应用分力合成方法提高系统性能指标的研究

提出了将柔性结构的分力合成主动振动抑制方法和反馈控制律结合使用来提高柔性结构控制系统性能指标的方法。应用该方法仅需要知道闭环系统及柔性振动的频率及阻尼，而且可以同时抑制任意多个振动模态（包括控制器引起的振动，柔性振动及其他形式的振动），分力合成方法对频率及阻尼的不确定性具有较强的鲁棒性，使该方法易于工程实现，文章针对单柔性杆，将分力合成主动振动抑制方法和反馈控制相结合，设计了不同形式的大角度机动控制律，数值仿真和试验结果充分验证了方法的有效性。     

利用平滑约束复原方法处理CCD相机遥感图像

重点研究了频域平滑约束复原方法以及该方法对遥感领域中的实际应用，文章先介绍了平滑约束复原方法的理论基础，然后用该方法对CCD相机的遥感图像进行了复原处理，讨论了遥感器系统调制传递函数（MTF）曲线的拟合，遥感器系统MTF矩阵的构造以及复原参数的选择。可以得出结论，在一定条件下，利用平滑约束复原方法可以有效地改善整个系统的调制传递函数，从而使图像变得清晰。     

微结构谐振传感器

阐述了频率输出的新型谐振传感器的发展方向之一——微型化。评价性地论述了热激励硅谐振压力传感器和热激励谐振膜质量流量传感器。重点讨论了热激励的原理,特点等。指出我国应对传感器的这一发展趋势给予足够的重视。     

扭叶片型面在线检测的研究

以汽轮机700mm扭叶片为对象,在XK5040数控机床上,进行了型面误差在线检测的研究。     

基于小波包分解的早期碰摩故障诊断研究

研究了旋转机械转静件早期碰摩故障信号的检测问题.根据小波包分解能在所有频率范围聚焦,对信号奇异性非常敏感的特性,对比分析了不碰摩和早期碰摩信号的小波包分解细节分量,得出应用小波包分解可实现早期碰摩故障诊断.同时,还研究并实现了碰摩故障的定位问题.      

基于目标操作化的多引擎协作体系结构研究

基于目标操作化的域原子操作模型,研究分析了面向应用目标的系统设计与实现的基本问题,通过引入解释引擎,提出了面向目标的形式模型与应用软件设计实现的一体化机制;在系统级应用中间件之上,引入组件服务,提出了一个通过处理操作作业流实现目标的、多个操作服务引擎协作的体系结构,通过构造组件适配器,以满足操作服务引擎对异构组件服务的一致性访问.     

递推阻尼最小二乘及其在INS/双星组合中应用

由于双星系统的误差模型未知,且稳定性较差,采用Kalman滤波实现惯导(INS)/双星组合导航时,其滤波特性较差;而此时最小二乘法是实际工程应用中常用的方法,但易产生参数爆发现象.因此,提出了一种基于多输入-多输出(MI-MO)系统的递推阻尼最小二乘法,并将其应用到INS/双星组合导航系统中.仿真结果表明,利用递推阻尼最小二乘法能达到和递推最小二乘法同样的精度,且能明显抑制参数爆发现象.      

A comprehensive numerical model investigating the thermal-dynamic performance of scientific balloon

The increase of balloon applications makes it necessary for a comprehensive understanding of the thermal and dynamic performance of scientific balloons. This paper proposed a novel numerical model to investigate the thermal and dynamic characteristics of scientific balloon in both ascending and floating conditions. The novel model consists of a dynamic model and thermal model, the dynamic model was solved numerically by a computer program developed with Matlab/Simulink to calculate the velocity and trajectory, the thermal model was solved by the Fluent program to find out the balloon film temperature distribution and inner Helium gas velocity and temperature field. These models were verified by comparing the numerical results with experimental data. Then the thermal and dynamic behavior of a scientific balloon in a real environment were simulated and discussed in details.     

Characterization of ionospheric amplitude scintillations using wavelet entropy detrended GNSS data

The extensive monitoring networks of Global Navigation Satellite System (GNSS) ionospheric scintillation have been established to continuously log observation data. Further, the amplitude scintillation index and the phase scintillation index, which are derived from scintillation observations, are anticipated to accommodate the accuracy requirement of both the user level and the monitoring station level. However, raw scintillation observations essentially measure superposed waveform impairments of GNSS signals propagating through ionosphere and troposphere. It implies that fluctuations of raw scintillation observations are caused by multiple factors from the entire radio propagation environment. Hence, it is crucial to characterize ionospheric scintillations from GNSS observation data. And the characterization is implemented through extracting fluctuations of raw observations merely induced by ionospheric scintillations. Designed to address this problem by means of Fourier filtering detrending, the present work investigates the influence of varying detrending cutoff frequencies on wavelet statistical energy and wavelet entropy distributions of scintillation data. It consequently derives criteria on the optimum detrending cutoff frequency for three types of raw amplitude scintillation data, which are classified by their wavelet energy distributions. Results of the present work verify that detrending with specific optimum cutoff frequencies rather than the fixed and universally applicable one renders the validity and credibility of characterizing ionospheric scintillations as the part of GNSS observation fluctuations purely induced by ionosphere electron density irregularities whose scale sizes are comparable with or smaller than the Fresnel scale.     

Magnetar descendants in HMXBs?

We investigate the relation between the pulse and orbital periods in high-mass X-ray binaries (HMXBs), in order to find the candidates of magnetar descendants in HMXBs. We suggest that magnetar descendants can be found among the HMXBs with relatively shorter orbital periods and longer pulse periods.