Abstract
Random media pose limitations on the imaging capability of photoelectric detection devices. Currently, imaging techniques employed through random media primarily operate within the laser wavelength range, leaving the imaging potential of terahertz waves unexplored. In this study, we present an approach for terahertz bistatic three-dimensional imaging (TBTCI) of hidden objects through random media. By deducing the field distribution of bistatic terahertz time-domain spectroscopy system, and proposing an explicit point spread function of the random media, we conducted three-dimensional imaging of hidden objects obscured by the random media. Our proposed method exhibits promising applications in imaging scenarios with millimeter-wave radar, including non-invasive testing and biological imaging.
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Introduction
The limitations brought by the existence of random media are widely observed from industrial inspections to medical diagnosis1,2,3,4. For example, existing optoelectronic imaging devices face difficulties in accurately recovering the original appearance in the application such as material defect detection and security inspection5,6,7. Underwater imaging remains a challenge in hydrographic exploration8,9,10, while imaging through surface biological tissues poses difficulties for medical professionals11,12,13,14,15,16.
Scattering phenomena occur across various spectrums. With the transmission environment primarily being the atmosphere, random media in this context mainly comprise small water droplets and aerosol particles, typically on the scale of micrometers or smaller, this size range approximates the wavelength of visible light and infrared waves. As a result, scattering phenomena are pervasive in the optics band, leading to lots of research on imaging through random media. To our knowledge, there are four main approaches to address this issue. The first method involves selectively imaging using ballistic photons17,18,19. When light propagates through random media, there is a chance that some photons will not be scattered by the media. These photons are referred to ballistic photons. Ballistic photons propagate almost in a straight line and arrive ahead of other photons that pass through random media. To accurately capture ballistic photons, one approach is to employ time gating techniques18,19. Time gating technique sets an appropriate temporal gate to exclusively capture the desired light signals and reject those outside the designated time range. Another effective approach is coherent gating technique17,20,21. Coherent gating is a technique employed in optical coherence measurements to measure the intensity distribution of light returning from different depths by controlling the optical path length of the reference light. These methods bypass the effects of scattering but results in significant loss of photon utilization, especially when detecting ballistic photons in thick scattering media or media with strong scattering properties, it will be a severe challenge of detector sensitivity. The second approach involves calculating higher-order correlations of the scattering field22,23,24,25,26, which does not require dealing directly with the troublesome random media. The effectiveness of calculating higher-order correlations depends on the range of memory effects, and often have strict requirements, such as the requirement for the random media to remain static or the restriction on the movement range of the light source. However, recent advancements in research have overcome these constraints, rendering correlation imaging methods more stable and versatile25,26. The third approach establish the connection between image degradation before and after by designing complex and massive neural networks. This method typically requires a large amount of annotated data for training, which in turn demands significant computational resources and time. However, from traditional convolutional neural networks to recent generative adversarial networks, deep learning methods have demonstrated increasing proficiency in the field of imaging through scattering media area27,28,29,30,31,32,33. Finally, the method of accurately simulating the point spread function of random media has the advantages of reliability and low computational complexity, and thus holds significant potential for applications in the field of imaging through random media34,35. This method relies on extensive prior knowledge as support, usually requiring preliminary research to determine the mathematical form of the point spread function and parameter values through pre-calibration. In the terahertz wave and longer wavelength wave (wavelengths greater than 1 mm), water droplets and aerosol particles in the atmosphere have minimal impact. Consequently, imaging through random media is rarely discussed in terahertz wave bands. However, in various fields such as industrial inspection and medicine, synthetic fibers, plastic materials, and biological tissues still exhibit strong scattering effects on terahertz waves. This poses a significant challenge for terahertz detection systems in terms of computational imaging algorithms.
In addition, it is common for imaging through random media algorithms to be designed based on monostatic detection systems. However, to prevent signal aliasing, the monostatic terahertz radar usually uses a transceiver to control the emission and reception of terahertz pulses or a beam splitter to change the direction of terahertz wave propagation. These lead to an increase in measurement time or a decrease in received signal intensity.
In this study, in order to enhance the imaging capabilities of terahertz waves through random media and overcome the efficiency limitations associated with monostatic radar, we introduce a method for terahertz bistatic three-dimensional imaging (TBTCI) of hidden objects through random media. We model and invert the scattering of terahertz waves that travel through random media, propagate through free space to a hidden object, scatter back, and travel through random media again. We designed multiple random media occlusion scenarios and tested our method with various hidden object types, and in all cases, the hidden object images were recovered.
Experiment and methods
Experimental setup
Our experimental setup, illustrated in Fig. 1, employs a bistatic terahertz time-domain spectroscopy (TDS) system as the terahertz source and detector. In Fig. 1b, we present an overhead view of our experimental setup, depicting the coordinate system utilized in the calculation process, as well as the points, surfaces, and regions of significance. Set the z = 0 plane as the surface of the random media near the detector side. The terahertz source and detector are fixed in the detection region \(\Omega_{D} = \left\{ {\left( {x,y,z} \right) \in {\mathbb{R}} \times {\mathbb{R}} \times {\mathbb{R}}|z < 0} \right\}\) and symmetrically positioned about the x = 0 plane. The center lines of the terahertz beam and detector’s receiving region are pointed towards (0, 0,\(z_{o}\)), forming an acute angle of \(\theta\) with the x = 0 plane. In our experiment, we only emit and receive vertically polarized terahertz waves, allowing us to express the electromagnetic field in scalar form in the subsequent text. The random media is situated in the random media region \(\Omega_{RM} = \left\{ {\left( {x,y,z} \right) \in {\mathbb{R}} \times {\mathbb{R}} \times {\mathbb{R}}|0 \le z < d} \right\}\) between the target and terahertz time-domain spectroscopy system, while the hidden object is placed in the target region \(\Omega_{T} = \left\{ {\left( {x,y,z} \right) \in {\mathbb{R}} \times {\mathbb{R}} \times {\mathbb{R}}|z \ge d} \right\}\) with its geometric center located at (0, 0,\(z_{o}\)). In our system, \(\theta\) is approximately 10°, zo is 7 cm. By utilizing a 2-D displacement platform, we moved the hidden object across a two-dimensional plane, enabling the terahertz waves to illuminate different locations on the hidden object and allowing the detector to collect the corresponding time-domain waveforms. This process resulted in a set of three-dimensional data regarding the dimensions of x, y, t.
The terahertz TDS system utilized in our experiment is a T-ray 5000 produced by Advanced Photonix. The terahertz source employed in the experiment emitted pulses with a central frequency of 0.3 THz and a full width at half maximum (FWHM) of around 4 ps, featuring ultra-short Gaussian pulses. The detector used had a receiving aperture of 4 cm in diameter. The detector we utilized is the receiver module of the T-ray 5000. This module features a 700 ps temporal gate, a maximum sampling frequency of 100 Hz, and an adjustable optical delay system. To facilitate movement of the hidden object, we employed a 2-D displacement platform that moves hidden object within an M \(\times\) N grid area, in our experiment, M and N were both set to 32, resulting in a scanning area of approximately 10 cm \(\times\) 5 cm. The hidden objects were cut into special shapes from tin foil and attached to an acrylic board for fixation. Polypropylene plastic particles with an average diameter of 4 mm were used to fill an acrylic container, which measured 10 cm \(\times\) 10 cm \(\times\) 3 cm along x, y, z axes, serving as the random media. random media RM1 is placed between hidden objects and terahertz source, while random media RM2 is placed between hidden objects and detector. Both RM1 and RM2 shared the same composition and configuration in our experiments.
Our imaging scheme operates under the assumption that the signal returned from the hidden object can be temporally separated from the signal directly returned from the random media. When actively probing an object hidden behand random media, a portion of the terahertz waves will directly return from the random media due to the scattering effect, while others will return after reaching the object. In order to avoid interference from signals that directly return from random media and to maximize the reception of signals during a single detection process, we selected the maximum duration that the detection system can receive, specifically 700 ps, as the length of the temporal gate. Additionally, we adjusted the optical delay length of the system to set an appropriate opening time for the time gate in order to block signals that return from random media. When the object is closely adjacent to the random media or submerged within it, the signal returning from random media overlaps with the signal returning from the object, which distorts the latter signal. Consequently, it is essential to carefully adjust the opening time of the temporal gate. In order to mitigate this distortion, one possible solution could be pre-measuring a set of data without the object can be used as background, enabling the elimination of this background signal from the data obtained with the object. To avoid this distortion, the minimum time interval between the signal returning from random media and the signal returning from the object should exceed the full width at half maximum (FWHM) of the signal returning from the object, indicating the object should be separated from the random media by a certain distance, which corresponds to the FWHM of the signal returning from the object times the speed of light. In our experiment, it is necessary for the object to be separated from the random media by a minimum distance of 2 cm. Besides, as the opening time of the time gate and the emission time of terahertz waves are not consistent, we only focus on the relative position of the hidden objects within the time gate, rather than their absolute time position. We set time t = 0 as the opening time of the time gate.
Imaging method
The complete propagation path of terahertz wave is illustrated in Fig. 1b. To begin with, the terahertz wave emits from the terahertz source, reaches a point \({\mathbf{r}}_{0} \in {\mathbf{S}}_{0} = \left\{ {\left( {r_{0,x} ,r_{0,y} ,r_{0,z} } \right) \in {\mathbb{R}} \times {\mathbb{R}} \times {\mathbb{R}}|r_{0,z} = 0} \right\}\) in the z = 0 plane. In the bistatic terahertz TDS system we employed, the terahertz source field distribution is in the form of a Gaussian pulse, but terahertz waves are not normally incident random media, instead, the terahertz beam forms an angle \(\theta\) with the z-axis. Therefore, the terahertz source field distribution needs to be projected onto the coordinate adopted by our system. Here, we derive the z = 0 plane electric field distribution \(E_{0} \left( {t,{\mathbf{r}}_{0} } \right)\) in the bistatic terahertz TDS system.
To calculate \(E_{0} \left( {t,{\mathbf{r}}_{0} } \right)\), the terahertz source field distribution in the x direction needs to be multiplied by a factor of \(\cos \theta\), and The propagation factor \(t - \left( {{\mathbf{r}}_{0,z} - {\mathbf{r}}_{{0,z_{0} }} } \right)/c_{0}\) is replaced by \(t - \left( {\frac{{\left( {{\mathbf{r}}_{0,z} - {\mathbf{r}}_{{0,z_{0} }} } \right) - \left( {{\mathbf{r}}_{0,x} - {\mathbf{r}}_{{0,x_{0} }} } \right)\tan \theta }}{{\sqrt {1 + \tan^{2} \theta } }}} \right)/c_{0}\), in which \(\left| {\frac{{\left( {{\mathbf{r}}_{0,z} - {\mathbf{r}}_{{0,z_{0} }} } \right) - \left( {{\mathbf{r}}_{0,x} - {\mathbf{r}}_{{0,x_{0} }} } \right)\tan \theta }}{{\sqrt {1 + \tan^{2} \theta } }}} \right|\) is the distance between the point \(\left( {{\mathbf{r}}_{0,x} ,{\mathbf{r}}_{0,y} ,{\mathbf{r}}_{0,z} } \right)\) and the equiphase plane \(r_{0,z} = \tan \theta \left( {r_{0,x} - r_{{0,x_{0} }} } \right) + r_{{0,z_{0} }}\). \(c_{0}\) denotes the speed of light in vacuum. Taking these factors into account, the distribution of \(E_{0} \left( {t,{\mathbf{r}}_{0} } \right)\) can be expressed as:
whereas \(\sigma_{xy}\) represents the standard deviations of the Gaussian pulse distribution in dimensions x, y, and \(\sigma_{t}\) represents the standard deviations of the Gaussian pulse distribution in dimensions t. \(\omega_{0}\) denotes the main frequency of the Gaussian pulse.
Subsequently, the terahertz wave travels through RM1 and arrives at a point \({\mathbf{r}}_{1} \in {\mathbf{S}}_{d} = \left\{ {\left( {r_{1,x} ,r_{1,y} ,r_{1,z} } \right) \in {\mathbb{R}} \times {\mathbb{R}} \times {\mathbb{R}}|r_{1,z} = d} \right\}\) situated in the z = d plane of \(\Omega_{RM}\). The electric filed distribution \(E_{1} \left( {t,{\mathbf{r}}_{0} } \right)\) in this z = d plane can be expressed as:
while \(h_{{{\mathbf{RM}}_{1} }} (t,{\mathbf{r}}_{0} ,{\mathbf{r}}_{1} )\) is the point spread function of the random media RM1.
The scattered terahertz wave further propagates towards a point \({\mathbf{x}} \in \Psi = \left\{ {\left( {x,y,z} \right) \in {\mathbb{R}} \times {\mathbb{R}} \times {\mathbb{R}}|z \ge d} \right\}\) located on the hidden object. After reflecting off the hidden object, it reaches a point \({\mathbf{r}}_{2} \in {\mathbf{S}}_{d} = \left\{ {\left( {r_{1,x} ,r_{1,y} ,r_{1,z} } \right) \in {\mathbb{R}} \times {\mathbb{R}} \times {\mathbb{R}}|r_{1,z} = d} \right\}\) situated in the z = d plane. The electric filed distribution in the z = d plane can be described as follows:
where \(\chi_{{\text{o}}} \left( {t,{\mathbf{r}}_{2} - {\mathbf{r}}_{1} } \right)\) is the point spread function of the target region \(\Omega_{T}\). We make an approximation that the main lobe distribution of terahertz wave propagates almost unchanged in the target region. In other words, we consider \(\chi_{{\text{o}}} \left( {t,{\mathbf{r}}_{2} - {\mathbf{r}}_{1} } \right)\) to be the hidden object reflectance distribution \(R\left( {{\mathbf{x}};\theta } \right)\) in our system, in which the center lines of the terahertz beam and detector’s receiving region are aimed at (0, 0,\(z_{o}\)), and forms an acute angle of \(\theta\) with the x = 0 plane as shown in Fig. 1b.
The terahertz waves travel through RM2 and arrive at a point \({\mathbf{r}}_{3} \in {\mathbf{S}}_{0} = \left\{ {\left( {r_{0,x} ,r_{0,y} ,r_{0,z} } \right) \in {\mathbb{R}} \times {\mathbb{R}} \times {\mathbb{R}}|r_{0,z} = 0} \right\}\) in the surface z = 0. Eventually, terahertz waves reach the detector's receiving aperture for detection, as illustrated in the Fig. 1b. Consequently, the electric field received by the detector can be represented as:
where \(h_{{{\mathbf{RM}}_{2} }} (t,{\mathbf{r}}_{2} ,{\mathbf{r}}_{3} )\) is the point spread functions of the random media RM2. The simplified convolution form of \(E_{detection} \left( {t,{\mathbf{r}}_{3} } \right)\) can be expressed as:
\(\otimes\) represents a three-dimensional convolution operation along x, y, t dimensions. Based on Eq. (5), it is easy to use a Wiener deconvolution procedure to recover the hidden object reflectance distribution \(R\left( {{\mathbf{x}};\theta } \right)\). Let \(T(t,{\mathbf{r}}_{0} ,{\mathbf{r}}_{1} ,{\mathbf{x}},{\mathbf{r}}_{2} ,{\mathbf{r}}_{3} )\) represents \(E_{0} (t,{\mathbf{r}}_{0} ) \otimes h_{{{\mathbf{RM}}_{1} }} (t,{\mathbf{r}}_{0} ,{\mathbf{r}}_{1} ) \otimes h_{{{\mathbf{RM}}_{2} }} (t,{\mathbf{r}}_{2} ,{\mathbf{r}}_{3} )\). e is given by:
where \(\mathcal{F}\) and \(\mathcal{F}^{ - 1}\) represents the Fourier transform and inverse Fourier transform, while the superscript “\(*\)” denotes the complex conjugate operation. The operator \(\left| \cdot \right|^{2}\) performs the calculation of the squared magnitude.\(\left| {\mathcal{F}\left\{ T \right\}} \right|^{2} = \mathcal{F}\left\{ T \right\} \cdot \mathcal{F}\left\{ T \right\}^{*}\). Additionally, snr refers to the ratio of the signal power spectrum to the noise power spectrum. However, it is often challenging to obtain prior knowledge about these spectrums during the imaging process through random media. In such cases, a commonly used approximation method is to set snr as a constant value.
Results and discussion
We propose an explicit random media point spread function model \(h_{{{\mathbf{RM}}_{1} }} (t,{\mathbf{r}}_{0} ,{\mathbf{r}}_{1} )\) based on the work of Guy Satat et al.35. In our experiment, both random media RM1 and RM2 share the same size. Therefore, we assume that the form of \(h_{{{\mathbf{RM}}_{2} }} (t,{\mathbf{r}}_{2} ,{\mathbf{r}}_{3} )\) is consistent with \(h_{{{\mathbf{RM}}_{1} }} (t,{\mathbf{r}}_{0} ,{\mathbf{r}}_{1} )\).
here, \(\alpha\) is a field intensity scaling factor, \(f_{T} (t)\) denotes the probability density distribution function of the detected terahertz field at time t, \(f_{T} (t)\) describes the broadening of the temporal distribution of terahertz pulses when propagating through random media. \(W(x,y|t)\) represents the probability density distribution function of the detected terahertz field at position (x, y) given the time t, \(W(x,y|t)\) describes the broadening of the spatial distribution (x, y) of terahertz pulses when propagating through random media. As a result of the greater scattering and absorption of high-frequency terahertz waves in random media compared to low-frequency terahertz waves. This effect significantly suppresses the high-frequency components of the terahertz waves while allowing the low-frequency components to pass through. In Eq. (6), \(F\left( {\Delta \omega } \right)\) is low-pass filter for terahertz waves. We assume that the detected terahertz wave spectrum has the same Gaussian shape as the incident terahertz wave, By fitting the measurements, we obtained the center frequency of measurements as \(\omega_{d} = \omega_{0} - \Delta \omega\).\(f_{T} (t)\) and \(W({\mathbf{r}}_{0} ,{\mathbf{r}}_{1} |t)\) are both normalized. \(W({\mathbf{r}}_{0} ,{\mathbf{r}}_{1} |t)\) refers to a time-correlated Gaussian diffusion kernel, which can be expressed in the following form:
where D is a parameter related to the frequency of terahertz wave, as well as the scattering coefficient and absorption coefficient of the random media, c denotes the speed of light inside the random media,\(c = {{c_{0} } \mathord{\left/ {\vphantom {{c_{0} } n}} \right. \kern-0pt} n}\), while n represents the refractive index of random media, \(t_{0}\) accounts for the offset of the hidden object signal relative to the time gate opening time, and its specific value is determined through actual measurement data. Similarly, we follow the same approach as Guy Satat et al.35 to determining the specific value of parameter D using a line search method.
The distribution form of \(f_{T} (t)\) is given by:
\(\sigma_{t}^{\prime }\) is the standard deviation of \(f_{T} (t)\).
The parameters used in the experiment for the above-mentioned model are as follows:\(\alpha\) is \(9 \times 10^{ - 5}\) V/m, D is \(2.2 \times 10^{ - 4}\) m, \(c_{0}\) is \(3 \times 10^{8}\) m/s, \(\omega_{0}\) is \(2.5 \times 10^{11}\) Hz, \(\Delta \omega\) is \(1.7 \times 10^{11}\) Hz, \(\sigma^{\prime}_{t}\) is \(5.1 \times 10^{ - 12}\) s. \(\sigma_{t}\) is \(1.7 \times 10^{ - 12}\) s, \(\sigma_{xy}\) is \(2.1 \times 10^{ - 3}\) m.
To test the distortion effect of polypropylene plastic particles on terahertz waves, we first used a square aluminum foil with a side length of 1.5cm as the target, and measured the detection field distribution in the presence of RM1 and RM2 simultaneously, as shown in the Fig. 2. Figure 2a shows the distribution of the detection field when the target is not blocked by RM1 and RM2. Due to the wrinkles in the aluminum foil, the detection field distribution image shows an irregular shape. Figure 2b shows the detection field distribution when the target is blocked by RM1 and RM2. Figure 2c shows the comparison of the time-domain distribution of the detection field before and after the target is blocked. For ease of presentation, we take the maximum projection in the t direction in Fig. 2a,b. The full width at half maximum of Fig. 2b is 1.5cm which is the side length of the square aluminum foil. In Fig. 2c, the full width at half maximum of the detection field distribution when the target is blocked by RM1 and RM2 is three times greater than the target is not blocked. Due to the scattering effect of the random media, the maximum intensity value of Fig. 2b is less than 2% of that in Fig. 2a. Additionally, we have computed the Structural Similarity Index measure (SSIM) between Fig. 2a and b. SSIM evaluates the similarity between two images by computing brightness, contrast, and structural metrics. The range of SSIM values is from 0 to 1, where higher values indicate greater similarity. The SSIM index between Fig. 2a and b is only 0.1434, indicating a significantly low level of similarity.
We examine our imaging scheme in three imaging scenarios, as follows: Scene1, where both the terahertz source and detector are completely blocked by random media; Scene2, where only the terahertz source is blocked by random media; and Scene3, where only the detector is blocked by random media. These scenarios correspond to the presence of random media RM1, the presence of random media RM2, and the presence of both RM1 and RM2. When the random media is absent, we assume that the field distribution remains almost unchanged as terahertz waves propagate through this area. In Fig. 3, we display the recovered results of the numbers “207” in all three scenarios. These numbers are cut from tin foil, pasted on an acrylic board, and placed parallel to the x-o-y plane. In the experiment, all detection data and computations are carried out in three dimensions (x, y, t). For convenience in presentation, we take the maximum projection in the t direction of the three-dimensional matrix.
The results demonstrate that our proposed TBTCI method effectively recovers numbers “207” in the three scenarios, and improves the resolution of the numbers “207”, particularly in distinguishing numbers 2 and 0 in Scene2 and Scene3. Figure 3g,j illustrate that our method exhibits similar recovery ability in Scene2 and Scene3, which validates the rationality of using the same point spread function at RM2 and RM1. In Scene 1, due to the simultaneous presence of RM1 and RM2, the terahertz waves pass through the random media twice, resulting in a significantly weakened detection signal, reduced signal-to-noise ratio, and slight poor recovery result. Nevertheless, our method still enables the numbers “2” and “7” to be discernible.
Moreover, we also examined the recovery capability of our method for volumetric objects. These volumetric objects include the letters “UT”, which were created by cutting tin foil and affixing them to acrylic boards. They were then positioned on different z planes with a separation distance of 2 cm. Additionally, a combination of a metal cylinder and a metal sphere. The corresponding recovery results are shown in Figs. 4 and 5.
Figure 4 demonstrates that our method performs well in recovering objects situated on various planes. The concave portion in the middle of the letter “U” and the edges of the letter “T” exhibit sharpness and clarity in the recovery results. Furthermore, From the recovery results, we determine that the distance between two letters is 2.02 cm, however, due to the utilization of a bistatic measurement method, this distance needs to be divided by a factor of \(\cos \theta\). Therefore, the recovered distance \(\Delta \hat{z}\) is 2.05 cm.
In the case of the combination of a metal cylinder and a metal sphere, we conducted imaging experiments of these objects in Scene1 by adjusting their relative positions, as shown in Fig. 5. These relative positions are as follows: the sphere and cylinder are placed side by side with their front surfaces in the same z-plane; the sphere is placed on the side of cylinder, closer to the detector; and the sphere is in front of the cylinder. Due to the smooth surfaces of these objects, they predominantly reflect terahertz waves through specular reflection. Consequently, only the surfaces approximately perpendicular to the z-axis can be accurately reconstructed. As the metal sphere's surface normal changes along the x and y axes, it appears as a bright spot in the recovery results. On the other hand, the metal cylinder does not exhibit a surface normal change along the y-axis, resulting in a bright band representation. When the cylinder is obstructed by the sphere, there will be some discontinuous reflectivity areas in the recovery results, such as those observed in Fig. 5,k. Although these areas are adjacent in the ground truth image, the non-specular reflection portion of the metal sphere reflects terahertz waves in directions that cannot be detected. Our method effectively suppresses noise, enabling the recovery of reflectance variations with respect to the metal surface's normal direction, as well as the spatial positions of the reflection surfaces.
Conclusion
In this study, we conducted imaging experiments on objects obscured by random media using a bistatic terahertz time-domain spectroscopy system. By introducing an explicit point spread function of random media, we recover the image of hidden object obscured by the random media. We investigated three types of hidden objects under three random media occlusion scenarios, the experimental results convincingly demonstrate the effectiveness of our imaging method in recovering the images of these hidden objects. Our proposed technique, known as terahertz bistatic three-dimensional computational imaging (TBTCI) through random media offers a solution for imaging in the millimeter-wave range, particularly for applications such as non-invasive testing and biological imaging.
Data availability
The datasets generated during and/or analyzed during the current study are available from the corresponding author on reasonable request.
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This work is supported by Ministry of Science and Technology of China, 210222.
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Q.Y. and L.L. designed the experiments and developed the method; Q.Y. and H.C. performed the experiments; Q.Y., X.Z. and Z.L. analyzed the data; L.L. and H.Y. supervised the project. All authors were involved in preparing the manuscript.
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Yu, Q., Cai, H., Zhu, X. et al. Terahertz bistatic three-dimensional computational imaging of hidden objects through random media. Sci Rep 14, 6147 (2024). https://doi.org/10.1038/s41598-024-56535-y
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DOI: https://doi.org/10.1038/s41598-024-56535-y
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