航天器规避动态障碍物的自适应人工势函数制导

针对航天器近距离操作中的动态障碍物规避问题,研究了一种燃料较省、精度较高的规避动态障碍物的自适应人工势函数制导方法。首先,对于引入高斯函数形式斥力势会使势函数在收敛点处的值不为零的情况,对斥力势乘以修正项,使得在收敛点的势能为零,消除了平衡点的偏离;在规避静态障碍物的基础上,研究了规避动态障碍物的人工势函数制导。其次,根据速度与引力梯度之间的关系,设计负反馈,使引力势梯度“适应”速度的变化,研究了规避动态障碍物的自适应人工势函数制导。最后,采用精确的数学模型进行数值仿真,验证所设计的制导律的正确性和有效性,并与传统的人工势函数制导对比。仿真结果表明：采用修正势函数提高了收敛精度;自适应人工势函数制导控制脉冲作用施加更加合理,相比人工势函数而言,总速度脉冲消耗可节省30%,精度提高两个数量级。     

人因工程学在飞机驾驶舱空间布局设计中的应用

回顾了当前驾驶舱设计中人因工程学的研究进展,重点探讨了人因工程学研究方法在飞机驾驶舱空间布局设计中的具体应用,总结了设计中需要遵循的原则,并对驾驶舱设计进一步的研究提出了若干建议。     

反舰导弹命中精度评估方法

研究了基于Bayes方法的反舰导弹命中精度评估方法,提出了导弹命中点系统误差评估方法、Bayes检验方案和CEP评估方法。     

激光成像系统实验研究

为解决激光脚点（laser footprint）在光学图像中的定位问题,建立分析模型,构建了集成激光测距机和CCD摄像机的实验室激光成像系统;通过实验,对采集的数据进行了图像配准和融合,反演出被测目标三维图像,包含了被测目标高程与灰度信息。     

氟化处理工艺对TiAl合金氧化层组织的影响

文章研究了氟离子注入和NH₄F溶液处理对TiAl合金高温氧化层组织结构的影响规律。结果表明:TiAl合金高温氧化层的组织和致密度受氟化处理工艺和参数的影响很大;经过表面氟化处理的TiAl合金高温氧化抗力高于原始合金;随着表面氟含量增加,氧化层的钛元素含量增加,致密度下降,研究表明存在一个最佳的表面氟浓度。     

八水氢氧化钡相变材料储热性能实验

采用八水氢氧化钡（Ba（OH）₂·8H₂O）作为相变储热材料,经过150次熔化-凝固热循环实验,发现随着热循环次数的增加,Ba（OH）₂·8H₂O的相变点温度变化很小,但是该相变材料结晶时存在严重的过冷现象.通过扫描电子显微镜获得50次热循环后Ba（OH）₂·8H₂O与铝合金和紫铜金属材料之间的腐蚀情况图像,图像分析表明,Ba（OH）₂·8H₂O与紫铜有良好的相容性.搭建了含/未含泡沫铜的相变储能装置的实验台,对比实验结果表明,泡沫铜填充不仅可以提高相变材料的传热效率,而且能够有效地降低Ba（OH）₂·8H₂O的过冷度.      

The influence of the spatial and temporal collocation windows on the comparisons of the ionospheric characteristic parameters derived from COSMIC radio occultation and digisondes

GPS radio occultation (RO) ionospheric products obtained by Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) mission during the year of 2014 and the observations from 3 digisonde stations which are located at different latitudes are used to study the influence of different time and space collocation windows on the comparisons of the ionospheric characteristic parameters (ICPs), including the peak density and peak height, derived from the two techniques. The results show that the correlation coefficients (CC) and the standard deviation of the absolute biases (SDAB) between the ICPs derived from the two techniques vary distinctly under different spatial and time collocation windows. Generally, the CC (SDAB) of the ICPs decrease (increase) as the size of the collocation window increases in time dimension or in space dimension. The rate of change of the statistic parameters with the increase in the size of the collocation window in time dimension and space dimension is analyzed for each digisonde station. It is found that within the collocation window of $\left(60\mathrm{m}\mathrm{i}\mathrm{n},{20}^{°},{20}^{°}\right)$, the influence of the increase of $1^{°}$ in the space window on the statistical comparison is much more significant than that of the increase of 1?min in the time window, and it is suggested that there can be appropriate relaxation on the time window within the threshold of 60?min to get a balance between the quality of the comparison results and the number of the matched pairs. In addition, it is found that the same variations in the longitude window and in the latitude window may have different influences on the comparison results when the horizontal gradients in electron density are distinctly different along different directions at the digisonde station, and strict space collocation window is preferred when comparing the observations from COSMIC RO with those from the digisonde station in such cases.     

ADS与多雷达数据融合中的系统误差配准法

对空中交通管制中自动相关监视(ADS)与现有多雷达监视系统进行数据融合的模型进行了分析,在现有多雷达数据处理(MRDP)系统误差配准方法的基础上设计了一种利用最小平方估计(LSE)准则实现的ADS与雷达的系统误差配准算法,给出了其最优解.利用我国西部航路模拟航路点数据进行了系统仿真,仿真结果的分析表明,通过该方法的配准,ADS和雷达数据融合中的系统误差得到了有效的消除,提高了综合监视精度.     

基于ICA和小波脊的多辐射源调制类型识别

针对电子侦察中多个雷达辐射源信号混叠时的调制类型识别问题,利用独立分量分析将多个雷达辐射源信号进行分离,再对分离后的辐射源信号采用小波变换,提取信号时频分布的脊线,最后计算脊线特征值,通过脊线特征值来判断辐射源调制类型.仿真实验验证了该方法的正确性和有效性.     

The evolution of globular clusters

Taking a wide range of the initial conditions, including spatial density distribution and mass function etc, the dynamical evolution of globular clusters in the Milky Way is investigated in detail by means of Monte Carlo simulations. Four dynamic mechanisms are considered: stellar evaporation, stellar evolution, tidal shocks due to both the disk and bulge, and dynamical friction. It is found that stellar evaporation dominates the evolution of low-mass clusters and all four are important for massive ones. For both the power-law and lognormal initial clusters mass functions, we can find the best-fit models which can match the present-day observations with their main features of the mass function almost unchanged after evolution of several Gyr. This implies that it is not possible to determine the initial mass function only based on the observed ones today. Moreover, the dispersion of the modelled mass functions mainly depends on the potential wells of host galaxies with the almost constant peaks, which is consistent with current observations.