基于Gauss-Newton法的L1数据拟合

在数据拟合中，当个别数据存在较大测量误差时，采用Ｌ１准则对数据进行拟合要优于最小二乘准则。本文通过建立Ｌ１准则与最小二乘准则之间的关系，给出了一种基于Ｇａｕｓｓ－Ｎｅｗｔｏｎ法的Ｌ１数据拟合自满。计算结果表明，该方法易于理解，便于编程，具有一定的理论意义和现实意义。     

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.     

基于夏氏最小二乘的轨道控制力系数辨识

在航天器轨道捕获、轨道维持和空间目标碰撞规避中都需要进行航天器轨道机动。针对航天器轨道机动过程中推力器的推力系数为装订常数,没有根据在轨工作实际进行优化而导致出现较大误差的情况,对控制力拟合系数进行辨识,作为修正控制参数以补偿轨道控制误差的依据,提高轨道控制精度。统计分析在轨管理的典型航天器平台及其发动机的轨道控制历史数据,分析轨道控制理论和在轨控制数据拟合建立轨道控制经验模型,用当前可测量的系统输入和输出预测系统输出的未来演变,得到不同工作情况下实际轨道控制误差与控制参数及其他主要影响因素之间关系的经验公式,为轨道控制策略决策提供参考。选取轨道半长轴控制量300m以上和300m以下的两类近地卫星,对其轨道控制历史数据进行分析,经实际数据测试,采用夏氏法进行推力系数拟合后预测的速度变化量精度较高。该种计算方法利用了轨道控制历史数据,计算方法简单,提高了轨道控制速度增量的预测精度,对轨道控制实施具有参考意义。     

一种基于多项式拟合的VCO开环线性校正法

压控振荡器VCO(Voltage Controlled Oscillator)是输入控制电压影响输出频率的振荡电路,可用于产生调频信号.应用于安检成像时,其输出信号的线性度通过影响副瓣电平和距离分辨率,从而决定了安检成像的效果.为了提高安检成像效果,提出了一种基于多项式拟合的VCO开环线性校正法,使VCO的输出频率通过...     

简谐力激励下多组件结构系统的整体优化设计

多组件结构系统整体优化设计通过协同优化支撑结构拓扑构型和组件布局来使结构系统的位移响应最小。本文提出通过模态加速度法（MAM）求解多组件结构系统的位移响应,并以位移响应值最小作为优化目标;引入多点约束（MPC）方法模拟组件与设计域间的铆钉或螺栓连接形式;采用有限包络圆法（FCM）来避免组件之间及组件与设计域边界产生干涉。建立了多组件结构系统整体优化问题的数学模型,并对动响应目标函数关于设计变量的灵敏度进行了推导。最后,通过几个算例验证了整体优化方法在简谐力激励下求解问题的可行性及其在实际问题中的有效性。     

多模型GGIW-GLMB算法跟踪机动群目标

针对多个机动群目标跟踪问题,提出了一种多模型伽马高斯逆威夏特-广义标签多贝努利（MM-GGIW-GLMB）算法。采用多模型算法对群目标进行运动建模,利用最适高斯（BFG）近似在预测阶段对多模型进行融合,减小了多模型算法的运算量,为进一步提高算法在目标机动阶段的跟踪性能,引入强跟踪滤波器（STF）对BFG算法得到的预测状态协方差进行修正。利用最优次模式分配（OSPA）距离及其一倍标准差和航迹标签正确率衡量算法对机动群目标的跟踪性能。仿真结果表明,本文算法能够提升对机动群目标的跟踪精度和稳定性。      

基于曲率优化的14参数平面叶栅设计方法

为了避免型线曲率不连续所导致的气动损失,提出了一种基于曲率优化的平面叶栅设计方法,共包括了对气动性能有显著影响的进出口几何构造角、喉部宽度、弯折角,对强度有较大影响的前/尾缘半径、最大内切圆半径、位置等14个独立参数.分段表征了平面叶栅的压力面、吸力面型线,为保证其光顺性,利用基于优化的方法通过调整内切圆半径的夹角,实现了压力面、吸力面型线的曲率连续.进行了平面叶栅的设计,结果表明文中提出的方法可以灵活进行平面叶栅的设计.     

Alice: The rosetta Ultraviolet Imaging Spectrograph

We describe the design, performance and scientific objectives of the NASA-funded ALICE instrument aboard the ESA Rosetta asteroid flyby/comet rendezvous mission. ALICE is a lightweight, low-power, and low-cost imaging spectrograph optimized for cometary far-ultraviolet (FUV) spectroscopy. It will be the first UV spectrograph to study a comet at close range. It is designed to obtain spatially-resolved spectra of Rosetta mission targets in the 700–2050 Å spectral band with a spectral resolution between 8 Å and 12 Å for extended sources that fill its ～0.05^ × 6.0^ field-of-view. ALICE employs an off-axis telescope feeding a 0.15-m normal incidence Rowland circle spectrograph with a toroidal concave holographic reflection grating. The microchannel plate detector utilizes dual solar-blind opaque photocathodes (KBr and CsI) and employs a two-dimensional delay-line readout array. The instrument is controlled by an internal microprocessor. During the prime Rosetta mission, ALICE will characterize comet 67P/Churyumov-Gerasimenko's coma, its nucleus, and nucleus/coma coupling; during cruise to the comet, ALICE will make observations of the mission's two asteroid flyby targets and of Mars, its moons, and of Earth's moon. ALICE has already successfully completed the in-flight commissioning phase and is operating well in flight. It has been characterized in flight with stellar flux calibrations, observations of the Moon during the first Earth fly-by, and observations of comet C/2002 T7 (LINEAR) in 2004 and comet 9P/Tempel 1 during the 2005 Deep Impact comet-collision observing campaign.     

四杆机构转折圆及其应用

介绍了转折圆的运动学特性，论述了求铰链四杆机构的转折圆，以及利用转折圆进行铰链四杆机构近似直线导向设计的方法。     

LD端泵Nd：YVO4固体激光器双折射现象研究

通过对LD端泵Nd：YVO4固体激光器输出特性的研究，并运用传播圆和变换圆理论的分析，得出了晶体双折射是影响激光器输出特性重要因素，并与实验相吻合。