微型定位导航授时系统集成设计

针对定位导航与授时系统的微小型化、一体化应用需求,提出了一种微型定位导航授时(Micro-PNT)系统集成方案,该方案是微小飞行器在GNSS拒止条件下可靠工作的有效解决手段。系统基于电路刚挠一体化工艺和器件空间布局优化技术,集成了MEMS惯性仪表、芯片级原子钟、处理器、电源芯片等功能器件,实现了系统的微型化、一体化。文中阐述了系统的集成架构和软件工作流程。通过系统样机的研制,验证了集成方案的可行性。通过分析系统样机的集成特点,指出其微型化存在的问题。最后,结合关键器件和三维微系统集成技术发展,给出了Micro-PNT微系统集成架构。     

面向空间应用的大容量实时网络总线架构

针对未来空间综合电子系统总线网络发展需求，本文在介绍现有星载电子系统体系架构优缺点的基础上，提出了一种面向空间环境应用的高速高可靠实时网络总线架构。对网络协议架构、网络拓扑、工作原理及网络关键设备进行了详细介绍，该技术10 Gb/s的传输带宽、亚微秒时钟同步精度、多通道冗余传输机制能够满足未来空间环境应用需求，为未来空间电子系统网络架构研究提供借鉴。     

Switching and performance variations of on-orbit BDS satellite clocks

The information of the satellite clock switching and performance variations on-orbit of Chinese BeiDou-2 Navigation System (BDS) is not available for the public. In order to detect the BDS satellite clock switching and performances variation, we analyzed the precise clock offset products with a total duration of 5?years every BDS satellite equipped four atomic clocks from four different manufactures from January 2013 to October 2017. Three important contributions are concluded as follows. (1) It is found that the average time of on-orbit operation for BDS satellite clocks is about 1–2?years. There have been 22 times of clock switching for BDS satellites, of which the C05 and C08 satellites have been switched to the fourth (last) atomic clock. (2) There are frequent phase adjustments for BDS on-orbit satellite clocks, and the frequency series is relatively stable. Furthermore, there are semi-annual sinusoid cycles in the frequency drift series of C06 and C09 satellites. (3) The performances of MEO satellite clocks perform better than the IGSO and GEO satellite clocks. The average ten-thousand frequency stability of BDS satellite clocks is about 1E-13, which is worse than that of GPS and Galileo but better than that of GLONASS.     

原子磁强计原子气室无磁加热温控系统设计

介绍一种用于原子磁强计原子气室的无磁加热温控系统设计。针对温控系统加热电流产生的磁场干扰，设计了双层加热丝加热膜结构的加热器件，该加热器件利用同层平行反向电流和层间平行反向电流产生的磁场相互抵消以减小加热电流磁场噪声；设计了滑动平均滤波器对采集的温度信号实施滤波以减小随机噪声的干扰；结合设计的高频加热信号的产生电路、幅度控制电路和功率放大电路开展了实验测试。测试结果表明，研制的双层加热丝加热膜结构加热器件相比单层加热丝加热膜结构加热器件的电流磁场噪声抑制能力提高了约16倍，实现的无磁加热温控系统的温控能力达到1.2‰。     

基于EtherCAT通信的双直线电机位置联动控制系统设计

针对传统脉冲、模拟量控制系统在实时性、稳定性和同步性方面的不足,提出了一种基于EtherCAT工业实时以太网通信的双直线电机位置联动控制方案。设计了3种位置联动控制模式,详细分析了EtherCAT的分布时钟补偿算法,并搭建了联动控制试验平台,对所设计的控制系统进行了试验验证。试验结果表明,采用EtherCAT通信的双直线电机位置联动控制系统实时性高,双轴同步、交替响应性能良好,适用于同步精度和响应速度要求都较高的应用场合。     

一种基于信道模拟的测速精度评估方法

为了评估单向多普勒测速动态测量精度,构建了一种基于卫星信道模拟器的测速精度评估系统,通过在卫星信道模拟器装订卫星飞行轨迹,利用卫星信道模拟器对上行信号加入传播时延、多普勒频率,对卫星在轨飞行状态下的单向多普勒测速进行场景仿真,并对场景仿真获取的测速数据进行O-C残差序列分析,得到动态测量条件下的测速精度。给出了O-C残差序列的计算方法,分析了单向多普勒测速体制下时钟偏差对测速结果的影响,并给出了一种简单的时钟误差修正方法。     

核磁共振陀螺技术研究进展

核磁共振陀螺是基于量子操控技术的前沿研究新进展。具有高精度、微小型、对加速度不敏感、纯固态等特点,是未来发展高精度、微小型陀螺的主要技术发展方向之一。围绕核磁共振陀螺技术的最新研究进展,重点介绍了核磁共振陀螺的基本工作原理及其硬件构成,分析了核磁共振陀螺在上个世纪的主要技术发展路线与面临的技术发展瓶颈,综述了核磁共振陀螺近年来取得的研究进展及实现的技术突破,最后对核磁共振陀螺技术的未来发展进行了展望。     

LiHe spectra from brown dwarfs to helium clusters

The detection of Li I lines is the most decisive spectral indicator of substellarity for young brown dwarfs with masses below about 0.06 solar mass. Due to the weakness of the Li resonance lines, it is important to be able to model precisely both their core widths and their wing profiles. This allows an adequate prediction of the mass at which Li lines reappear in the spectra of brown dwarfs for a given age, or reversely an accurate determination of the age of a cluster. We report improved line profiles and the dependence of line width on temperature suitable for modeling substellar atmospheres that were determined from new LiHe molecular potential energies. Over a limited range of density and temperature, comparison with laboratory measurements was used to validate the potential energies which support the spectral line profile theory.     

Collisional line broadening versus collisional depolarization: Similarities and differences

Within the impact approximation, collisional line broadening parameters and depolarizing and polarization transfer (population, orientation, alignment transfer) rates are complementary: both include the effect of collisional transitions between the Zeeman sublevels of a given level, or between fine or hyperfine structure levels of a given term. However, there are several differences: in line broadening, the two levels connected by the radiative transition contribute to the broadening, and there is also an interference term between these two levels, whereas only one level or two close levels are concerned in the depolarization. Another difference lies in the fact that purely elastic collisions contribute also to the line broadening, whereas they do not contribute to the depolarization. The nature of these two kinds of coefficients are recalled. Then the possibility to find some relationships or systematic trends concerning depolarization versus collisional broadening is considered. This is to answer some current questions which come from the polarization community.     

Stark broadening data for spectral lines of rare-earth elements: Nb III

The electron-impact widths for 15 doubly charged Nb ion lines have been theoretically determined by using the modified semiempirical method. Using the obtained results, we considered the influence of the electron-impact mechanism on line shapes in spectra of chemically peculiar stars and white dwarfs.