An imaging algorithm based on keystone transform for one-stationary bistatic SAR of spotlight mode
© Qiu et al.; licensee Springer. 2012
Received: 8 March 2012
Accepted: 2 September 2012
Published: 12 October 2012
This article proposes an imaging algorithm based on Keystone Transform for bistatic SAR with a stationary receiver. It can efficiently be applied to high-resolution spotlight mode, and can directly be process the bistatic SAR data which have been ranged compressed by the synchronization reference pulses. Both simulation and experimental results validate the good performance of this algorithm.
Bistatic SAR is more flexible in data acquisition geometry compared with traditional monostatic SAR. However, this flexibility is gained at the cost of increasing system complexity, which not only refers to increasing hardware system complexity due to synchronization needs of transmitter and receiver, but also refers to increasing processing complexity. As for the synchronization, the easy to realize and commonly used strategy is using an additional antenna to receive the direct pulses from transmitter, and then using these directly received pulses as a reference for range compression. As for bistatic SAR imaging, a number of studies have been done and several kinds of imaging algorithms have been proposed for different configurations [1–9]. Furthermore, a number of bistatic SAR experiments with different configurations [10–15] have successfully been carried out till now.
Among the various configurations of bistatic SAR, the so-called one-stationary configuration, which is usually formed by an existing moving transmitter (i.e., spaceborne SAR, airborne SAR, or even navigation satellite ) and a stationary passive receiver, is, in the authors’ opinion, one of the most practical configurations. On the one hand, it is inexpensive to build, and on the other hand, it can easily be extended to multi-receiver stations and then obtain multi-baseline interferometric SAR images to rebuild accurate DEM of regions of interest.
The main difficulty of imaging processing for the one-stationary bistatic configuration has been pointed out and solved to some extent in the authors’ previous publication [17, 18]. However, the former algorithm mainly aims at the stripmap mode and may not be suitable for the high-resolution spotlight mode. In spotlight mode, the pulse repetition frequency (PRF) is usually smaller than the Doppler bandwidth of a single target. So, the dechirp method is commonly used for efficient processing. Meanwhile, if range compression is done by the directly received pulses from the synchronization channel, the dechirp in azimuth has already been done within this range compressing step. After this dechirp step, the residual range and phase histories are still range–azimuth variant, while the linear term is predominant. In the high-resolution case, the range histories are bending more severely as the range bins are smaller. Hence, the differential range histories for those targets with the same bistatic range will exceed one range gate; therefore, the precondition of the NLCS algorithm based on azimuth perturbation in  is no longer valid. Till now, almost all the published images of the one-stationary bistatic SAR experiments have been focused by the universal back-projection (BP) algorithm [10, 16]. Although good quality images can be obtained using this algorithm, the main shortcoming is its computational inefficiency. The computation load of BP algorithm for producing an image, whose size is M * M and the synthetic aperture length is K, is on the order of M*M*K (i.e., O(M*M*K)). This can be very large for a big size high-resolution image.
In this article, an efficient imaging algorithm based on the Keystone Transform for one-stationary bistatic SAR, whose computation load is on the order of M2log2M, is proposed. The Keystone Transform is usually used in ISAR processing. The idea of using this transform to correct the azimuth variant range cell migration (RCM) in medium-earth–orbit SAR imaging has been proposed in the authors’ another article (H Lijia, Q Xiaolan, H Donghui, D Chibiao, A novel algorithm based on keystone transform and azimuth perturbation for medium-earth-orbit SAR, submitted). In this study, we propose to use the Keystone Transform for bistatic SAR imaging. The approach can directly be performed on bistatic SAR data which has been range compressed by the synchronization reference pulses, which makes it convenient to use. The experimental data of the HITCHHIKER system at University of Siegen/ZESS is used to test this algorithm, and good bistatic SAR images are obtained by this algorithm.
This article is organized as follows: “Geometry and signal model” section describes the one-stationary bistatic SAR geometry, and builds the signal model; “Imaging algorithm based on Keystone Transform” section introduces the proposed imaging algorithm step-by-step and shows the block diagram of the algorithm; “ Simulation and experimental results” section validates the imaging algorithm through simulations and experimental results, and “Conclusion” section concludes the article.
Geometry and signal model
One-stationary bistatic SAR geometry
where p(τ) represents the transmitted waveform; τ represents the fast time (range time), whose origin is when the pulse is transmitted; ϕ T is the phase error of the transmitter oscillator; σ(r) is the scattering coefficient of target r; w D (η ,τ) and w(η ,τ ; r) mean the weight due to the transmitter and receiver antenna pattern, propagation loss, etc. Without loss of generality, w(η ,τ ; r) and w D (η ,τ) are considered as constants here and are ignored in the following analysis.
where ϕ R is the phase error of the receiver oscillator.
The approximation in the above equation comes from omitting of the phase difference between and , which can usually be ignored.
It can be seen from Equation (9) that, after range compression using the reference signal from the direct channel, the time synchronization problem is solved because all the received echo pulses are aligned to the known R D (η). The frequency synchronization problem is solved because the direct and the echo pulses are generated by the same transmitter. The phase synchronization is also solved as long as no additional phase difference is introduced by the two receive channels. This is because the phase errors caused by the transmitter are the same in direct and echo pulses and hence can be counteracted; besides, as the direct and the echo pulses are received with small time difference, the phase errors caused by the receiver in direct and in echo pulses are nearly the same and also can be counteracted. So, as has been said in the introduction, this is the easiest and commonly used synchronization method. Therefore, it is reasonable to start bistatic SAR focusing from s1(η ,τ).
It can be seen that, if the receiver is near the scenario, the higher order terms in R bic (η ; r) will be much smaller than those in the original range history R bi (η ; r), so the Doppler bandwidth of the targets after range compression by the reference pulses is much smaller than the original Doppler bandwidth. For example, in the spaceborne-ground bistatic SAR configuration, such as in TerraSAR-X/HITCHHIKER experiment, the original Doppler bandwidth is about 5192 Hz, but after the range compression using the direct pulses, the residual Doppler bandwidth shrinks to be about 62 Hz. Therefore, if traditional imaging algorithms, which correct RCM in the azimuth frequency domain, are applied, a Doppler wideband signal rebuilding step should be adopted, which makes them not very convenient to use. In the next section, an algorithm based on the Keystone Transform which does not need Doppler signal rebuilding will be introduced.
Imaging algorithm based on Keystone Transform
Keystone Transform for linear RCM correction
It can be seen that A(r) nearly linearly depends on y, which means it is strongly azimuth variant, while B(r) depends on |r − R T (0)| and θ T (r), which is more slightly azimuth variant than A(r). The higher-order terms are much smaller than the first two-order terms, so here we pay more attention to A(r) and B(r).
In case of a complex trajectory, these parameters can numerically be obtained by polynomial fit to the residual range history.
where λ = c /f0T.
where subscript ref means the value calculated at the reference position (usually to be the scene center). Here, we denote S2(ξ, f ) = S1(ξ, f )Hcomp(ξ, f ).
This ensures that in each processing area, all targets r at each ξ have quadratic phase error that smaller than π/4, so the imaging quality is guaranteed.
Residual RCM correction
is satisfied for any r, then residual RCM correction step can be omitted. If this cannot be satisfied for the whole scene, then the sub-swath strategy can be used to deal with the azimuth variance and interpolation in two-dimensional time domain can correct the range variance of RRCM r (ξ; r i ).
It can be seen that the azimuth sub-swath can be restricted through θ T (r), and the limitation of θ T (r) is variant with range.
If the azimuth variation of ψ A h (ξ ; r) is larger than π/4, an additional step of sub-segment azimuth processing is needed. This means to cut the above image into several small segments along azimuth direction (according to the azimuth variation of ψ A h (ξ ; r)), and then to perform an inverse Fourier transform to get the azimuth time domain signal for each segment. The differential phase between ψ A h (ξ ; r) of this segment and the phase of HAc(ξ ; r) for each range gate can be calculated through range history, and be compensated for this segment. Finally, all the segments are transformed to the frequency domain and combined together to get the final fine focused image.
As can be seen from Equation (34), the axes of the focused image are τ and f ξ , whose limitations are [τ1 : 1 / f s : τ1 + (N r − 1) / f s ] and [−fPRF / 2 : fPRF / N a : fPRF / 2], respectively. Here, N r is the image size in range direction and N a is the size in azimuth direction. f s is the sample rate and fPRF is the PRF. τ1 corresponds to the sample delay of the first range gate after range compression. When trigger time of the echo channel is the same as that of the direct pulse channel, then τ1 = R D (0) / c.
Here, V T is the transmitter velocity vector in the Earth-fixed coordinates. If a DEM of the scenario is provided, then geocoding can be done according to Equations (1), (2), (10), (35), and (36).
Block diagram of the algorithm
Simulation and experimental results
To testify this algorithm, both simulated bistatic SAR data and the real experimental data of HITCHHIKER are processed using this algorithm, and results are analyzed and compared in this section.
Point target simulation
Transmitter and receiver parameters for simulation
Data acquisition time
Azimuth pulse number
Range sample number
Interferometry phases of the simulated targets
Differential phase (degree)
Measured from images
Experimental data processing and results
This article proposed an imaging algorithm for the one-stationary bistatic SAR in spotlight mode. The main property of the algorithm is using the Keystone Transform to correct the linear part of the two-dimensional variant RCM. The algorithm can directly be applied to the bistatic SAR data which has been range compressed by the reference pulses; therefore, it is efficient and convenient to use. Both simulation and experimental data processing results validate the algorithm.
Xiaolan Qiu (M’09) received the B.S. degree in electronic engineering from the University of Science and Technology of China in 2004 and the Ph.D. degree in signal and information processing from the Graduate University of the Chinese Academy of Sciences, Beijing, China, in 2009. Since 2009, she has been working in the Institute of Electronics, Chinese Academy of Sciences (IECAS). From May to October 2011, she was supported by K.C. Wong Education Foundation Hong Kong and being a guest scientist in the Center for Sensorsystems (ZESS), University of Siegen. Her current research interests include mono- and bistatic SAR signal processing, SAR interferometry and geostationary orbit SAR.
Florian Behner received the Dipl.Ing. degree in electrical engineering from the University of Siegen, Siegen, Germany, in 2009. He is a research assistant at the Center for Sensorsystems, University of Siegen, Siegen, Germany since 2009 and member of the MOSES postgraduate programme. His current research interests include radar sensor development, bistatic SAR processing and noise SAR. Mr. Behner is member of the DPG (German Physical Society).
Simon Reuter received the Dipl.Ing. degree in electrical engineering from the University of Siegen, Siegen, Germany, in 2009. He is a research assistant at the Center for Sensorsystems, University of Siegen, Siegen, Germany since 2009 and member of the MOSES postgraduate programme. His current research interests include radar sensor development, bistatic SAR processing and noise SAR. Mr. Reuter is member of the VDE Association for Electrical, Electronic and Information Technologies.
Holger Nies(M'10) received the Diploma degree in electrical engineering and the Dr. Eng. degree, from the University of Siegen, Siegen, in 1999 and 2006, respectively.
Since 1999 he is a member of the Center for Sensorsystems (ZESS) at the University of Siegen and a lecturer in the Department of Signal Processing and Communication Theory. Since 2010 he is executive director of the International Postgraduate Programme (IPP) "Multi Sensorics" and of the NRW Research School on Multi-Modal Sensor Systems for Environmental Exploration and Safety (MOSES) at the university of Siegen. He is team leader of the SAR group of the ZESS.
He worked in the project sector “Optimal Signal Processing, Remote Sensing - SAR” of ZESS since 1999. He was involved in some project work for Daimler AG (Stuttgart, Germany) in the field of engine modeling and optimization. He was working in the area of SAR interferometry for the German TerraSAR-X mission. Currently he is leading a BMBF funded project regarding optimal processing of TanDEM-X data. His current research interests include bistatic SAR processing, SAR interferometry and distributed data fusion.
Otmar Loffeld(M’05–SM’06) received the Diploma degree in electrical engineering from the Technical University of Aachen, Aachen, Germany, in 1982 and the Eng. Dr. degree and the “Habilitation” in the field of digital signal processing and estimation theory from the University of Siegen, Siegen, Germany, in 1986 and 1989, respectively.
In 1991, he was appointed as a Professor for digital signal processing and estimation theory at the University of Siegen. Since then, he has given lectures on general communication theory, digital signal processing, stochastic models and estimation theory, and synthetic aperture radar. In 1995, he became a Member of the Center for Sensorsystems (ZESS), which is a central scientific research establishment at the University of Siegen (http://www.zess.uni-siegen.de), where he has been the Chairman since 2005. In 1999, he became the Principal Investigator (PI) on baseline estimation for the X-band part of the Shuttle Radar Topography Mission, where ZESS contributed to the German Aerospace Center’s baseline calibration algorithms. He is the PI for the interferometric techniques in the German TerraSAR-X mission, and together with Prof. Ender from FGAN, he is one the PIs for a bistatic spaceborne airborne experiment, where TerraSAR-X serves as the bistatic illuminator while FGAN’s PAMIR system mounted on a Transall airplane is used as a bistatic receiver. In 2002, he founded the International Postgraduate Program “Multi Sensorics,” and based on that program, he established the “NRW Research School on Multi Modal Sensor Systems for Environmental Exploration and Safety (http://www.moses-research.de)” at the University of Siegen as an upgrade of excellence, in 2008. He is the Speaker and the Coordinator of both doctoral degree programs, hosted by ZESS. Furthermore, he is the university’s Scientific Coordinator for “Multidimensional and Imaging Systems.” He is the author of two textbooks on estimation theory. His current research interests include multisensor data fusion, Kalman filtering techniques for data fusion, optimal filtering and process identification, SAR processing and simulation, SAR interferometry, phase unwrapping, and baseline estimation. A recent field of interest is bistatic SAR processing.
Prof. Loffeld is a member of the Information Technology Society of the Association for Electrical, Electronic and Information Technologies and a senior member of the IEEE/GRSS. He was the recipient of a Scientific Research award from Northrhine-Westphalia (“Bennigsen-Foerder Preis”) for his works on applying Kalman filters to phase estimation problems such as Doppler centroid estimation in SAR, and phase and frequency demodulation.
Lijia Huang(M’10) received the B.S. degree in electronic engineering from Beihang University, Beijing, China, in 2006 and the Ph.D. degree in signal processing and information science at the Graduate University of Chinese Academy of Sciences, Beijing, China, in 2011.
Since 2011, she has been working in the Institute of Electronics, Chinese Academy of Sciences (IECAS). Her current research interests include geostationary orbit SAR and SAR interferometry.
Donghui Hu received the B.S. degree from Peking University, Beijing, China, in 1992, and the M.S. degree from the Beijing Institute of Technology, Beijing, in 2001.
He is currently an Associate Research Fellow with the Institute of Electronics, Chinese Academy of Sciences, Beijing.
His main research interests include SAR signal processing, SAR interferometry and SAR calibration.
Chibiao Ding received the B.S. and Ph.D. degrees in electronic engineering from Beihang University, Beijing, China, in 1997.
Since then, he has been working with the Institute of Electronics, Chinese Academy of Sciences, Beijing, where he is currently a Research Fellow and the Vice Director. In 2006, he got the first prize in China's State Technological Invention Award.
His main research interests include advanced SAR systems, signal processing technology, and information systems.
This study was supported in partly by the Special Foundation of President of the Chinese Academy of Sciences, the National Science Foundation of China (No. 61101200), and the authors are gratefully acknowledging the support of K.C. Wong Education Foundation Hong Kong.
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