组合卫星导航系统的快速选星方法

分析了选星数目与几何精度因子(GDOP, Geometry Dilution of Precision)及导航运算量的关系,基于遗传算法提出了一种以满足用户定位精度需求为条件的快速选星方法——快速遗传选星法.根据用户需求确定选星数目初值、选星数目最大值和GDOP阈值,构造选星方案的初始种群,在进化代数上限为1的条件下对种群进行选择、交叉和变异运算,获得初始选星解,根据初始解的GDOP与阈值的关系确定是否依据GDOP最小原则对初始解进行优化,直至满足算法终止条件,输出选星解.仿真结果表明,该算法可以在一次进化之内以不低于92.45%的概率满足GDOP阈值在2.5~6的要求,同时可有效降低54.75%以上的导航运算量.      

基于编队形状的反舰导弹预定目标选择模型特点

相比传统的预定目标选择方法,基于编队形状的反舰导弹预定目标选择方法是一类新方法。为了便于进一步研究具体算法,需要研究基于编队形状的反舰导弹预定目标选择模型的特点。该类方法的实质是将目标选择问题转化为点集匹配问题,因而文章从点集的信息来源、点集之间的变换关系、点集之间的映射关系、点集之间的距离函数等方面分析了模型特点,并根据这些特点将基于编队形状的反舰导弹预定目标选择算法分为2类：即基于迭代收敛的预定目标选择算法和基于变换位置集合的预定目标选择算法。     

Relay selection based on MAP estimation for cooperative communication with outdated channel state information

In this paper, we consider an amplify-and-forward (AF) cooperative communication system when the channel state information (CSI) used in relay selection differs from that during data transmission, i.e., the CSI used in relay selection is outdated. The selected relay may not be actually the best for data transmission and the outage performance of the cooperative system will deteriorate. To improve its performance, we propose a relay selection strategy based on maximum a posteriori (MAP) estimation, where relay is selected based on predicted signal-to-noise ratio (SNR). To reduce the computation complexity, we approximate the a posteriori probability density of SNR and obtain a closed-form predicted SNR, and a relay selection strategy based on the approximate MAP estimation (RS-AMAP) is proposed. The simulation results show that this approximation leads to trivial performance loss from the perspective of outage probability. Compared with relay selection strategies given in the literature, the outage probability is reduced largely through RS-AMAP for medium-to-large transmitting powers and medium-to-high channel correlation coefficients.     

月球返回再入着陆场位置选择限定因素分析

月球返回再入着陆场不仅影响月-地返回转移和返回再入飞行,同时也影响整个月球飞行任务的规划和设计.文章首先分析了航天器与地-月间的相对位置关系;结合月-地返回转移及返回再入轨道特性,理清了月球、地球着陆场和航天器三者在惯性空间内相对位置的内在约束关系;最后分析并通过仿真研究,明确了制约航天器返回再入着陆场位置选择的限定因...     

基于突变理论的机场选址评价研究

针对机场选址评价中大多采用模糊评价方法需要确定指标体系权重,使得评价结果带有较强主观性的问题,将突变理论应用到民用机场选址的合理性及可持续发展评价中来。在对影响机场选址因素进行分析的基础上进行各因素的分解排序,将底层评价指标进行标准量化后,运用突变理论的归一化公式进行计算,得到机场选址合理性及可持续性的突变评价值。针对突变评价值偏高的缺点,给出转换公式,运用Matlab对评价值进行转换计算。实例计算验证了该方法的可行性、有效性和实用性。     

基于飞行品质的飞机控制增稳系统参数估计

提出了一种控制增稳系统参数的设计方法,即利用低阶等效系统和飞行品质边界,通过搜索算法确定满足对应飞行品质的参数集合,再利用多种飞行品质确定的参数集合的交集和数据的插值算法,确定控制增稳系统的控制律参数。通过纵向增稳系统设计仿真表明,所提方法简化了传统设计方法通过性能指标反复选择参数和验证系统飞行品质的过程,为控制增稳系统的设计提供一种简单有效的方法。     

A Fast Global Node Selection Algorithm for Bearings-only Target Localization

In the target tracking, the nodes aggregate their observations of the directions of arrival of the target. The network then uses an extended Kalman filter （EKF） to combine the measurements from multiple snapshots to track the target. In order to rapidly select the best subset of nodes to localize the target with the minimum mean square position error and low power consumption, this paper proposes a simple algorithm, which uses the location information of the target and the network. The lower botmd of localization error is utilized according to the distances between the target and the selected active nodes. Furthermore, the direction likelihoods of the active nodes is predicted by way of the node/target bearing distributing relationships.     

基于光谱信息散度的光谱解混算法

光谱解混是高光谱遥感定量化的关键,提出了一种基于光谱信息散度和光谱混合分析的光谱解混改进算法(SID-SMA,Spectral Information Divergence-Spectral Mixed Analysis).以光谱信息散度判定最优端元子集,端元选择时采用端元的初选和二次选择来提高端元选择的精度,得到较小的丰度估计误差.通过光谱库模拟数据的结果可以看出,SID-SMA的端元选择精度和丰度估计精度要优于其他算法,当信噪比为100∶ 1时,算法端元选择正确率达到了99.8%,29个端元的丰度估计总误差小于0.1,并且算法的速度较快.     

Application of support vector machine combined with K-nearest neighbors in solar flare and solar proton events forecasting

The support vector machine (SVM) combined with K-nearest neighbors (KNN), called the SVM-KNN method, is new classing algorithm that take the advantages of the SVM and KNN. This method is applied to the forecasting models for solar flares and proton events. For the solar flare forecasting model, the sunspot area, the sunspot magnetic class, and the McIntosh class of sunspot group and 10 cm solar radio flux are chosen as inputs; for the solar proton event forecasting model, the inputs include the longitude of active regions, the flux of soft X-ray, and those for the solar flare forecasting model. Detailed tests are implemented for both of the proposed forecasting models, in which the SVM-KNN and the SVM methods are compared. The testing results demonstrate that the SVM-KNN method provide a higher forecasting accuracy in contrast to the SVM. It also gives an increased rate of ‘Low’ prediction at the same time. The ‘Low’ prediction means occurrence of solar flares or proton events with predictions of non-occurrence. This method show promise for forecasting models of solar flare and proton events.     

基于黎曼距离的编队飞行卫星姿态控制系统故障检测数据优选方法

为突破星上资源的严苛约束、提升编队飞行卫星故障检测能力,提出了一种适用于编队飞行卫星姿态控制系统的故障检测数据优选方法,通过利用黎曼距离衡量无故障情况和故障情况下系统测量信息之间的差距,构建了编队飞行卫星姿态控制系统故障检测能力的评价指标。在此基础上,提出了故障检测数据优选方法,为系统输出信息结构优化提供了理论依据。仿真表明,所提出的方法能够在星上资源受限的情况下有效提升编队飞行卫星姿态控制系统的故障检测能力。