涡扇发动机极值限制保护闭环控制设计

现代高性能涡扇发动机采用分段组合多变量控制计划,以发挥发动机工作在整个飞行包线范围内的气动热力设计潜力。为保证发动机在过渡态工作的安全性,控制系统中必须考虑极值限制保护控制的设计问题。为避免直接限制保护控制引发的不同控制通道切换带来的系统震荡问题,提出1种高回路稳态增益的滞后-超前频域校正间接极值限制保护控制器设计方法,在保证限制回路足够的稳态精度和抗噪声能力的同时,又避免了引入积分环节导致相角裕度损失过大的缺点。通过发动机线性模型和非线性模型的控制系统仿真,验证了所述方法设计限制控制器的有效性。     

航路网络生成及优化

空中交通流运行的安全性和成本取决于航路网络结构。基于节点度实现航路网络枢纽节点和干线节点分层,利用全局耦合生成主干网络,运用距离连接概率实现干线节点社区化,采用连接概率生成社区网络;采用DBSCAN聚类算法,基于角度和距离实现航路网络优化;以中国大陆空域为例,实现了主干航路网络和局部干线航路网络的生成及优化,验证了方法的可行性。在与相关研究对比,基于节点度的枢纽节点选取更加客观合理,所构建的分层航路网络结构符合机场点的分布特性,采用DBSCAN聚类算法优化效率明显提高。     

涡轴发动机双回路PI控制器多发功率匹配

为了应对多个发动机共同驱动同一直升机时,单个发动机性能衰退所引发的输出功率不平衡问题,以控制2个转子转速的双回路结构PI控制器为基础,将外回路改为直接功率控制回路,搭配能够计算旋翼在一定转速下需求功率的机载模型,构建了1种涡轴发动机多发功率平衡匹配控制系统.内回路分别采用燃气发生器转子转速控制回路和动力涡轮转子转速控制回路,得到参数不同的控制器并进行了仿真验证和对比.结果表明:所设计的双回路PI控制器能够在保证涡轴发动机动力涡轮转速恒定的同时,使性能衰退程度不同的2台发动机输出相同的功率.     

基于载体姿态测量的微伺服吊舱

针对微小型无人机光电吊舱对光轴稳定与目标跟踪的需求,研究了一种基于载体姿态测量的光学平台稳定技术.该技术利用吊舱基座上的速率陀螺测量机体三轴姿态运动,通过控制光学平台的俯仰和偏航两通道伺服系统实现对光轴的惯性空间稳定.该系统使用步进电机来当执行机构,根据步进电机的特性,可以推导得到控制量与转速的关系,由此省去了在一般捷联稳定技术中的微分测速环节,得出了一种新的基于前馈控制的不变性原理.设计了解耦指令分配算法,将一个两轴耦合系统,转换为两个独立的单轴系统.在单轴控制中,分别设计了比例控制及比例积分控制算法实现对光轴的稳定控制和跟踪.最后通过在Matlab/Simulink环境下的仿真,以及实际的摇摆台试验,证明了基于载体姿态测量的稳定技术能够实现微小型无人机光电吊舱的光轴稳定.     

主流攻角对双射流孔气膜冷却特性的影响

应用压力敏感漆技术,在平板上测量了不同主流攻角(i=-30°,-20°,-10°,0°,10°,20°,30°)下双射流孔的气膜冷却效率,并利用计算流体动力学(CFD)计算得到的流场对气膜冷却效率的规律进行了解析。所研究的双射流孔结构的孔间无量纲横向距离为0.5,孔间无量纲流向距离为3;射流与主流密度比为1.0,吹风比分别为0.5、1.0、1.5、2.0。结果表明小的主流攻角(i=-10°,0°,10°)下,流场中存在反肾型涡对或挤压作用,气膜层与壁面贴附良好,气膜冷却效率最高;大正值攻角(i=20°,30°)下,虽然气膜覆盖面积大,但反肾型涡对退化,气膜冷却效率下降;大负值攻角(i=-20°,-30°)下,流场中有肾型涡对,且气膜横向覆盖受限,气膜冷却效率最低。     

不同纤维预制体结构对SiC_f/PyC/SiBCN复合材料力学性能的影响

使用不同织造方式(二维机织,法向增强2.5维机织和三维五向编织)制备了3种SiC纤维预制体,采用树脂转移模塑(RTM)和聚合物浸渍裂解(PIP)工艺制备了SiC_f/PyC/SiBCN复合材料。观察复合材料的显微组织,测试弯曲强度、拉伸强度、压缩强度等力学性能,探究不同预制体结构对复合材料力学性能的影响行为。结果表明:同一预制体结构在不同方向的纤维分布不同导致材料力学性能的各向异性;不同预制体结构对材料力学性能有着显著的影响。     

Calculation of flight vehicle main support wheel vibrations taking into account brake forces

A model of the main support of the aircraft landing gear is presented and its dynamics is studied using the equations for the distributed motion of a wheel equipped with a brake. Stability of the support wheel rolling motion is analyzed and the brake parameter values which may cause stability loss are found. The results of numerical experiments are presented.     

Ground Compatibility Tests for Gravity Measurement of SELENE: Accuracies of Two- and Four-Way Doppler and Range Measurements

The Japanese lunar mission Selenological and Engineering Explorer (SELENE) was launched in September 2007 and continued its mission until June 2009, when the main orbiter impacted with the surface of the Moon. SELENE consisted of three satellites: Main, Rstar, and Vstar. Rstar’s tasks were to forward up-link signals from the Usuada Deep Space Center (UDSC) to Main, and to down-link returning signals from Main to UDSC. We refer to this tracking sub-system as a four-way Doppler measurement. In contrast, conventional tracking systems between Rstar and UDSC as well as between Main and ground stations are referred to as two-way Doppler and range measurements. Using Main and Rstar, we successfully observed the gravity field over the farside of the Moon. Because four-way Doppler measurements via a relay sub-satellite were a fundamental experiment in space for Japanese space agencies, compatibility of radiometric instruments onboard Main and Rstar to UDSC were carefully examined at the UDSC using components manufactured for flight models. These tests not only proved the feasibility of the four-way Doppler measurements but also provided biases and variations of the four-way Doppler and two-way Doppler and range measurements that were later taken into account during the processing of tracking data and the analysis of the lunar global gravity field.     

注射成型和注射压缩成型角窗的残余应力比较

基于粘性流体力学基本方程和粘度模型,建立了注射成型和注射压缩成型的残余应力计算模型,然后对角窗的注射成型和注射压缩成型进行了计算模拟,结果表明,注射成型角窗的残余应力大,且分布范围宽;注射压缩成型角窗的残余应力相对较小,且分布范围较窄,这种特征与注射压缩成型时熔体流动阻力小、型腔压力和体积温度分布均匀有关。最后采用偏振光法对实际注射成型和注射压缩成型角窗的应力分布进行了测试,进一步验证了注射压缩成型制品的低残余应力特点。     

The Magnetic Electron Ion Spectrometer (MagEIS) Instruments Aboard the Radiation Belt Storm Probes (RBSP) Spacecraft

This paper describes the Magnetic Electron Ion Spectrometer (MagEIS) instruments aboard the RBSP spacecraft from an instrumentation and engineering point of view. There are four magnetic spectrometers aboard each of the two spacecraft, one low-energy unit (20–240 keV), two medium-energy units (80–1200 keV), and a high-energy unit (800–4800 keV). The high unit also contains a proton telescope (55 keV–20 MeV). The magnetic spectrometers focus electrons within a selected energy pass band upon a focal plane of several silicon detectors where pulse-height analysis is used to determine if the energy of the incident electron is appropriate for the electron momentum selected by the magnet. Thus each event is a two-parameter analysis, an approach leading to a greatly reduced background. The physics of these instruments are described in detail followed by the engineering implementation. The data outputs are described, and examples of the calibration results and early flight data presented.