This disclosure relates to horn lens antennas.
Horn antennas, also known as microwave horns, include a flaring metal waveguide shaped like horn that directs radio waves in a beam. Horn antennas have multiple uses, including small-aperture antennas to feed reflectors to large-aperture antennas used by themselves as medium-gain antennas.
The performance of horn antennas is based on the shape and size of the horn. When designing the horn antenna, other considerations are taken into account, such as the fluctuation in temperature, humidity, dust and impurities in the surrounding air and other related factors. These factors affect the propagation of the signals. Therefore, to achieve a better signal, the antenna is designed to provide high gain. High gain generally implies that the antenna size is large. In some examples, size requirements prevent designing the antenna according to the needed size to achieve the required gain. In such instances, other adjustments to the design are considered.
One aspect of the disclosure provides an antenna that includes a receiver, a horn, a lens, and an anti-reflection layer. The horn has a first end disposed on the receiver and a second end defining an aperture positioned opposite the receiver. The lens is disposed within the aperture of the horn and has a first surface facing inward toward the receiver and a second surface opposite the first surface and facing outward away from the horn. The anti-reflection layer includes a dielectric material and is disposed on the first surface of the lens. Moreover, the anti-reflection layer defines holes arranged in a 50/50 material to void ratio and that have a thickness of a quarter wavelength of a signal received by the antenna.
Another aspect of the disclosure provides a method of making a horn antenna, the method includes: forming a lens having a first surface and a second surface opposite the first surface; forming an anti-reflection layer having a dielectric material; disposing the anti-reflection layer on the first surface of the lens; and positioning the lens within an aperture defined by a horn. The anti-reflection layer defines holes arranged in a 50/50 material to void ratio and has a thickness of a quarter wavelength of a signal received by the antenna. The horn has first and second ends, where the first end receives a receiver and the second end defines the aperture. The lens is positioned so that the first surface of the lens faces the receiver.
Implementations of the disclosure may include one or more of the following features. In some implementations, the horn defines a frustoconical shape, a pyramidal shape, an h-plane sectoral shape, or an E-shape sectoral shape. The anti-reflection layer may be integral with the lens. In such cases, the lens defines the holes in its first surface facing the receiver, where the holes have a depth equal to the thickness of the anti-reflection layer. Moreover, the holes may have a diameter of less than or equal to a tenth of the wavelength of the signal received by the antenna. In some examples, the lens and the anti-reflection layer is a cross linked polysterene microwave plastic or a Polytetrafluoroethylene. Other materials are possible as well. The second end of the horn may define a groove configured to receive the lens. The horn may define a frustoconical shape having a flare angle of about 45 degrees.
In some examples, the holes of the anti-reflection layer have one or more of a circular cross-sectional shape, a square cross-sectional shape, a diamond cross-sectional shape, an oval cross-sectional shape, or a rectangular cross-sectional shape. The holes may be arranged in a two-dimensional array.
The details of one or more implementations of the disclosure are set forth in the accompanying drawings and the description below. Other aspects, features, and advantages will be apparent from the description and drawings, and from the claims.
Like reference symbols in the various drawings indicate like elements.
A horn antenna gradually transitions waves from a tube into space allowing the impedance of the tube to match the impedance of free space. Referring to
The horn 110 may be flared at a constant flare angle θ or exponentially. The pyramidal horn 100b defines a four-sided pyramid (sides S1, S2, S3, S4) having a rectangular cross section where the parallel sides S1 and S3 have a greater length than the other parallel sides S2 and S4. All sides of the pyramidal horn 100b are flared. The pyramidal horn 100b is used with rectangular waveguides and radiates linearly polarized radio waves. The sectoral horn 100c, 100d (including the H-plane sectoral horn 100c and the E-plane sectoral horn 100d) has a pyramidal horn shape with four sides S1-S4; however, only one pair of the sides is flared while the other pair is parallel. Sectoral horns 100c, 100d are generally used as feed horns for wide search radar antennas. As shown in
Referring back to
In some examples, the inner surface 110a of the horn 100 defines parallel slots or grooves (not shown) positioned throughout the inner surface 110a of the horn 100 and perpendicular to the center axis 111. Such corrugated horn antennas 100 are mainly used as a feed horn for satellite dishes and radio telescopes.
Referring to
Δ=D−√{square root over (D2−a2)} (1)
where a equals half the width W of the horn 110 (a=W/2).
In some examples, the second end 112b of the horn 110 may define a groove 114 configured to receive a lens 200. The groove 114 may be perpendicular to the center axis 111 and extending throughout the inner surface 110a of the horn 110. The lens 200 may be releasably removed from the groove 114. In other examples, an adhesive is applied to the edges of the lens 200 (or the inner surface 110a) allowing the lens 200 to adhere to the inner surface 110a of the second end 112b of the horn 110. Other methods ol securing the lens 200 within the horn 110 may also be used.
The horn antenna 100 focuses or concentrates power by strengthening the power of signals in one direction and reducing the power in another direction. For example, the horn antenna 100 strengthens the power of signals exiting the aperture 112 of the horn antenna 100 in a forward direction F and weakens signals received by the aperture 112 of the horn antenna 100 in a rearward direction R.
The dimensions of the horn antenna 100 directly affect the gain G of the horn antenna 100. Horn antenna gain or power gain G is a relative value of an antenna's ability to direct or focus radio frequency energy in the forward direction F or backward direction B. The gain G is measured in decibels relative to an isotropic radiator (dBi) or Decibels relative to a dipole radiator (dBr). The isotropic radiator is the reference point P (apax) that radiates energy equally (equal power) in all directions.
When configuring the wide-band horn antenna 100 to fit within a desired volume, the axial length L of the horn 110 chosen may affect an aperture efficiency of the aperture 112. For example, shortening the axial length L of the horn 110 by increasing the flare angle θ, introduces phase error to the horn aperture 112 (e.g., spherical wave propagation), which affects the gain G. An increase of the flare angle θ to 45 degrees may reduce the axial length of the horn 110 to a minimal practical length D/2 (e.g., 87.5 mm), which increased phase error. Phase error occurs due to the difference between the slant length D of the horn 110 and the axial length L. The phase error at the horn aperture 112 translates directly to degraded aperture efficiency, reducing the gain G of the horn antenna 100.
To mitigate and/or compensate for the phase error, the horn antenna 100 includes a lens 200 (e.g., made of a dielectric material) at the horn aperture 112 where the lens 200 compensates and equalizes the phase distribution over the aperture 112. The lens 200 compensates and/or equalizes the phase distribution over the aperture 112. In other words, the lens 200 corrects phase aberrations that may occur when reducing the axial length L of the horn 110 in an attempt to achieve a constant phase distribution over the aperture for a much shorter horn length L. The larger the flare angle θ of the horn 110, the more correction may be needed up to a maximum flare angle θ (e.g., a 45 degree flare). Moreover, a dielectric lens 200, by virtue of the dielectric material, causes a signal wave propagating towards an entrance plane of the dielectric lens 200 to have a discontinuity in its propagation. The discontinuity is due to some portion of the signal wave reflecting back and some portion of the signal wave transmitting through the dielectric lens 200, resulting in reflection losses and impairing aperture efficiency. The lens 200 may have a maximum thickness T at and measured along the center axis 111 of the horn 110. The thickness of the lens 200 may be tuned to achieve certain downlink and uplink performance of the antenna 100.
Referring to
The anti-reflective layer 210 defines a plurality of holes 220. The holes 220 may envelop about 50% (by volume) of the surface of the lens 200. In some examples, the holes 220 are of equal size and shape (as shown in FIGS, 2A-2E). While in other examples, the holes 220 have different sizes and/or a different shape while maintaining 50% of the matter. The holes 220 may define a square, rectangular, polygonal, circular, or elliptical cross-sectional shape. Other shapes are possible as well. The holes 220 are arranged to mitigate and compensate for phase error by equalizing the phase distribution over the aperture 112. In some examples, the holes 220 may have different cross-sectional shapes while maintaining the 50% ratio. The holes 220 may be arranged in a random or ordered manner. The holes 220 are used to counter the reflections caused by the lens 200. In addition, the holes 220 allow the horn 110 to receive or output most of the signals, i.e., the signals are not reflected by the lens 200, instead they are absorbed (in either forward direction F or backward direction B).
The anti-reflective layer 210 defines holes 220 versus grooves or other elongated indentations or voids to provide a relatively even disbursement of the material-to-void ratio (e.g., 50/50). Grooves or elongated voids (e.g., slots having a length of at least 3 or more times a width) result in comparatively degraded performance, due to the lack of a relatively even disbursement of the material-to-void ratio. As discussed below, the use of holes 220, as described herein, improves the downlink performance by 90% or up to 92% and the uplink performance by 80% or up to 90%, and are therefore not a mere design choice.
As shown in
The anti-reflection layer 210 may be a quarter wave impedance transformer. A quarter wave impedance transformer (λ/4) is a waveguide component that is one-quarter of a wavelength long and terminates at a known impedance. The anti-reflection layer 210 has a dielectric constant (i.e., relative permittivity) ∈T that may be the geometrical average of the medium prior to a point of reflection (i.e., of the material preceding the lens 200 inside the horn 110) and the medium past the point of reflection (i.e., of the material of the lens 200). In this case:
∈T=√{square root over (∈r
where ∈T is the dielectric constant of the anti-reflection layer 210, ∈r
The thickness LD [mm] of the anti-reflection layer 210 may be determined using the following equations:
which is a Quarter wave in matter. When the anti-reflection layer 210 is formed integral with the lens 200 (e.g., via molding), the holes 220 have a depth of the thickness LD of the anti-reflection layer 210 in the first surface 202 of the lens 200. Moreover, the holes 220 may have a diameter DH (
In some examples, the lens 200 defines a two-dimensional array or grid of holes 220 having a substantially square cross-sectional shape or a substantially circular cross-sectional shape (as shown in
The holes 220 within the anti-reflection layer 210 provide a low cost horn antenna 100 with an improved efficiency for uplink and down links. For example, the addition of the lens 200 with the anti-reflection layer 210 allows for a shorter axial length L of the horn 110.
Referring to
In some examples, the lens 200 is a cross linked polysterene microwave plastic. The lens 200 may maintain a dielectric constant of 2.53 through 500 GHz with low dissipation factors. In some examples, the lens 200 may include a Polytetrafluoroethlyene (PTFE), which is a synthetic fluoropolymer of tetrafluoroethlyene. PTFE is a flurocarbon solid with a high-molecular weight compound made of carbon and fluorine. PTFE has a low coefficient of friction against any solid, and is hydrophobic (i.e., repels water).
Referring to
A number of implementations have been described. Nevertheless, it will be understood that various modifications may be made without departing from the spirit and scope of the disclosure. Accordingly, other implementations are within the scope of the following claims.
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