基于超螺旋二阶滑模的双馈风力发电机控制策略

传统双馈风力发电机(DFIG)控制存在抖振现象,容易造成系统的不稳定。为了减轻控制抖振现象,提高控制的稳定性,在分析了DFIG动态特性的基础上,建立了DFIG的数学模型,设计了超螺旋二阶滑模控制器,并研究了突变风的情况下滑模控制器的控制性能。通过MATLAB/Simulink工具进行了仿真验证。仿真结果证明:滑模控制器具有良好的最优转矩跟踪能力和无功调节能力,与一般的控制方法相比鲁棒性较强,转子控制电压连续,控制产生的抖振可以大幅减轻,系统的稳定性大大提升。     

Early analysis of precise orbit and clock offset determination for the satellites of the global BeiDou-3 system

Eight new-generation BeiDou satellites (BeiDou-3) have been launched into Medium Earth Orbit (MEO), allowing for global coverage since March 2018, and they are equipped with new hydrogen atomic clocks and updated rubidium clocks. Firstly, we analyzed the signals for the carrier-to-noise-density ratio (C/N0) and pseudorange multipath (MP) by using international GNSS (Global Navigation Satellite System) Monitoring and Assessment System (iGMAS) station data, and found that B1C has a lower C/N0, and B2a has the same level of C/N0 as the B1I and B3I signals. For pseudorange multipath, compared with the BeiDou-2 satellites, the obvious systematic variation of MP scatters related to the elevation angle is greatly improved for the BeiDou-3 and BeiDou-3e satellites signals. For the signals of the BeiDou-3 satellites, the order of the Root Mean Square (RMS) values of multipath and noise is B3I?<?B1I?<?B2a?<?B1C. Then, the comparison of the precise orbit determination and clock offset determination for the BeiDou-2, BeiDou-3, and BeiDou-3 experimental (BeiDou-3e) satellites was done by using 10 stations from iGMAS. The 3D precision of the 24?h orbit overlap is 24.55, 25.61, and 23.35?cm for the BeiDou-3, BeiDou-3e, and BeiDou-2 satellites, respectively. BeiDou-3 satellite has a comparable precision to that of the BeiDou-2 satellite. For the precision of clock offset estimation, the Standard Deviation (STD) of the BeiDou-3 MEO satellite is 0.350?ns, which is an improvement of 0.042?ns over that of the BeiDou-2 MEO satellite. The stabilities of the BeiDou-3 and BeiDou-3e onboard clocks are better than those of BeiDou-2 by factors of 2.84 and 1.61 at an averaging time of 1000 and 10,000?s, respectively.     

通信拓扑切换下的多飞行器协同拦截方法

针对通信拓扑切换条件下的多飞行器协同拦截问题，提出了一种基于扩张状态观测器的协同制导方法。建立协同制导设计模型，将协同拦截问题转换为视线稳定条件下的剩余飞行时间调节问题。为解决机动目标状态不确定的问题，将目标的状态视作扰动，设计扩张状态观测器来估计机动目标的状态，并在制导律中对目标的机动进行补偿。利用有限时间一致性理论进行一致性控制协议的设计，实现各飞行器剩余飞行时间的有限时间一致，并利用Lyapunov稳定性理论分析通信拓扑切换情况下闭环系统的有限时间稳定性，给出了系统一致收敛时间。仿真结果表明，在通信拓扑变换的情况下，设计的观测器能够有效估计目标状态，且协同制导律能够满足对剩余飞行时间的控制要求，进而实现协同拦截。     

基于点云数据的发动机管路最小间距计算方案

为检测整机发动机管路是否满足最小间距的设计要求,提出了一种基于点云数据的发动机管路最小间距计算方案,方案包含5个步骤:①从点云数据中划分出不同管路的数据;②基于管路点云数据的空间分布构造等间隔栅格,计算栅格中心点作为管路的趋势线数据;③在管路各趋势线数据点位置上构造垂直平面,将管路点云数据投影到最近的垂直平面上,获得各个垂直平面上呈圆弧状分布的投影点数据;④对各垂直平面上的投影点数据进行最小二乘圆拟合,得到拟合圆圆心及其半径值,将拟合圆圆心作为管路中心线数据;⑤采用遍历法计算两条管路中心线数据的最小间距,中心线最小间距分别减去两条管路的半径值则得到两条管路的表面最小间距。通过12条管路验证了方案的准确度。实验结果表明:管路最小间距偏差在-0.35~0.46mm之间,管路半径偏差在-0.08~0.22mm之间。该方案的实施有助于管路间距数字化检测的实现,且方案的计算结果具有较好的鲁棒性。      

高主流湍流度下密度比对涡轮导叶全气膜冷却特性的影响

为了研究高主流湍流度下二次流密度比对涡轮导叶全气膜冷却特性的影响,使用热色液晶测量了在主流湍流度为15%,二次流密度比为1.0和1.5下三维涡轮导叶的气膜冷却效率和换热系数。二次流与主流质量流量比为7.0%和12.5%。结果表明:二次流密度比增大可以降低冷气射流的动量,小流量比工况下,在叶片前缘和压力面前半段,动量较低的二次流在高主流湍流度的影响下更易耗散,增大二次流密度比使冷却效率明显降低;大流量比工况下,二次流动量降低使气膜孔后区域冷气贴附性增强,气膜冷却效率和冷气覆盖效果均得到提升。小流量比工况下,二次流密度比增大对叶片表面换热的影响较小;大流量比工况下,二次流密度比增大使吸力面中弦区域和压力面后半段的平均换热系数比分别降低15%和25%。     

航天器视场遮挡分析方法研究

敏感器视场遮挡分析是航天器构型布局设计的重要组成部分，针对大型在轨变构型航天器敏感器视场遮挡分析工作量大、出错率高、遮挡率无法量化等特点，本文提出一种基于敏感器第一视角的视场遮挡快速分析方法。该方法通过设置第一视角图像蒙版及图像映射，模拟方锥形、圆锥形、球形等各类敏感器视场，通过逐个像素比对，计算视场遮挡率和遮挡方位。使用此方法建立了空间站敏感器视场遮挡分析系统，结果表明新方法能够显著提高视场遮挡分析效率和准确率，并且为机构类部件运动过程对敏感器视场遮挡的分析提供了有效工具。     

Multi-level virtual prototyping of electromechanical actuation system for more electric aircraft

Electromechanical actuators (EMAs) are becoming increasingly attractive in the field of more electric aircraft because of their outstanding benefits, which include reduced fuel burn and maintenance cost, enhanced system flexibility, and improved management of fault detection and isolation. However, electromechanical actuation raises specific issues when being used for safety-critical aerospace applications like flight controls: huge reflected inertia to load, jamming-type failure, and increase of backlash with service due to wear and local dissipation of heat losses for thermal balance. This study proposes an incremental approach for virtual prototyping of EMAs. It is driven by a model-based system engineering process in order to enable simulation-aided design. Best practices supported by Bond graph formalism are suggested to develop a model’s structure efficiently and to make the model ready for use (or extension) by addressing the above mentioned issues. Physical effects are progressively introduced, and the realism of lumped-parameter models is increased step-by-step. In particular, multi-level component models are architected to ensure continuity between engineering activities. The models are implemented in the AMESim simulation environment, and simulation responses are given to illustrate how they can be used for preliminary sizing, control design, thermal balance verification, and faults to failure analysis. The proposed best practices intend to provide engineers with fast, reusable, and efficient means to assess performance virtually and enhance maturity, performance, and robustness.     

振动试验极限控制应用实例

介绍了某产品振动应力筛选试验，通过对产品采用极限控制，并组合配以虚拟参考点（2点控制）以及响应点（2点控制）的方式，保证产品在试验过程中不会受到过强的力学应力，避免产品内部敏感元件的损坏。这种振动试验与常见的振动试验有很多不同点，从某产品振动试验实践，阐述此类试验有关技术问题。     

Application of small-size antennas for estimation of angles of arrival of HF signals scattered by ionospheric irregularities

A modification of the Doppler Interferometry Technique is suggested to enable estimating angles of arrival of comparatively broadband HF signals scattered by random irregularities of the ionospheric plasma with the use of small-size weakly directional antennas. The technique is based on the measurements of cross-spectra phases of the probe radiation recorded at least in three spatially separated points. The developed algorithm has been used to investigate the angular and frequency-time characteristics of HF signals propagating at frequencies above the maximum usable one (MUF) for the direct radio path Moscow-Kharkiv. The received signal spectra show presence of three families of spatial components attributed, respectively, to scattering by plasma irregularities near the middle point of the radio path, ground backscatter signals and scattering of the sounding signals by the intense plasma turbulence associated with auroral activations. It has been shown that the regions responsible for the formation of the third family components are located well inside the auroral oval. The drift velocity and direction of the auroral ionosphere plasma have been determined. The obtained estimates are consistent with the classical conception of the ionospheric plasma convection at high latitudes and do not contradict the results of investigations of the auroral ionosphere dynamics using the SuperDARN network.