Establishment of atmospheric weighted mean temperature model in the polar regions

Due to the special geographical location and extreme climate environment, the polar regions (Antarctic and Arctic) have an important impact on global climate change. Atmospheric weighted mean temperature (Tm) is a crucial parameter in the retrieval of precipitable water vapor (PWV) from the zenith wet delay (ZWD) of ground-based Global Navigation Satellite System (GNSS) signal propagation. In this paper, the correlation between weighted mean temperature and surface temperature (Ts) is studied firstly. It is shown that the correlation coefficients between Tm and Ts are 0.93 in the Antarctic and 0.94 in the Arctic. The linear regression Tm model and quadratic function Tm model of the Antarctic and the Arctic are established respectively using the radiosonde profiles of 12 stations in the Antarctic and 58 stations in the Arctic from 2008 to 2015. The accuracies of the linear regression Tm model, the quadratic function Tm model and GPT2w Tm model which is a state-of-the-art global Tm model are verified using the radiosonde profiles from 2016 to 2018 in the Antarctic and Arctic. Root Mean Square (RMS) errors of the linear regression Tm model, the quadratic function Tm model and GPT2w Tm model in the Antarctic are 3.07 K, 2.87 K and 4.32 K respectively, and those in the Arctic are 3.53 K, 3.38 K and 4.82 K, which indicates that the quadratic function Tm model has a higher accuracy compared to linear regression Tm model, and the accuracies of the two regional Tm models are better than that of GPT2w Tm model in the polar regions. In order to better evaluate the accuracy of Tm in the PWV retrieval, the PWV values of radiosondes are used for comparisons as the reference value. The RMS errors of PWV derived from the two Tm models are similar for 1.28 mm in the Antarctic and 1 mm in the Arctic respectively. In addition, the spatial and temporal variation characteristics of Tm are analyzed in the polar regions by spectral analysis of Tm data using fast Fourier transform. The results show that the Tm has obvious seasonality and annual periodicity in the polar regions, and the maximum difference between warm season and cold season is about 63 K. After comparing and analyzing the influences of latitude, longitude and elevation on the Tm in the polar regions, it is found that latitude and elevation have a greater influence on the Tm than the longitude. As the latitude and elevation increase, the Tm decreases, and vice versa in the polar regions.     

紧凑型横向变焦系统关键器件的设计方法与功能验证

变焦系统可实现连续的光学变焦，可对不同景深的目标实现连续成像。在焦深延拓和光学检测等领域具有广泛地应用和发展潜力。本文提出了一种紧凑型可实现连续变焦功能的扁平化位相衍射元件，并设计分析和验证了横向调制相位型变焦衍射元件的功能。通过标量衍射基本理论模型，借助菲涅尔波带和多台阶相位衍射元件的设计方法，实现了横向变焦关键器件的设计仿真和实验验证。并以多波长响应的空间光调制器为基础，搭建了器件相位调制验证实验系统，通过测试证明了所设计器件的变焦能力，仿真和实验测试均可实现5倍变焦目标的有效调制。     

微型化半球陀螺制备工艺发展现状及趋势分析

因低噪声、高性能、无磨损的优势，半球陀螺已成为航空、航天领域内的最佳导航陀螺。半球陀螺的微型化是微机电陀螺领域的研究热点，全球各研究单位设计了多种形态的谐振器结构，开发了各具特色的加工工艺，其选用的材质也各不相同，并研制出了形态各异的微半球陀螺结构。对半球陀螺微型化的历程和方式进行了综述，着重对微型化半球陀螺壳体谐振器的结构形态、工艺制备方法和选材进行了对比和分析，并对各微型化途径的特点进行了讨论和展望。     

空间站燃烧科学实验系统设计

建立空间站燃烧实验系统，可满足未来空间微重力燃烧实验系统需求.通过空间站微重力燃烧实验研究，可拓展空间燃烧学研究.根据所要实现的功能及燃烧实验需求，对中国空间站燃烧柜的燃烧科学实验系统进行了设计和分析.燃烧科学实验系统由8个子系统组成，是一个适合开展气、液、固多种燃料燃烧实验的综合性实验系统.考虑到强度设计要求，在完成方案设计后，对系统进行了有限元分析，并在研制的结构件上进行了力学环境实验.实验与分析结果表明，本文设计的实验系统能够满足环模实验的要求，结构合理可行.      

直线模拟加载系统的研究进展与发展趋势

直线模拟加载系统是一种用于在实验室条件下模拟承载对象工作时所受直线负载力的半实物仿真系统，可用于模拟各类飞行器关键部件在工作过程中所受的气体阻力载荷。针对目前常用的机械式、电液式和电动式直线模拟加载系统，分析其基本加载原理和研究进展，结合自行研制的电动式直线模拟加载系统进行了深入探讨。针对多余力抑制方法的关键问题，详细论述了直线负载模拟器的结构补偿方法和控制策略。最后，展望了直线模拟加载系统的发展趋势，归纳了电动式直线模拟加载系统的高精度、大载荷发展方向。     

Estimating inter-system biases for tightly combined Galileo/BDS/GPS RTK

The overlapping carrier frequencies L1/E1, L5/E5a and B2/E5b from GPS/Galileo/BDS allow inter-system double-differencing of observations, which shows a clear advantage over differencing of the observations of each constellation independently. However, the inter-system biases destroy the integer nature of the inter-system double-differencing ambiguities. Two methods of direct rounding and parameter estimation are used to determine the ISB value. By analyzing data collected from Curtin University from 2015 to 2018, the phase and code inter-system bias (ISB) are related to the receiver type, firmware version and the selected overlapping frequency. Upgrade of receiver firmware version results in changes of ISB values. For example, the upgrade of Javad firmware in Dec, 15, 2017 causes the difference of 0.5 cycles ISB between BDS GEO and non-GEO satellites. By comparing the three dynamic models which include white noise process, random walk process, and random constant in the parameter estimation method, the ISB determined by the random constant model is consistent with the value obtained by the direct rounding method. After the calibration of ISBs, the performances of tightly combined positioning are assessed. The success rate of ambiguity resolution and accuracy of positioning for the tight combination (TC) are significantly improved in comparison with that for the loose combination (LC) over short baselines. For L5/E5a, on which only few satellites can be observed, the maximum increase in success rates of ambiguity resolution can reach 31.7%, i.e., from 54.9% of LC to larger than 86.6% of TC, and the positioning accuracies can even be increased by 0.13 m, i.e., from 0.208 of LC to 0.074 m of TC in East direction for the mix-receiver TRIMBLE NETR9-SEPT POLARX4 in 2018.     

基于动态补偿的多电机控制算法

多电机协调控制达到转速一致是电机控制中的一个关键难题，外加负载变动和电机参数变化时会引起电机性能的下降，达不到良好的控制效果。为使电机间保持转速同步，建立了永磁同步电机d-q坐标系下的矢量控制数学模型，基于转速跟随控制，提出一种基于单神经元PID的变增益速度补偿器进行偏差耦合控制。在MATLAB/Simulink建立了3台永磁同步电机的仿真模型。仿真结果表明，与传统PID固定增益速度补偿器算法相比，单神经元PID的变增益速度补偿器具有更强的鲁棒性以及更快的收敛性。     

基于最小约束系统的分布式协作定位研究

5G移动通信系统中,设备到设备的通信方式产生了节点间的信号测量,可用于提升无线定位的覆盖范围和定位精度。提出了一种基于最小约束系统的分布式协作定位方法,该方法首先利用已有算法估计节点参考位置,并据此构建最小约束确定网络的位置及朝向,然后在该约束下极大化由节点间测量引出的似然函数,获得位置估计。理论研究表明,该方法将由节点间测量确定的相对位置拟合到参考位置处,在参考位置等于真实位置时达到最优效果。仿真结果表明,该方法可有效提高定位精度,并具有分布式和可扩展等优点。     

同步双小行星系统共振轨道设计

研究了同步双小行星系统中共振轨道的设计方法及演化规律。首先，基于双椭球模型建立探测器运动方程，并给出共振轨道初值选取方法。然后，利用改进并行打靶法，提出一种双小行星系统平面共振轨道两步修正方法。同时结合稳定性理论及分岔理论，给出双小行星系统三维共振轨道生成和延拓方法；最后，以双小行星系统1999KW4为例，设计了共振比为1∶1,1∶2,1∶3,1∶4,2∶3的平面和空间共振轨道族，并分析了共振轨道的特性及轨道周期和轨道能量的变化规律。给出的双小行星系统中共振轨道的设计方法具有普适性，对未来双小行星系统探测任务中的轨道设计具有一定的参考意义与借鉴价值。     

电铸镍Wolter I型光学系统制造技术发展综述

摘要： 为满足未来脉冲星导航和空间天文观测任务对X射线望远镜的载荷需求，Wolter I光学系统的研制正逐渐成为新的研究热点，电铸镍方案是当前国内外X射线光学系统镜筒制造的主要技术方案.文章对电铸镍X射线光学系统制造工艺、国内外研制现状、未来应用需求进行了介绍和整理，梳理了电铸镍X射线光学系统研制遇到的关键技术和难点，提出了后续研究发展建议，以促进中国在 X射线脉冲星自主导航、空间探测领域的快速发展.