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Localization of NarrowBand Sources in Unknown Spatially Correlated Noise
EURASIP Journal on Advances in Signal Processing volumeÂ 2010, ArticleÂ number:Â 732591 (2010)
Abstract
In subspacebased method for directionofarrival (DOA) estimation of signal wavefronts, the additive noise term is often assumed to be spatially white or known to within a multiplicative scalar. When the noise is nonwhite but has a known covariance matrix, we can still handle the problem through prewhitening. However, the problem turns to be complex when the noise field is completely unknown. In this paper, we study the localization of the sources, when the noise covariance matrix is one unknown band matrix. An iterative denoising algorithm based on the noise subspace spanned by the eigenvectors associated with the smallest eigenvalues is developed. The performance of the proposed algorithm is evaluated by computer simulations. We also test the proposed algorithm with some experimental data recorded during an underwater acoustic experiment.
1. Introduction
Array processing is used in diverse areas such as radar, sonar, communications, and seismic exploration. Usually the parameters of interest are the directions of arrival of the radiating sources. The highresolution subspacebased methods for directionofarrival (DOA) estimation have been a topic of great interest. The subspacebased methods welldeveloped so far require a fundamental assumption, which is that the background noise is uncorrelated from sensor to sensor, or known to within a multiplicative scalar. In practice this assumption is rarely fulfilled and the noise received by the array may be a combination of multiple noise sources such as flow noise, traffic noise, or ambient noise, which is often correlated along the array [1, 2]. However, the spatial noise is estimated by measuring the spectrum of the received data when no signal is present. The data for parameter estimation is then prewhitened using the measured noise. The problem with this method is that the actual noise covariance matrix varies as a function of time in many applications. At low signaltonoise ratio (SNR) the deviations from the assumed noise characteristics are critical and the degradation may be severe for the localization result. A maximum likelihood algorithm is presented in [3], where the spatial noise covariance is modeled as a function of certain unknown parameters. Also in [4, 5] a maximum likelihood estimator is analyzed. The problem of incomplete prewhitening or colored noise is circumvented by modeling the noise with a simple descriptive model. As opposed to AR and ARMA models used in [6] this gives the advantages of incorporating prior knowledge into the model [5, 7]. There are other approaches to the problem of spatially correlated noise: one is based on the assumption that the correlation structure of the noise field is invariant under a rotation or a translation of the array, while another is based on a certain linear transformation of the sensor output vectors [8â€“13].
In this paper, we present an algorithm to estimate the noise with band covariance matrix. This algorithm is based on the noise subspace spanned by the eigenvectors associated with the smallest eigenvalues of the covariance matrix of the recorded data. The goal of the present study is to investigate how the perturbations due to the noise covariance matrix affect the accuracy of the narrowband signal DOA estimates [14â€“18].
The remainder of the paper is as follows. Section 2 presents the high resolution algorithm. Section 3 proposes the model of the additive noise. Section 4 introduces the covariance matrix of the band noise. Section 5 presents the proposed algorithm. Sections 6 and 7 present some comparative results concerning the proposed algorithm exemplified using simulated data and realworld signals in a noisy environment. Section 8 gives the conclusions.
In this paper, we denote by, a scalar, a vector, and X a matrix.
2. Problem Formulation
Consider an array of sensors which receive the signals in one wave field generated by sources in the presence of an additive noise. The received signal vector is sampled and the DFT algorithm is used to transform the data into the frequency domain. We represent these samples by
where , , and are, respectively, the Fourier transforms of the array outputs, the source signals, and the noise vectors. The matrix , with dimensions , is the transfer matrix of the sourcesensor array systems with respect to some chosen reference point. The sensor noise is assumed to be independent of the source signals and partially spatially correlated. The sources are assumed to be uncorrelated. The covariance matrix of the data can be defined by the dimensional matrix
where denotes the expectation operator, superscript represents conjugate transpose, is the noise covariance matrix, and is the signal covariance matrix. The above assumption concerning the noncorrelation of the sources means that is full rank.
The highresolution algorithms of array processing assume that the matrix is diagonal with constant element. The subspacebased techniques are based on these properties. For example the Multiple Signal Classification (MUSIC) [10] nullspectrum is defined by
and it is expected that has maximum points around , where are the directions of arrival of the sources. Therefore, we can estimate the DOA by taking the local maximum points of .
In this paper, we consider that the matrix is not diagonal because the noise realizations are spatially correlated and then the performances of these methods are considerably degraded [16â€“19].
3. Modeling the Noise Field
A fundamental limitation of the standard parametric array processing algorithms is that the covariance matrix of background noise cannot, in general, be estimated along with the signal parameters. So this leads to a unidentifiable parametrization, the measured data should always be regarded to consist on only the noise with a covariance matrix equal to that of the observed samples. This is a reason for imposing a model on the background noise. Several parametric noise models have been proposed in some literatures recently. Here, as well as in [8, 20], a descriptive model will be used, that is, the spatial noise covariance matrix is assumed to be a linear combination of some unknown parameters, which are weighted by known basis matrices. There are two different noise phenomenons to be described. We can model the noise as follows.

(i)
An internal noise generated by the sensors socalled thermal noise. This noise is assumed to be independent [8, 11] from sensor to sensor, but not necessarily spatially white. Then the spatial covariance matrix of this noise denoted is diagonal.

(ii)
An external noise received on the sensors, whose spatial covariance matrix is assumed to have the following structure [8, 11, 12, 19], , where are unknown parameters and are complex weighting matrices, are chosen such that is positive definite and of band structure.
Consequently, the additive noise is the sum of these two noise terms and the spatial covariance matrix is
4. Modeling the Covariance Matrix of the Band Noise
In many applications when a uniform linear array antenna system is used, it is reasonable to assume that noise correlation is decreasing along the array (see Figure 1). This is a widely used model for colored noise. We can then obtain a specific model for noise correlation under the following assumptions:

(i)
the correlation length is which means that the spatial correlation attains up to the sensor;

(ii)
the noise realizations received by sensors which are separated with a distance no less than , where is the distance between sensors, are considered uncorrelated.
The noise correlation model which is obtained is represented on Figure 1.
In this paper the noise covariance matrix is modeled as a Hermitian, positivedefinite band matrix , with halfbandwidth . The element of is with
where ; , are complex variables, , is the noise variance at the sensor, and denotes complex conjugate.
In the following section, an algorithm to estimate the band noise covariance matrix is developed for narrowband signals.
5. Estimation of the Noise Covariance Matrix
5.1. Proposed Algorithm
Several methods have been proposed for estimating the directions of arrival of multiple sources in unknown noise fields. Initially the noise covariance matrix is measured, when signals of interest are not present. Other techniques [5, 7, 21] based on the maximum likelihood algorithm are developed, which incorporate a noise model to reduce the bias for estimating both the noise covariance matrix and the directions of arrival of the sources. In this paper, our approach is realized in two steps. Using an iterative algorithm, the noise covariance matrix is estimated, then this estimate is subtracted from the covariance matrix of the received signals.
As the noise is supposed to be uncorrelated with the source signals, using (3), one can see that element of
where is the element of the matrix . These equations show that the element for â€‰â€‰ and is not impaired by the additive noise. We know also that [12]
where is a diagonal matrix containing the largest eigenvalues and where the matrix contains the corresponding eigenvectors of the covariance matrix . So, we have
Using (9), we obtain a constraint for estimating correctly the largest eigenvalues and the corresponding eigenvectors. Indeed by minimizing the error we can estimate the eigenelements by an iterative algorithm. Then by using (10) we calculate the noise covariance matrix. The proposed method for estimating the noise covariance matrix can be summarized as follows.
Step 1.
Estimate the covariance matrix of the received signals using snapshots: . Calculate the eigendecomposition of this matrix: with and , where , and are, respectively, the eigenvalue and the corresponding eigenvector.
Initialize the noise covariance matrix by, .
Step 2.
Calculate , and . is the matrix of the eigenvectors associated with the first largest eigenvalues of calculated at the first iteration. is the diagonal matrix containing the dominant eigenvalues.
Let .
Step 3.
Calculate the element of the current noise covariance matrix
Step 4.
Eigendecomposition of the matrix . The new matrices and are calculated using the previous steps. Repeat the algorithm until a significant improvement of the estimated noise covariance matrix is obtained.
Stop Test
The iteration is stopped when or the Frobenius norm calculated only with the elements such that for and is a fixed threshold. Symbol stands for Frobenius norm and the superscript "" indicates the iteration.
5.2. Estimation of the Spatial Correlation Length
In the previously proposed iterative algorithm, the spatial correlation length of the noise is supposed to be known. In practice, this is aforehand uncertain, therefore the search for a criterion of an estimate of is necessary. In [21], one algorithm which jointly estimates the number of sources and the spatial correlation length of the noise is presented. We propose to vary the value of until the stability of the result is reached, that is, until the noise covariance matrix does not vary when varies. The algorithm incorporating the choice of the correlation length is presented in Figure 2. In the stop test, we check whether or not.
6. Simulation Results
In the following simulations, a uniform linear array of omnidirectional sensors with equal interelement spacing is used, where is the midband frequency and is the velocity of propagation. The number of independent realizations used to estimate the covariance matrix of the received signals is . The signal sources are temporally stationary zeromean white Gaussian processes with the same frequency . Three equipower uncorrelated sources impinge on the array, with the . The noise power is taken as the average of the diagonal elements of the noise covariance matrix .
To demonstrate the performance of the proposed algorithm, the following three situations are considered:

(i)
BandToeplitz noise covariance matrix, with each element given by a modeling function;

(ii)
BandToeplitz noise covariance matrix with the elements arbitrary chosen;

(iii)
Band noise covariance matrix used in [16].
In each case, two spatial correlation lengths are studied: and .
6.1. Noise Covariance Matrix Estimation and Results Obtained
To localize the directions of arrival of sources and to evaluate the performance of the proposed algorithm, the highresolution methods such as MUSIC [9, 10] are used after the preprocessing, with priori knowledge of the exact number of sources ().
Example 1 (BandToeplitz noise covariance matrix).
In this example, the spatial correlation between the noises is exponentially decreasing along the antenna array and the elements of the noise covariance matrix are expressed as
where is the noise variance equal for every sensor and is the spatial correlation coefficient. The values which are retained are, and .
In each of the two studied cases ( and ), the noise covariance matrix is estimated with a fixed threshold value after a few iterations and we notice that the number of iterations for is greater than that of .
Example 2 (BandToeplitz noise covariance matrix with the elements arbitrary chosen).
In this example, the covariance matrix elements are chosen such that their values are decreasing along the array of antenna. The noise covariance matrix has the same structure as in Example 1

(i)
The parameters used are in the case , , , and . Using the proposed algorithm, the three complex parameters of the noise covariance matrix can be perfectly estimated.

(ii)
For : , , , , and . The proposed algorithm gives good estimates of the simulated parameters.
Example 3 (Band noise covariance matrix using model in [16, Example ]).
The configuration of this experiment contains a tenelement uniform rectilinear array with three sources at , , and (angles are measured with respect to the normal of the array). One hundred snapshots of array data were taken.
Example 3 o (typical correlated noise with sensor spacing ).
where is the noise variance equal for every sensor and is the spatial correlation coefficient. Figure 3 shows the rootmeansquared error versus sensor noise correlation factor over the range from 0 to 0.9. The SNR is held constant at , the number of sensor and the noise spatial correlation length .
Figure 4 presents the rootmeansquared error and the CramerRao bound (CRB) [22] versus signaltonoise ratio over the range from to dB.
Figure 5 shows the RMSE performances of the tested algorithms and the CRB with respect to the number of snapshots.
Figures 4 and 5 show that it is possible to mitigate the estimation error if SNR and/or the number of snapshots increase.
Example 3 t.
In order to study the influence of the estimation of the spatial correlation length on the localisation of the sources, we have considered the same data as in the previous example. The value of is varied over the range 1 to and for each value the number of the sources (number of largest eigenvalues) is estimated after applying the proposed algorithm. Figure 6 shows that the estimation of the number of the sources is sensitive to the choice of . The number of the sources is correctly even the value of is overestimated . Figure 7 shows the variations of the bias of the estimated angles for different values of . When is equal to 5 we obtain good resultsâ€” and very small value of a biasâ€”this conclusion is observed for several scenarios.
Figure 8 shows the norm of the vector difference between the 10 elements of the principal diagonal of the simulated matrix and those of the estimated matrix for and .
Comparing these results, we can remark that when increases the estimation error increases. However, the estimation is still small.
Figures 9(a), 9(b), 10(a), 10(b), 11(a), and 11(b) show the localization results of the sources before and after the preprocessing. Before the preprocessing, we use directly the MUSIC method to localize the sources. Once the noise covariance matrix is estimated with the proposed algorithm, this matrix is subtracted from the initial covariance matrix of the received signals, and then we use the MUSIC method to localize the sources. The three simulated sources are , , and for Figure 9;, , and for Figure 10;, , and for Figure 11. For Figure 10, the SNR value (10â€‰dB) is greater than those of Figures 9 and 11 (â€‰dB).
The comparison of the results of Figures 10 and 11 comes to the conclusion that the MUSIC method cannot separate the close sources without the preprocessing when the SNR is low, so in Figure 10 we can only detect two sources before preprocessing. And for each case we can note that there is an improvement in the results obtained with the preprocessing. Comparing the results of with that of for each figure, we can also reconfirm that when increases, the estimation error increases on the estimated noise covariance matrix, so we obtain better results with the preprocessing for than for .
In order to evaluate the performances of this algorithm, we study, below, the influence of the involved parameter .
6.2. Performance of the Proposed Method versus Noise Spatial Correlation Length
Figure 12 shows the variations of the estimation error of the noise covariance matrix when the spatial correlation length of the noise is increasing from to for two numbers of the sources and with and . This error is defined by, .
These results show that independently of the value the estimation error is null until and increases with value. This increasing estimation error is larger for greater values of .
To study the influence of on the localization, we draw, see Figure 13, according to the spatial correlation length of the noise, the variations of the bias of estimate of the azimuths in the case of three sources localized at , and .
We define that the bias of the estimated directions of the arrival of the sources is calculated by
where
with the number of trials .
The experimental results presented in Figure 13 show that the correlation length also influences the estimate of the DOA values.
The spatial correlation length authorized by the algorithm is a function of the number of sensors and the number of sources. Indeed, the number of parameters of the signal to be estimated is , and the number of parameters of the noise is . In order to estimate them it is necessary that and that . In the limit case: , we have , which corresponds to a bidiagonal noise covariance matrix. If the model of the noise covariance matrix is bandToeplitz [5, 21], the convergence of the proposed algorithm is fast, and the correlation length of the noise can reach .
7. Experimental Data
The studied signals are recorded during an underwater acoustic experiment. The experiment is carried out in an acoustic tank under conditions which are similar to those in a marine environment. The bottom of the tank is filled with sand. The experimental device is presented in Figure 14(a). A source emits a narrowband signal (). In addition to the signal source a spatially correlated Gaussian noise is emitted. The signaltonoise ratio is . Our objective is to estimate the directions of arrival of the signals during the experiment. The signals are received on one uniform linear array. The observed signals come from various reflections on the objects being in the tank. Generally the aims of acousticians is the detection, localization and identification of these objects. In this experiment we have recorded the reflected signals by a single receiver. This receiver is moved along a straight line between position and position with a step of in order to create a uniform linear array (see Figure 14(b)).
Two objects are placed at the bottom of the tank and the emitting source describes a circular motion with a step of by covering the angular band going from to . The signals received when the angle of emission is are shown in Figure 15. This figure shows that there exists two paths, which may correspond to the reflected signals on the two objects. The results of the localization are given in Figure 16. We note that in spite of the presence of the correlated noise our algorithm estimate efficiently the DOA of the reflected signals during the experiment.
Figure 16(a) shows the obtained results of the localization using MUSIC method on the covariance matrices. The DOA of the reflected signals on the two objects are not estimated. This is due to the fact that the noise is correlated.
Figure 16(b) shows the obtained results using our algorithm. The two objects are localized.
8. Conclusion
In this paper the problem of estimating the direction of arrival (DOA) of the sources in the presence of spatially correlated noise is studied. The spatial covariance matrix of the noise is modeled as a band matrix and is supposed to have a certain structure. In the numerical example, the noise covariance matrix is supposed to be the same for all sources, which covers many practical cases where the sources are enclosed.
This algorithm can be applied to the localization of the sources when the spatialspectrum of the noise or the spatial correlation function between sensors is known. The obtained results show that the proposed algorithm improves the direction estimates compared to those given by the MUSIC algorithm without preprocessing. Several applications on synthetic data and experiment have been presented to show the limits of these estimators according to the signaltonoise ratio, the spatial correlation length of the noise, the number of sources, and the number of sensors of the array. The motivation of this work is to reduce the effect of the additive spatially correlated noise for estimating the DOA of the sources.
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The authors would like to express their thanks to the anonymous reviewers for their careful reading and their helpful remarks, which have contributed in improving the clarity of the paper.
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Bourennane (EURASIPMember), S., Fossati, C. & Marot, J. Localization of NarrowBand Sources in Unknown Spatially Correlated Noise. EURASIP J. Adv. Signal Process. 2010, 732591 (2010). https://doi.org/10.1155/2010/732591
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DOI: https://doi.org/10.1155/2010/732591