基于径向基函数神经网络的自由曲面重构

根据径向基函数神经网络（RBFNN）具有很强的非线性逼近能力的优点，本文采用RBF网络模型进行自由曲面重构，建立了适应于曲面重构的径向基函数网络模型，讨论了基函数对重构曲面连续性的影响，并与多自由曲面重构，建立了适应于曲面重构的径向基函数风络模型，讨论了基函数对重构曲面连续性的影响，并与多层感知器神经网络的性能进行对比。理论分析和仿真实验结果表明：常用的几种径向基函数重构的曲面都具有很好的连续性，径向基函数网络用于曲面重构，不论是在拟合精度，还是网络的训练速度都明显优于多层感知器网络，具有一定的实用价值。     

单一基准径向圆跳动误差的新测量法

用传统的测量方法不能得到单一基准径向圆跳动误差的准确值。根据单一基准径向圆跳动误差的定义建立了该项误差的正交最小二乘评定数学模型。在万能工具显微镜上得到了采样数据并给出了微机数据处理结果。     

高强钛合金中的微动损伤与疲劳

本文对高强钛合金Ti-10V-2Fe-3Al在不同温度下的微动损伤和疲劳特性进行了研究。试验结果表明,该合金对微动损伤十分敏感,常温疲劳强度下降达50％。微动损伤的主要机制是疲劳脱层,这是由作用在材料次表层的交变切应力引起的,它将导致疲劳裂纹的萌生和早期断裂。疲劳裂纹的扩展方向可根据接触应力分析得到解释。在较高试验温度下,由于接触面形成的氧化层的保护作用,微动损伤程度减弱。     

TC4钛合金的微动磨损及防护

对Ｔｉ－６Ａｌ－４Ｖ合金在１８℃，１００℃２５０℃下的微动磨损特性及防护工艺进行了研究。表明：该合金微动磨损的主要磨损形式是疲劳脱层，其磨损量随温度升高而下降，高渐微动磨损量与磨损区表面所形成的氧化层的性质及厚度有关。     

机翼连接耳片微动疲劳裂纹萌生机制

 对歼击机机翼全尺寸模拟疲劳试验的耳片断口进行了观察和分析,从断裂处存在磨痕和磨屑的形貌及耳片受力变形状态,证明耳片属于微动疲劳断裂。本文提出铝合金耳片和钢衬套接触时,微动疲劳裂纹萌生过程的模型。     

确定微动疲劳寿命的附加应力法

通过引进新的微动疲劳参数 ,对微动疲劳寿命进行定量分析。将微动作用的效果作为一种附加应力 ,与普通力学分析中得到的宏观应力一起作为总应力作用于构件。用这个总应力按疲劳寿命计算公式或对照疲劳寿命S -N曲线得到疲劳寿命 ,这个疲劳寿命就是微动疲劳寿命。这种方法称为附加应力法。     

涡轮高压导叶流场结构及损失分析

采用具有TVD性质有三阶精度Godumov格式，数值模拟了某型涡轮高压导叶流场，并对流场损失及涡系结构进行分析，结果表明由于强烈的径向流，使低能流体大量地迁移到下端壁，使得下端部的损失显著增大，从而引起了总损失的增加。因此在高压导叶设计中，当采用低展弦比叶片时，应注意削弱叶片出口附近流场的严重径向窜流。     

Effect of protrusion amount on gas ingestion of radial rim seal

In this paper, the effect of different amount of protrusion on various parameters in rotor–stator system was experimentally studied by measuring CO₂ concentration and pressure, in order to obtain the optimal protrusion amount. The parameters of different dimensionless sealing flow were measured under the condition that the annulus Reynolds number was 4.39 × 10⁵ and the rotating Reynolds number was 1.05 × 10⁶. The results show that the change of the amount of protrusions has little effect on the static pressure in the cavity, and the static pressure change near the sealing ring is almost negligible. But the total pressure and sealing efficiency increase first and then decrease with the increase of the amount of protrusion. The variation of power consumption is the same. A complex vortex structure will appear at the high radius region when the protrusion is installed. On the other hand, the protrusion can effectively reduce the minimum sealing flow of the rotor–stator cavity. Furthermore, considering the sealing efficiency and power consumption, the best range of the protrusion amount is about 36. The ratio near this range can optimally balance the alleviation of the gas ingestion and the reduction of the power consumption.     

Application of improved active disturbance rejection control algorithm in tilt quad rotor

The Tilt Quad Rotor (TQR) has complex dynamics characteristics, especially in conversion mode. It is difficult to build the dynamic model of the TQR and the environmental factors have a great influence on it. To solve the problem of control in conversion mode of TQR, this paper carries out the design of the controller based on improved Active Disturbance Rejection Control (ADRC). According to the characteristics of flight in conversion mode, Tracking Differentiator (TD) with explicit model is used to solve the problem of multiple integrals when the system is high-order system. Extended State Observer (ESO) with Radial Basis Function (RBF) neural network is used to estimate and compensate for internal and external uncertainties, and the adaptive sliding mode control in Nonlinear State Error Feedback (NLSEF) is used to improve the response speed of the controller and reduce the parameters which should be tuned. Through the flight control simulation of the TQR, the validity and rationality of the control system are verified.     

A statistical study of C IV regions in 20 Oe-stars

In this paper, using the Gauss-Rotation model (GR model), we analyse the UV C IV resonance lines in the spectra of 20 Oe-stars of different spectral subtypes, in order to detect the structure of C IV region. We study the presence and behavior of absorption clouds and analyse their characteristics. From this analysis we can calculate the values of a group of physical parameters, such as the apparent rotational and radial velocities, the random velocities of the thermal motions of the ions, the Full Width at Half Maximum (FWHM), the optical depth, as well as the absorbed energy and the column density of the independent regions of matter, which produce the main and the satellite clouds of the studied spectral lines. Finally, we present the relations between these physical parameters and the spectral subtypes of the studied stars and we give our results about the structure of the C IV region in their atmosphere.