JI Bingren,WANG Yong,ZHAO Bin,and XU Rongqing
School of Electronics and Information Engineering,Harbin Institute of Technology,Harbin 150001,China
Abstract: This paper concentrates on super-resolution imaging of the ship target under the sparse aperture situation.Firstly,a multi-static configuration is utilized to solve the coherent processing interval (CPI) problem caused by the slow-speed motion of ship targets.Then,we realize signal restoration and image reconstruction with the alternating direction method of multipliers(ADMM).Furthermore,we adopt the interferometric technique to produce the three-dimensional (3D) images of ship targets,namely interferometric inverse synthetic aperture radar (InISAR)imaging.Experiments based on the simulated data are utilized to verify the validity of the proposed method.
Keywords: multi-static,sparse aperture,signal recovery,interferometric inverse synthetic aperture radar (InISAR),ship target,alternating direction method of multipliers (ADMM).
Inverse synthetic aperture radar (ISAR) is able to operate normally regardless of time limitation and weather conditions [1−5].As we all know,ISAR imaging achieves high resolutions in the range direction by transmitting wideband signals and in the azimuth direction by processing the large Doppler frequency generated by the target’s effective rotational motion.Usually,long coherent processing interval (CPI) is a good way to acquire enough Doppler frequency shift.
In recent years,phase array radar has been increasingly deployed to carry out multiple tasks with the help of time control mechanisms [6].By continuously adjusting the directions of the radar beams,the system can track,recognize,and image different targets in a relatively short time.However,in order to monitor the status of different targets,long and continuous radar beam illumination for any single target cannot be achieved at all time,which will lead to the sparse aperture situation for the echoed data.
In addition,the complex motions of targets and deliberate interference can also lead to the missing of echoes and then result in the degeneration of imaging performance,and failure of sequential automatic target recognition (ATR).Thus,how to acquire super-resolution ISAR images under the sparse aperture situation has attracted a lot of attention recently [7].
To overcome the sparse aperture imaging challenge,the first problem we have to solve is motion compensation of the observed target under sparse aperture situation.Range alignment and phase adjustment are two processes in motion compensation,which aim to eliminate the misalignments and phase errors between pulses.These two steps can guarantee the focus of image and the retention of target features.Numerous range alignment methods have been presented in [8,9].However,when facing sparse aperture conditions,approaches such as the scatterer point referencing algorithm lose efficacy,while the global minimum entropy-based method can produce acceptable performance.In addition,most phase-adjustment methods such as the phase gradient autofocus algorithm [10] and the weighted least-squares algorithm [11]become inapplicable due to the loss of coherence between different pulses under the sparse aperture condition.The eigenvector-based autofocus method [12,13],on the other hand,is still suitable in this case,and is used in this paper.
Then,we should solve the problem of data missing.The existing sparse aperture ISAR imaging techniques include linear prediction methods,modern spectrum estimation methods,and sparse signal recovery methods.The performance of the former two methods are easily affected by the signal to noise ratio (SNR) [14].Among the third category,the compressive sensing (CS) method is exempt from the limitation of the Nyquist sampling theory [15−17].The number of dominant scatterers in ISAR images is small compared to the whole image,which allows the echo signals in the image domain to be considered as compressible.The alternating direction method of multipliers (ADMM) is an emerging technique,which can solve the signal reconstruction problem by utilizing the proximal splitting strategy [18−20].In this paper,we adopt the ADMM algorithm to restore the missing parts of the signal,which can produce excellent imaging performance.
In fact,the observed targets sometimes sail along the radar light of sight (RLOS) deliberately,leading to the loss of relative rotational motion between the target and the RLOS,which brings trouble to ISAR imaging [21].In addition,for slow-velocity targets,for example,ship targets,imaging fails when they move within a small angle of LOS [22].If we adopt a long CPI to solve this issue,the system will require large data storage and long processing time,which is not suitable for real time processing.Furthermore,ship target motion states could be complex in the rough sea condition with a long CPI.Thus,we make use of the multi-static configuration to solve aforementioned problems.With the separation of the transmitter and the receivers,the relative motion of the target to the receiver is accentuated compared with the mono-static situation.In addition,multi-static radar system can also increase the battle survival rate due to the separation of the transmitter and the receivers.
Normally,the target mapped onto the image projection plane (IPP) forms the ISAR image.The imaging results could be different when selecting different IPPs or imaging time.In addition,the complex motion of targets also brings trouble to target recognition [23−26].To overcome these shortness,we adopt the interferometric ISAR(InISAR) method to produce the three-dimensional (3D)imaging results.
In this paper,we attempt to combine the multi-static configuration and InISAR techniques with the signal recovery method ADMM to deal with the ship 3D imaging problem under the sparse aperture situation.
The remaining sections are organized as follows:The signal model is established in Section 2.Section 3 introduces the ADMM signal recovery algorithm and illustrates the flow chart of multi-static InISAR imaging for the ship target with sparse aperture situation.In Section 4,experiments with the simulated model are provided to verify the validity of the proposed method.Finally,conclusions are drawn in Section 5.
Fig.1 shows the multi-static InISAR imaging system.TransmitterT,receiverB,and receiverAlocate in the axisU,while the receiverClocates in the axisW.The axisVis perpendicular to the plane formed by axisUand axisW.We define receiverAas the originOof the coordinate system.The baseline length is |AB|=|AC|=Lrand the length betweenOand transmitterTis |AT|=Ltr.The target is situated in the reference system (O′,X,Y,Z).The radar system(O,U,V,W) and the reference system(O′,X,Y,Z)are parallel to each other.P is one of the scatterers on the ship and |PA|=RPA,|PB|=RPB,|PC|=RPC,|TP|=RTP.η,ξ,ζ denote the three axes of rotation.wr,wp,wyare the roll,pitch,and yaw rotations.Besides,Mis in the middle between receiverAand receiverBwith |PM|=RPM.The observed targets usually locate in the far field,therefore,RPA+RPB≫LrandRPA+RPB≈2RPM.
Fig.1 Multi-static InISAR radar system
Consider that the signal transmitted from the transmitter is a linear frequency modulation (LFM) signal:
where rect(t) is the rectangle function,TPmeans the pulse width,andkstands for the chirp rate.tm=mTr(m=0,1,2,···,M)denotes the slow time.is the fast time,andMrepresents the echoes’ number.fcis the initial frequency.
The returned signal from the ship target can be shown as
whereq=A,B,C,Rq(tm)=RTP(tm)+Rpq(tm),Pis the number of all the target’s scatters,c denotes the light velocity,and σprepresents the reflectivity of scatterp.
Assume thatRref(tm) represents the reference distance andTrefstands for the pulse width.The reference signal is expressed as
After the de-chirp process,the signal is expressed as
where
Then,fast Fourier transform (FFT) is carried out with regard to,
The second exponential term in (6) can lead to the migration through resolution cell and needs to be eliminated with the keystone transform,while the last term stands for the residual video phase,which may degrade the imaging quality and should be erased.After removing the last two exponential terms,(6) can be abbreviated as
To obtain the coordinates of the target’s scatterers,interferometric processing is implemented with regard to the signaland signal
whereudenotes the distance between the scattererpandMalong theUaxis.
Similarly,by interferometricly processing the signalsandthe scattererp’s coordinate in theWaxis can be acquired.The scattererp’s coordinate in theVaxis is obtained through the range information.Next,we take the following transformation to convert the scatterer’s radar system coordinates to the target coordinates,taking into consideration the target’s rotational motion:
where [ξ,η,ς]and [U,V,W] denotethe coordinatesofthe scatterers inthe coordinatesystems(O′,ξ,η,ς)and(O,U,V,W)respectively.Rot represents the rotation matrix of the ship target.Moreover,θr(t),θp(t),θy(t) represent the instantaneous angles caused by the roll,pitch,yaw of the ship. θr0,θp0,θy0are the angles of rotation at timetm=0.
In addition,as the result of the multi-static configuration,the coordinates derived above would be distorted and another coordinate transformation is needed to recover the true coordinates [22].
The sparse aperture situation usually contains two types:random and gap.Fig.2 gives the schematic of the random case,where the blue squares indicate the valid data and the white ones denote the empty data.
Fig.2 Geometry of sparse aperture signal
In this section,we first give the details of the ADMM method.Then the angular motion compensation and the flow of the proposed method are described,respectively.
From (7),we can obtain the range compressed data in thenth range bin as
whereNdenotes the range bins’ number.
Equation (11) can be further expressed as
Equation (12) can be described as an unconstrained optimization problem:
where λ denotes the regularization coefficient.
We utilize the ADMM method to split (13) into subproblems,which is an effective way in solving this kind of problem.
The augmented Largrangian function can be expressed as
whereδis the penalty parameter,γ represents the Lagrangian multipliers,and µ stands for the auxiliary variable.
The ADMM method decouples (14) into several subproblems,and updates the variables alternately.The updating processes are
where superscriptidenotes theith iteration.
After some mathematical derivations,the solutions for the sub-problems (15)−(17) are
Then,we can make the ADMM method to all the range bins and obtain the restored ISAR images.
In the multi-static condition,there exist phase differences between different images.Hence we should make the image registration.
From Fig.1,as the different locations of receiversAandB,the path length difference can be expressed as
Since the angle θAB(t) is small in this situation,(19) can be approximated to
Take Taylor expansion to the angle θAB(t):
Making FFT with regard totmin (8),we can obtain
wherefpAdenotes the scatterp’sfrequencyinreceiverA,σABdenotes the amplitude,andTcmeanstheimaging time.To achieve the image co-registration,we need to compensate the termin (22) as
From(23),we can see that the estimation of θAB(t) is a necessary step.In this paper,we employ the method in [22] to carry out the compensation process.
Furthermore,sinceLris usually much smaller thanLtr,the phase of estimatedhas ambiguity and should be unwrapped as
The angular motion compensation is completed when the phase unwrapped processing is finished.
To achieve a satisfactory performance of 3D ISAR imaging for the observed ship under the sparse aperture situation,many processes need to be carried out.The concrete procedures are enumerated as follows:
Step 1Acquire the original data from three receivers and making de-stretch process.
Step 2Adopt the envelope alignment method based on minimum entropy and the phase correction method based on eigenvector to realize motion compensation under sparse aperture.Since the coherency between the three received signals is a key requirement to achieve 3D reconstruction,the aforementioned motion compensation methods need to be implemented for all three channel signals together.
Step 3Perform ADMM to the sparse aperture data after motion compensation.By setting appropriate parameters,we can obtain the high resolution ISAR images.
Step 4Carry out angular motion compensation and phase unwrapping process to the reconstructed signals to realize image co-registration.Then,matched images of targets can be obtained.
Step 5Carry out the interferometric processing with respect to the images from three channels and obtain the 3D imaging results of the ship target with multi-static configuration under sparse aperture.
The details of this procedure are illustrated in Fig.3.
Fig.3 Flowchart of multi-static 3D imaging method under sparse aperture
In this section,we conduct simulations to validate the proposed method.First,we utilize a sinusoidal signal to check out the performance of the ADMM algorithm under different SNRs and different sparsity rates (SRs).The parameters λ andδare set as 0.1 and 1.0,respectively.The signal is formulated as
whereadenotes the amplitude,f,Ts,tsrepresent signal frequency,sampling interval,and sampling index,respectively.
Fig.4 gives the ADMM method’s root mean square error (RMSE) values versus different SNRs and SRs.When the estimated signal is close to the original signal,the RMSE will be small and vice versa.
From Fig.4(a),we can see that the RMSE result decreases as the SNR increases.On the other side,Fig.4(b) illustrates that the RMSE result increases when the sparsity rate goes up.
Fig.4 RMSEs of the ADMM method
Then,we utilize a simulated ship target to explore the validity of the ship target.The ship target is modelled in Fig.5.Fig.5(a)–Fig.5(c) are the ship’s three-view drawings.Fig.5(d) illustrates the 3D model of the ship.
Fig.5 Model of the ship
The parameters of radar system simulated in the paper are listed in Table 1.Referring to Fig.1,the transmitterT,the receiverA,and the receiverBare situated in theUaxis,while the receiverCis located in theWaxis.The distance between transmitterTand the origin is 5 km.The initial target’s coordinates in the coordinate system(O,U,V,W) are (U0=0 m,V0=10 km,W0=0 m).The coordinate system (O,U,V,W) is parallel to the coordinate system (O',X,Y,Z).The ship’s translational speed is 600 knots.The ship target is moving at an angle of 72° with regard to theUaxis.
Table 1 Parameters of the radar system
Firstly,we explore the proposed method’s effectiveness with one-rotational motion dominant.Table 2 illustrates the ship’s three-dimensional rotation parameters with yaw motion being the dominant.Fig.6 shows the ship’s 3D multi-static InISAR images under the sparse aperture situation,with 128 echoes disappearing.It can be seen that the ADMM method is valid in signal reconstruction and its imaging performance under the sparse aperture condition with 50% missing data is satisfactory compared to the model and the imaging results with the whole data.Next,we demonstrate the validity of the proposed method with complex target motion.The relative ship’s 3D rotational parameters are shown in Table 3,with large motion amplitudes in all pitch,roll,and yaw directions.The sparse situation is also 50% randomly missing data.
Table 2 3D rotation parameters of the ship with one dimension dominant
Table 3 3D rotation parameters of the ship with all dimensions dominant
Fig.6 Three dimensional InISAR images of the ship under sparse aperture with one dimension dominant
Fig.7 shows the 3D multi-static InISAR ship target’s images with complex target motion.The imaging results in Fig.7 show that the recovered positions of points are similar to the original ones and the ones with no missing data,which demonstrates that the proposed method is still applicable when the target undergoes complex threedimensional motion.
Fig.7 Three dimensional InISAR images of the ship under sparse aperture with all dimensions dominant
Furthermore,in order to quantitatively access the proposed method’s performance,we utilize the RMSE as the quantitative criterion.
The RMSE between the InISAR image obtained with the proposed method and the target model is defined as
where (xp,yp,zp) denotes the scattererp’s coordinates in the target model.denotes the coordinates of the scattererpin the InISAR image acquired with the proposed method.
Similarly,the RMSE between the InISAR image obtained with the whole data and the target model is defined as
Table 4 gives the RM and RM1 results of Fig.6 and Fig.7.
Table 4 RMSE results of Fig.6 and Fig.7
From Table 4,we can see that the RM results are close to the RM1 results in both situations,which further validate the effectiveness of the proposed method.
In this paper,we adopt the multi-static configuration to realize the ship targets’ imaging under sparse aperture.The ADMM algorithm is utilized to restore the whole signal and produce the super resolution ISAR image.Furthermore,the InISAR technique is introduced to enhance the target recognition efficiency.Experimental results with the simulated data verify the validity of the proposed method.
Journal of Systems Engineering and Electronics2022年3期