTA) vehicles such as manned airships (blimps), unmanned airships, or tethered aerostats have been used as platforms for radar and radio communication relays. However, since LTA lift capacity is reduced as the vehicle operates at higher altitudes, LTA vehicles require extremely lightweight antenna systems to function in this role at very high altitudes. Adding to the complexity of such antenna installations is the requirement for ballonets, or buoyancy control systems, to control the lifting force and allow controlled ascent and descent of the LTA vehicle. As the maximum altitude of the LTA increases, these ballonets occupy a larger fraction of the total volume within the LTA envelope. Ideally, the antenna would be collapsed or folded when the LTA is at low altitude (ballonets fully expanded) and the antenna would be fully deployed when the LTA is at high altitude (ballonets fully collapsed).
Scanning antennas utilizing transreflectors of spherical, parabolic, elliptical, or other toric sections are described in U.S. Pat. No. 2,835,890—Bittner, U.S. Pat. No. 2,989,746—Ramsay, and U.S. Pat. No. 4,214,248—Cronson et al. However, these antennas are not designed to be collapsible, are fabricated from thick metal rods or wires, or are comprised of multiple singly curved, reflective/transmissive surfaces. An inflatable spherical reflector is described in U.S. Pat. No. 4,364,053—Hotine but it is not collapsible nor capable of 360 degree scanning. A planar inflatable/collapsible antenna is described in U.S. Pat. No. 5,132,699—Rupp.
Although no published documentation is presently in hand, it is also believed others have previously recognized that an RF reflective conductive surface can have a thickness less than one RF skin depth.
A collection of possibly relevant prior art documents are identified below:
This invention provides, among other things, an exemplary embodiment using a transreflector-based antenna that is inflatable and which can be collapsed when not in use. This substantially eases integration of the antenna into an airship which can be the primary antenna platform. Several other types of inflatable antennas (including one spherical reflector, e.g., see U.S. Pat. No. 4,264,053—Hotine) are described in the prior art, but none are designed to be collapsible and have wide scan (e.g., 360-degree) capabilities.
Another feature of an exemplary embodiment of this invention is a possibly reinforced thin-film, single-wall spherical reflector construction with a thin metallized linear transreflector grating pattern. The metallized strips of the grating preferably have a width that is about half their center-to-center spacing which is, in turn, much less (e.g., <⅛) the shortest RF wavelength to be utilized by the antenna. This provides an extremely lightweight implementation for a transreflector.
In an exemplary embodiment, the metallization of the grating pattern can be much thinner than the RF current skin depth at a particular frequency to help minimize the transreflector weight.
An exemplary antenna capable of scanning a pencil beam through 360 degrees in azimuth and limited scan in elevation includes a stationary (with respect to a platform) transreflector, which may be an annulus of an inflatable/collapsible sphere. The surface of the sphere includes a thin, non-metallic film with thin, flexible metallization in a linear grating pattern oriented at 45 degrees with respect to the equator and increasing inclination with respect to the latitudes of the sphere as the grating “lines” approach the poles. A folding RF feed system can be used to illuminate a portion of the annulus as the feed system rotates about a concentric focal sphere or spherical annulus (whose radius is approximately half the transreflector sphere radius). The movable feed can produce an illumination pattern that is shaped to maximize gain and minimize sidelobes and to radiate with a polarization vector which is parallel to the reflective grating.
The preferred exemplary transreflector maintains a spherical shape owing to internal inflation gas pressure and the shape of the thin film membrane used to construct the transreflector surface. When this pressure is relieved, the reflector collapses around the feed system (which may also be folded for minimum total collapsed antenna volume).
The preferred exemplary folding RF feed system may provide a plurality of illuminating RF beams, possibly at differing radio frequencies. Such a plurality of beams may be utilized to increase the effective scan rate for a given feed system rotation rate or to decrease the feed system rotation rate for a given scan rate. In one exemplary embodiment, a turntable system of rotating feeds with constant rotation rate provides a surveillance function at one (lower) frequency while a separate set of independently steerable feeds positioned radially from the sphere center can provide dedicated tracking of a number of targets at a higher frequency. As the optimum feed radius decreases with increasing radio frequency of illumination, the two sets of feeds may avoid collision with each other. Each feed of an exemplary embodiment of the invention may be any of either horn, dipole, patch, notch, waveguide aperture, array or other radiator element whose polarization can be oriented at approximately 45 degrees with respect to the sphere's equator.
An exemplary embodiment of this invention allows the antenna to be readily collapsed to a much smaller volume than when in the fully deployed state, permitting the antenna to share the fully deployed volume when not in use with other structures that may be required for a vehicle which carries such an antenna. Since inflatable structures tend to approach a spherical shape, the single-wall inflatable sphere is the simplest and lightest shape for a stationary 360 degree scanning reflector antenna. The thin film sphere and thin grating metallization allows for an exceedingly lightweight structure that is much lighter than other transreflector shapes and construction methods to provide scanning capability over 360 degrees.
A presently preferred exemplary embodiment of this invention uses an inflatable-collapsible, spherical reflector antenna (specifically, a transreflector which substantially reflects RF waves from one internal side and which is substantially transparent to RF waves at an opposing side). The spherical transreflector 10 approximates an ideal parabolic shape over a limited portion 12 of the sphere that is illuminated by the feed(s) 14 (i.e., RF ports) as shown in
The beam is steered by moving the feed relative to the reflector rather than by moving the entire antenna structure (i.e., feed plus reflector) as is commonly done for conventional parabolic reflectors. An exemplary embodiment is used as a search radar antenna wherein scanning can be accomplished by sweeping the feed across the reflected image of the searched region. Since the transreflector is stationary (relative to the supporting antenna platform), it can be made from extremely lightweight RF transparent films (e.g., Mylar or other similar material).
An exemplary transreflector surface can be constructed as an inflatable sphere using thin, non-metallic film with patterned, thin metallization strips 20 (as shown in
As will be appreciated by those in the art, because it is an RF reflecting surface and not an RF current conducting surface, the metallization film traces can be much thinner than the RF current skin-depth required for low-loss transmission lines, further minimizing weight. However, the surface resistance of the metallization should be as low as possible for maximum grating efficiency.
To form a spherical inflatable surface, typically, specially cut pieces (or “gores”) of flat material are used to create the doubly curved spherical surface (e.g., just like a basketball is sewn together from flat gores, e.g., see
The scan capability of the exemplary system is unlimited in the azimuthal plane (the sphere's equatorial plane), while scanning in the elevational plane is limited by non-ideal orientation of the grating lines at opposite sides of the sphere which limits transreflector efficiency. A near-ideal grating orientation is only achieved when the beam is scanned along the sphere's equator. However, the grating orientation can be adjusted, if desired, at locations away from the equator to more closely achieve the desired orthogonality between the grating on reflection and transmission sides of the sphere when the beam is scanned away from horizontal. The polar caps of the sphere may be left free of metallization to reduce weight or one polar cap (typically the top) may be completely metallized while the opposite polar cap can be left free from metallization to allow expanded elevation scanning, even to vertical.
The exemplary transreflector 10 maintains a nearly spherical shape (as shown in
An advantage of the exemplary reflector design is that it can be quite broad-band, a capability that can be exploited by adding separate feeds at different frequencies or by using wideband feeds. For maximum efficiency over a wide frequency range, the center-to-center spacing of the grating strips should be a small fraction (e.g., <⅛) of the shortest RF wavelength used. This is schematically depicted by an <λ/8 arrow which also serves to indicate the grossly exaggerated scale of the grating as depicted in
To support and scan the feeds within the spherical transreflector, several different exemplary embodiments are described. The first exemplary embodiment uses feeds mounted on radial boom(s) 40 from the center of the sphere as shown in
As shown in
The exemplary embodiments so far described employ a large-aperture spherical transreflector with separate movable point feeds and, optionally, a multi-beam array feed. As depicted in
Another advantage of the exemplary transreflector design is that it is quite broad-band, a capability that can be exploited by adding separate feeds at other frequencies or adding high-range-resolution waveforms such as in combat ID modes. These capabilities also help in providing clutter and ECM resistance.
To produce high-gain radar beams, scannable over 360° in azimuth, a spherical transreflector is used, similar to the parabolic dome antenna suggested in 1953 [1] and built in 1956 [2]. As shown in
As earlier noted, we have determined that a spherical transreflector is our preferred shape. One reason is reduced gain loss with scan. Another reason is that to get a non-spherical shape using inflatable technology requires a lenticular construction resulting in a true torus (donut) shape. This would be heavier (requiring sturdy rings at top and bottom and a means to maintain precise separation of the rings) and be more complicated to build and deploy. The spherical transreflector suffers only slightly in terms of peak gain, has much wider scan capability, is lighter and easier to fabricate than non-spherical shapes. Nevertheless, in cases requiring limited elevation scanning, a non-spherical toroidal shape may be preferred.
Some background and underlying rationale for our conclusion regarding a preferred spherical shape for the transreflector are set forth below. In the following section, UHF band (500 MHz) applications are assumed. It may be desirable to choose a higher frequency such as L-band (1 GHz) in other designs. All that is required for changing or adding frequencies is to change or add feed horns (or broader-band feeds) for the desired frequencies.
The primary issues for this antenna may be associated with (1) finding a reflector shape with good wide-angle focusing ability, (2) designing an efficient wide-bandwidth transreflector grating, and (3) providing sufficient surface accuracy with an inflatable structure.
To achieve 360° of azimuthal coverage, the reflector must be a surface of revolution in azimuth. Limited elevation scanning allows more freedom in choosing the shape. Let us first compare the focusing ability of a parabola and a circle. In the vertical plane, a circular cross section may still be desirable for ease of fabrication and lighter mass as previously mentioned. A variety of options for the shape of the vertical plane of the reflector may be considered.
The focusing characteristics of a parabola and circle can be compared by geometric ray tracing. First consider a focus-fed parabola.
For a compact reflector (F/D<0.5), the scan range is limited to a few beamwidths. Larger values for F/D would increase the scan range, but be less compact and require bigger feeds to efficiently illuminate the small angular extent of the reflector.
Now consider a circle fed from a point near its half radius.
(F/D)min−0.18*(R/?)0.25 (1)
For a 10-meter-radius circle, the minimum useful F/D at 500 MHz is about 0.36. This low value of F/D means that a large portion of the circle can be used (the result of this calculation is shown in the next section). One advantage that the circle has over any other curve is that the wave can be scanned without further degradation of the phase front.
The preferred curvature in the vertical plane depends on how far the beams need to be scanned in elevation. For the HAA application, since the radar is at high altitude, significant elevation scanning may be required, depending on the mission. Without scanning it might appear that a parabola is best, while significant scanning would favor the circle. However, somewhat surprisingly, even without a requirement to scan in elevation, an ellipse is slightly better than the parabola due to lower diagonal plane phase errors [6]. The next section will quantify these tradeoffs.
This section compares the beamforming performance (directivity) between spherical and parabolic-torus reflectors, as computed by a geometric optics code obtained from C. J. Sletten [7].
To maximize computation speed, only the most heavily illuminated portion of the reflector was modeled (the circular region within the 0 to 10 dB range), shown as D in
The feed pattern was assumed to have a cosm(θ) pattern variation. Changing parameter “m” varied the size of the illuminated aperture, D. In general, increasing D leads to a larger effective aperture and higher directivity until the maximum phase error exceeds about 90°, when the directivity tops out and then begins to decrease.
For a specific case, first consider a spherical reflector fed from the optimum point slightly outside the half-radius. At UHF, due to lower phase errors, the optimum value of D is about 12 meters, which is predicted by Equation 1. The directivity is plotted against effective illuminated aperture diameter for a variety of sphere sizes in
The optimum feed point for the sphere used in computing the directivity changes with frequency. This provides a convenient means of avoiding collision between feeds operating in different bands.
In this section, computed antenna patterns for a spherical reflector are given to show that phase errors do not pose a significant limitation on sidelobe level. Here the entire reflecting half of the transreflector (modeled as a solid reflector) is used in the computations to ensure that all phase error effects are accounted for. This is a hemisphere with the poles trimmed off by planes at ±6 meters from the equator. All of the computations presented here used a physical optics code modified from one obtained from D. Paolino of NAWC [9].
For a military application where an interference nulling array might be used, we are more concerned with the average sidelobe level [11]. An estimate of the average sidelobe level can be obtained by assuming that whatever power is not in the main beam must be in the sidelobes.
SLLavg=10 log10[4π(1−Pbeam)/(4π−Abeam)]dBi (2)
where
Now consider gain patterns at 500 MHz. Assume a two-element end-fire array of half-wave dipoles spaced by 0.20 λ oriented for 45° linear polarization. The computed reflector gain patterns over the azimuth, elevation, and diagonal planes are shown in
Aperture blockage will reduce the gain and increase the sidelobe levels. A first-order estimate of this effect can be computed by subtracting the fields radiated by the blocked portion of the aperture [12]. The effect of blockage is very small until it exceeds about 5% of the effective aperture. From the computed directivity for the 20-meter-diameter spherical reflector, 5% of blockage equates to 4.5 m2 at UHF.
A conservative first-order estimate of the maximum number of feeds that can be accommodated by the reflector can be calculated using the cross-sectional area of the transmission lines leading to the feeds. The feed support structure can be neglected since the supports can be built from non-metallic materials designed for low blockage. The coax transmission lines will have widths of about 2.5 cm at UHF. Assuming a direct path from the feed across the aperture, each feed line would contribute about 0.15 m2 of blockage at UHF, using a 12-meter-diameter aperture. The maximum number of feeds for less than 5% blockage is on the order of 30 beams for UHF. We note that radially supported feeds tend to exhibit more deleterious pattern effects due to the concentration of blockage in the center, or peak amplitude, portion of the antenna pattern.
While the invention has been described in connection with what is presently considered to be the most practical and preferred embodiments, it is to be understood that the invention is not to be limited to the disclosed exemplary embodiments, but on the contrary, is intended to cover various modifications and equivalent arrangements included within the spirit and scope of the appended claims.
This non-provisional application claims the priority benefit under 35 U.S.C. § 119(e) of provisional application 60/516,280 filed Nov. 3, 2003 (entitled LARGE-APERTURE, LIGHTWEIGHT ANTENNAS FOR LIGHTER-THAN-AIR PLATFORMS) the entire content of which is hereby incorporated hereinto by reference.
Parts of this invention were described in a February 1996 proprietary proposal to a Federal agency by Toyon Research Corporation. Parts of this invention were also described in a related February 1998 report by Toyon Research Corporation with “Distribution limited to U.S. Government agencies only/Test and Evaluation; February 1998. Other requests for this document must be referred to Commander, U.S. Army Missile Command, Attn: AMSMI-RD-WS-DP, Redstone Arsenal, Ala. 35898-35248.” This report covered studies by Toyon sponsored by Defense Advanced Research Projects Agency (Information Technology Office), DARPA Order No. E175101, issued by U.S. Army Missile Command Under Contract No. DAAH01-96-C-R203.
Number | Date | Country | |
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60516280 | Nov 2003 | US |