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IEEE TRANSACTIONS ON ANTENNAS AND PROPAGATION, VOL. 54, NO. 5, MAY 2006
Center Feed Single Layer Slotted Waveguide Array
Sehyun Park, Member, IEEE, Yasuhiro Tsunemitsu, Student Member, IEEE, Jiro Hirokawa, Senior Member, IEEE,
and Makoto Ando, Fellow, IEEE
Abstract—A center feed configuration is newly introduced to enhance the bandwidth as well as to suppress the frequency dependent
beam squinting in single layer slotted waveguide arrays. A multiple-way power divider consisting of cross-junctions is installed at
the center of the aperture in an alternating-phase fed waveguide
slot array to reduce the long line effect in the radiating waveguide.
Each radiating slot is equipped with an inductive wall for reflection
canceling, which dispenses with the beam tilting technique for
suppressing cumulative reflection and assures the boresight beam.
All these are equipped in single layer and are potential for low cost
mass-production as is usual the case with alternating phase-fed
arrays. The test antenna is fabricated at 26 GHz band for FWA
system. A 30.5 dBi gain with 46% efficiency with the main beam
staying in the boresight is obtained. The sidelobes of 9.5 dB associated with the aperture blockage for the center feed is suppressed
to below 14.7 dB at the design frequency, by applying a genetic
algorithm for controlling the slot excitation.
Index Terms—Center feed, reflection canceling, waveguide arrays.
I. INTRODUCTION
S
INGLE layer slotted waveguide arrays are attractive candidates for high-gain and high-efficiency planar antennas in
millimeter-wave since the transmission loss of a hollow waveguide is quite small even in millimeter-wave band [1]. One
example of alternating phase fed array is presented in Fig. 1(a).
This antenna has been commercialized for FWA(Fixed Wireless
Access) system of 26 GHz band in Japan. The simple structure
consisting of only two parts, that is a slot plate and a grooved base
plate, is suitable for mass-production with low-cost. Radiation
waveguide with slots have been fed from their ends by a feed
waveguide consisting of cascaded and T-junctions, in co-phase
and alternating phase fed arrays, respectively [2], [3]. This end
feed configuration is associated with long radiation waveguides
and gives rise to narrow frequency bandwidth; the long line effect
as well as the beam squinting is notable as the electrical size of
arrays become larger, as is usual the case with traveling wave
antennas. Fig. 1(b) shows frequency dependent main beam direction of conventional end feed waveguide array. This array consists
. The main beam direcof 20-element which are spaced by
tion is tilted about 1.6 [deg.] for 0.5 [GHz] frequency shift
from center frequency 25.5 [GHz]. This means degradation of
gain in the main beam direction. To overcome these problems,
Manuscript received February 4, 2004; revised October 25, 2005
S. Park is with Samsung Advanced Institute of Technology, Kyungki-do 440600, Korea.
Y. Tsunemitsu is with the Electrical and Electronic Engineering Department,
Tokyo Institute of Technology, Tokyo 152-8552, Japan and also with Japan
Radio Co., Ltd., Tokyo 181-8510, Japan.
J. Hirokawa and M. Ando are with the Tokyo Institute of Technology, Tokyo
152-8552, Japan.
Digital Object Identifier 10.1109/TAP.2006.874310
Fig. 1. End feed single layer slotted waveguide arrays. (a) End feed single
layer slotted waveguide array for alternating phase (T-junction) and (b) typical
beam squinting in end fed slotted waveguide arrays.
the authors have proposed the center feed single layer slotted
waveguide arrays as is shown in Fig. 2 [4]. By feeding the array
not from its end, but from the center of the waveguide arrays,
the long line effect is halved and the bandwidth enhancement is
expected. The symmetrical structure of the center feed would
also contribute to the main beam staying in the boresight. The
key components that have been developed for this new array are
1) A cross junction with four inductive posts was designed
for exciting two radiation waveguide on both sides of the
feed waveguide [4]; a cascaded cross junctions composes
0018-926X/$20.00 © 2006 IEEE
PARK et al.: CENTER FEED SINGLE LAYER SLOTTED WAVEGUIDE ARRAY
1475
Fig. 2. Center feed single layer slotted waveguide arrays.
Fig. 3. Slot and an inductive wall.
a multiple-way power divider to be installed in the center
of the alternating phase fed arrays.
2) Several types of reflection canceling element such as slot
pair, slot set, circular pit [5], [6] and inductive post [7]
have been designed for suppressing the cumulative slot
reflection at the input port and for dispensing with the well
known beam tilting technique [1].
In this paper, the above two devices are assembled to realize a
center feed alternating phase fed single-layer slotted waveguide
arrays, for the first time. As a reflection canceling element, a
slot with an inductive wall is newly designed by the Galerkin’s
method of moment [7] for simple fabrication and mass production by die-casting etc [8]. One difficulty of the center feed
array is the blockage occupied with the feed waveguide in
the center of the array aperture which results reduction in the
efficiency as well as the high sidelobes [9], [10]; sidelobe suppression by controlling slot excitation is also conducted here
by using genetic algorithm. The model array for FWA system
at 26 GHz band is fabricated and the 30.5 dBi gain with 46%
efficiency with the main beam staying in the boresight is obtained. The sidelobes of 9.4 dB associated with the aperture
blockage for the center feed is suppressed to below 14.7 dB
at the design frequency.
if the beam is directed at the boresight. EM design of a slot
and an inductive wall is performed by MoM with uniform line
current approximation on the inductive wall surface. A choke
is accommodated in the periphery of the antenna, which prevents the leakage through the gap between the slot plate and
the groove structure at the periphery of the array [11]. It dispenses the electrically perfect contact and the screws are used
for the simple assembly. In summary, the structure of center
feed arrays has higher degree of symmetry than the conventional end feed ones. One difficulty is the blocked area in the
center of the aperture occupied with the cross junctions; the
typical blockage is about 2.1 free space wavelength in width.
The growing sidelobes as well as the efficiency decrease should
be taken into account in the design.
II. STRUCTURE OF A CENTER FEED ARRAY
The overall configuration of the center feed alternating phase
fed single layer slotted waveguide array is explained in Fig. 2.
The feed waveguide, which works as a multiple-way power divider consisting of cascade of cross-junctions, is installed at the
center of the array. Each cross-junction has four inductive posts
to control the amplitude and phase of the divided power [4].
An antenna input aperture is cut on the bottom at the center of
the feed waveguide. The radiation waveguides are placed with
a spacing of half the guide wavelength in the feed waveguide
for excitation in alternating phase. The radiating shunt slots
are longitudinally spaced by a half the guide wavelength while
they are transversally offset on both sides of the waveguide
axis. Each radiating element consists of a slot and an inductive
wall which cancels out the reflection from slot; the radiation
waveguide is free of cumulative reflection at the input even
III. COMPONENT DESIGNS
A. Reflection Canceling Slot With Inductive Wall
In the design of a traveling wave array, we developed a simple
design method in two steps as in [5]. The design of a radiation
unit for controlling radiation and suppressing reflection comes
first and then it is utilized to synthesize the array with desired
illumination. This paper adopted it but the unit design is conducted in the isolated environment. An analysis model of a slot
with an inductive wall is shown in Fig. 3. The longitudinal slot
which is parallel with respect to -axis is adopted for linear polarization. The length and the width of the slot are and . The
-position, -position and thickness of inductive wall are ,
and , respectively. In the analysis procedure, an electric current
on the wall surface and an equivalent magnetic current on the
slot aperture are assumed. The unknown expansion coefficients
of basis function are determined by the Galerkin’s method of
moment [7]. Then, the radiation power as well as the reflection
of the slot and an inductive wall is estimated.
The predicted reflection as well as the slot parameters and
wall positions are presented in Fig. 4 as functions of radiation
power. The other parameters are given as follows:
,
,
and
. The longitudinal slot
with resonant length of 5.8 mm is used. For wide range of
coupling power, the low reflection below 30 dB is realized
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Fig. 4. Slot and an inductive wall parameters for reflection canceling.
Fig. 5.
Fig. 6.
Suppressed sidelobe level by using genetic algorithm.
Efficiency and sidelobe level as function of antenna size.
Fig. 7. Slot excitation determined by genetic algorithm.
by varying the wall location. In the later discussion of sidelobe
level control, Fig. 4 provides the reflection canceling element
design for various radiation power of slot, specified in the array
design.
B. Suppression of Sidelobes Due to Aperture Blockage by
Center Feed Waveguide
A center feed waveguide arrays has typical blockage region
at the center of the aperture with the width of 2.1 free space
wavelength. This give rises to high side lobe levels. Fig. 5 shows
the prediction of antenna efficiency and the sidelobe levels as
functions of array size. A square aperture
and magnetic dipole source model is used in the calculation. The sidelobe of a center feed waveguide arrays mainly depends on the
ratio of array size and blockage region. It is required to increase
the number of slot for some application requiring lower sidelobe. The efficiency degradation as well as the sidelobe level
growth is associated with the blocking area ratio. For example,
the aperture
in 26 GHz band has
the initial first side lobe level of 13 dB for 20-slot design of
uniform illumination is increased to 9.4 dB with 2.1 free space
wavelength blockage as shown in Fig. 5. Here, the first side lobe
level is suppressed by using genetic algorithm [12]. In this step,
only the excitation amplitudes are optimized for half side array
due to symmetry structure. The genetic algorithm optimized a
10-element array with 6-bit amplitude accuracy. The maximum
relative-sidelobe level is used for cost function [13], [14]. Sometimes, GA give us unacceptable slot illumination with large fluctuation even though sidelobe level is suppressed enoughly. To
avoid this, the initial value of slot excitation amplitude set to
be taylor distribution of 20 dB sidelobe level. The parametric
range of amplitude has dynamic range 0.3 compare to taylor
distribution. Fig. 6 shows the resulting H-plane radiation pattern
after GA optimization compare to uniform illumination. The radiation pattern has a reduced sidelobe level of 16 dB though
the inevitable gain degradation due to tapered illumination about
1 dB is observed. The optimized excitation amplitude is given
in Fig. 7. Fig. 8 shows the slot and inductive wall parameters
to realize desired excitation amplitude and reflection canceling.
The end-most slot is specially designed as a “matching slot”
which radiates all the residual power with the reflection suppressed [15], [16].
PARK et al.: CENTER FEED SINGLE LAYER SLOTTED WAVEGUIDE ARRAY
1477
Fig. 11.
Near field distribution of the aperture field at 25.5 GHz.
Fig. 8. Slot parameters for desired slot coupling.
as 10 dB at the design frequency 25.3 GHz. It also includes
the result by HFSS simulator applied for 1/4 structure of the full
array based upon the symmetry. The reason for this degradation
of return loss was intensively discussed numerically and experimentally by authors [17]. The mutual coupling of inner-most
slots, which are strongly excited according to GA design, has
been identified as the source of reflection. However, they are remarkable agreement though the structure is very large and complicated. This implies that the fabrication of parts, the slot plate,
the base plate and the posts in cross junctions, as well as the
contact by the choke with simple screw is accurate and works
well.
Fig. 9.
Fabricated model antenna.
B. Near Field Distribution
Fig. 10. Reflection at the feed point of the antenna.
IV. EXPERIMENTAL RESULTS
A. Reflection
A test antenna of the center feed waveguide arrays is designed
and fabricated at 26 GHz band as shown in Fig. 9. The antenna
consists of two sets of radiation waveguides, one on each side
of the feed waveguide. Each set consists of 16 radiation waveguides, and each radiation waveguide has 10 slots. The aperture
area is around 160 180 mm. Fig. 10 shows the frequency dependence of the overall reflection at the input port. It is as high
Fig. 11 shows the two-dimensional amplitude distribution at
25.5 GHz. The feed waveguide with cascaded cross junctions is
placed at the center along the vertical axis. As is expected, weak
amplitude is observed at the center of the arrays because there is
no slot above on the feed waveguide. The one-dimensional amplitude and phase distribution along the feed waveguide, measured at the center of the antenna, is shown in Fig. 12(a) and (b),
respectively. Uniform amplitude and phase distributions with
small ripples are observed at 25.5 GHz. These confirm the desired operation of the cross-junction feed waveguide. The frequency characteristics are slightly shifted to higher than design
one of 25.3 GHz. Figs. 13(a) and (b) shows those along the radiation waveguides. The amplitude has the blocking at the center
and is tapered down toward the aperture end following the design as shown in Fig. 7 for sidelobe suppression, while the uniform phase is observed.
C. Radiation Pattern
Fig. 14 shows the measured H-plane pattern for 16 dB
sidelobe suppression design. This pattern is associated with the
excitation of the radiating slot array. The maximum sidelobe
of measured result is 14.7 dB at design frequency 25.3 GHz.
It is slightly higher than calculated one of 16 dB but reasonable agreement was obtained. The measured radiation pattern
in E-plane coincides with that for uniform illumination with
the sidelobe 13 dB as shown in Fig. 15. As an important advantage of the center feed array confirmed in these figures, the
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IEEE TRANSACTIONS ON ANTENNAS AND PROPAGATION, VOL. 54, NO. 5, MAY 2006
Fig. 12. Amplitude and phase distribution in parallel with the feed waveguide.
(a) Amplitude and (b) phase.
Fig. 13. Amplitude and phase distribution in perpendicular with the feed
waveguide. (a) Amplitude and (b) phase.
main beam direction in E- and H-plane stays in the boresight in
wide frequency range and is not squinted with the frequency.
Generally, slot array has very high polarization purity. This advantage is independent of feed structure. The measured XPD
of center feed waveguide array is more than 45 dB as shown
in Fig. 16.
D. Gain and Efficiency
Fig. 17 shows the frequency characteristics of the gain and efficiency of the antenna. The measured gain is compared with the
end feed waveguide array for commercial use of FWA system.
The enhancement of frequency bandwidth is observed as expected. The maximum gain is 30.5 dBi which correspond 46%
efficiency for the aperture size. This is a bit lower than the end
feed waveguide arrays. The degradation of the gain and efficiency comes from the blockage region and the aperture tapering for sidelobe suppression. These are roughly estimated
as aperture blockage 0.5 dB, tapered illumination 1 dB, return
loss 0.5 dB, and the slot excitation (amplitude/phase) error due
to mutual coupling 0.5 dB. The former two are inherent to this
specific design of the array while the latter two may be reduced
by the advanced slot design taking the mutual coupling effects.
Fig. 14.
Radiation pattern in the yz -plane (H-plane).
V. CONCLUSION
We have proposed a center feed single layer slotted waveguide array. The main advantage of this antenna is a wide
bandwidth and the stable boresight main beam. The main beam
direction in H-plane is not squinted for frequency change.
PARK et al.: CENTER FEED SINGLE LAYER SLOTTED WAVEGUIDE ARRAY
1479
to 46% efficiency is obtained. The inductive posts will be
replaced with walls to simplify fabrication in the near future.
The advanced slot design taking the mutual coupling effects
into account, should be developed for gain enhancement as
well as input VSWR improvement.
REFERENCES
Fig. 15.
Radiation pattern in the xz -plane (E-plane).
Fig. 16.
Measured cross polarization (E-plane).
Fig. 17.
Gain and efficiency of the antenna.
A cross-junction is used for multiple-way power divider. A
reflection canceling slot with inductive walls is introduced to
escape from the beam tilting technique and a waveguide arrays
with boresight main beam is realized. The sidelobe which is
a bit higher than conventional end feed waveguide array is
suppressed by genetic algorithm. The maximum sidelobe is
suppressed below 14.7 dB. A gain of 30.5 dBi corresponding
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Sehyun Park (S’01–M’04) was born in Kyeongnam,
Korea, on February 2, 1973. He received the B.S. degree in control and instrumentation engineering and
the M.S. degree in radio sciences and engineering
from Korea Maritime University, Busan, Korea,
and the D.E. degree in electrical engineering from
the Tokyo Institute of Technology, Tokyo, Japan in
2003.
From 2003 to 2004, he was Postdoctoral Research
Fellow at the Tokyo Institute of Technology. He is
currently a Senior Research Engineer at the Samsung
Advanced Institute of Technology, Kyungki-do, Korea.
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IEEE TRANSACTIONS ON ANTENNAS AND PROPAGATION, VOL. 54, NO. 5, MAY 2006
Yasuhiro Tsunemitsu (S’05) was born in Kanagawa,
Japan, on September 1, 1976. He received the B.S.
degree in electrical engineering from Takushoku University, Tokyo, Japan, in 2000, and the M.S. degree in
electrical and electronic engineering from Yokohama
National University, Yokohama, Japan, in 2002. He
is currently working toward the D.E. degree at Tokyo
Institute of Technology, Tokyo.
He works at Japan Radio Co., Ltd. His current research interests are in slotted waveguide array antenna.
Mr. Tsunemitsu is a member of the Institute of Electronics, Information and
Communication Engineers (IEICE), Japan and the Applied Computational Electromagnetics Society (ACES).
Jiro Hirokawa (S’89–M’90–SM’03) was born in
Tokyo, Japan, on May 8, 1965. He received the B.S.,
M.S., and D.E. degrees in electrical and electronic
engineering from the Tokyo Institute of Technology
(Tokyo Tech.), Tokyo, Japan, in 1988, 1990, and
1994, respectively.
He was a Research Associate from 1990 to 1996,
and is currently an Associate Professor at Tokyo
Tech. From 1994 to 1995, he was with the antenna group at Chalmers University of Technology,
Gothenburg, Sweden, as a Postdoctoral Fellow, on
leave from Tokyo Tech. His research area has been in analyzes of slotted
waveguide array antennas.
Dr. Hirokawa is a Member of the Institute of Electronics, Information and
Communication Engineers (IEICE), Japan. He received an IEEE AP-S Tokyo
Chapter Young Engineer Award in 1991, a Young Engineer Award from IEICE
in 1996, a Tokyo Tech. Award for Challenging Research in 2003, and a Young
Scientist Award from the Minister of Education, Cultures, Sports, Science and
Technology of Japan in 2005.
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Makoto Ando (SM’01–F’03) was born in Hokkaido,
Japan, on February 16, 1952. He received the B.S.,
M.S., and D.E. degrees in electrical engineering
from Tokyo Institute of Technology, Tokyo, Japan,
in 1974, 1976, and 1979, respectively.
From 1979 to 1983, he was with Yokosuka Electrical Communication Laboratory, NTT, and was engaged in development of antennas for satellite communication. He was a Research Associate with Tokyo
Institute of Technology from 1983 to 1985, and is
currently a Professor. His main interests have been
high-frequency diffraction theory such as physical optics and geometrical theory
of diffraction. His research also covers the design of reflector antennas and
waveguide planar arrays for DBS and VSAT. His latest interest includes the
design of high-gain millimeter-wave antennas.
Dr. Ando is a Member of the Institution of Electrical Engineers (IEE) London,
U.K., and the Institute of Electronics, Information and Communication Engineers (IEICE), Japan. He has been a Member of the Scientific Council for the
Antenna Centre of Excellence (ACE) in EU’s Sixth Framework Programme for
research a network of excellence since 2004. He received the Young Engineers
Award of the Institute of Electronics, Information and Communication Engineers (IEICE), Japan, in 1981, the Fifth Telecom Systems Award in 1990, the
Eighth Inoue Prize for Science in 1992, the Achievement Award and the Paper
Award from IEICE Japan in 1993, and the Meritorious Award on Radio, the
Minister of Public Management, Home Affairs, Posts and Telecommunications
in 2004. He has been the Vice-Chair and Chair of Commission B of the International Union of Radio Science (URSI), for 1999 to 2002 and 2002 to 2005,
respectively. He is the Chairman of the Board of Association of Radio Industries
and Businesses (ARIB) in 2004. He served as the Chairman of the Technical
Program Committee of the International Symposium on Antennas and Propagation (ISAP) in 2000, the Technical Program Co-Chair for the 2003 IEEE
Topical Conference on Wireless Communication Technology, the Vice-Chair of
ISAP 2004, the Chair of 2004 URSI International Symposium on Electromagnetic Theory, and the Co-Chair of 2005 IEEE ACES International Conference
on Wireless Communications and Applied Computational Electromagnetics. He
is the Chair of the IEICE Electronic Society’s Technical Group of Electromagnetic Theory for 2004 to 2005 and the IEICE Communication Society’s Technical Group of Antennas and Propagation for 2005 to 2007. He is a Member of
the Administrative Committee of the IEEE Antennas and Propagation Society
for 2004 to 2006. He served as the Guest Editor-in-Chief of the Special Issue
on Innovation in Antennas and Propagation for Expanding Radio Systems in
IEICE Transactions on Communications in 2001 and the Special Issue on Wave
Technologies for Wireless and Optical Communications in IEICE Transactions
on Electronics in 2004. He has also been appointed Guest Editor-in-Chief for
several special issues in Radio Science and IEICE Transactions on Electronics
in 2005.