MULTIMODE HORN
United States Patent 3680145
Multimode horn enabling to obtain a radiation pattern the phase of which is practically nil within a wide range of values of the radiation angle, characterized by the fact that the length of the paths of the modes according to the geometrical axis of the horn is such as phase differences exist between the said modes at the center of the horn aperture.
US Patent References:
Low-noise single aperture multimode monopulse antenna feed system
Webb - March 1968 - 3373431


Application Number:
05/129229
Publication Date:
07/25/1972
Filing Date:
03/29/1971
View Patent Images:
Assignee:
International Standard Electric Corporation (New York, NY)
Primary Class:
International Classes:
H01Q13/02; H01Q13/00; H01Q13/00
Field of Search:
343/772,779,786
Primary Examiner:
Lieberman, Eli
Parent Case Data:


This is a continuation of application Ser. No. 743,527, filed July 9, 1968.
Claims:
What is claimed is

1. A multimode horn having excited modes TE10 + TE30 wherein mode TE30 is excited by mode TE10 by a broadening of the height dimension of a single guide, comprising:

2. Apparatus according to claim 1 in which said phase difference PO at the center of said aperture is less than zero degrees.

3. Apparatus according to claim 1 in which said phase difference at the center of said aperture is defined as PO ≅ - 10°.

Description:
The present invention concerns improvements to multimode horns and more particularly a process enabling to obtain, by means of such horns, a radiation pattern the phase of which is close to zero degree within a large range of values of the radiation angle.

The horn radiators or "horns" constitute the extension of the waveguides and assure the transition between the waveguides and the free space, particularly where it concerns velocities of propagation of these two media. The horns may be used either as main sources of radiation or, more generally, as sources known as primary sources associated to a reflecting surface or reflector in order to form a directive aerial system. It will be observed that several horns may be used in one same aerial system in order to obtain the required radiation pattern. It is clear that the radiation pattern of such antennae using horns depends mainly upon the distribution of the electromagnetic fields in the mouth or aperture plane of the one or several horns, this distribution being itself a function of the modes which propagate in the waveguide, the horn of which is the extension, as well as upon the shape of the horn. Thus, in the case of a rectangular waveguide, the horn may be flared, either according to one of its two dimensions in order to form a sectoral horn, or according to the two dimensions at the same time, to form a pyramidal horn. In the case of a sectoral horn, the flare is defined usually with respect to the plane of the electrical field vector E (plane E) or with respect to the magnetic field vector (plane H); the plane E is for instance the plane which contains the direction of propagation of the waves and which is parallel to the electrical field vector. Therefore, it will be said that the horn is flared in the plane E when only the sides at cross angle with this plane E have been moved. Owing to this flare, the waves located in the plane of the aperture of the horn are no longer in phase, but it is generally admitted that a phase shift of 45° between the electrical field present at the center of the aperture and that present at the ends, does not disturb noticeably the ideal radiation pattern calculated without taking into account the phase. However, in certain applications, such a phase shift is not permissible.

In order to compensate phase variations in the aperture of the horn, the use of lenses which introduce an important delay at the center and a delay nil at the ends, has been proposed. Such lenses present the drawback of increasing the losses and of dismatching the horn. Furthermore, they must, in certain applications, be made in a very homogeneous material from the point of view of its dielectric constant and must be machined with very tight tolerances.

One of the objects of the present invention is thus to achieve a multimode horn in which means implemented to compensate the phase variations in the horn aperture do not present the drawbacks quoted hereabove.

Another object of the present invention is to achieve a multimode horn which presents a radiation pattern the phase of which remains practically nil within a large range of values of the radiation angle.

According to a feature of the present invention, in a multimode horn provided for propagating two modes, the length of the path of the said modes according to the geometric axis of the horn is chosen in such a way as it exists a phase shift between these two modes at the middle of the horn aperture, the value of this phase shift depending upon the types of modes used.

According to another feature of the present invention, in a multimode horn comprising means for propagating more than two modes, means are provided for obtaining phase shifts between the different modes, the values of these phase shifts being chosen in such a way as the phase of the vectorial sum of the modes in the horn aperture, varies little within the whole useful range of values of the radiation angle.

The above mentioned and other features and objects of this invention will become apparent by reference to the following description taken in conjunction with the accompanying drawings in which:

FIG. 1 illustrates a rectangular waveguide;

FIG. 2 illustrates a cross section of a multimode horn;

FIG. 3 illustrates curves of the electrical field for two types of modes and their sum;

FIG. 4 illustrates curves of the phase of the field radiated by the multimode horn;

FIG. 5 illustrates amplitude curves of the field radiated by the multimode horn.

FIG. 1 shows the aperture 1 of a rectangular waveguide 2 of width a and height c. When the dimensions a and c, with respect to the wavelength d in free space, are such as (d/2) < a < d and c < (d/2), the only mode which propagates in the waveguide is a mode with transversal electrical field, i.e., a mode the electrical field vector of which is at cross angle with the propagation direction Oz. In the plane of the aperture, the distribution of the electrical field has the pattern of the curve 3 which constitutes the envelope of the electrical field vectors 4. Such a mode is called mode TE 10 or H 10 , the indices 1 and 0 meaning that there is a maximum electrical field according to the axis Ox and no maximum at all of the said field according to the axis Oy. By keeping the same wavelength d in free space and by increasing the dimension a of the waveguide 2, other modes may be propagated which will be called modes TE mo or H mo . More generally, if the dimensions a and c of the waveguide are increased, other modes appear and these modes may be with transversal electric field and are called TE mn (H mn ), or with transversal magnetic field and are called TM m n (E m n ). It will be observed that in the case of the modes E m n the indices m' and n' are always different from zero.

By using this FIG. 1, one may define an electric plane E as the one containing Oy and Oz, and a magnetic plane H as the one containing Ox and Oz, i.e., a plane at cross angle with the electrical plane E.

In order to assure the transition between the waveguide and the free space, the waveguide is flared either according to one of the two dimensions in order to form a sectoral horn, or according to the two dimensions in order to form a pyramidal horn. This flare is generally defined in relation with the electrical plane E and the magnetic plane H, and it is said that the horn is flared in the magnetic plane H when the sides at cross angle with this plane have been moved. Thus, in the case of FIG. 1, a flare in the magnetic plane H corresponds to move one from the other the sides 5 and 6 of the waveguide.

In order to modify the radiation pattern of a horn, it is sometimes interesting to make appear simultaneously several modes in the horn aperture, each one of these modes having a determined amplitude. It is clear that in a horn, the different modes are set up as the dimensions of the aperture increase, however the amplitude of each one of these modes are not defined with accuracy. In order to obtain modes of accurate relative amplitudes, one resorts to successive widenings by steps, then when the different modes required have been obtained, the transition between the last waveguide and the free space is carried out by a horn. In the specialized literature concerning the antenna technique, a "multimode" horn designates the whole assembly constituted by the different waveguides of increasing cross sections and by the horn.

FIG. 2 gives a cross section of a multimode horn. This multimode horn has been obtained from the waveguide 2 of FIG. 1, the dimensions a and c of this guide being such as only the mode H 10 or fundamental mode, propagates. The larger side has been extended to a value b such as the mode H 30 appears, viz. (3d/2) < b < 2d. The ratio k of the amplitude of the mode H 30 to the amplitude of the mode H 10 depends upon the values of a and b at a given frequency, this ratio k is called harmonic rate. The waveguide of side b, referenced 10, is then flared in the magnetic plane H in order to form a sectoral horn 11 the width of the aperture 12 of which is A. FIG. 2 is thus a cross section of the multimode horn in the magnetic plane.

In the part 11 of the multimode horn, other modes different from the modes H 10 and H 30 appear, but these new modes are of small amplitude and it may be considered that their effect over the aperture distribution of the electromagnetic field and thus on the radiation pattern, is negligible. The aperture distribution of the electrical field is thus given by the sum of the electrical fields of the modes H 10 and H 30 the electrical fields being expressed with their amplitude and their phase.

FIG. 3 gives the amplitude curves in the aperture 12 of the horn, of the modes H 10 (curve 15), H 30 (curve 16) and of their sum (curve 17) assuming that the said modes are in phase at the middle of the aperture. The axis X'QX is graduated according to the values of the ratio between the abscissa measured with respect to the center of the aperture and the half-width A/2 of the aperture, this ratio will be called standard abscissa X.

It is possible to calculate the phase difference P between the modes H 10 and H 30 introduced by the path of the said modes in the multimode horn, this phase difference P is made up with a first phase shift P1 due to the path L1 in the part 10 and of a second phase shift P2 due to the path L2 in the flared part. The following is thus obtained : ##SPC1##

by assimilating the flared part 11 to a rectangular guide the large side of which would have the dimension (A + b)/2 . It will be observed that if a higher accuracy is required in the calculation of P2, another formula for the phase shift must be used. Thus, for instance, it may be demonstrated that the phase shift introduced by the part 11 of the horn, in the case of a mode H mo , is given by :

In the technique of multimode horns, one proceeds in such a way as the modes H 10 and H 30 are in phase at the middle point N of the horn aperture, i.e., that the phase shift P is equal to an integer number of times 360° . This phasing is obtained generally by varying the length L1, and for this reason, the part 10 is called "phasing section."

More precisely, if G1(X) designates the function which defines the aperture distribution of the electrical field of the mode H 10 , and G3(X) designates the function which defines the aperture distribution of the electrical field of the mode H 30 , one may write the general expression G(X) of the electrical field in the aperture under the form:

G(X) = G1(X) + ke JPO G3(X) (1);

in which formula X is the standard abscissa according to the width of the aperture and thus varies between - 1 and + 1, PO is the phase shift between the two modes at the point N, j is the complex term such as j 2 = - 1, k is the harmonic rate defined hereabove.

On the other hand, the functions G1(X) and G3(X) may be written :

G1(X) = cos (πX/2) e -jBX and G3(X) = cos (3π X/2 ) e -jCX (2),

b and C designating the maximum phase shifts appearing on the edges of the aperture respectively for the modes H 10 and H 30 . The equations (1) and (2) enable to calculate the radiated field G according to the angle r, i.e., the bearing angle, and one obtains:

G(r) = │ G1(r) │ e jP1 (r) + ke jP0 │ G3(r) │ e jP3 (r) = │ G(r) │ e jP (r).

FIG. 4 gives phase curves P(r) for different values of PO and FIG. 5 gives amplitude curves G(r) for the same values of the phase PO. These curves have been plotted by taking k = 0, 4. In FIG. 4, the phase curves have been referenced 20 for PO = - 20°, 21 for PO = - 10°, 22 for PO =0° and 23 for PO = + 20°. The bearing r has been brought on the abscissa axis and the phase shift P(r) on the ordinate axis. In FIG. 5, the amplitude curves have been referenced 25 for PO = - 20°, 26 for PO = - 10°, 27 for PO = 0° and 28 for PO = + 20°; the bearing r has been plotted on the abscissa axis, and the amplitude G(r) has been plotted in decibels on the ordinate axis. The different values of PO are obtained generally by varying the length L1 of the part 10 (FIG. 2).

The curve 22 (PO = 0°) of FIG. 4 shows that the phase of the field radiated by the multimode horn varies substantially when the bearing r varies. However, it will be observed that by choosing PO = - 10°, the curve 21 is obtained which gives a practically constant phase close to zero for r ranging between 0° and 35°. Besides, the curve 26 of FIG. 5 shows that the curve of corresponding amplitude differs very little from the curve 27 plotted for PO = 0°. In a general way, the amplitude curves vary very little in accordance with the phase shift PO of the modes according to the geometric axis of the horn.

By way of indication, the curves 24 and 29 of the FIGS. 4 and 5 show respectively the phase and amplitude curves of the field radiated by the mode H 10 alone. It will thus be observed that the phase varies quickly with respect to the bearing and that the radiation pattern (FIG. 5) is more directive.

The invention has been described assuming that the modes used were the modes H 10 and H 30 , however it is clear that it is applied also when other modes are used. Besides, the number of modes may be higher than two. It is also clear that it is applied to horns the radiation pattern of which is not in horizontal plane and is located in particular in the vertical plane. The characteristics of the invention may also be implemented in pyramidal horns.

While the principles of the above invention have been described in connection with specific embodiments and particular modifications thereof it is to be clearly understood that this description is made by way of example and not as a limitation of the scope of the invention.




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