基于Rao-Blackwellized蒙特卡罗数据关联的检测跟踪联合优化

提出了基于Rao-Blackwellized蒙特卡罗数据关联的雷达目标检测跟踪联合优化算法。Rao-Blackwellization方法将单目标跟踪与数据关联分开处理,将序贯蒙特卡罗方法（粒子滤波）用于数据关联,实现杂波与虚警量测中的多目标跟踪。同时,根据粒子的分布范围确定波门大小。在考虑粒子权重的前提下,利用检测单元与所有粒子的相对位置对检测门限进行修正,提高检测率。将本文算法与已经实现的基于空域特性的杂波抑制算法相结合,分别应用于仿真数据、S波段相参与非相参雷达实测数据。实验结果表明,本文算法能够在粒子数较少的情况下,实现对小弱目标的检测与跟踪。      

中国大豆进口贸易影响因素的实证分析

近年来我国大豆需求及进口数量逐年增长,大豆的对外依存度也逐年提高。文章选取国内大豆产量、大豆进口量、豆油及豆粕产量、国内外价格比等指标,利用Johansen检验法确定各变量之间的协整关系,采用Granger因果检验法确定中国大豆进口贸易的影响因素。研究证实,国内大豆产量、豆粕和豆油需求、国内外大豆价格比是影响我国大豆进口的重要因素,提出了控制大豆进口规模、积极生产非转基因大豆等政策建议。     

联合交互式多模型概率数据关联算法

通过对交互式多模型（IMM）算法和概率数据关联（PDA）算法的研究,指出Bar-Shalom和Blom等提出的IMMPDA算法结构和理论上存在的问题。根据全局最优的思想,设计了一个最优波门,从而得到全局最优的量测集合,保证了系统的理论完整性和结构合理性。推导完成了新的联合IMMPDA算法--C-IMMP-DA算法。大量仿真计算验证了C-IMMPDA算法在减少计算量的同时,总体性能上较之原IMMPDA算法有大幅度提高。     

多目标无源跟踪中的多特征模糊综合数据关联算法

提出了一种多目标无源跟踪中的数据关联算法———多特征模糊综合数据关联算法。首先基于目标特征关联因子模型,进行单跟踪门的多特征数据关联模糊评估,得到单跟踪门内的有效观测与真实目标的模糊关联程度,在此基础上,进行了多目标数据关联模糊综合评估,得到多目标整体模糊关联程度,最后进行多目标关联判决。由于该算法综合利用了目标更多的特征信息,所以比传统的NN方法有更好的关联性能,计算机仿真表明,它比NN方法的错误关联率约低15%。     

基于模糊ISODATA*的关联规则聚类算法

在对模糊ISODATA算法分析的基础上,提出了一种适用于关联规则聚类ISODATA^*算法。本文首先分析了距离聚类的不足,然后结合关联规则的表示形式,提出了基于属性权重实现规则聚类的思想,并给出了相应的实现算法。最后采用国际上的UCI数据库进行了实验。实验表明该算法能有效地对关联规则进行聚类。     

残差滤波及其在密集多回波环境下机动多目标跟踪中的应用

 修正概率数据关联滤波（MPDAF）是目前解决密集多回波环境下机动多目标跟踪较为有效的方法,但当回波密度增高时,该方法容易失跟。本文针对此特点,在MPDAF基础上,提出了残差滤波（RF）方法,分别从理论和Monte carlo仿真两方面揭示了RF与数据关联的内在机理,结果表明该方法能大幅度提高跟踪滤波器捕捉目标和剔除关联域内多余回波的能力以及跟踪的性能,是一种解决高密集多回波环境下机动多目标跟踪的有效方法。     

Identification of uncatalogued LEO space objects by a ground-based EO array

A ground-based electro-optical (EO) array, deployed at the Jilin Space Tracking Base of Changchun Observatory, China, has been in operation since April 2017. The array has 8 small telescopes, each has an aperture of 15 cm and a field of view of 14° × 14°. On average, the array can collect angles data over 3–4 thousand Very Short Arcs (VSAs) of Low Earth Orbit (LEO) space objects each night. Correlation of the VSA angles data with the NORAD catalogue objects results in about 85% of all the VSAs being correlated to NORAD objects. The remaining 15% VSAs angles data could be supposed from uncatalogued objects. The Initial Orbit Determination (IOD) solutions of the VSAs with the range-search method and the association results of the IODs with the geometrical method are presented. The mean IOD success rate is about 91% and the True Positive (TP) rate is more than 86%. In addition, the classical Gauss, Laplace, Gooding and Double-r angles-only IOD methods are applied to process VSA angles data and their performance is assessed. The CBTA method is used to associate the IOD tracks and compared with the geometrical method. A set of procedures for identifying the uncatalogued objects based on the VSA angles data is designed. Processing of the VSA angles data from Aug 4 to Sep 30, 2017 reveals there are possibly 415 uncatalogued LEO objects.     

Track Association for Dynamic Target Tracking System Based on AP Algorithm

Track association of multi-target has been recognized as one of the key technologies in distributed multiple-sensor data fusion system,and its accuracy directly impacts on the performance of the whole tracking system.A multi-sensor data association is proposed based on aftinity propagation(AP)algorithm.The proposed method needs an initial similarity,a distance between any two points,as a parameter,therefore,the similarity matrix is calculated by track position,velocity and azimuth of track data.The approach can automatically obtain the optimal classification of uncertain target based on clustering validity index.Furthermore,the same kind of data are fused based on the variance of measured data and the fusion result can be taken as a new measured data of the target.Finally,the measured data are classified to a certain target based on the nearest neighbor ideas and its characteristics,then filtering and target tracking are conducted.The experimental results show that the proposed method can effectively achieve multi-sensor and multi-target track association.     

卫星星座的空域覆盖性能计算模型

空域覆盖性能计算是星座覆盖性能分析的重要组成部分。分析了星座的关注区域,参考美国的SMTS系统,归纳了空域覆盖性能的主要影响因素;提出了Walker—delta星座最小覆盖重复周期的简化计算,以及基于最小覆盖重复周期内的经纬度覆盖等效性,这两方面可为空域覆盖性能计算中的仿真时间界定和空间采点提供依据;最后举例详细阐明了星座空域覆盖性能的基本特征．并基于此得出星座空域覆盖性能的评价角度,以此作为星座空域覆盖特性的本质表现。