星载稀布阵对小角度内辐射源的实时测向研究

星载侦察在现代战争中的作用日益显著,对相关技术的研究也成为热点。由于受到有效载荷的限制,星载接收阵列一般采取稀疏阵,因此分析稀疏阵对地面辐射源的测向性能具有重要的现实意义。分析了典型结构稀布阵对地面辐射源的测向性能及测向的实时性问题,所得结果表明5元稀布L阵能够实现对地面辐射源的实时高精度测向。     

Modeling of unsupervised knowledge graph of events based on mutual information among neighbor domains and sparse representation

Text event mining, as an indispensable method of text mining processing, has attracted the extensive attention of researchers. A modeling method for knowledge graph of events based on mutual information among neighbor domains and sparse representation is proposed in this paper, i.e. UKGE-MS. Specifically, UKGE-MS can improve the existing text mining technology's ability of understanding and discovering high-dimensional unmarked information, and solves the problems of traditional unsupervised feature selection methods, which only focus on selecting features from a global perspective and ignoring the impact of local connection of samples. Firstly, considering the influence of local information of samples in feature correlation evaluation, a feature clustering algorithm based on average neighborhood mutual information is proposed, and the feature clusters with certain event correlation are obtained; Secondly, an unsupervised feature selection method based on the high-order correlation of multi-dimensional statistical data is designed by combining the dimension reduction advantage of local linear embedding algorithm and the feature selection ability of sparse representation, so as to enhance the generalization ability of the selected feature items. Finally, the events knowledge graph is constructed by means of sparse representation and l₁ norm. Extensive experiments are carried out on five real datasets and synthetic datasets, and the UKGE-MS are compared with five corresponding algorithms. The experimental results show that UKGE-MS is better than the traditional method in event clustering and feature selection, and has some advantages over other methods in text event recognition and discovery.     

压缩感知稀疏重构对星图的影响

稀疏重构是压缩感知理论的核心内容之一,为了将稀疏重构有效地应用于星敏感器的压缩成像过程中,从星图图像误差和星点特征误差两个方面分析稀疏重构对星图的影响。在图像误差方面,利用峰值信噪比评价指标考察星图在不同重构算法、不同压缩比下的重构质量;在特征误差方面,从理论上分析稀疏重构对星点特征的影响机理,提出星点特征重构误差的评价指标,考察星点的质心、亮度和数量特征的重构误差。结果表明,在所选算法各压缩比下,星图相比一般图像能够获得更高的重构质量,重构星点能够在很大程度上保持可用于姿态确定的特征信息,结论保证了利用重构星图进行姿态计算的正确性,进一步验证了压缩感知理论在星敏感器中应用的可行性,为实现星敏感器的压缩成像提供了现实依据。