基于码分复用的超空间分辨率成像技术

在遥感类光电成像系统中,光学镜头可实现较高空间分辨率,而光电探测器件空间分辨率不足,焦面图像的采样不满足Whittaker-Shannon抽样定理,频谱之间的混叠导致实际分辨率下降。基于此问题,提出了一种通过编码技术标识来自物空间的不同频率,再通过像空间的解码来消除频谱混叠的影响,进而实现超分辨率成像的方法。该方法在光路中没有微镜扫描等机械运动部件,同时具备在一定程度上降低噪声的特点。文中对频谱编码实现超分辨率的机理进行了仿真,依据仿真模型和结果对影响频谱编码效果进行了相关分析。     

基于CPLD的TMS320C6727B外设重叠地址空间解析方法的研究与实现

针对TMS320C6727B扩展外设无法基于其硬件资源直接访问的问题，提出了一种重叠地址解析的外设扩展方法，可满足多个外设、外设多个寄存器或端口地址的访问控制。对外设地址空间构成解析、地址映射CPLD的逻辑控制、用户程序中外设寄存器或端口的访问控制等问题，进行了详细的研究分析，并给出了寄存器或端口逻辑控制和用户程序访问的实现方法。硬件平台测试验证了利用重叠地址解析实现外设访问控制方法的可行性。     

大斜视滑动聚束方位向波束指向控制策略

对星载电扫合成孔径雷达斜视滑动聚束模式，采用传统波束扫描策略中出现的方位向分辨率沿方位向空变大及方位扫描角度过大的问题展开研究。首先，分析采用传统斜视滑动聚束扫描策略情况下，方位向分辨率沿方位向出现空变的原因，探究方位向分辨率与扫描策略、扫描角度的关系。然后，提出基于全局搜索增强鲸鱼优化算法的斜视滑动聚束波束扫描策略，控制不同时刻下的方位向扫描角速度，降低方位向分辨率沿方位向的空变程度，减小天线最大方位向扫描角度，缩短数据录取时间，有效降低系统代价，提升系统性能。最后，通过仿真验证所提策略的有效性，方位向分辨率空变降低至1%以下，数据录取时间与总扫描角度相较于原有方法降低10%以上。     

基于冲突分类与消解的多智能体路径规划算法设计CSCD

多智能体路径规划应用广泛但求解困难。为更好地处理多智能体路径规划中的路径冲突问题,提高求解效率,将冲突进一步分类为相向顶点冲突和交叉顶点冲突,并提出了对应的消解方式。相向顶点冲突的消解方法采用提前添加约束的方式,避免在消解其冲突的过程中产生另一个可预见的冲突;交叉顶点冲突的消解方法采用寻找最佳等待时间的方式,在消解其冲突的同时消解其他存在的冲突。两种冲突消解方法均可减小约束树的规模,在一定程度上减少算法的计算量。并提出了基于冲突搜索算法的高层节点冲突搜索算法。实验结果表明,所提出的冲突分类及消解方式有效地减小了算法高层中约束树的规模,降低了算法计算量,并在智能体密集的环境下表现出更大的优势。     

Target localization method of non-cooperative spacecraft on on-orbit service

With the explosion of the number of meteoroid/orbital debris in terrestrial space in recent years, the detection environment of spacecraft becomes more complex. This phenomenon causes most current detection methods based on machine learning intractable to break through the two difficulties of solving scale transformation problem of the targets in image and accelerating detection rate of high-resolution images. To overcome the two challenges, we propose a novel non-cooperative target detection method using the framework of deep convolutional neural network.Firstly, a specific spacecraft simulation dataset using over one thousand images to train and test our detection model is built. The deep separable convolution structure is applied and combined with the residual network module to improve the network’s backbone. To count the different shapes of the spacecrafts in the dataset, a particular prior-box generation method based on K-means cluster algorithm is designed for each detection head with different scales. Finally, a comprehensive loss function is presented considering category confidence, box parameters, as well as box confidence. The experimental results verify that the proposed method has strong robustness against varying degrees of luminance change, and can suppress the interference caused by Gaussian noise and background complexity. The mean accuracy precision of our proposed method reaches 93.28%, and the global loss value is 13.252. The comparative experiment results show that under the same epoch and batchsize, the speed of our method is compressed by about 20% in comparison of YOLOv3, the detection accuracy is increased by about 12%, and the size of the model is reduced by nearly 50%.     

基于多层次特征的高分影像海岸带地物分类

针对高分辨率影像地物光谱丰富复杂的问题，文章提出了一种结合像元-对象-空间格局特征的水域、盐田等海岸带精细地物分类方法。首先基于像元和空间格局特征分别利用遗传算法优化随机森林参数进行分类；其次将两种分类结果采用D-S证据理论融合；然后基于不同地物斑块的空间上下文信息，采用粒子群算法优化支持向量机（Support Vector Machine，SVM）参数实现面向对象的二次分类。为验证方法的有效性，收集山东省莱州湾海岸带附近区域的“高分二号”卫星影像，开展了水域及水利设施用地、盐田、工矿用地、交通运输用地、住宅用地、沿海滩涂、海域与耕地8类地物的分类实验，总体精度达到97.21%，Kappa系数为0.964 2。实验结果表明，文章提出的高分影像海岸带地物分类方法兼顾像元、对象及空间格局特征优点，能够实现多层次细致分类，并同时兼具较短的训练时长与较高的分类精度。该研究成果可为中国海岸带生态环境监测与土地利用规划提供一定技术支撑。     

Precise orbit determination and baseline consistency assessment for Swarm constellation

Precise orbit determination (POD) and precise baseline determination (PBD) of Swarm satellites with 4 years of data are investigated. Ambiguity resolution (AR) plays a crucial role in achieving the best orbit accuracy. Swarm POD and PBD based on single difference (SD) AR and traditional double difference (DD) AR methods are explored separately. Swarm antenna phase center variation (PCV) corrections are developed to further improve the orbit determination accuracy. The code multipath of C1C, C1W and C2W observations is first evaluated and clear variations in code noise related to different receiver settings are observed. Carrier phase residuals of different time periods and different loop tracking settings of receiver are studied to explore the effect of ionospheric scintillation on POD. The reduction of residuals in the polar and geomagnetic equator regions confirms the positive impact of the updated carrier tracking loops (TLs) on POD performance. The SD AR orbits and orbits with float ambiguity (FA) are compared with the Swarm precise science orbits (PSOs). An average improvement of 27 %, 4 % and 16 % is gained in along-track, cross-track and radial directions by fixing the ambiguity to integer. For Swarm-A/B and Swarm-B/C formations, specific days are selected to perform the DD AR-based POD during which the average distance of the formation satellites is less than 5000 km. Satellite laser ranging (SLR) observations are employed to validate the performance of FA, SD AR and DD AR orbits. The consistency between the SD AR orbits and SLR data is at a level of 10 mm which shows an improvement of 25 % when comparing with the FA results. An SLR residuals reduction of 15 % is also achieved by the DD AR solution for the selected days. Precise relative navigation is also an essential aspect for spacecraft formation flying missions. The closure error method is proposed to evaluate the baseline precision in three dimensions. A baseline precision of 1–3 mm for Swarm-A/C formation and 3–5 mm for Swarm-A/B and Swarm-B/C satellite pairs is verified by both the consistency check and closure error method.     

Assessing the performance of BDS-3 for multi-GNSS static and kinematic PPP-AR

As of 2021, a total of four different GNSS constellations – namely, GPS, GLONASS, Galileo, and BDS-3 – can be used with Full Operational Capability (FOC). In this work, the contribution of BDS-3 FOC to GPS + GLONASS + Galileo (GRE) PPP-AR is investigated, considering the three different cut-off angles (7°, 30°, and 45°) and different lengths of static observation sessions (24-, 12-, 6-, 3-, 1-, 0.5-, 0.25-hour). The data of 31 IGS-MGEX stations is processed with GRE PPP-AR and GREC3 (GPS + GLONASS (using float mode) + Galileo + BDS-3) PPP-AR modes. The results showed that BDS-3 degraded the horizontal (except for 24-h sessions) and vertical accuracy of static GRE PPP-AR solutions regardless of the elevation cutoff angle and observation time. The kinematic results showed that BDS-3 significantly contributed to the accuracy of GRE kinematic PPP-AR for 30° and 45° cutoff angles. The convergence time analysis showed that BDS-3 only contributes to GRE kinematic PPP-AR for the vertical component.     

天基海表精细探测微波载荷性能分析与展望

海表精细探测是海洋卫星未来发展的重要方向。介绍卫星海表参数探测的特点与优势，总结海表温度、海表高度、海表盐度等要素，分析天基探测载荷的发展现状。根据海表参数时空变化特性，分析高时空分辨率微波探测载荷性能需求。在此基础上，针对美国和欧洲相关卫星系统发展计划，分析了高时空分辨率、高精度天基微波探测载荷可实现性与未来发展趋势，针对海表精细探测天基微波载荷的发展提出了建议。     

大气环境监测卫星激光雷达技术

星载激光雷达是高精度测量全球大气CO2柱浓度和气溶胶垂直廓线的重要手段，大气环境监测卫星大气探测激光雷达(ACDL)在一套激光雷达中集成了2种探测体制，采用1 572 nm积分路径激光差分吸收方法测量全球CO2柱浓度，采用532 nm高光谱探测(HSRL)方法测量气溶胶和云的垂直廓线，均为国际首次在星载平台成功验证，是国际首个星载CO2探测激光雷达和国际首个高光谱气溶胶探测激光雷达。在国际已发射的星载激光雷达中，ACDL激光雷达是探测体制最全、波长最多、能量最高、频率最稳和精度最准的激光雷达，实现了创新跨越。大气探测激光雷达在轨连续工作，首次获得了全天时精度优于1 ppm的全球CO2柱浓度、精度优于20%的气溶胶廓线等遥感数据。本文介绍了ACDL激光雷达的工作原理、系统参数以及相关的定标测试结果。