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an author's https://oatao.univ-toulouse.fr/22991

https://doi.org/10.1109/RADAR.2015.7131013

Bidon, Stéphanie and Lasserre, Marie and Besson, Olivier and Le Chevalier, François Bayesian sparse estimation of targets with range-Doppler grid mismatch. (2015) In: IEEE Radar Conference (RadarCon 2015), 10 May 2015 - 15 May 2015 (Arlington, United States).

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Bayesian Sparse Estimation of Targets

with range-Doppler grid mismatch

St´ephanie Bidon, Marie Lasserre, Olivier Besson

DEOS University of Toulouse/ISAE Toulouse, France Email: firstname.lastname@isae.fr

Franc¸ois Le Chevalier

MS3

Delft University of Technology Delft, The Netherlands Email: F.LeChevalier@tudelft.nl

Abstract—In this paper, we study the problem of estimating the target scene via a signal sparse representation (SSR) scheme in the range-Doppler domain. As compared to a range-gate by range-gate SSR analysis, this bidimensional approach can take into account targets straddling two range-gates. Here, we propose a robust SSR Bayesian algorithm that considers the well known grid mismatch problem in both the range and Doppler dimensions. Our algorithm implements a bidimensional approach to a previous described algorithm. Numerical simulations are performed with synthetic and experimental data to demonstrate the benefit of estimating the grid mismatch with the proposed technique.

I. INTRODUCTION

A significant attention has been lately devoted by the radar community to the design of sparse representation techniques. SSR methods are applied when the radar signal can be described by a small set of atoms from a dictionary. Due to its deconvolving property, the SSR approach allows for the signal of interest to be represented without sidelobes thereby enhancing the contrast of the estimated radar scene.

The SSR is of particular interest to represent moving targets in the Fourier basis; assuming the latter can be modeled by point-like scatterers in the Doppler domain. Nonetheless, performing a range-gate by range-gate SSR analysis can yield to unsatisfactory representation if a target is not precisely centered in a range-gate. In that case, the same scatterer can be either estimated on several gates or missed due to range-gate straddling loss. A bidimensional analysis may prevent the splitting effect or the miss-detection if the problem of grid mismatch is taken into account.

In case of a sparse Fourier analysis, this phenomenon arises whenever the frequency of a scatterer lies off the Fourier grid. It leads to important performance degradation if not taken into account by the SSR technique [1]. Several strategies of robustification have been proposed accordingly in the literature. These include: i) the local refinement of the grid [2] ii) the estimation of the grid mismatch [3]–[7] iii) the use of grid-free based methods [8].

The work of S. Bidon and O. Besson is supported by DGA/MRIS under grant 2012.60.0012.00.470.75.01.

The work of M. Lasserre is supported by DGA/MRIS under grant 2014.60.0045. x y σ2 εd, εr (β0, β1) (γ0, γ1) w σ2 x

Fig. 1. Graphical representation of the proposed Bayesian model. Parameters circled have to be set by the radar operator.

In this paper, we chose to adopt the second strategy. More specifically, we propose to extend a recently published algo-rithm [9] using a bidimensional approach. Within a Bayesian framework, the 2D-grid mismatch is described for each bin of analysis by two random variables that are jointly estimated with the target amplitude.

In this paper, Section II and III describe the hierarchichal Bayesian model and its estimation procedure. Numerical sim-ulations are provided in Section IV while the last Section includes some concluding remarks.

II. BAYESIAN MODEL

The hierarchical Bayesian model proposed in this paper is represented graphically in Fig. 1 and detailed herein. As compared to [9], the technical novelty resides in the modeling of a bidimensional grid mismatch.

A. Observation model

1) SSR approach: We consider a measurement matrix Y of size K × M that represents data collected by a radar system in the fast-frequency/slow-time domain and where M and K are the number of pulses and range frequency bins to be processed. The KM -length vector that stems from the row vectorization of the matrix Y was annoted y. In an SSR framework, one attempts to interpret the signal of interest (here the targets)

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as a small number of atoms in a given dictionary which is equivalent to the following model

y = Hx + n where

H is the sparsifying dictionary;

x is a sparse vector that ideally entails as many nonzero elements as there are target scatterers;

n is the noise vector.

In radar applications, a common approach is to consider targets as a set of discretes in the fast-time/slow-frequency domain, namely in the range-Doppler map. For a narrowband radar system, a natural SSR dictionary is thus

H = F

where F is a 2D-Fourier matrix of size KM × ¯K ¯M . More specifically, F operates an inverse Fourier transform on the slow-frequency dimension and a Fourier transform on the fast-time domain so that the ¯K ¯M -length vector x represents the target amplitude vector in the range-Doppler map. Once fixed by the radar operator, the parameters ¯K and ¯M set the number of points for analysis in the range-Doppler domain as depicted in Fig. 2(a). A regular spaced grid is usually considered.

2) Modeling of bidimensional grid mismatch: Ideally, in absence of grid mismatch, each target is located at the center of a range-Doppler bin of analysis. An appropriate choice for the sparsifying dictionary F is hence

F =f0 . . . fK ¯¯M −1 

where the ith element of the ¯ith column is for i = {0, . . . , KM − 1} and ¯i = {0, . . . , ¯K ¯M − 1} [f¯i]i = 1 √ KM exp  −2jπ ¯ k ¯ Kk  expn2jπm¯¯ Mm o . (1)

In (1), we have used the notation i = m + kM

where i is the linear index equivalents to the row and column subscripts k ∈ {0, . . . , K − 1} and m ∈ {0, . . . , M − 1} for a matrix of size K × M . Likewise, we have used the notation

¯i = ¯m + ¯k ¯M

where ¯i is the linear index equivalents to the row and column subscripts ¯k ∈ {0, . . . , ¯K − 1} and ¯m ∈ {0, . . . , ¯M − 1} for a matrix of size ¯K × ¯M . Subscript- or index-based notations were used interchangeably in the remainder of the paper. In real world applications, target scatterers are most likely located off the range-Doppler grid. We propose to model this mismatch by defining two perturbation vectors

εd=εd 0 . . . εd¯i . . . εdK ¯¯M −1 T εr=εr 0 . . . ε¯ri . . . ε r ¯ K ¯M −1 T

where εd and εr entail the grid errors with respect to the Doppler (superscript d) and range (superscript r) axes. The

range bin Doppler bin ¯ k ¯ K − 1 ¯ m M − 1¯ 0 0 (a) ¯ k ¯ m 0, 0 − .5 − .5 + .5 + .5 εr ¯i εd ¯i

true target location within the (¯k, ¯m)th bin

target location

in absence of grid mismatch

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Fig. 2. Representation of the grid error. (a) 2D frequency grid in the

range-Doppler domain. (b) Zoom on the (¯k, ¯m)th frequency bin.

mismatch modeling is represented for the (¯k, ¯m)th bin in Fig. 2(b). Accordingly, we redefine the sparsifying dictionary so that it incorporates the grid errors, i.e.,

F , F (εd, εr) =f0(ε d 0, ε r 0) . . . fK ¯¯M −1(ε d ¯ K ¯M −1, ε r ¯ K ¯M −1) 

where the ith element of the ¯ith column is parameterized by εd ¯i, ε¯ri as follows [f¯i(ε d ¯i, ε r ¯i)]i= 1 √ M exp ( 2jπm + ε¯ d ¯i ¯ M m ) ×√1 Kexp ( −2jπ ¯ k + ε¯ri ¯ K k ) .

In the remaining of this paper, the following equivalent nota-tion is also used, i.e.,

i(ε¯di, ε¯ri) = fkr¯(ε¯ri) ⊗ fdm¯(ε d ¯i) where ⊗ is the Kronecker product, fr¯k(ε¯ri) and f

d ¯

m(ε¯di) are respectively the K-length and M -length vectors such that

[fdm¯(ε d ¯i)]m= 1 √ M exp ( 2jπm + ε¯ d ¯ i ¯ M m ) (2) [fr¯k(ε r ¯i)]k = 1 √ Kexp ( −2jπ ¯ k + ε¯ri ¯ K k ) .

Remark 1 (Size of the 2D-grid): In [9], it has been shown in the 1D-case that, with a parametric model as in (2), up-sampling the grid does not improve the reconstruction quality of the target scene. Applied to the present 2D-case, it means that one can already limit the study to ¯K = K and ¯M = M . Nonetheless, we maintain the notations ¯K and ¯M throughout this paper to distinguish the dimension of the measurement from that of the SSR analysis.

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3) Likelihood: The noise background is assumed to be adequately modeled by a white Gaussian noise with power σ2. The likelihood function is thus given by

f (y|x, εd, εr, σ2) = 1 (πσ2)KM exp  −ky − F (ε d, εr)xk2 2 σ2  . (3) Note that such modeling will ensure that the SSR algorithm interprets the clutter component (if any) as discretes.

B. Prior pdfs of the parameters

To pursue the description of our Bayesian model, prior probability density functions (pdf) need to be assigned to the unknown parameters x, εd, εr, σ2. Pfds are chosen to comply with the physical constraints of the problem (e.g., sparsity of the targets scene) while preserving some mathematical tractability [10]. As previously mentioned, the novelty of our approach lies in the description of the 2D-grid error prior.

1) Target amplitude vector: A sparsity inducing prior is chosen for x. More specifically as in [9], the elements of x are supposed to be independent and identically distributed (iid) according to a complex Bernoulli-Gaussian density, namely

π(x¯i|w, σx2) = (1 − w)δ(|x¯i|) + w 1 πσ2 x exp  −|x¯i| 2 σ2 x  (4) where x¯i , [x]¯i for ¯i = {0, . . . , ¯K ¯M − 1} and δ() is the Delta Dirac function. Therefore, a target scatterer is a priori present in the (¯k, ¯m)th range-Doppler bin with probability w and power σ2

x. The pdf (4) is denoted by x¯i|w, σx2 ∼ Ber CN w, 0, σ2

x.

2) Grid errors: Similarly to the target amplitude vector x, we assume that the grid errors εd

¯i, ε¯ri are a priori independent from one range-Doppler bin to another so that

π(εd, εr|x) = Y ¯i=0,..., ¯K ¯M −1

π(ε¯di, ε r

¯i|x¯i). (5)

Note that in (5) we have described the grid errors εd ¯i, εr¯i conditionally to the target amplitude x¯i. This allows us to propose a scheme where the grid errors are estimated only if a target is present at the corresponding range-Doppler bin. Particularly, we assume that, conditionally to x¯i, the grid errors on the Doppler axis ε¯di and on the range axis ε

r ¯i are independent and such that

π(ε¯di, ε r ¯i|x¯i= 0) = δ(ε d ¯i)δ(ε r ¯i) (5a) π(ε¯di, ε¯ri|x¯i6= 0) = I[−.5,.5](ε¯di)I[−.5,.5](ε¯ri) (5b) where IA(.) is the indicator function of the set A.

3) Noise power: An inverse Gamma prior distribution is assumed for the white noise power σ2, viz

π(σ2|γ0, γ1) ∝

e−γ1/σ2

(σ2)γ0+1I[0,+∞)(σ

2) (6)

where ∝ means proportional to, γ0, γ1 represent the shape and scale parameters of the pdf respectively. The latter can be tuned to obtain a noninformative (e.g., γ0 = γ1 = 0), a moderate or a very informative prior. The pdf (6) is denoted by σ2|γ0, γ1∼ IG (γ0, γ1).

C. Prior pdfs of the hyperparameters

Since the probability w and the target power σx2 are un-known, a hierarchical step is added to the Bayesian model, where in turn they are considered as random variables with given prior probabilities.

1) Target signal power: An inverse Gamma pdf is chosen to describe σ2x a priori, i.e., σ2x|β0, β1 ∼ IG (β0, β1). The shape and scale parameters β0, β1 can be tuned to obtain a noninformative, a moderate or a very informative prior about the average target power. In Section IV, β0, β1are adjusted to obtain the desired a priori mean mσ2

x and standard deviation

stdσ2 x.

2) Level of occupancy: If no information is available to the radar operator about the sparsity level of the target scene, a uniform pdf over the interval [0, 1] serves as a convenient prior, i.e., w ∼ U[0,1].

III. BAYESIAN ESTIMATION A. Principle

According to the Bayesian model described in Sec-tion II, the unknown parameters to be estimated are θ = h

xT, εdT, εr T, σ2, w, σ2 x

iT

. Particularly, we propose to study the minimum mean square error (MMSE) estimator of x, εd and εr. By definition, the MMSE estimator of θp is

ˆ

θp,MMSE= Z

θpf (θp|y)dθp

where θp refers to the pth element of θ and f (θp|y) is its posterior distribution. Given our data model, it seems impossible to obtain analytically the MMSE estimators of x, εd and εr. Nonetheless, one can resort instead to a numerical solution, namely a Monte-Carlo Markov chain (MCMC) method [11]. The MCMC generates iteratively sam-ples x(t), εd(t), εr (t), σ2(t), w(t), σ2x

(t)

according to their con-ditional posterior distribution f (θp|y, θ−p) where θ−p is the vector θ whose pth element has been removed. After a burn-in period of Nbi iterations, the samples θp(t) are distributed according to their posterior distribution f (θp|y). The MMSE estimator of θp can thus be obtained as an empirical mean

ˆ θp,MMSE, Nr−1 Nr X t=1 θp(t+Nbi)

provided that a sufficient number of samples, say Nr, are collected.

The conditional posterior distributions can be easily ob-tained from the joint posterior pdf which is given by

f (x, εd, εr, σ2, w, σx2|y) = f (y|x, εd, εr, σ2) × π(εd, εr|x)π(x|w, σ2 x)π(σ 2) × π(w)π(σ2 x).

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Specifically, since the vectors x, εd, εr are sampled elemen-twise in the proposed estimation scheme, it is of interest to express the following joint conditional pdf

f (x¯i, ε¯di, ε¯ri|y, x−¯i, εd−¯i, εr−¯i, σ2, w, σx2) ∝ exp−σ−2|x ¯i|2− 2<x¯∗if¯i(ε d ¯i, ε r ¯ i) He ¯i  × π(ε¯di, ε r ¯ i|x¯i)π(x¯i|w, σ 2 x) (7) where we have used f¯i(εd¯i, ε¯ri)Hf¯i(ε¯di, ε¯ri) = 1 and defined the KM -length vector

e¯i= y − X

¯ι6=¯i

x¯ιf¯ι(ε¯dι, εr¯ι).

In (7), ()∗ is the element-wise complex conjugaison operator. B. Sampling ofεr, εd

Using (7), the conditional posterior distribution of (εd ¯i, ε

r ¯i) is, under the hypothesis x¯i= 0, given by

f (ε¯di, ε r ¯i|y, x, ε d −¯i, ε r −¯i, σ 2, w, σ2 x; x¯i= 0) = δ(ε d ¯i)δ(ε r ¯i) which means that εd

¯i = 0 and εr¯i = 0. Alternatively under the hypothesis x¯i 6= 0, following the same path as in [9] it becomes f (ε¯di, ε¯ri|y, x, εd−¯i, εr−¯i, σ2, w, σ2x; x¯i6= 0) ∝ K−1 Y k=0 M −1 Y m=0 exp  κm+kMcos  2π m¯ Mε d ¯i − k ¯ Kε r ¯i  − φm+kM  I[−.5,.5](εd¯i)I[−.5,.5](ε¯ri) (8) with κm+kM = |[z¯i]m+kM| and φm+kM = ∠[z¯i]m+kM where ∠ is the phase angle of a complex number and z¯i is the KM -length vector

i = 2 x¯∗i σ2f

¯i(0, 0) e¯i.

Given the equation (8), we propose to sample jointly εr ¯i, ε¯di when x¯i 6= 0. However the pdf (8) does not belong to any familiar class of distributions. Therefore, we resort to a Metropolis-Hastings (MH) move. The MH algorithm is an iter-ative procedure that simulates samples distributed according to a target distribution using samples from a proposal distribution with a given acceptance ratio [11]. The closer the proposal pdf to the target distribution, the more efficient the sampling. To find an adequate proposal pdf, the target distribution (8) is depicted in Fig. 3 for high and low signal-to-noise ratio (SNR). The (postprocessing) SNR is defined as

SNR = |x¯i|2/σ2. (9)

Note that the target pdf peaks around the true value of the grid errors ε¯ri, ε

d

¯i at high SNR while it tends to be noninformative at low SNR. We thus make the following choice for the proposal pdf

• a uniform distribution at low SNR

q(ε¯di, ε¯ri) = I[−.5,.5](ε¯di)I[−.5,.5](ε¯ri) • a bivariate Gaussian distribution at high SNR

q(ε¯di, ε¯ri) ∼ N2(m, Σ)

where m and Σ are the mean and the covariance matrix respectively. They are obtained given that when the SNR (9) is high, the concentration parameters κm+kM in (8) tend to be large too so that the following approxi-mation can be made in the support of (8)

exp  κm+kMcos  2π m¯ Mε d ¯i − k ¯ Kε r ¯i  − φm+kM  ≈ exp ( κm+kM " 1 − 1 2  2π m¯ Mε d ¯i − k ¯ Kε r ¯i  − φm+kM 2#) . In the numerical simulations, we consider as a rule of thumb that the SNR is low when < 10 dB.

C. Sampling of x,σ2,w,σ2 x The sampling of x, σ2, w, σ2

x is similar to the procedure described in [9] and can be summarized as follows

x¯i|y, x−¯i, εd, εr, σ2, w, σx2∼ Ber CN w¯i, µ¯i, η¯i2  where η¯2i = σ −2+ σ−2 x −1 µ¯i= η¯2i σ2f¯i(ε d ¯i, ε¯ri)He¯i w¯i= w (1 − w)σ2x η2 ¯i expn−|µ¯i|2 η2 ¯i o + w . and σ2|y, x, εd, εr∼ IG γ 0+ KM, γ1+ ky − F (εd, εr)xk22  w|x ∼ Be (1 + n1, 1 + n0) σx2|x ∼ IG β0+ n1, β1+ kxk22 

where n1 is the number of nonzero elements of x and n0= ¯

K ¯M − n1.

IV. NUMERICAL EXAMPLES

We highlight herein several numerical examples to illustrate the performance of the SSR algorithm proposed in Section III. A. Synthetic data

In what follows, N = 7 target scatterers are generated synthetically with possible grid errors in a white noise back-ground. The target scene ˆxMMSE, ˆεdMMSE, ˆε

r

MMSE assessed by our estimation technique is represented in Fig. 4 with diamond markers. Each gray rectangle represents a 2D-frequency bin of the analysis grid while the circles indicate the actual location of each scatterer. For simplification purposes, grid error values increase from the bottom left to the top right hand corner. Furthermore, the mismatch is introduced either in one dimension (the Doppler or the range) or in both dimensions.

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(a)

(b)

Fig. 3. Shape of the conditional posterior distribution

f (εd ¯i, ε r ¯i|y, x, ε d −¯i, εr−¯i, σ2, w, σx2; x¯i 6= 0). M = 16, K = 20, ¯

M = M , ¯K = K. Only one target is present in the data at the ¯ith bin with

εd

¯

i = 0.15, ε

r

¯i = 0.25. (a) High SNR |x¯i|2/σ2 = 25 dB. (b) Low SNR

|x¯i|2/σ2= 5 dB.

For comparison purposes, we also depict the target scene estimated with the algorithm of Section III except that the grid errors are not estimated but set to zero.

As expected, when the grid errors are not estimated, the SSR algorithm splits the scatterer power on the surrounding bins. More specifically, as soon as there is a mismatch in one dimension, a split occurs in that same dimension. Moreover, the greater the mismatch, the more significant the target spreading. The sparsity level of the reconstructed scene is thus degraded which may prevent a proper interpretation of the target scene. On the contrary, the proposed SSR technique estimates with sufficient accuracy both grid errors and target

(a)

(b)

Fig. 4. SSR of synthetic target scene: 7 scatterers with SNR of 25 dB,

M = 16, K = 20, σ2= 1, ¯M = M , ¯K = K. (β

0, β1) chosen such that

mσ2

x= 20 dB and stdσ2x= 10 dB. (γ0, γ1) = (0, 0) (i.e., noninformative

prior on σ2). 2D-APES processing as a transparent background [12]. Location

and amplitude of targets are indicated by a circle. Gray rectangle represents

a 2D-frequency bin. (a) Target amplitude vector ˆxMMSE with estimated

mismatch (ˆεdMMSE, ˆεrMMSE) (diamond marker). (b) Target amplitude vector

ˆ

xMMSE without mismatch estimation (εd= 0, εr= 0) (diamond marker).

amplitudes and gives a satisfactory sparse representation of the target scene. Note that the split phenomenon can still occur (e.g., scatterer located in the (4, 12)th bin) but is less frequent and less pronounced.

B. Experimental data

Finally, we describe our results obtained from our experi-mental data. The data set considered here was collected with the PARSAX radar system [13] on November 2010. The radar antenna was pointing at a freeway during a heavy traffic time. The estimated target scene is represented in Fig. 5(a) with grid

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errors estimated from our proposed technique and in Fig. 5(b) with grid errors that are ignored. Since the ground truth is unknown, the output of the APES technique is also depicted as a transparent background to give an indication of the radar scene [12]. Remarks done previously in the synthetic case still hold here. Note that by ignoring the mismatch, some scatterers seem to split on several bins (e.g., scatterer at range gate 643 and Doppler bins -7/-6) and may also be almost missed by the sparse recovery algorithm (e.g., scatterer at range gate 650 and Doppler bin -7). Finally, for this data set, ground clutter seems to be correctly modeled by a finite set of scatterers located at zero Doppler.

V. CONCLUSION

In this paper, we introduce an estimation technique able to give a sparse representation of a bidimensional signal in the Fourier basis. Particularly, this algorithm is suited for sparse estimation of the radar scene in the range-Doppler domain. To ensure robustness towards the grid mismatch phenomenon, two grid error vectors were introduced in the data model. They both represent the mismatch with respect to each of the two dimensions (i.e., Doppler and range). This mismatch description is integrated in a complete hierarchi-cal Bayesian data model. Accordingly, the MMSE estimator of the radar scene can be derived. Numerical results from both synthetic and experimental data validate the benefit of estimating the 2D-mismatch with the proposed technique. We intend to extend this work to wideband radar data in which a cross-coupling phenomenon occurs between the range and Doppler dimensions. Note that this phenomenon will need to be accounted for in the data model.

ACKNOWLEDGMENT

The authors are very grateful to Oleg Krasnov at TU-Delft for kindly providing the PARSAX experimental data.

REFERENCES

[1] Y. Chi, L. Scharf, A. Pezeshki, and A. Calderbank, “Sensitivity to basis mismatch in compressed sensing,” IEEE Trans. Signal Process., no. 5, pp. 2182–2195, May 2011.

[2] D. Malioutov, M. Cetin, and A. Willsky, “A sparse signal reconstruction perspective for source localization with sensor arrays,” IEEE Trans. Signal Process., vol. 53, no. 8, pp. 3010–3022, Aug. 2005.

[3] H. Zhu, G. Leus, and G. Giannakis, “Sparsity-cognizant total least-squares for perturbed compressive sampling,” IEEE Trans. Signal Pro-cess., vol. 59, no. 5, pp. 2002–2016, 2011.

[4] L. Hu, Z. Shi, J. Zhou, and Q. Fu, “Compressed sensing of complex sinusoids: An approach based on dictionary refinement,” IEEE Trans. Signal Process., vol. 60, no. 7, pp. 3809–3822, Jul. 2012.

[5] Z. Yang, L. Xie, and C. Zhang, “Off-grid direction of arrival estimation using sparse Bayesian inference,” IEEE Trans. Signal Process., vol. 61, no. 1, pp. 38–43, Jan. 2013.

[6] L. Hu, J. Zhou, Z. Shi, and Q. Fu, “A fast and accurate reconstruction algorithm for compressed sensing of complex sinusoids,” IEEE Trans. Signal Process., vol. 61, no. 22, pp. 5744–5754, Nov. 2013.

[7] Z. Tan and A. Nehorai, “Sparse direction of arrival estimation using co-prime arrays with off-grid targets,” IEEE Signal Process. Lett., vol. 21, no. 1, January 2014.

[8] G. Tang, B. Bhaskar, P. Shah, and B. Recht, “Compressed sensing off the grid,” IEEE Trans. Inf. Theory, vol. 59, no. 11, pp. 7465–7490, Aug. 2013.

(a)

(b)

Fig. 5. SSR of experimental target scene (PARSAX data): range resolution of 3 m, carrier frequency 3.315 GHz, pulse repetition frequency 1 kHz,

M = 16, K = 20, σ2 ≈ 1 (pre-normalization of the data), ¯M = M ,

¯

K = K. (β0, β1) chosen such that mσ2

x = 35 dB and stdσ2x = 10 dB.

(γ0, γ1) = (0, 0) (i.e., noninformative prior on σ2). 2D-APES processing

as a transparent background [12]. (a) Target amplitude vector ˆxMMSE with

estimated mismatch (ˆεdMMSE, ˆεrMMSE) (diamond marker). (b) Target amplitude

vector ˆxMMSE without mismatch estimation (εd = 0, εr = 0) (diamond

marker).

[9] M. Lasserre, S. Bidon, O. Besson, and F. Le Chevalier, “Bayesian sparse Fourier representation of off-grid targets with application to experimental radar data,” Signal Processing, vol. 111, pp. 261–273, Jun. 2015.

[10] S. M. Kay, Fundamentals of statistical signal processing, Vol. I:

Estima-tion Theory, ser. Signal Processing. Upper Saddle River, NJ: Prentice

Hall, 1998.

[11] C. Robert and G. Casella, Monte Carlo Statistical Methods. Springer,

2004.

[12] J. Li and P. Stoica, “An adaptive filtering approach to spectral estimation and SAR imaging,” IEEE Trans. Signal Process., vol. 44, no. 6, pp. 1469–1484, Jun. 1996.

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[13] O. A. Krasnov, G. P. Babur, Z. Wang, L. P. Ligthart, and F. van der Zwan, “Basics and first experiments demonstrating isolation improvements in the agile polarimetric FM-CW radar – PARSAX,” International Journal of Microwave and Wireless Technologies, vol. 2, pp. 419–428, 8 2010.

Figure

Fig. 1. Graphical representation of the proposed Bayesian model. Parameters circled have to be set by the radar operator.
Fig. 2. Representation of the grid error. (a) 2D frequency grid in the range- range-Doppler domain
Fig. 4. SSR of synthetic target scene: 7 scatterers with SNR of 25 dB, M = 16, K = 20, σ 2 = 1, ¯ M = M , ¯ K = K
Fig. 5. SSR of experimental target scene (PARSAX data): range resolution of 3 m, carrier frequency 3.315 GHz, pulse repetition frequency 1 kHz, M = 16, K = 20, σ 2 ≈ 1 (pre-normalization of the data), ¯ M = M , K = K

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