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In recent years there has been an increasing demand for antenna calibrations at millimeter wave frequencies. Because of this the National Institute of Standards and Technology (NIST) has been developing measurement capabilities at millimeter wave frequencies. The development of gain and polarization measurement capabilities have been previously reported. This paper reports on the development of the capability to measure an antenna pattern which has been achieved during the last year. Measurement accuracies of better than 4 dB have been achieved for sidelobes which are 40 dB below the mainbeam peak. NIST is now providing a new measurement service for antenna patterns in the 30-50 GHz frequency range.
To perform antenna measurements, it is necessary that the entire antenna structure is illuminated by a uniform plane wave. Since almost all sources radiate spherical waves, plane wave field configurations can be achieved locally only at very large distances from the source. The proliferation of compact range designs have reduced the distance required to achieve nearly plane wave field configurations to distances which can be satisfied by indoor facilities. While most compact ranges have been designed to create a nearly plane wave field configuration, at Arizona State University an operational compact range exists which creates a nearly cylindrical wave field structure. The pattern measured under cylindrical wave illumination is transformed, using analytical and numerical methods, to obtain the plane wave response of the antenna system. Measurements have been performed, using the cylindrical wave compact range, of a 15 GHz axial waveguide antenna on a 1/10 scale Advanced Attack Helicopter model. The measurements were then transformed and compared with those made of the same antenna system in a plane wave compact range facility.
Implementing an antenna test range has traditionally been viewed as a major and costly undertaking, requiring significant long term facility planning, computer hardware interfacing, and software development. This paper describes a complete low cost, yet high accuracy portable near-field measurement system that was privately built for less than $2,000 and interfaced to a PC compatible computer. The design and operation of this system, including the scanner, microwave hardware, and computer system will be described. This system has since been extended into a commercial product capable of providing rapid and accurate measurements of small to medium size feeds and antennas within a small office or lab space at significantly lower cost than standard antenna test techniques. The system has demonstrated an equivalent sidelobe noise level of less than -50 dB, includes a probe corrected far-field transform and holographic back projections, and can output pattern cuts, contour plots, 3D plots, and grey scale images of antenna performance.
Evaluation methods for analyzing the performance of anechoic chambers have typically been limited to field probing, free space VSWR and pattern comparison techniques. These methods usually allow the users of such chambers to qualify or determine the amount of measurement accuracy achievable for a given test configuration. However, these methods in general do not allow the user to easily identify the reasons for limited or degraded performance. This paper presents a method based on synthetic aperture imagery which has been found usable for finding and identifying anechoic chamber performance problems. Photographs and illustrations of a working SAR imaging/mapping system are shown. Discussions are also given regarding the method's advantages and disadvantages, system requirements and limitations, focusing processing requirements, calibration techniques, and hardware setups. Both monostatic and bistatic configurations are considered and both RCS and antenna applications are discussed. The SAR system constructed to date makes use of a portable HP-8510 based radar placed on a hydraulic manlift for easy system maneuverability and flexibility. The radar antenna is mounted on an 8 foot mechanical scanner directed toward the area to be mapped. An image is processed after each scan of the receive antenna. Measured data and example results obtained using the mapping system are presented which demonstrate the system's capabilities.
Due to the limited size of a compact range, an antenna with low sidelobes, broad bandwidth, broad beam, small physical signature, low scattering level and reasonably high power handling are required. Historically, slot line antennas are circuit board type antennas noted for their thin cross-section, low cost of fabrication, scalability and high package density in array applications. A broadband version, fed by a microstrip line (and therefore easily connected to microstrip transceiver circuits etched on the same circuit board) is described in this paper. Test models with different shapes and using different dielectric materials were built and tested. The measured VSWR, radiation and scattering patterns of the various antenna designs are presented.
The design, fabrication, and testing of a high directivity, constant beamwidth feed horn is presented in this paper. The subject feed horn is designed to illuminate a shaped reflector compact range operating from 140 to 170 GHz. Design considerations related to pattern control and VSWR are discussed. Fabrication challenges are also considered. Primary pattern test results are presented and compared to predictions. Integration (into the reflector system) considerations are reviewed and quiet zone performance is discussed.
Currently many new compact range facilities are being constructed for making antenna pattern measurements indoors. Limited suppression of stray signals ~ due to range layout, confined surroundings and residual absorbing material reflectivity ~ represents a limitation on the accuracy of the measurements made in these facilities. Time-gating of the compact range signal appears to be a very attractive technique to reduce unwanted reflections. The authors have carried out an experimental investigation of time gating in a compact range. It is demonstrated that time-gating can improve the uniformity of the aperture field by removing the feed backlobe radiation; and, it is demonstrated that time-gating can remove the effects on a pattern of certain room reflections and of feed backlobes. When compared to conventional methods of reducing reflections based on placement of absorber, time gating appears equivalent. It does not appear however that time gating improves the conventional methods, except for measuring wide beamwidth antennas.
A technique to determine the radiation centers of large reflector antennas in a given direction is presented in this paper. Coherent processing is used to determine various radiation centers based on far zone pattern data of the antennas provided that adjacent centers are separated far enough so that their locations can be resolved. Numerical results for processing of two reflector antennas, a prime focus fed and a Cassegrainian, are presented to validate this technique. The diagnostic value of this technique for reflector antennas is demonstrated by processing the actual measured pattern and identifying some unexpected radiation centers. One can also use this technique to fine tune numerical pattern simulations of reflector antennas.
This paper describes the measurement requirements of a phased array comprised of three sub-arrays and the test system built to measure it. To evaluate the performance of the array, it is necessary to measure the radiation patterns of all three outputs at various azimuth scan angles. Because the relative phase and amplitude between the elements is an important performance parameter, if data is to be taken "on the fly", then high speed measurements are required. In addition, when taking elevation patterns through the peak of the beam, which has been scanned in azimuth, the polarization of the antenna under test changes with elevation angle. Consequently, since the patterns are to be measured to matched polarization, the transmit antenna polarization must be varied as a function of elevation angle. To complicate matters, this is a non-linear relationship. The test system architecture and resultant performance capabilities are presented.
In this paper a new system consisting of a single parabolic reflector and a point source will be presented. Such a system is capable of producing a cylindrical wavefront over a wide frequency range. Moreover, physically large text-zone dimensions can be realized. The principle of operation is identical to that of the near-field/far-field cylindrical scanning, however, the far-field antenna pattern or RCS response can be computed more efficiently by performing a simplified transformation procedure in one dimension only. It will be shown that such a system is suitable for both antenna and RCS measurements. Finally, experimental RCS data will be presented.
This paper describes how corrugated feed horns are designed for compact ranges with tight pattern control. Both the amplitude and phase of the horn pattern must be invariant over a wide frequency band. A horn synthesis computer program has been developed using the JPL HYBRIDHORN computer program as the analysis module which is driven by a Harris developed synthesis code (OPTDES). This paper also discusses launching techniques used to generate the HE(11) hybrid mode in the corrugated horn as well as design methods to eliminate ringing effects observed in both the input waveguide circuits and corrugated horns when used for RCS measurements.
The utility of absorber-lined tunnels to control the sidelobe levels of horns has previously been demonstrated. The use of such a tunnel gives the designer the option of designing a broadband feed, for example, and later tailoring the sidelobe level to meet a given specification. In this paper, a technique for calculating the radiation characteristics of a horn in an absorber-lined tunnel will be presented. The analysis is based on an absorbing phase screen approximation which has been used by one of the authors in analyzing the diffraction of signals around rocket plumes. Propagation through the tunnel is treated as if the wave travels through a sequence of layers in which the absorption depends on the transverse coordinates. The absorbing phase screen model will be developed, and then applied to the analysis of a Narda standard gain horn in a square tunnel which is lined with wedge absorbing material. For the determination of E and H-plane pattern cuts, a two dimensional model can be utilized. In order to determine the radiation pattern over the full range of theta and phi as is required for illuminating a reflector, a three dimensional model is needed. All calculations were implemented in Fortran on an IBM personal computer.
A far-field antenna range has been assembled on the roof of the Electrical Engineering building at Virginia Tech. Antenna radiation patterns and polarization patterns can be measured. The system consists of two Scientific-Atlanta azimuth positioners, a Scientific-Atlanta 1711 receiver, a Scientific-Atlanta 1832A amplitude display unit, a DC motor controller, a synchro-to-digital converter, an IBM PC, and signal sources. The DC motor controller has been interfaced to the PC along with the synchro-to-digital converter, forming a closed loop positioning control system that can be used with either of the azimuth positioners. One of the positioners is used for the antenna under test while the other positioner controls the polarization of the transmit antenna. The receiver and amplitude display provide a 60 dB dynamic range for antenna measurements. The PC has been programmed in TURBO Pascal to control the antenna positioner, record antenna patterns, store pattern data on disk, and provide antenna pattern plots. This modular approach provides permanent storage on PC disk of all measurements as well as allowing many plot combinations including linear or logarithmic form and rectangular or polar format.
For the past two years the National Bureau of Standards (NBS) has been developing the capability to perform on-axis gain and polarization measurements at millimeter wave frequencies from 33-65 GHz. This paper discusses the error analysis of antenna measurements at these frequencies. The largest source of error is insertion loss measurements. In order to make accurate insertion loss measurements, flanges on antennas need to be flat and perpendicular to the waveguide axis to within approximately 0.001 cm (0.0005 in). In addition, waveguide screws need to be tightened with a device that supplies constant torque. For antennas with gains less than about 25-30 dB (probes) we can measure on-axis gains within an uncertainty of 0.14 dB in the 33-50 GHz frequency band and within 0.16 dB in the 55-65 GHz frequency band using the three-antenna technique on the extrapolation range. For antennas with larger gains we can measure on-axis gains within an uncertainty of 0.21 dB in the 33-50 GHz frequency band and within 0.24 dB in the 55-65 GHz band using the planar near-field technique. NBS in continuing development of its measurement capabilities, including measuring probe correction coefficients required in planar near-field processing, in order to provide accurate pattern measurements at these frequencies.
For over a decade the National Bureau of Standards (NBS) has used the planar near-field method to accurately determine the gain, polarization and patterns of antennas either transmitting or receiving cw signals. Some of these calibrated antennas have also been measured at other facilities to determine and/or verify the accuracies obtainable with their ranges. The facilities involved have included near-field ranges, far-field ranges, and compact ranges. Recently, NBS has calibrated an antenna to be used to evaluate both a near-field range and a compact range. These ranges are to be used to measure an electronically-steerable antenna which transmits only pulsed-cw signals. The antenna calibrated by NBS was chosen to be similar in physical size and frequency of operation to the array and was also calibrated with the antenna transmitting pulsed-cw. This calibration included determining the effects of using different power levels at the mixer, the accuracy of the receiver in making the amplitude and phase measurements, and the effective dynamic range of the receiver. Comparisons were made with calibration results obtained for the antenna transmitting cw and for the antenna receiving cw. The parameters compared include gain, sidelobe and cross polarization levels. The measurements are described and some results are presented.
Near-field testing of a very low sidelobe, L-band, 32-element, linear phased array antenna was conducted. The purpose was to evaluate testing and calibration techniques which may be applicable to a much larger, space borne phased array antenna. Very low sidelobe performance in a relatively small array was achieved by use of high precision transmit/receive modules. These modules employ 12-bit voltage controlled attenuators and phase shifters operating at an intermediate frequency (IF) rather than at RF. Three array calibration techniques are discussed. One technique calibrates the array by means of a movable near-field probe. Another method is based on mutual coupling measurements. The last technique uses a fixed near-field source. The first two calibration methods yield substantially the same results. Module insertion attenuation and phase can be set to 0.02 dB and 0.2 degrees, respectively. Near-field measurement derived antenna patterns were used to demonstrate better than -20 dBi sidelobe performance for the phased array. Application of increasing Taylor array tapers showed the limitations of the measurement systems to be below the -35 dBi sidelobe level. The effects of array ground plane distortion and other array degradations are illustrated.
The direct far field pattern measurement of an aperture antenna becomes more difficult as the size of the aperture increases. Recent measurements on reflector antennas with 2D2/? =1500’ at The Ohio State University ElectroScience Laboratory have demonstrated the usefulness of the compact range in obtaining the complete far field pattern of antennas with large far field distances.
Techniques developed for the design of shaped, off-set reflector antennas have been applied to the design of compact ranges. Shaped optics which map an axially symmetric feed pattern into an elliptical aperture distribution have been designed. Some of the major design considerations for this type of system are examined in this paper. The design has been verified both analytically and experimentally.
When performing antenna pattern measurements on far-field antenna test ranges or in anechoic chambers, one of the main problems concerning the pattern accuracy is range reflections. Previous works dealing with this have been limited to the one-dimensional case.
An antenna radiation pattern measurement technique which allows near real time pattern capture is presented. This technique uses relatively simple field probles and detectors to cover a reasonably broad operating band. The captured pattern data is digitized with a resolution of 1.0 degree and has an angular range of 150 degrees. Many captured patterns or snap-shots could be recorded during a given time interval and later viewed for diagnostic evaluations where rapid changes in the pattern are expected.