no. ?,o tof .2- C6HKKKCE ROOM 'pGJNGERIW ANTENNA LABORATORY Technical Report No. 20 /OF ILLINOIS U88ANA, ILLINOIS FREQUENCY INDEPENDENT ANTENNAS MWHHBE ROOM TH-'-Ui, COL i by V. H. RUMSEY 25 October 1957 Contract No. AF 33 (6161-32 20 Project No. 6(7-4600) Task 40572 WRIGHT AIR DEVELOPMENT CENTER ELECTRICAL ENGINEERING RESEARCH LABORATORY ENGINEERING EXPERIMENT STATION UNIVERSITY OF ILLINOIS URBANA, ILLINOIS 36Q Antenna Laboratory Technical Report No. 20 FREQUENCY INDEPENDENT ANTENNAS by V.H. Rumsey 25 October 1957 Contract AF33( 616) -3230 Project No. 6(7-4600) Task 40572 WRIGHT AIR DEVELOPMENT CENTER Electrical Engineering Research Laboratory Engineering Experiment Station University of Illinois Urbana, Illinois ii sin <£ CONTENTS Page Abstract iii Acknowledgement iv 1. Antennas Specified by Angles 1 2 . The General Approach 3 3. The Pattern 5 4. The Impedance 7 5. Pseudo-Frequency- Independent Antennas 9 Bibliography 11 Appendix Surfaces for Which a Rotation is Equivalent to an Expansion 12 Distribution List Digitized by the Internet Archive in 2013 http://archive.org/details/frequencyindepen20rums iii ABSTRACT There is a class of antennas whose pattern as well as impedance is practically independent of frequency for all frequencies above a certain value. The general formula for their shape is r = e F(#) where r ; 0,f> are the usual spherical coordinates, a and

with the o same a . The general problem is to find all surfaces which have the property that a change in the unit of length is equivalent to a certain rotation. Then if we construct a metal antenna whose surface is one of these surfaces, its performance will be the same at all wavelengths except for a rotation of the coordinate system. This problem is analyzed in the appendix. The solution can be written in the form „,,-„, ^ \ r = e a (? + ?°> F(e) (13) where in principle F(0) can be any function of Q. The shapes represented by (13) can be very complicated because in general an increase of 2?T t in p does not give the same r: as <£> ranges from - oo to the surface weaves around through all space. Figure 3 illustrates a simple example which gives a practical antenna design. Figure 4 illustrates the case where In F(0) is periodic in 9 with period 27Ta . This gives a simple surface like a screw thread which is uniformly expanded in proportion to the distance from the origin: an increase of 27T in and ^ are defined in Fig. 5. The formula for a symmetrical plane sheet antenna consisting of two triangles with a common apex at the terminals is 189 K(cos 40 K(sin ip) \ X **< Cone FIGURE 5 where K represents the elliptic integral defined by .1 dt (1 - t*) (1 - x^t*) and V represents the half angle of the triangular strips measured from the common axis. In connection with the impedance, we should note an interesting property which was pointed out by Mushiake in one of the Tohoku University reports. It is that the impedance of any plane sheet antenna whose shape is the same as the shape of its complement (except for a trivial change of coordinates) is independent of frequency and equal to 60-77 = 189 ohms. The complementary antenna is defined as the portion of a metal plane which is not covered by the original antenna: when the antenna and its complement are fitted together they completely cover the whole plane without over- lapping. The constant impedance of a "self -complementary" antenna follows Q from the relation Z ][ Z 2 = (607T) 2 between the impedance Z of the antenna and the impedance Z of its comple- ment. Figure 6 gives some examples of self -complementary shapes. 5. PSEUDO-FREQUENCY- INDEPENDENT ANTENNAS The idea of a pseudo-frequency-independent antenna is illustrated by the horn antenna shown in Fig. 7. It consists of metal sheet perforated by holes of uniformly expanding size: any hole is exactly like its neigh- bor on the left except for a fixed expansion. The idea is that the effective size of the horn remains roughly independent of wavelength because the metal sheet becomes approximately transparent once the holes become greater than about half a wavelength square. More precisely, it can be seen that if the horn started from a point and extended to infinity, it would "look" the same to any two wavelengths whose ratio was equal to the expansion factor. Some interesting examples of pseudo-frequency— independent antennas are described 3 in the paper by R H. DuHamel and D.E. Isbell . Terminals 10 FIGURE 6 FIGURE 7 11 BIBLIOGRAPHY 1. S.A. Schelkunoff, Electromagnetic Waves, D. Van Nostrand Co., Inc., New York, 1943. 2. Ohio State University Research Foundation Reports 510-4 and 510-5, May 1953. 3. R.H. DuHamel and D.E. Isbell, "Broadband Logarithmically Periodic Antenna Structures," University of Illinois Electrical Engineering Technical Report No. 1£, Contract AF33(616)-3220, May 1, 1957. 4. J.D. Dyson, "The Equiangular Spiral Antenna," USAF Antenna Symposium, University of Illinois, October 1955. 5. R.L. Carrel, "Conical Spiral Antenna," University of Illinois Electrical Engineering Technical Report No. 22, Contract AF33( 616) -3220, May 25, 1957. 6. V.H. Rumsey, "The Characteristic Impedance of Two Inclined Cones," IRE Trans . on . Antennas . To be published. 7. R.L. Carrel, "The Characteristic Impedance of the Fin Antenna of Infinite Length," University of Illinois Electrical Engineering Technical Report No. 16, Contract AF33(616)-3220, January 1957. 8. H.G. Booker, "Slot Aerials and Their Relation to Complementary Wire Aerials, (Babinet's Principle) ," JIEE, Part IIIA, 1946. 12 APPENDIX SURFACES FOR WHICH A ROTATION IS EQUIVALENT TO AN EXPANSION A surface can be represented by the equation r = f(0/P) (14) where r, and tp are the conventional spherical coordinates. The condition that a uniform expansion be equivalent to a rotation can be written as K f(0 ; P) = f(e;P') or Kr = r* (15) where K is the expansion factor and (0|^P') represents the direction after rota- tion of the line represented by (0^), eg., for a rotation about the z axis (0=0), 1 = 0, and ^ iQ.' = T p_ (19) where T is a (3 X 3) matrix independent of e 1 > e 2 ,d l'®2' ' To ex P ress T we introduce / cos c sin c 0\ J (c) = -sin c cos c oj 1 1/ (20) 13 It is easily verified that«/(c) /D represents a rotation through the angle c about the z axis. Now the general rotation can be taken as a rotation c about the z axis followed by a rotation c about the y axis followed by a rotation c about the z axis. In effect, the latter two rotations define the direction of the axis of rotation, and the first defines the angle of rotation about that axis. Since z \ /0 it /x X - = 10 y =•• W Q., where i y / \0 1 0/ [0 l\ \ ml u = 10 \0 1 0/ (21) and UU = 1 (22) (U denotes the transpose of U) , it is easily verified that these three rotations are represented by T =/( Cl ) fy (c 2 ) u/(c 3 ). (23) To find the solutions of (15) we note that it must be valid for all 9 ,QJ& S&' 1 and all expansions K and the corresponding rotations specified by c 1 > c ^c 3 - Thu s dr d r ' dr' 9e i* K W. a©, a©.' a©. ^ ; i i j i with the understanding that summation is implied over any repeated suffix, such as j in (24) . The matrix M and the vector a are defined by M. . = w^ (25) Then (24) becomes Also from (15) 8r 8r' Q i " 85. i «l' = W ■ (26) K a = M a' (27) 3K 8r' 8r' ^j , N i i j i 14 The matrix S and the vector (3 are defined by s ij - ST <29) (*i - 5r ■ (30) i Then (28) becomes r p = S a' . (31) Our aim now is to eliminate a_ from (27) and (31) and thus obtain a set of differential equations for r in terms of and . This requires that 1 £ M and S be expressed in terms of and , which is accomplished as follows: From (19) W = T W or "Se^ = T ">J 3e~ * (32) i i i i H-=Hv^o r ^- = ^-^ . (33, i J i i j i ap • , %,' Define A. . = ^ ; A ±J = -ggj- • (34) Then (32) and (33) give T A = A ' M or A T = M A* . (35) Bp ' dp ' be.' y *7 ^=W7^ 8p ' 8t and jgf- = ^ P^ (37) i i whence S A = N (38) 3t. where N ±j = ^- 0^ (39) 15 * Note that (35) and (39) comprise 15 equations for the 16 elements of M A and S. In addition we have A ' = from (34) and (17)^ so that in principle we have enough equations to proceed.. At this point j we can simplify the analysis by choosing the coordinate system so that the axis of rotation is the z axis, i.e. ; Cj = 0) c 2 = o ; c 3 = c (40) and T =^(c) . (41) d This does not. involve any less of generality provided -g — is carried out before (40). It is easily verified that (41) is equivalent to e i = 8 1 ; @ 2 = ®2 + ° ' (42) Hence from (25) M = 1 (43) /- (27) gives K a = a/ „ (44) Substitution in (31) gives r J3 = K S a (45) which can be expressed more concisely by defining if{- In r and k = In K * (46) Then, from the definitions of a and (3 in (26) and (30), (45) can be expressed as ¥ 3 2 Again there is no non-trivial solution. The rotation therefore has only one degree of freedom. Therefore T is a function of only one variable which we shall call t. Now since T T = 1 |T| = Determinant T = 1 (69) •'• 4^=0. (70) dt But (70) is the condition that there be some Q_ and p ' satisfying dp' Jm -sr = £ e» - ° • <71) dt dt Ha „\ /2 ' is independent of t. The rotation therefore has a fixed axis represented by Q_ ' = Q. . Thus (59), (60) and (61) reduce to (61), giving the solution (62) where f(© ) is an arbitrary function. From (61) we also obtain k = - Dc . 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