一种新型的低噪声硅微机械陀螺电容读出电路

陀螺系统的微机械敏感结构部分的性能提升受到成本、工艺的限制，有较高难度，故提升接口电路的各项性能成为提升整个系统性能的关键。因此，电容读出电路作为微机械陀螺系统中非常重要的组成部分，该电路性能的优劣直接决定着陀螺的测量精度。为实现硅微陀螺高精度检测，设计了一款低噪声的电容读出电路。在陀螺与读出电路之间设计斩波开关，基于斩波技术进行低噪声设计，采用相关双采样技术用来降低关键的第一级放大电路的低频闪烁噪声和开关噪声。采用了一种简化的陀螺测试模型，用于读出电路的独立测试。读出电路在0.18μm CMOS工艺下设计流片，测试结果表明，该电容读出电路输出噪声为-122.8dBV/Hz1/2，可实现0.06aF/Hz1/2的电容分辨率。     

基于波长控制的光纤陀螺标度因数温度性能提高方法

光纤陀螺的标度因数与光纤环的长度、直径及光源的平均波长有关。在温度条件下，光纤环的长度、直径及光源的平均波长均会发生变化，进而导致光纤陀螺在高低温下的标度因数不同，影响温度环境下的光纤陀螺标度因数的重复性。提出了一种基于光纤陀螺波长控制的标度因数温度性能提高方法，该方法在光源驱动电路的桥式回路中增加了铂电阻组件，从而可自动调节光纤陀螺光源的管芯温度，进而控制光源平均波长的变化，以抵消光纤环有效面积因温度变化而对标度因数产生的影响，提高温度环境下光纤陀螺的标度因数重复性。试验表明，该方法将未补偿情况下光纤陀螺全温范围内的标度因数重复性(1σ)由271×10-6~280×10-6减小到了32.5×10-6~43.5×10-6，标度因数重复性误差减小了84%~88%，并验证了该方法的有效性。     

表贴式永磁同步电机直接转矩控制变幅值预测控制研究

基于以电压矢量幅值为变量的表贴式永磁同步电机(SPMSM)磁链和转矩方程,采用预测控制计算得出施加不同电压矢量幅值的下一时刻磁链和转矩值,选择使磁链和转矩误差目标函数最小的电压矢量幅值作为最优值,从而确定下一时刻施加的电压矢量。仿真结果表明:在电压矢量变幅值预测下,SPMSM直接转矩控制(DTC)系统运行良好,定子磁链轨迹为理想圆,磁链和转矩均符合控制要求,转速跟踪良好,定子电流波形正弦。预测控制需要从备选电压矢量幅值集合中选择最优幅值。理论上,备选电压矢量幅值个数越多,系统优化效果越好,但也带来更大的计算负担。研究了9种等分电压矢量情况下变幅值预测控制系统的控制效果。根据控制效果和计算负担,提出变幅值预测控制将电压矢量幅值三等分较为理想。     

一种基于观测站数目最小化的TDOA/FDOA无源定位算法

在三维（3D）运动目标无源定位系统中，无模糊定位最少需要4个观测站。而传统的两步加权最小二乘（TSWLS）及其改进的闭式算法至少需要5个观测站进行求解，当减少一个观测站时，这些闭式算法往往无法提供可靠解。针对这一问题，提出一种最小化观测站数目的到达时间差（TDOA）与到达频率差（FDOA）定位算法。该算法是一种闭式解法并且能够在三维场景下仅使用4个观测站进行定位。该算法分为两步：第1步分离传统的TSWLS算法中未知参数空间，建立了一组新的等式，并且利用加权最小二乘（WLS）算法得到目标位置与速度的初始值；第2步利用泰勒级数展开算法将中间变量线性化，对目标位置和速度初始值进一步校正。理论分析证明了在适当的噪声水平下该算法能够达到克拉美罗界（CRLB）。此外，计算机仿真表明仅使用4个观测站时，该算法对于近场以及远场目标参数的估计精度在测量噪声较小时可以实现CRLB；并且还表明使用5个观测站估计时，该算法比TSWLS及其改进算法能更好地适应大的测量噪声。     

Modeling and analysis of mover gaps in tubular moving-magnet linear oscillating motors

A tubular moving-magnet linear oscillating motor (TMMLOM) has merits of high efficiency and excellent dynamic capability. To enhance the thrust performance, quasi-Halbach permanent magnet (PM) arrays are arranged on its mover in the application of a linear electro-hydrostatic actuator in more electric aircraft. The arrays are assembled by several individual segments, which lead to gaps between them inevitably. To investigate the effects of the gaps on the radial magnetic flux density and the machine thrust in this paper, an analytical model is built considering both axial and radial gaps. The model is validated by finite element simulations and experimental results. Distributions of the magnetic flux are described in condition of different sizes of radial and axial gaps. Besides, the output force is also discussed in normal and end windings. Finally, the model has demonstrated that both kinds of gaps have a negative effect on the thrust, and the linear motor is more sensitive to radial ones.     

Stability of relative equilibria of the full spacecraft dynamics around an asteroid with orbit–attitude coupling

The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered.     

Orbital stability close to asteroid 624 Hektor using the polyhedral model

We investigate the orbital stability close to the unique L4-point Jupiter binary Trojan asteroid 624 Hektor. The gravitational potential of 624 Hektor is calculated using the polyhedron model with observational data of 2038 faces and 1021 vertexes. Previous studies have presented three different density values for 624 Hektor. The equilibrium points in the gravitational potential of 624 Hektor with different density values have been studied in detail. There are five equilibrium points in the gravitational potential of 624 Hektor no matter the density value. The positions, Jacobian, eigenvalues, topological cases, stability, as well as the Hessian matrix of the equilibrium points are investigated. For the three different density values the number, topological cases, and the stability of the equilibrium points with different density values are the same. However, the positions of the equilibrium points vary with the density value of the asteroid 624 Hektor. The outer equilibrium points move away from the asteroid’s mass center when the density increases, and the inner equilibrium point moves close to the asteroid’s mass center when the density increases. There exist unstable periodic orbits near the surface of 624 Hektor. We calculated an orbit near the primary’s equatorial plane of this binary Trojan asteroid; the results indicate that the orbit remains stable after 28.8375?d.     

硅半球深腔结构无损检测技术

半球深腔的加工质量是决定硅基MEMS半球陀螺精度的关键因素之一，及时检测半球深腔的形貌参数并将其反馈至加工过程，是确保高性能MEMS半球陀螺研制成功的重要措施。由于硅半球深腔的深度较大，台阶仪和光学显微成像系统无法对半球深腔的形貌特征进行有效测量。因此,需要将硅深腔结构剖开后采用扫描电镜(SEM)进行检测。这种检测方式时间周期长，且属于破坏性的样本检测，效率和测试精度都较低。提出以硅半球深腔为模具，利用PDMS铸模将硅半球深腔的结构尺寸和表面形貌转移到PDMS凸起的半球模型上，通过检测PDMS半球模型的尺寸结构和表面形貌，即可反推出硅半球深腔的尺寸特征。经实验验证，脱模后的PDMS模型可以准确地反映出半球深腔的尺寸信息，测量结果的不确定度小于5‰，有效解决了硅半球深腔无损检测的难题。     

过氧化氢/紫外线/臭氧氧化技术处理肼类污水的应用

采用放大试验规模（处理量1 m³/h）的H₂O₂（过氧化氢）/UV（紫外线）/O₃（臭氧）氧化技术处理肼类推进剂污水，在30.0±1.6 ℃，pH=9.0±0.2的条件下，研究肼类的过氧化氢增强光解臭氧化降解。对比不同氧化技术的协同效应以及对污水降解的影响，重点考察过氧化氢、紫外线、臭氧和初始浓度等工艺参数对降解效果的影响，对氧化技术的应用进行了优化。研究结果表明：该技术可使COD去除率提高27.66%，肼类的降解速率随着过氧化氢投加量、紫外线辐射强度、O₃投加速率和水质地提高而升高，随着初始质量浓度的提高而下降。在最佳工艺下，处理5 000 mg/L质量浓度的废水，处理60 min时，COD去除率分别为98.62%（偏二甲肼）、99.17%（甲基肼）、99.94%（肼）和93.25%（单推-3）。     

GNSS观测数据ZTD建模的质量控制方法

针对目前基于GNSS观测数据的对流层天顶总延迟(ZTD)模型缺乏有效质量控制手段的现状,提出了一套综合考虑数据量、网格分辨率以及模型稳定性的ZTD建模质量控制方法,并采用内华达大地测量实验室(NGL)解算的高空间分辨率GNSS对流层数据,选取了近十年德国及周边区域[47°N-55°N,5°E-15°E]183个测站的实测ZTD,对该方法进行了校验。实验结果表明:在该质量控制方法下建立的新模型精度稳定,平均均方根误差(RMS)为3.4 cm,相对于UNB3m、EGNOS、GPT2w+Saas平均改善了42.4%、35.8%、33.3%。本文提出的质量控制方法有效提升了基于GNSS观测数据的ZTD模型的性能,对于ZTD建模研究具有一定的参考价值。