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Diss / (Springer Series in Information Sciences 25) S. Haykin, J. Litva, T. J. Shepherd (auth.), Professor Simon Haykin, Dr. John Litva, Dr. Terence J. Shepherd (eds.)-Radar Array Processing-Springer-Verlag

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292 T.V. Ho and J. Litva

Dr. Bill Gabriel for carefully reading the chapter and for his comments on the completeness of the material contained herein. As well, we wish to thank Dr. Terry Shepherd for providing a critical and valuable review of the chapter. Finally, we wish to thank a close colleague, Dr. S. Haykin, for helpful suggestions and comments.

References

6.1R.A. Monzingo, T.W. Miller: Introduction to Adaptive Arrays (Wiley, New York 1980)

6.2S. Haykin (ed.): Array Signal Processing (Prentice-Hall, Englewood Cliffs, NJ 1985)

6.3c.R. Ward, A.J. Robson, P.J. Hargrave, J.G. McWhirter: Application of systolic arrays to adaptive beamforming, lEE Proc. Vol, 131, Pt. F, 638--645 (1984)

6.4c.R. Ward, P.J. Hargrave, J.G. McWhirter: A novel algorithm and architecture for adaptive digital beamforming. IEEE Trans. AP-34, 338-346 (1986)

6.5J.V. McCanny, J.G. McWhirter: Some systolic array developments in United Kingdom. IEEE

Comput. Mag. 20 (7), 1-63 (1987)

.

6.6D.M. Boroson: Sample size considerations for adaptive arrays. IEEE Trans. AES-16, 842-845 (1980)

6.7W.F. Gabriel: Spectral analysis and adaptive array superresolution techniques. Proc. IEEE 68, 654-666 (1980)

6.8R.T. Compton, Jr.: Improved feedback loop for adaptive arrays. IEEE Trans. AES-16, 159-168 (1980)

6.9D.J. Chapman: Partial adaptivity for large array. IEEE Trans. AP-24, 685-695 (1976)

6.10E. Brookner, J.M. Howell: Adaptive-adaptive array processing. Proc. IEEE, 74, 602-607 (1986)

6.11V.U. Reddy, A. Pauiraj, T. Kailath: Performance analysis of the optimum beamformer in the presence ofcorrelated sources and its behaviour under spatial smoothing. IEEE Trans. ASSP- 35,927-936(1987)

6.12T.J. Shan, T. Kailath: Adaptive beamforming for coherent signals and interferences. IEEE Trans. ASSP-33, 527-536 (1985)

6.13W.F. Gabriel: Using spectral estimation techniques in adaptive processing antenna systems. NRL Report 8920 (October 1985)

6.14A.P. Howells: Intermediate frequency side-lobe canceller. U.S. Patent 3202990 (Aug. 24, 1965)

6.15S.P. Applebaum: Adaptive arrays. Syracuse Univ. Res. Corp., SPL TR 66-1, (Aug. 1966)

6.16B. Widrow, P.E. Mantey, L.J. Griffiths, B.B. Goode: Adaptive antennas systems, Proc. IEEE 55,2143-2159 (1967)

6.17L.J. Griffiths: A simple adaptive algorithm for real-time processing in antennas arrays. Proc. IEEE 57,1696-1704 (1969)

6.18O.L. Frost III: An algorithm for linearly constrained adaptive signal processing. Proc. IEEE 60, 926-935 (1972)

6.19M. Klemes: A practical method for obtaining constant convergence rates in LMs adaptive arrays. Trans. IEEE AP-34, 440-446 (1986)

6.20I.S. Reed, J.D. Mallett, L.E. Brennan: Rapid convergence rate in adaptive arrays. IEEE Trans. AES-IO, 853-863 (1974)

6.21J. Capon: Probability distributions for estimators of the frequency wavenumber spectrum. Proc. IEEE 58, 1785-1786 (1970)

6.22J.E. Hudson: Adaptive Array Principles (Peregrinus, Stevenage, UK 1981)

6.23B. Widrow, S.D. Steams: Adaptive Signal Processing (Prentice-Hall, Englewood Cliffs, NJ 1985)

6.24R.T. Compton, Jr.: Adaptive Antennas: Concepts and Performance (Prentice-Hall, Englewood Cliffs, NJ 1988)

6.25S. Haykin: Adaptive Filter Theory (Prentice-Hall, Englewood Cliffs, NJ 1986)

6.26Special Issue on Adaptive Arrays. IEEE Trans. AP-24, (Sept. 1976)

6. Two-Dimensional Adaptive Beamforming

293

6.27Special Issue on Adaptive Processing Antenna Systems. IEEE Trans. AP-34, (March 1986)

6.28W.F. Gabriel: Adaptive arrays-an introduction. Proc. IEEE 64, 239-272 (1976)

6.29H.T. Kung, W.M. Gentleman: Matrix triangularization by systolic arrays, in Real-Time Signal Processing IV, Proc. SPIE 298, 19-26 (1981)

6.30J.G. McWhirter: Recursive least-squares minimization using a systolic array, in Real-TJme Signal Processing VI, Proc. SPIE 431, 105-112 (1983)

6.31R.T. Compton: An adaptive array in a spread-spectrum communication system. Proc. IEEE 66, 289-298 (1978)

6.32J.H. Winters: Spread spectrum in a four-phase communication system employing adaptive antennas. IEEE Trans. COM-30, 929-936 (1982)

6.33H. Steyskal, J.F. Rose: Digital beamforming for radar systems. Microwave 32, 121-136 (1989)

6.34G.H. Golub: Numerical methods for solving linear least-squares problems. Numer. Math. 7, 206-216 (1965)

6.35W. Givens: Computation ofplane unitary rotations transforming a general matrix to triangular form. J. SIAM 6, 26-50 (1958)

6.36W.M. Gentleman: Least-squares computations by Givens transformations without squareroots. J. Inst. Math. Appl. 12,329-336 (1973)

6.37T.V. Ho, J. Litva: Systolic array for 2D adaptive beamforming, IEEE Int'I Conf. on Systolic Arrays, San Diego, CA, May (1988)

6.38M.M. Hadhoud, D.W. Thomas: The two-dimensional adaptive LMS algorithm. IEEE Trans. CAS-35, 485-494 (1988)

6.39S.T. Alexander, S.A. Rajala: Image compression results using the LMS adaptive algorithm. IEEE Trans. ASSP-33, 712-714 (1985)

6.40Y.L. Hong, C.c. Yeh, D.R. Ucci: The effect of a finite-distance signal source on a far field steering Applebaum array-two-dimensional array case. IEEE Trans. AP-36, 468-475 (1988)

6.41M.P. Ekstrom: Realizable Wiener filtering in two-dimensions. IEEE Trans. ASSP-30, 31-40 (1982)

7. The Radio Camera

B.D. Steinberg

With 11 Figures

The radio camera is an instrument for taking high-resolution two-dimensional pictures with long wavelengths. The wavelength with which the experimentation reported in this chapter has been accomplished is 3 em, which is 4-5 orders of magnitude longer than optical or near infrared radiation. The resolution of an imaging instrument is the order of the wavelength divided by the size of the aperture. Hence, microwave apertures need to be 4-5 orders ofmagnitude larger than optical apertures to achieve the same resolving power. The 50 mm diameter lens of a small telescope has a resolution of 10 J.1rad or 2 arc sec. At a wavelength of 3 cm, an aperture of 3 km is required to achieve the same resolution.

The reason for the use of the long wavelength is its ease of penetration of weather; the penalty is the huge antenna size required., and the concomitant engineering problems that result.

7.1 Problems

There is one fundamental problem, and several key problems ofpracticality. The fundamental problem is the mechanical or geometric instability of a large system. The required surface tolerance of a diffraction limited aperture is about one-tenth wavelength to prevent degeneration of the main lobe of the radiation pattern; it is three to ten times finer than that to ensure that the sidelobes do not appreciably deteriorate [7.1]. Thus, the surface tolerance must be held to one part in 106 to one part in 107 of the aperture size. An imaging aperture of hundreds of meters to tens of kilometers in size will surely be a phased array rather than a dish. The locations of the centers of phase of the antenna elements must be known to within this tolerance. Furthermore, variations in the driving point impedances of the antenna elements due for example to differences in the electromagnetic coupling of the antenna elements to their local environments must also be taken into account in the tolerance budget. The same is true for phase variations in the receiver channels following the elements, drifts in the local oscillators and mistunings of phase detectors.

Many of the electrically induced phase errors can be corrected by tuning based upon the electrical insertion of signals at the front end. The situation is

Springer Series in Information Sciences, Vol. 25

Radar Array Processing

Eds.: S. Haykin J. Litva T. J. Shepherd

© Springer-Verlag Berlin, Heidelberg 1993

296 B.D. Steinberg

different for mechanically-induced phase errors resulting from geometric distortion. For this situation signals must arrive at the distorted array from outside the system; these signals must be measured by the system after all the distortioninducing sources have operated, and a wavefront or phase aberration correction deduced from the measurements.

This procedure is called adaptive beamforming, to which the acronym ABF is given in this chapter.

The remaining difficult problems are matters of practicality. A two-dimen- sional optical aperture 105 wavelengths in diameter is a relatively simple device. The corresponding microwave phased array is a horror, however. Its area is the order of 1010 square wavelengths, with elements spaced A./2 to ensure the avoidance of grating lobes. The number of antennas, phase-shifters for beam steering, and receivers are about 4 x 1010Drastic thinning by several orders of magnitude is required to constrain cost. Thinning can be periodic, provided that procedures are introduced that avoid the problems of grating lobes, or aperiodic.

A second practical problem is the cost and complexity of the intra-array communications subsystem. Its function is to transfer the signals received at the array elements to the signal processor. The number of communication channels equals the number of antenna elements. Call this number N. Each channel is sampled at the rate B, which is the order of the signal bandwidth. Each sample is quantized into b bits. The product N Bb is the data transmission rate. It is easily shown that this number can be excessively large. Consider a one-dimensional linear array of 105 wavelengths designed to provide a resolution cell of 1 meter in both range and cross range. The number of antenna elements in a filled array is N = 2L/A., and the signal bandwidth is 150 MHz. Each I/Q component of the coherently demodulated signal will be quantized to 6-8 bits. Therefore, b = 12-16. The product NBb exceeds 1014 bps, which is larger by several orders of magnitude than the transmitter frequency, and is hopelessly beyond our technological capability. N is reduced by thinning; b can also be reduced to some extent.

7.2 Adaptive Beamforming: Dominant Scatterer Algorithm

Figure 7.1 shows a badly distorted receiving antenna array in the upper-left portion. Each receiving element drives a coherent receiver, whose outputs are sampled and stored. The transmitter, also shown in the upper-left, radiates a short pulse toward the target area to be imaged. A prominent scatterer, modeled as a corner reflector in the figure, is in the general direction of the target region. The illuminating beam is broad in azimuth, as is common in radar; the beamwidth is typically a few degrees. This beamwidth defines the instantaneous field of view of the imaging system. That is, the system can only image those targets that are illuminated by the transmitter. A typical received waveform is

298 B.D. Steinberg

the dominant reflector are very small compared to Ro. Not so with the phases, however. A shift in element position by only one-halfwavelength in the direction toward the corner reflector changes the two-way phase delay by a full wavelength. Thus, the amplitudes at range Ro are nearly constant, while the phases vary randomly from element to element.

The capability for imaging with conventional electronic scan. is lost under this condition. However, the random set of phases in the Ro column carries information disclosing the effect of the distortion; these phases reflect the differential distances, modulo wavelength, of the two-way paths between the transmitter and the receiving elements. By introducing a weight vector into the set of receivers, whose components are the negatives ofthe phases of the received signals, proper compensation is effected. This process is called phase conjugation. A superior procedure is to assign the complex conjugate of the column vector at Ro to the weight vector in the receiver.

Either process counter-phase rotates all the echo samples in the Ro column to a common phase, which may be taken to be O. This 0 is exactly the process performed by a conventional phased array system (or a lens or a microwave dish) when focusing upon a target; that is, all signals from the target are cophased within the system, in preparation for adding them to form the output.

Phase conjugation, then, focuses the badly distorted system upon the reference reflector. The system can be refocused simultaneously to all range bins by applying the Fresnel (quadratic) connection to the phases. The beam, pointing in the direction of the reference reflector and focused simultaneously at all ranges, is then scanned from left to right by conventional electronic scan procedures.

The steps in the algorithm are summarized in Table 7.1. A detailed description of the process is found in [7.2J.

Table 7.1. Steps in radio camera imaging. (From [7.2])

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7.3 Experiments

This algorithm has been used repeatedly at the Valley Forge Research Center of the University of Pennsylvania over the last decade and a half. It is a very robust procedure. The echo from the dominant scatterer need only be 4 dB larger than the sum of all the echoes from the clutter. Figure 7.2 shows a high-resolution image of a street of row houses in a town about 6 km from the laboratory [7.4J. The phased array was highly distorted; the distortion was estimated to be about one wavelength rms in all dimensions. The diffraction-limited image obtained with the dominant scatterer algorithm exhibits cross range resolution of 3 m,

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300 B.D. Steinberg

consistent with the antenna size (83 m), wavelength (3 em) and target range. The range resolution was 3 m, determined by the duration of the 20 ns pulse. The lower portion of the figure shows the image from the same data set without adaptive beamforming. It is a useless jumble of pixels. Adaptive beamforming converted a hopeless condition into a useful imaging procedure. Figure 7.3

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7. The Radio Camera

301

shows a suburban housing development 4.5 km from the laboratory. Each clump of pixels is a single house. The houses are spaced by approximately 20 m. Streets and backyards are evident. The cross range resolution in Figs. 7.2 and 3 is comparable to human vision.

The same algorithm can be applied to a succession of pulse echoes received from a moving target by a monostatic radar. The technique is called inverse synthetic aperture radar (ISAR). The line of sight direction to the target changes from pulse to pulse due to the target motion (Fig. 7.4, left). From a frame of reference on the target (right), the apparent location of the radar moves from pulse to pulse. This sequence of apparent locations forms a synthetic aperture. The pulse sequence received by the radar is treated as if each pulse train came from a different antenna element. The data are laid down in a store exactly as in Fig. 7.1, and are processed as in Tablet.l. An example of the result is shown in Fig. 7.5, which is a high-resolution two-dimensional image of a Boeing 727 flying into Philadelphia International Airport. This ISAR image was obtained with adaptive beamforming. The bottom of the figure is the image of the same data when adaptive beamforming was not included. Again, the comparison is striking.

The two techniques can be performed simultaneously to provide a combined spatial-temporal radio camera. Figure 7.6 shows the result of such an experiment. The receiver was a two-element interferometer in which the elements were spaced at 25 m. Eighty-five echo traces were obtained from each receiver from a

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Fig. 7.4. It is also possible to apply radio camera processing to a sequence of echoes from a moving target, received by a single antenna. An inverse synthetic aperture is formed. Adaptive beamforming corrects for distortion in the synthetic aperture caused by flight-path deviations. Image processing is the same as in the spatial radio camera. (From [7.5])