Research Article  Open Access
Jiaqi Song, Haihong Tao, Jian Xie, Chenwei Sun, "Mixed FarField and NearField Source Localization Algorithm via Sparse Subarrays", International Journal of Antennas and Propagation, vol. 2018, Article ID 3237167, 15 pages, 2018. https://doi.org/10.1155/2018/3237167
Mixed FarField and NearField Source Localization Algorithm via Sparse Subarrays
Abstract
Based on a dualsize shift invariance sparse linear array, this paper presents a novel algorithm for the localization of mixed farfield and nearfield sources. First, by constructing a cumulant matrix with only directionofarrival (DOA) information, the proposed algorithm decouples the DOA estimation from the range estimation. The cumulantdomain quarterwavelength invariance yields unambiguous estimates of DOAs, which are then used as coarse references to disambiguate the phase ambiguities in fine estimates induced from the larger spatial invariance. Then, based on the estimated DOAs, another cumulant matrix is derived and decoupled to generate unambiguous and cyclically ambiguous estimates of range parameter. According to the coarse range estimation, the types of sources can be identified and the unambiguous fine range estimates of NF sources are obtained after disambiguation. Compared with some existing algorithms, the proposed algorithm enjoys extended array aperture and higher estimation accuracy. Simulation results are given to validate the performance of the proposed algorithm.
1. Introduction
In recent years, passive source localization has become a key topic in array signal processing [1]. Various localization algorithms have been proposed for farfield (FF) source, whose wavefronts are plane waves, such as the multiple signal classification (MUSIC) method [2], the estimation of signal parameters via rotational invariance technique (ESPRIT) [3], and their derivatives. Nevertheless, when the radiating sources are located in nearfield (NF) source, whose wavefronts are spherical waves, both the DOA and the range parameters should be determined to localize these radiating sources. As a result, traditional FF DOA estimation algorithms are no longer applicable for NF source localization. Fortunately, many advanced methods have been presented under the NF assumption, including the 2D MUSIC algorithm [4], the highorder ESPRIT algorithm [5, 6], the covariance approximation (CA) method [7, 8], the weighted linear prediction method [9], the generalized ESPRIT algorithm [10, 11], and the signal reconstruction for nearfield source localization [12]. In addition, we also proposed a novel method of passive localization for nearfield noncircular sources [13].
However, both FF and NF sources may coexist in many interested situations such as speaker localization using microphone arrays, seismic exploration, and electronic surveillance. Most of the algorithms, which deal with pure NF or pure FF sources, may fail in the scenarios of mixed sources.
Recently, mixed source localization problem has been an important research topic in array signal processing [14–19]. A twostage MUSIC (TSMUSIC) algorithm [14] was first advanced to localize mixed FF and NF sources. Based on fourthorder cumulant, the TSMUSIC algorithm can successfully estimate the parameters of mixed sources. However, its computational complexity is high due to the construction of highorder cumulant matrices and the spectral search. To relieve the computational burden, an efficient MUSICbased algorithm is proposed in [15], which only utilizes secondorder statistics. Unfortunately, this algorithm suffers from severe array aperture loss and 1D spectral search in both DOA and range estimation. Based on [10], Liu and Sun presented another GESPRITbased algorithm to alleviate the array aperture and obtain a reasonable classification result [16]. Our early works on mixed localization focused on unknown source numbers [17] and unknown mutual coupling [18].
As is well known, the estimation accuracy is directly correlated with the array aperture size that a larger array would produce more precise estimates. However, most of the existing methods limit the array element spacing to be within a quarter wavelength to avoid DOA ambiguity. Recently, a mixedorder MUSIC (MOMUSIC) algorithm [19] was proposed to extend the array aperture by a special nested sparse linear array (SLA), which can improve the estimation accuracy.
In this paper, a novel fourthorder cumulantbased dualsize shift invariance (CDSSI) algorithm is presented to solve the mixed source localization problem. Our technique utilizes a SLA of the dualsize spatial invariance method [20] which was designed by M. D. Zoltowski and K. T. Wong. Furthermore, they also proposed MUSIC/MODE null spectrum disambiguation algorithm [21] aiming to realize more accurate disambiguation. Unlike most of the existing algorithms, our technique utilizes a SLA of dualsize spatial invariance. As a result, the novel method enjoys significant promotion in DOA and range estimation accuracy by extending the intersubarray spacing. Furthermore, the proposed method avoids any 1D or 2D spectral searching and therefore has lower computational complexity.
The rest of the paper is organized as follows. In Section 2, the mixed FF and NF signal model based on SLA is presented. The proposed CDSSI algorithm is described in Section 3. In Section 4, we compare CDSSI with some recently developed ones, and computer simulations are conducted in Section 5 to validate the performance of the proposed algorithms. Finally, we conclude this paper in Section 6.
Notation. The complex conjugate, transpose, Hermitian transpose, and pseudoinverse are denoted by , , , and , respectively. symbolizes the Kronecker product and represents the KhatriRao product (or columnwise Kronecker product), that is, . is a identity matrix.
2. Data Model
Suppose that independent narrowband sources (FF and NF) impinge upon a symmetric SLA, as shown in Figure 1. The array has a total number of sensors, which are composed of 3 subarrays and each subarray contains array sensors, with and being positive integers. This SLA configuration can be considered as a particularization of the sparse rectangular dualsize spatial invariance array in [20].
In Figure 1, the intersensor spacing is , and the intersubarray spacing is , where . The sensor position vector would have the following form, if we take as the length unit.
Let the array center be the phase reference point; the output of the th sensor can be approximated as [5] where represents the DOA of the th source, stands for the distance between the th source and the reference sensor, symbolizes the th source signal, denotes the additive Gaussian noise, and is the number of snapshots. It should be noted that, for the NF source scenario, the range parameter lies in the Fresnel region [22], with symbolizing the array aperture. For the FF source scenario, the range parameter approaches to and the associated parameter becomes 0 [14].
In a matrix form, the array data can be written as where
In the above equations, represents the array steering matrix, denotes the array steering vector for the th source, symbolizes the source signal vector, and is the noise vector.
Given the array data , a novel algorithm is proposed in Section 3 to obtain high performance in localizing and distinguishing the mixed sources successfully, under the following hypotheses. (i)The incoming signals are mutually independent, narrowband stationary, and nonGaussian, as well as nonzero kurtosis.(ii)The DOAs of all source signals differ from each other.(iii)The noise is zeromean, additive (white or color) Gaussian, and statistically independent from all impinging sources.(iv)In order to avoid the phase ambiguity, the intersensor spacing d should be within a quarter wavelength.
3. Algorithm Development
As is shown in Figure 2, the proposed algorithm has two main stages. In the first stage, by constructing a fourthorder cumulant matrix containing only the DOA information, we can decouple the DOA estimation from the range estimation. After the eigendecomposition of , dualsize shift invariance ESPRIT [20] could be applied to generate coarse (unambiguous) and fine (ambiguous) DOA estimates of both NF and FF sources. In the second stage, another fourthorder cumulant matrix needs to be constructed to overcome the rankdeficient phenomenon described in [14]. Moreover, the virtual steering matrix of can be decoupled into two parts and both the coarse and fine range estimates of these sources could be obtained. In both of the two stages, disambiguation is important for the final accurate and unambiguous localization of mixed FF and NF sources. The proposed CDSSI algorithm is described in detail in the following subsections.
3.1. DOA Estimation
3.1.1. Cumulant Matrix for the DOA Estimation
Similar to the TSMUSIC algorithm in [14], we first construct a fourthorder cumulant matrix to estimate the DOAs of the radiating sources in this subsection. However, there are some differences between the two algorithms. For example, (1) the uniform linear array (ULA) configuration in TSMUSIC is generalized to a SLA in Figure 1, which promotes the estimation accuracy effectively and (2) the proposed method utilizes ESPRIT to generate the DOA estimation, which avoids the spectral search procedure in TSMUSIC and therefore reduces the computational complexity.
According to the definition in [23], the fourthorder cumulant of the array outputs , , , and can be written as where symbolizes the kurtosis of the th source.
We can construct a cumulant matrix , with its th element being
Note that can be written in a matrix form where
From (1), can be written as where herein, is the virtual steering matrix for each subarray in the cumulant domain, with the following form:
Therefore, can be expressed as
The reason to rewrite it in this manner is that it has a similar form of dualsize invariance and therefore, ESPRIT could be applied to yield coarse and fine estimates of DOAs.
3.1.2. Fine DOA Estimates with Ambiguities
We firstly estimate the DOAs of the mixed FF and NF sources. By taking an eigendecomposition of (17), we have where and are diagonal matrices containing large eigenvalues and small eigenvalues, respectively. is the eigenvector matrix spanning the noise subspace of . is the signal subspace eigenvector matrix of , which can be expressed as where is a nonsingular matrix.
To obtain highaccuracy DOA estimates, we may form two matrices that are related by the extended intersubarray spacing along the axis. As is illustrated in Figure 3, by taking the first and the last rows of , we have the following two matrices. where and are the first and the last 2 rows of and . Since is contributed by the cumulant domain data from all sensors at and and is contributed by the cumulant domain data from all sensors at and , fine DOA estimates can be found from due to the extended invariance relationship.
From (20), we have , which means that there is a rotational invariance between and , that is, . Therefore, the diagonal elements of , , correspond to the eigenvalues of . As and , we can find a series of ambiguous DOA estimates where is an integer and and represent the ceil (round toward positive infinity) and floor (round toward negative infinity) operation in MATLAB, respectively. returns the phase angle of the operand, which lies between .
3.1.3. Coarse DOA Estimates without Ambiguities
For the purpose of disambiguation, unambiguous but coarse DOA estimates must be obtained as references to the ambiguous fine estimates in the previous subsection. From Figure 4, by extracting the cumulant domain information of the first and the last sensors in each subarray, the quarterwavelength spatial invariance of the array geometry can be exploited to generate unambiguous coarse DOA estimates. This can be easily done by defining a permutation matrix where signifies the th column of the identity matrix .
By taking the first and the last rows of , we obtain the following two matrices. where and are the first and the last rows of , respectively. . Since is contributed by the cumulant domain data from the first sensors in each subarray and is contributed by the cumulant domain data from the last sensors in each subarray, unambiguous DOA estimates with quarterwavelength spatial invariance can be found from .
From (26), we have , which means that there is a rotational invariance between and , that is, . Therefore, the diagonal elements of , , correspond to the eigenvalues of . The unambiguous coarse DOA estimates of mixed FF and NF sources are given by and may be paired by the method in [20].
3.1.4. Disambiguation
The coarse estimates could be used as references to disambiguate the cyclic ambiguities in . Mathematically, we obtain the disambiguated angle estimates as where the estimate of is given by
Note that is solved through searching over a few discrete points and the searching range is given by (22).
3.2. Range Estimation
3.2.1. Cumulant Matrix for the Range Estimation
In order to derive the range estimates, another fourthorder cumulant matrix needs to be constructed to overcome the rankdeficient phenomenon described in [14]. The virtual steering matrix for range estimation in [5] has the following form
If the th source is in FF, the electrical angle will become 0 and the th column of will be . When the number of FF sources is more than one, will drop rank and thus the algorithm will fail to localize radiating sources.
In this section, a new fourthorder cumulant matrix is defined, with its th element being
Note that can be expressed as where is the steering matrix in (6) and is the kurtosis diagonal matrix of sources as defined in (12). When the th source is in FF, the corresponding column vector becomes
Therefore, will still be of full column rank when there are multiple FF sources.
3.2.2. Unambiguous and Ambiguous Range Estimations
From (1) and (7), can be decoupled as where is a matrix which only contains the DOA information and is a column vector which only depends on .
By taking an eigendecomposition of , we can obtain a signal subspace matrix and a noise subspace matrix , where is composed of the principle eigenvectors of and contains the remaining eigenvectors.
According to [4], the 2D MUSIC spectrum for DOA and range estimation is given by
Substituting the disambiguated DOA estimates into the above equation, the 2D spectrum search can be reduced to the 1D ones. Therefore, the estimates of are given by
Actually, (37) implies that is the eigenvector associated with the minimum eigenvalue of the Hermitian matrix . Through the eigendecomposition of , we can obtain an estimation of .
In order to generate the coarse range estimates unambiguously, can be estimated as where represents the th element in . From (3), the coarse range estimate is given by where is the disambiguated DOA estimation. According to the definition of the Fresnel region, NF sources are located in the range of . As a result, when is in this region, the corresponding source is classified as a NF one; otherwise, it is regarded as a FF one.
Similarly, through the extended aperture size between each subarray, fine range estimates with ambiguity can be generated. From (35), we have
Therefore, we can find a series of ambiguous range estimates
3.2.3. Disambiguation
In an analogous manner to that of Section 3.1.4, the coarse estimates could be used as references to disambiguate the cyclic ambiguities in . Mathematically, the disambiguated range estimates are where the estimate of is given by
Note that is solved through searching over a few discrete points, and the searching range is given by (42).
4. Discussion
In this section, we compare CDSSI with some recently developed mixed source localization algorithms, including TSMUSIC [14], the generalized ESPRITbased (GESPRIT) algorithm [16], and MOMUSIC [19]. All of the four methods are analysed from the following aspects:
4.1. Array Aperture
Both TSMUSIC and GESPRIT employ an ULA which requires the intersensor spacing to be within a quarter wavelength. Therefore, with the same sensor number, SLA enjoys extended array aperture size, producing better estimation accuracy for the proposed algorithm. MOMUSIC also utilizes a special nested SLA in the development of the algorithm. However, according to the array model described in [19], the array aperture of MOMUSIC equals to when and (9 sensors in all), while the array aperture of CDSSI, with the same number of sensors, could be extended by spacing subarrays apart at tens of quarter wavelengths or more [20].
4.2. Maximum Number of Sources That Can Be Resolved
In CDSSI, the coarse and fine DOA estimates are derived from two matrices and two matrices, respectively; therefore, the maximum number of sources that can be resolved is . For MOMUSIC algorithm, a virtual ULA with sensors can be constructed. However, it has a half aperture loss in the formation of a Toeplitz matrix, and therefore, it can resolve sources at most. With a element ULA, TSMUSIC is capable of resolving up to sources, while GESPRIT can resolve a maximum number of sources.
4.3. Computational Complexity
Only the major computation load is considered in this comparison, including construction of the cumulant matrices, eigenvalue decomposition (EVD), and spectral search. The searching steps for the angle parameter and the range parameter are denoted as and . Let and symbolize the snapshot number and sensor number, respectively. For MOMUSIC, we assume that , and therefore, the sensor number is . TSMUSIC involves computing two fourthorder matrices with dimensions and , two EVDs, and spectral search for DOA estimation. The GESPRIT algorithm requires the construction of two secondorder covariance matrices, two EVDs, and spectral search for DOA and range estimation. MOMUSIC requires the construction of a fourthorder cumulant matrix and a secondorder covariance matrix, two EVDs, and spectral search for DOA and range estimation. CDSSI does not need any spectral search operation but requires two fourthorder cumulant matrices with dimension , EVDs on , , , , and ( times). The computational complexity of the four methods is listed in Table 1.

Compared with the secondorderbased methods, CDSSI requires more computations in constructing the fourthorder cumulant matrix and EVDs. However, it avoids any 1D or 2D complicated spectral search. Since the search steps need to be dense enough for the spectral searchbased algorithms to approach their theoretical bounds, the computation load of these algorithms will in turn increase dramatically.
4.4. Performance in Correlated Noise
Both TSMUSIC and the proposed algorithm are capable of suppressing additive Gaussian colored noise since they apply fourthorder cumulant in the whole estimation procedure, while GESPRIT and MOMUSIC, which rely on the secondorder statistics, will degrade in the presence of spatially correlated noise.
4.5. Arc Length and FirstOrder Curvature
Furthermore, knowledge of the “manifold shape” not only is essential for the investigation of ambiguities and assessment of the detectionresolution capabilities of an array but it may also prove useful in developing new and more effective methods for its search process. We studied on the two array manifold properties, namely, arc length and firstorder curvature, and analyse the accuracy and resolution capabilities of mixed sources [24].
It has been shown that the response of sparse array towards a farfield/nearfield source emitting narrowband spherical wavefront from azimuth and range can be written as where the associated parameter is , , and is the sensor position vector.
For the farfield source scenario, the range parameter approaches to and the associated parameter becomes 0.
The rate of change of arc length and firstorder curvature of the parameter curves are as follows: where implies differentiation with respect to and the arc length is defined as
The CramerRao lower bound under the assumption of spatially and temporally uncorrelated large number of snapshots may be written as where the unitnorm tangent vector to the array manifold has been substituted for .
The expression of the asymptotic () variance for a single emitter of unit power can be written as
The variance asymptotically approaches the CRB for high SNR or large N and has a similar dependence on .
Figures 5, 6, and 7 show the CramerRao lower bound capabilities of our proposed sparse array. Figures 5 and 6 indicate the variation of theoretical CRB with respect to the change of . Figure 7 shows the theoretical CRB with respect to the change of snapshot. From Figures 5 and 6, we can see that the smaller the angle with the normal direction of array, the less the estimation error and when the range between the array and source is enlarged, the theoretical estimation performance becomes worse. And we can conclude that more sample data can improve estimation performance from Figure 7.
In addition, the angle and range estimation accuracy is not only related to the intersubarray spacing of sparse but also related to the possibility of disambiguation. As the intersubarray spacing increases, the possibility of wrong disambiguation increases simultaneously. The MIE method [25] can be used to predict MSE performance; the angle and range estimation can be represented as where and denote the estimation value and true value of angle and range parameters, is the possibility of right disambiguation, and is the possibility of wrong disambiguation.
5. Simulation Results
In this section, numerical simulations are conducted to validate the performance of the proposed algorithm relative to TSMUSIC, GESPRIT, and MOMUSIC. In the following experiments, we consider a SLA composed of elements with for the proposed algorithm, a quarterwavelengthspaced ULA consisting of 15 elements for TSMUSIC and GESPRIT, and a sparse nested array with 9 elements for the MOMUSIC algorithm. NF sources are set to lie in a common Fresnel region of these algorithms. Moreover, the source signals are equipower, statistically independent, and of the form , where the phase is uniformly distributed between . The performance is measured by the root mean squared error (RMSE) of 500 independent Monte Carlo trials. The RMSE is defined as where stands for the DOA or the range and denotes the estimation of in the th trial.
In the first experiment, we consider two equipower sources that are located at and , that is, a mixed FF and NF scenario. The number of snapshots equals to 500, and the SNR varies from −10 dB to 20 dB in steps of 3 dB. The RMSEs of the four algorithms as a function of SNR are plotted in Figure 8. From these figures, one can observe that the coarse DOA and range estimates of the proposed algorithm have higher RMSEs due to the quarterwavelength spatial shift invariance. However, after disambiguation, the fine estimates have superior estimation accuracy than those of the other three algorithms. Moreover, RMSEs of the DOA and range estimates decrease as the SNR increases.
(a)
(b)
In the second experiment, we investigate the RMSEs of the four algorithms with the variation of the number of snapshots. The parameter settings are the same as those of the first experiment except that SNR is set equal to 10 dB and the number of snapshots varies from 100 to 10,000. From Figure 9, it is obvious that, as a result of the extended aperture, CDSSI outperforms the other three algorithms in DOA and range estimation accuracy for all snapshot numbers. In addition, both the DOA and range estimation performance of all four algorithms improves as the snapshot number increases. This is because that larger sample support will produce better estimate of the covariance matrix for stationary data.
(a)
(b)
In the third experiment, the scenario of two NF sources is investigated, with the source location parameters being and . The snapshot number is fixed at 500 and the SNR varies from −10 dB to 30 dB in steps of 5 dB. Figure 10 leads to a similar conclusion as in the first experiment that the proposed algorithm achieves the best performance owing to its extended aperture. Additionally, from the second figure, one can observe that the range estimation accuracy of the first source, which is closer to the array, is better than that of the second source. This result is consistent with the theoretical analysis developed in [6].
(a)
(b)
In the fourth experiment, we study the dependence of DOA and range estimation accuracy upon the angular gap between two NF sources. varies form to in steps of , while , , and , with the snapshot number and the SNR equal to 500 and 10 dB, respectively. The RMSEs of the angle and range estimation are shown in Figure 11. From these figures, one can see that CDSSI is superior to the other three algorithms in the performance of both DOA and range estimation for all values. In addition, there is a similarity in Figure 11 that the range estimation accuracy of the first source decreases with the growth of , while that of the second source remains almost constant. This phenomenon can be explained as follows: in all the four algorithms, range estimates are based on the estimation of DOAs and the DOA estimation errors are propagated to the subsequent range estimation.
(a)
(b)
In the fifth experiment, the range parameter of the first source varies from to in steps of , while the range of the second source is fixed at . The DOAs of the two sources are and . Let the snapshot number and SNR be 500 and 10 dB, respectively. The influence of on the DOA and range estimation is shown in Figure 12. From the first figure, it is obvious that the DOA estimation performance is insensitive to the change of the range parameter, since the DOA estimation is decoupled with the range estimation in all these algorithms. However, the GESPRIT algorithm behaves abnormally when the range of the first source approaches to (the range parameter of the second source). This is because when the two sources are symmetrical with respect to the broadside, that is, and , the GESPRIT algorithm will generate image sources, which are misidentified as real ones. Moreover, the second figure reveals that (1) the range estimation performance of the second source is hardly affected by the range variation of the first source and (2) the range estimation accuracy of the first source (closer to the array) is superior to that of the second one, which corroborates the theoretical analysis in [6]. Finally, from Figure 12, it is clear that the proposed algorithm outperforms the other three methods in both DOA and range estimation for all range parameters.
(a)
(b)
In the last experiment, two FF sources are considered with their location parameters being and . The snapshot number is fixed at 500 and the SNR varies from −10 dB to 20 dB in steps of 3 dB. Note that the intersubarray spacing is extended from to without introducing additional sensors. The RMSEs of the DOA estimates with the variation of SNR are shown in Figure 13. From this figure, it is seen that all of the four algorithms are still effective in the multiple FF source scenarios and CDSSI outperforms the other three in the performance of DOAs estimation. Also, one can observe that as the intersubarray spacing becomes larger, the accuracy of the proposed method turns better compared with the results demonstrated in Figure 2.
6. Conclusion
In this paper, an efficient and highperformance algorithm is proposed for the mixed farfield and nearfield source localization problems. Based on a sparse linear array of dualsize spatial invariance, the proposed algorithm can offer enhanced accuracy due to the extended aperture size. Moreover, the proposed method has lower computational complexity because it does not require any 1D or 2D spectral search. According to the simulations, the proposed algorithm outperforms the conventional ones in the performance of both angle and range estimation.
Conflicts of Interest
The authors declare that there is no conflict of interest regarding the publication of this paper.
Acknowledgments
This work is supported by Natural Science Foundation of China (no. 60971108 and no. 61601372).
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Copyright © 2018 Jiaqi Song et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.