Abstract

Linear sparse arrays (coprime and nested arrays) have been studied extensively as a means of performing direction of arrival (DoA) estimation while bypassing Nyquist sampling theorem. However, rectangular sparse arrays have few studies, most of which are based in lattice theory. Although the multiple signal classification (MUSIC) alogrithm can be applied to lattice theory-based sparse arrays, fewer DoAs can be estimated for these arrays than for a full array with the same aperture. One contribution of this paper is the formulation of symmetry-imposed rectangular coprime and nested array designs that have wider contiguous lags than lattice-based arrays. Also, existing algorithms for rectangular arrays employ the direct sample covariance matrix estimate, which has low accuracy. Another contribution of this paper is an alternate method for estimating the covariance matrix that ensures the matrix is block-Toeplitz. Using the proposed covariance matrix estimate, we integrate a MUSIC-based DoA estimation method that applies to both full arrays and sparse arrays. The results show that the covariance estimates produced by the proposed method have higher accuracy than the traditional sample covariance estimates. The results also demonstrate that symmetry-imposed sparse arrays have higher resolution than full rectangular arrays with the same number of sensors.

Highlights

  • Estimation of a propagating signal’s direction of arrival (DoA) is a vital task used by applications including sonar, radar, radio astronomy, and seismology

  • We stressed the importance of the block-Toeplitz property for the spatial covariance matrix of a rectangular array

  • We provided an algorithm to estimate the covariance matrix that applies to all three arrays—URA, symmetry-imposed RNA (SIRNA), and symmetry-imposed rectangular coprime array (SIRCA)

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Summary

INTRODUCTION

Estimation of a propagating signal’s direction of arrival (DoA) is a vital task used by applications including sonar, radar, radio astronomy, and seismology. A fascinating feature of coprime and nested arrays is that they have a contiguous (hole-free) coarray with approximately the same length as a full uniform linear array (ULA) with an equal aperture This feature facilitates the estimation of all elements of the covariance matrix estimate. A limitation of both sparse and full arrays is that existing two-dimensional DoA estimation algorithms use the direct sample covariance matrix, which has low accuracy. This paper overcomes both these limitations, making the following contributions: 1) New two-dimensional coprime and nested array designs, designated SIRNA (Section III-C) and SIRCA (Section III-F), in which the range of contiguous lags is comparable to that of a full URA with equal aperture. FPD(A) denotes the fundamental paraellepiped of A [39], [41]

LAGS AND COVARIANCE MATRIX OF A
SYMMETRY-IMPOSED RECTANGULAR NESTED ARRAY
BIAS REMOVAL FROM ACF ESTIMATES MATRIX
BLOCK-TOEPLITZ CONVERSION FOR
IMPLEMENTATION OF MUSIC WITH THE ESTIMATED COVARIANCE MATRIX
EVALUATION OF THE SPATIAL PSEUDOSPECTRUM WITH FULL URA
COMPARISON OF THE MEAN SQUARED ERRORS
Findings
CONCLUSION
Full Text
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