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Phased Array
Automated Near-Field Antenna Test Set for Phased Array Production
D. Staiman (Government Systems Division), November 1979
The AEGIS AN/SPY-1A antenna system is an S-band monopulse phased array system designed for monopulse operation. Its high performance and manifold capabilities have placed stringent demands on the test system used in its evaluation. This paper will describe the AEGIS Near-Field Antenna Test Set (ANFATS) currently being implemented for acceptance testing production models of the antenna, a system designed for operation by manufacturing test personnel
Calibration measurements of an 80 element linear phased array antenna
L.D. Poles (Rome Air Development Center), November 1983
An 80 element linear phased array antenna was measured in the nearfield. The insertion phase and amplitude for each element were measured while the 8-bit ferrite phase shifters were individually stepped through their degrees for freedom.
Phased array testing in the compact antenna range
K.M. Parsons, November 1983
Acceptance testing of the AN/SYR-1 Electronically Steered Phased Array (ESPA) antenna in a Compact Antenna Range is described. Unique to the testing described are (1) generation of the beam steering commands to the phased array as well as control of the positioner and recording equipment by a single desktop computer and (2) the recording of S-band antenna patterns after down-conversion to a 300 MHz IF. Modifications and interfaces to the standard Compact Antenna Range equipment for testing of the multi-element planar phased array are described.
Preliminary development of a phased array near field antenna coupler
D. D. Button (Sanders Associates, Inc.), November 1984
End-to-end testing of electronic warfare (EW) equipment at the organizational or flight lines level is accomplished by use of an antenna coupler which is placed over the EW system antenna. The coupler is used to inject a stimulus signal simulating a signal emanating from a distant radar, and to receive and detect the EW system response (EW transmit) signal. The coupler is used to determine the EW receiver sensitivity over a swept frequency coverage and the EW transmit gain and effective radiated power (ERP) versus frequency characteristics, as well as to determine the operating integrity of the EW antenna and transmission lines.
Pulsed, computer-controllable receiver and exciter having wide instantaneous bandwidth for testing active-element phased arrays
P.N. Richardson (Texas Instruments Incorporated), November 1985
This paper describes a receiver and exciter built by Texas Instruments for automated testing of electronic-scan antennas. The equipment is suitable for both near-field and far-field testing, and is programmable through a General-Purpose Interface Bus (GPIB) conforming to IEEE Standard 488. A two-channel design is described, but the technology is equally applicable to receivers from one to three (or more) channels. The receiver outputs are digitized as 10-bit I and Q (In-phase and Quadrature) components.
Measurement of element pattern and its usage in the development of multi-beam arrays
P. Kirshner (ELTA Electronic Industries),I. Oz (ELTA Electronic Industries), November 1986
Electronic scanning phased arrays are being used more and more in radar, EW and communication systems. The development of such an array can be divided into two separate parts: development of the radiating elements and development of the beam forming network. The development of these two parts is often done in parallel and the radiating elements should always be developed taking into consideration the whole array and not only single elements.
Displaced phase center antenna measurements for space based radar applications
H.M. Aumann (Massachusetts Institute of Technology),A.J. Fenn (Massachusetts Institute of Technology), F.G. Willwerth (Massachusetts Institute of Technology), November 1986
An investigation of the use of array mutual coupling measurements, to evaluate displaced phase center antenna (DPCA) performance, is made. The details of a subscale space based radar (SBR) DPCA phased array and the array mutual coupling technique are discussed. DPCA results are quantified experimentally under a number of test conditions. It is shown that the test array beam decorrelation computed from array mutual coupling data, is in good agreement with both theoretical predictions, planar near field measurements and direct far field measurements.
Near-field testing of a low-sidelobe phased array antenna
H.M. Aumann (Massachusetts Institute of Technology/Lincoln Laboratory),F.G. Willwerth (Massachusetts Institute of Technology/Lincoln Laboratory), November 1987
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.
High speed pattern measurements of a multi-port phased array
R.E. Hartman (Flam & Russell, Inc.),M.E. Burdack (Flam & Russell, Inc.), November 1988
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.
Scale model aircraft/phased array measurements
M. O'Brien (Loran Randtron Systems),R. Magatagen (Loran Randtron Systems), November 1989
This paper describes the techniques applied to a fully automatic computer controlled, HP8510 based, range gated digital data acquisition system used to provide scale modeled large aperture synthesis, evaluation of aircraft blockage effects, array patterns, element cancellation ratios, as well as providing a large accurate data base for radar simulation exercises.
Measurement of phased array patterns by near-field focusing
H.M. Aumann (Massachusetts Institute of Technology),F.G. Willwerth (Massachusetts Institute of Technology), November 1989
Performance verification of an adaptive array requires direct, real-time sampling of the antenna pattern. For a space-qualified array, measurements on a far-field range are impractical. A compact range offers a protected environment, but lacks a sufficiently wide field of view. Conventional near-field measurements can provide antenna patterns only indirectly. This paper shows how far-field antenna patterns can be obtained in a relatively small anechoic chamber by focusing a phased array in the near-field. The focusing technique is based on matching the nulls of far-field and near-field antenna patterns, and is applicable to conformal or nonuniform phased arrays containing active radiating elements with independent amplitude and phase control. The focusing technique was experimentally verified using a 32-element, linear, L-band array. Conventionally measured far-field and near-field patterns were compared with focused near-field patterns. Very good agreement in sidelobe levels and beamwidths was achieved.
Alignment measurements using a special purpose phased array antenna
L.D. Poles (Rome Air Development Center), November 1989
A special purpose 80 element linear phased array antenna was aligned using an iterative phase cycling method. First, the array was aligned to yield maximum main-beam power in the reactive near-field zone and then in the far-field zone. A record of the phase-shifters settings achieved for each zone was kept for use as look-up table during operation. In situ electronic main-beam steering was performed to compare sidelobe performance for the two cases. This report describes the measured results obtained using the phased cycling alignment procedure and compares the measured one-way radiation pattern for the two distance conditions.
Measurement of phased array gain-to-temperature ratio using the solar method
J. Harris (Georgia Tech Research Institute), November 1989
The gain-to-temperature ratio (G/T) is a fundamental parameter used in describing the performance of a receiving antenna. This single parameter is sufficient to describe the antenna's contribution to the sensitivity of the receiving system because it includes the antenna gain as well as noise producing factors such as sidelobes and ohmic losses. The G/T of a phased array antenna is determined by the size of the aperture and the aperture distribution as well as the ohmic losses, electronic gains and noise figures of the components in the array assembly. Measurement of phased array G/T is an important means of verifying that the integrated assembly is performing to the level equivalent to the sum of the subassemblies. One method of measuring antenna G/T uses the sun as a source of radio frequency noise. This method is equivalent to the hot/cold source method used to measure the noise figure of a two port device. The sun is used as the hot source and the clear sky is used as the cold source. The difference in the noise output from the antenna with it pointed at the hot sun and the cold sky is used along with the known solar flux density and appropriate correction factors to calculate the G/T. The measured G/T is corrected for the antenna beamwidth and losses in the post antenna measurement system. This paper describes the solar method used to measure the G/T of a large S-Band airborne phased array designed and built by the Georgia Tech Research Institute (GTRI). The measurement results are compared to the G/T values calculated knowing the performance of the components that make up the array assembly.
Design of a short range for testing large phased arrays
L. Goldstone (Norden Systems), November 1989
Large arrays require large separations between the transmit antenna and the antenna under test (AUT) to measure pattern parameters in the far field. For the subject AUT, a range of 6 miles with a spurious signal level of -58 dB was necessary to obtain the required accuracy. Measurements have been performed on a significantly shorter range without serious degradation. The antenna was focused for the angle of electronic scan and the resulting pattern measured. The theoretical far field patterns were compared with the calculated focused patterns for the short range. The maximum sidelobe error of 1/2 dB occurred at 60 degrees scan. There was no noticeable degradation in beamwidth, gain, or foresight at any scan angle. A 6-mile range would have produced a 2-dB sidelobe error. The measured range reflection level was -50 dB. The transmit dish with sidelobes of 22 dB was replaced with an array that had 40 dB sidelobes. This change reduced the reflections to below the required -58 dB. The antenna was focused using a range calibration technique and the measurements substantiated the theory.
Holographic diagnostics of a phased array antenna from near field measurements
P.A. Langsford (GEC-Marconi Research Centre),M.J.C. Hayes (GEC-Marconi Research Centre), R. Henderson (GEC-Marconi Research Centre), November 1989
A 400 element phased array antenna has been constructed at the GEC-Marconi Research Centre. Each radiating element is fed from its own phase shifter. The radiation patterns of this array have been measured using a recently constructed Cylindrical Near Field Test Facility. The radiation pattern is obtained on a two dimensional grid and contains both amplitude and phase information. It is therefore possible to transform these data back to the array aperture to obtain the array excitation amplitudes and phases. The spatial resolution obtained in the aperture is a function of the angular coverage of the radiation pattern used. The effect of deliberately introduced phase errors on the calculated aperture data is shown.
Mesar active phased array antenna pattern acquisition
E.H. England (Admiralty Research Establishment),R. Young (Plessey Radar Limited), November 1989
Separation of the Antenna from the remainder of the system is not possible with a fully active phased array such as MESAR, since each array element has an associated electronic module which contains amplifiers (separate for transmit and receive), phase shifters, switches, etc. The "antenna" is therefore not reciprocal and it also requires a control system. As a result, the system used for pattern acquisition is considerably more complex than that used for testing conventional antennas and some of the traditional parameters are either not obtainable or require redefining. The methods used for testing the MESAR antenna are given together with details of the range equipment involved.
Aramis - a flexible near-field antenna test facility
O. Silvy (Electronique Serge Dassault), November 1989
A flexible near-field antenna test-facility is presented. This system gathers all that is necessary to design, to debug and to validate the high performance antennas which are made by ESD. ARAMIS has been operational since January 1988. Its applications are: - Near-field measurements (for diagrams): * planar, * cylindrical. - High speed field mapping (for default analysis): * planar radiating surface, * cylindrical radiating surface. - Generation of element excitation (active phased array testing): * planar antennas, * cylindrical antennas. - Direct far-field measurements (probes, small antennas), - Circuit measurement (S parameter). The facility features a specially designed scanner. Thanks to its six degrees of freedom, this positionner allows the differents types of measurements to be made. The instrumentation is based upon the HP 8510 B network analyzer. A single computer performs the measurements, transforms the data and presents the graphics (linear diagrams, color maps, three-dimensional colored projections). In order to grant a high scan speed, the system uses the FAST CW mode of the HP 8510 B. An external trigger is provided during the motion process of the probe. A rate of 500 measurements/sec. has been proved. This on-the-fly process is clearly depicted. Experimental results are presented which include: - Low sidelobe (-38 dB) antenna diagrams. - Default analysis through: * Amplitude mapping (leakage short-circuit in a microstrip antenna). * Phase mapping (out-of band comparison between two radiating element technologies). * Measurement of excitation laws. * 3-D transformation. - Simultaneous on-the-fly acquisition of up to three antenna outputs.
Error suppression techniques for near-field antenna measurements
G. Hindman (Nearfield Systems Incorporated),D. Slater (Nearfield Systems Incorporated), November 1989
This paper describes techniques for coherently suppressing multipath and other error sources in planar near-field measurements. Of special interest is a simple, yet effective technique of suppressing axial multipath and mutual coupling between the nearfield probe and an antenna. This is of particular value in the testing of low sidelobe antennas. Traditionally, self comparison tests with different separations between the probe and the antenna under test are used to identify the magnitude of multipath errors. What is not generally realized is that these tests can be used to produce a coherent estimate of the induced error, which can often be suppressed. A series of tests was performed with a small X-band phased array antenna, resulting in a reduction of the sidelobe noise background from a 25 dB level to better than 50 dB.
G/T measurement technique for low directivity wide beam antennas
R.P. Heon (Texas Instruments),S. Sanzgiri (Texas Instruments), November 1990
The end-to-end G/T performance of an antenna system has typically been measured using celestial bodies. The technique requires high G/T performance ( 10 dB/K) to obtain accuracies of 0.5 dB. In addition, the measurement is dependent on several atmospheric and environmental conditions. This paper describes a technique for measuring the G/T performance of a low directivity, wide beamwidth antenna. The discussion details the measurements, extrapolation technique to demonstrate performance at specified atmospheric conditions, measurement uncertainties, and test results. This new G/T measurement technique offers advantages over the existing technologies. Measurements are limited to the output port of the antenna so as to include all interactions between components within the system. This allows for accurate characterization of phased array performances. In addition, testing can be performed on indoor antenna ranges under environmentally controlled conditions.
A New implementation of the planar near-field back projection technique for phased array testing and aperture imaging
D. Garneski (Hughes Aircraft Company, Radar Systems Group), November 1990
A new implementation of the planar near-field back projection technique for phased array testing and aperture imaging is described. In the alignment of phased arrays, the aperture field is treated as a continuous distribution rather than using idealized array concepts. The continuous field is then sampled to obtain element excitations. In this way, nonrectangular arrays can easily be accommodated. The method also produces highly interpolated images of apertures that can offer much insight into their nature. Also, any polarization of the aperture field may be obtained if the probe pattern has been characterized. The technique uses large FFTs which are computed very quickly by a workstation located in the facility. Results from an iterative phase alignment of a 12x18 phased array are presented, as well as highly interpolated images of apertures and results which demonstrate the polarization selection.

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