同步发电机励磁功率单元中可控整流桥的故障工况研究

分析了三相全控桥式整流电路的各种故障工况,得出故障下触发角与输出励磁电压之间的定量关系,并提出了相应的解决措施。通过对MATLAB/Simulink搭建的同步发电机励磁功率单元模型进行仿真,结果表明,所提措施能有效减轻故障对系统的不利影响,在脉冲丢失时,可以为备用设备切换赢得时间;晶闸管发生故障时,有利于调控发电机平稳退出运行以避免产生稳定性问题。     

Adaptive robust cubature Kalman filtering for satellite attitude estimation

This paper is concerned with the adaptive robust cubature Kalman filtering problem for the case that the dynamics model error and the measurement model error exist simultaneously in the satellite attitude estimation system. By using Hubel-based robust filtering methodology to correct the measurement covariance formulation of cubature Kalman filter, the proposed filtering algorithm could effectively suppress the measurement model error. To further enhance this effect and reduce the impact of the dynamics model error, two different adaptively robust filtering algorithms, one with the optimal adaptive factor based on the estimated covariance matrix of the predicted residuals and the other with multiple fading factors based on strong tracking algorithm, are developed and applied for the satellite attitude estimation. The quaternion is employed to represent the global attitude parameter, and three-dimensional generalized Rodrigues parameters are introduced to define the local attitude error. A multiplicative quaternion error is derived from the local attitude error to maintain quaternion normalization constraint in the filter. Simulation results indicate that the proposed novel algorithm could exhibit higher accuracy and faster convergence compared with the multiplicative extended Kalman filter, the unscented quaternion estimator, and the adaptive robust unscented Kalman filter.     

基于X射线脉冲星导航试验卫星观测数据的到达时间估计

中国首颗X射线脉冲星导航试验卫星（X-ray Pulsar Navigation-1, XPNAV-1）搭载了两种体制的X射线探测器,其主要任务是在轨开展X射线脉冲星的探测以及进行脉冲星导航体制的验证。为了实现到达时间（Time of Arrival,TOA）的高精度估计,提出了利用阵列信号处理领域的多重信号子空间分类（Multiple Signal Classification,MUSIC）方法进行脉冲星导航的TOA估计,进行了试验仿真验证,并且对XPNAV-1观测到的蟹状星云（Crab）脉冲星的光子数据进行处理。在观测时间为协调世界时（Coordinate Universal Time,UTC）57727.0约简儒略日（Modified Julian Day,MJD）到UTC57812.0MJD内,选取了0.5~10keV频段内的121段光子观测数据,对这些数据进行了脉冲轮廓折叠,得到了Crab脉冲星的折叠轮廓,然后分别利用互相关法和MUSIC方法进行折叠轮廓的TOA估计,最后对比了两种方法的估计结果。     

An estimation of Envisat’s rotational state accounting for the precession of its rotational axis caused by gravity-gradient torque

The rotational state of Envisat is re-estimated using the specular glint times in optical observation data obtained from 2013 to 2015. The model is simplified to a uniaxial symmetric model with the first order variation of its angular momentum subject to a gravity-gradient torque causing precession around the normal of the orbital plane. The sense of Envisat’s rotation can be derived from observational data, and is found to be opposite to the sense of its orbital motion. The rotational period is estimated to be $(120.674\pm 0.068)·\exp \left((4.5095\pm 0.0096)\times {10}^{-4}·t\right)\text{s}$, where t is measured in days from the beginning of 2013. The standard deviation is 0.760?s, making this the best fit obtained for Envisat in the literature to date. The results demonstrate that the angle between the angular momentum vector and the negative normal of the orbital plane librates around a mean value of $8.53°\pm 0.42°$ with an amplitude from about $0.7°$ (in 2013) to $0.5°$ (in 2015), with the libration period equal to the precession period of the angular momentum, from about 4.8?days (in 2013) to 3.4?days (in 2015). The ratio of the minimum to maximum principal moments of inertia is estimated to be $0.0818\pm 0.0011$, and the initial longitude of the angular momentum in the orbital coordinate system is $40.5°\pm 9.3°$. The direction of the rotation axis derived from our results at September 23, 2013, UTC 20:57 is similar to the results obtained from satellite laser ranging data but about $20°$ closer to the negative normal of the orbital plane.     

基于公共余数最优估计的多通道干涉SAR高程重建方法

针对多通道干涉SAR高程重建方法计算效率较低的问题,提出了一种基于公共余数最优估计的多通道干涉SAR快速高程重建方法。该算法首先对干涉相位去除平地效应后,得出每幅干涉图像任意一个像素对应的缠绕干涉相位,构造出关于干涉相位模糊数的同余方程组;然后利用最优估计法求解出带噪声余数的公共余数的最优估计值,求解出各目标的高程值;最后再利用改进措施得到更高精度的高程重建结果。试验数据处理结果表明,该方法使得多通道干涉SAR高程重建的计算效率有了显著提升。     

面向装备RUL预测的平行仿真技术

装备平行仿真是系统建模与仿真领域的新兴仿真技术,已经成为研究热点。在装备维修保障领域中,分析了装备剩余寿命（RUL）预测存在的突出问题,即模型参数固定、不具备自适应演化能力,成为阻碍实现装备剩余寿命自适应预测的首要因素。结合装备平行仿真理论,在建模分析的基础上提出了面向装备剩余寿命预测的平行仿真框架,该框架以Wiener状态空间模型为基础仿真模型,在动态注入的装备退化观测数据驱动下,利用期望最大化（EM）算法在线更新模型参数,并利用卡尔曼滤波（KF）算法实现仿真输出数据与观测数据的同化（DA）,从而实现仿真模型动态演化,使得仿真输出不断逼近装备真实退化状态,为准确预测剩余寿命提供高逼真度仿真模型和数据输出。以某轴承性能退化数据为数据驱动源,对该框架进行了验证,仿真结果表明平行仿真方法能准确仿真装备性能退化过程,在提高预测精度的基础上实现了装备剩余寿命的自适应预测,有力证明了平行仿真方法的可行性和有效性。      

压缩感知OFDM稀疏信道估计导频设计

为提高稀疏信道估计性能, 基于压缩感知(CS)理论, 研究了正交频分复用(OFDM)系统中的导频设计问题。由于已有方法不能准确衡量采样矩阵重建性能, 从而导致根据已有方法设计的导频具有较差的信道估计性能, 因此提出以互相关矩阵元素的立方和为准则准确评价采样矩阵的重建性能。针对OFDM系统信道估计导频设计为离散组合优化问题, 提出了一种并行完全树分组替换搜索算法用于搜索最优的导频。在算法的每次循环中, 先将导频索引集合分组, 再根据每一组替换的结果更新导频, 提出的方法扩大了导频搜索空间, 避免了导频搜索的局部最优问题。仿真结果表明, 提出的评价方法相比现有方法能够准确评价采样矩阵重建性能, 使用提出的准则设计的导频与现有互相关准则相比信道估计均方误差可减小约3 dB。同时, 所提出的导频搜索算法具有更快的收敛速度和最优的导频搜索性能。      

姿态异常下的星体自旋角速度确定方法

摘要： 针对在轨姿态异常后星体高速自旋情况,开展星体自旋角速度确定方法研究.提出一种基于太阳敏感器测量数据确定自旋角速度的方法,并对自旋角速率确定误差进行分析,得到各误差源对确定精度的影响关系;基于角速率确定误差分析结论,给出根据角速度大小选取不同时间间隔测量数据的策略,通过大时间间隔测量数据的选取,保证小角速度情况下的确定精度.所提出方法的有效性通过数学仿真验证,并在实际应用中基于太阳敏感器遥测数据获取在轨姿态异常卫星角速度.     

求根传播算子方法及其在ARM抗诱偏中的应用

反辐射导弹（ARM）抗有源诱偏问题中,多源信号在空、频域的强相关性往往造成导引头对信源数目欠估计,从而导致传统超分辨算法的测向性能下降。针对这一问题,提出了一种求根的传播算子方法,该算法首先在信源数过估计情况下计算信号到达角,然后利用每个角度对应的信号功率来剔除虚假角度。求根传播算子方法不需要预先估计信号源数目,而且在信号高度相关的情况下具备很好的角度分辨性能,因此适用于解决ARM抗诱偏问题。仿真实验结果表明,求根传播算子方法在提高ARM抗诱偏能力方面的表现优于MUSIC算法。