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摘要: 随着我国空间利益拓展与在轨资产规模增长,非合作空间暗弱目标的高精度探测已成为空间安全防御与碎片清除的核心瓶颈。传统光学或雷达探测手段受限于衍射极限与信噪比约束,对“快、远、小、暗”目标的探测与识别精度不足,激光雷达凭借其高精度、抗干扰等优势,逐渐成为空间目标高精度探测的核心技术手段。通过突破传统激光雷达系统的物理限制,亚像素扫描、合成孔径和反射层析等技术能够实现远距离超分辨成像。该文从总结梳理关键问题和关键技术出发,追踪了3种激光雷达超分辨成像技术的关键技术研究进展,分析了典型实验系统和实验结果,并结合空间探测、遥感测绘等任务需求,阐述了各体制的特点、优势和不足,展望了其应用前景和发展趋势。Abstract: With the expansion of China’s space interests and the growth in the scale of on-orbit assets, high-precision detection of dark and weak targets in noncooperative space has become the core bottleneck in space security defense and debris removal. Traditional optical or radar detection technologies are limited by diffraction limit and signal-to-noise ratio constraints, and the detection and identification accuracy of “fast, far, small, and dark” targets is insufficient. Light Detection and Ranging (LiDAR), with its high precision and anti-jamming advantages, has gradually become the core technical means of accurately detecting space targets. Technologies such as sub-pixel scanning, synthetic aperture, and reflective tomography enable long-range super-resolution imaging by breaking through the physical limitations of conventional LiDAR systems. This paper begins by summarizing and sorting the critical problems associated with LiDAR super-resolution technology. The key technological research progress is then reported, typical experimental systems and experimental results are analyzed, and the characteristics, advantages, and shortcomings of each system are described with respect to requirements of space exploration, remote sensing, and mapping missions. Finally, the application prospects and development trends are presented.
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图 3 准直照明与聚焦照明成像原理[27](a)准直照明(b)聚焦照明
Figure 3. Collimated and Focused Illumination Imaging Principles (a) Collimated illumination (b) Focused illumination
图 6 Pawlikowska三维单光子激光雷达对6.8 km目标重建效果[44](a) 可见光波段近景图像(b)和(c)为通过最小二乘寻峰法对6.8 km 桥塔深度强度重建图,(b)和(c)设置阈值不同
Figure 6. Effect of Pawlikowska 3D single-photon LiDAR on 6.8 km target reconstruction[44] (a) Close-up image in the visible band (b) and (c) Depth intensity reconstruction of the 6.8 km bridge tower by the least-squares peak-finding method, with different thresholds in (b) and (c)
图 7 中国科学技术大学徐飞虎团队机载单光子激光雷达系统[45](a) 系统总体外观 (b) 系统与陀螺稳定件 (c) 光学收发装置细节 (d) 实例230 m×470 m 成像结果
Figure 7. Airborne single-photon LiDAR system by USTC Feihu Xu’s team[45] (a) Overall design of the airborne single-photon LiDAR system (b) Main components of the system installed on the gyro stabilization mount (c) Details of the transceiver optics (d) Example 3D imaging result of a 230 m × 470 m region
图 12 Buck团队[77]机载SAL实验(a) 机载平台,(b) 机载系统外观,(c) 机载系统内部结构,(d) 目标光学图像,(e) 无角反射器SAL成像结果,(f) 使用角反射器校正相位误差SAL成像结果
Figure 12. Buck’s team[77] airborne SAL experiment (a) Airborne platform, (b) Airborne system outside, (c) Inside, (d) Target optical image, (e) SAL imaging results without corner, (f) SAL imaging results using corner reflector to correct for phase error reflector
图 16 百公里级SAL成像实验[84](a) 实验场景 (b) 目标及SAL成像结果 (c) 6个角锥的摆放场景(其中两端角锥相距11 m)以及SAL成像结果
Figure 16. SAL experimental scene and imaging results[84] (a) Experimental scene (b) The targets and their SAL imaging result (c) The scene showing the placement of 6 pyramids (where the two end pyramids are 11 m apart) and the SAL imaging
图 17 1 km RTL远场实验不同算法对比[102](a) 重建目标 (b) 全角度采样重建 (c) 间隔20°采样重建 数字1~5代表不同重建算法(1) Inverse Radon (2) FBP (3) ART (4) sparse ART with OMP (5) TV sparse reconstruction with ART
Figure 17. Comparison of different algorithms for 1 km RTL outfield experiments[102] (a) Reconstruction target (b) Full angle sampling reconstruction (c) 20° spaced sampling reconstruction (Numbers 1~5 represent different reconstruction algorithms) (1) Inverse Radon (2) FBP (3) ART (4) Sparse ART with OMP (5) TV sparse reconstruction with ART
图 20 胡以华团队[119]10.38 km激光反射层析室外实验(a) “NUDT”艺术字 (b) 艺术字重建结果 (c) 空间碎片目标 (d) 空间碎片重建结果,(e) 实验装置
Figure 20. 10.38 km laser reflection tomography outdoor experiment by Hu Yihu’s team[119] (a) “NUDT”artwork (b) Artwork reconstruction result (c) Space debris target (d) Space debris reconstruction result (e) Experimental set-up
表 1 典型激光扫描成像系统对比
Table 1. Comparison of typical laser scanning imaging system
文献 年份 距离(km) 分辨率 光源 探测器 系统 图像重建方法 [43] 2013 4.5 — 1550 nm
1.6 mWInGaAs/InP
PDE 26%
DCR16000 /cpsGalvanometer
Scan mirrorpixel-by-pixel
time-correlated cross-correlation[44] 2017 10.5 0.28 m 1550 nm
10 mWInGaAs/InP
PDE 30%
—Galvanometer
Scan mirrorImage mosaicking
TV restoration[46] 2017 0.9 — 532 nm
28 mWSi
PDE 55%
—Galvanometer Scan mirror
Aperture 78 mmModified TV restoration [24] 2020 45.0 0.6 m 1550 nm
120 mWInGaAs/InP
PDE 15%
DCR2200 /cpsGalvanometer Scan mirror
Aperture 279 mmSub-pixel scanning
3D- Deconvolution[25] 2020 201.5 — 1550 nm
600 mWInGaAs/InP
PDE 29%
DCR ~100/cpsGalvanometer Scan mirror
Aperture 279 mmSub-pixel scanning
3D-Deconvolution[47] 2021 3.1 0.11 m 1064 nm
6 μJSi
—
DCR 100/cpsAll-fiber
Rotation platform
Aperture 20.5 mmSub-pixel scanning
3D-Deconvolution[45] 2024 2.1 0.4 m 1550 nm
150 mWInGaAs/InP
PDE 20%
DCR 2000/cpsThree 64×64 SPAD arrays
Aperture 47 mmSub-pixel scanning
3D-Deconvolution*PDE: Photon Detection Efficiency, DCR: Dark Count Rate 表 2 典型SAL系统对比
Table 2. Comparison of typical SAL systems
文献 年份 分辨率 距离 激光参数 相位补偿与成像方法 系统参数 [77] 2011 3.3 cm 1.6 km 1.5 W @ 1550 nm
Phase coding 7 GHzPGA
ConventionalAirborne SAL
Swath 1~2 m (1.67 mrad)
Single- channel[78] 2016 ~ 5 cm 3 km 20 W @ 1030 nm
Galvanometer-frequency 650 HzAttitude compensation
Cross-Track ResamplingAirborne Down look SAL
Swath 14.5 m (4.8 mrad)
Single-channel[79] 2018 12.7 mm×9.2 mm 3.4 km 3 W @ 1030 nm
Galvanometer-frequency 760 Hz
PGA
Envelope alignmentGround down look ISAL
Single-channel[81] 2016 1.8 cm 1.1 km 10 W@ 1550 nm
EOM 4 GHz—
—Ground ISAL
Single-channel[80] 2016 4 cm 2 km 1550 nm
EOM 4 GHzSub-aperture PGA splicing Airbone SAL
Single-channel[72] 2021 ~1 cm 4.3 km 20 W@ 1550 nm
5 GHz—
Time-space stitchingGround ISAL
10-channel array[84] 2024 15.6 mm×1.7 mm 101.8 km 101.3 W
10 GHz—
—Ground ISAL
4×4 micromirror-lens array
Swath 11 m*Res: Resolution, EOM: Electro-Optic Modulation 表 3 典型RTL成像系统对比
Table 3. Comparison of typical RTL imaging systems
文献 年份 距离 分辨率 回波探测方法 激光波长/脉宽 回波处理方法/重构算法/后处理技术 [99] 1989 5.4 km — Doppler
detection10.6 μm
——
Inverse Radon transform
—[113] 2001 500 km 0.2 m Heterodyne
detection11.15 μm
1.5 ns—
FBP
Thresholding[98] 2010 22.4 km 0.15 m Coded aperture —
——
Inverse Radon transform
—[115] 2012 53 m — TCSPC 1.5 μm
4 ps—
FBP
Convex hull mask[119] 2022 10.4 km 0.02 m Direct detection 1.06 μm
73 ps
Feature tracking
FBP
—[102] 2022 1 km — Direct detection 1.06 μm
100 psFeature tracking
TV-ART
—*TCSPC:Time-Correlated Single Photon Counting 表 4 激光雷达超分辨成像技术对比
Table 4. Comparison of LiDAR super-resolution imaging techniques
成像技术 超分辨原理 优势 局限 扫描成像 二维亚像素扫描 技术成熟、效果稳定、成像灵活 分辨率受扫描步进、阵列像素间距、
激光光斑大小等因素限制,随探测距离下降SAL 多个成像口径相干合成 理论分辨率与探测距离无关 需要平台与目标相对运动,对平台稳定度、
激光相干性等要求高,工程难度大RTL 多角度层析重建 理论分辨率与探测距离无关,可与多体制结合 非直视平面成像,需要采集尽可能多的角度回波信息,
平台与目标需相对旋转 -
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