机身上壁板复合材料蒙皮数字化成型工艺

为解决树脂基复合材料复杂结构件工艺难以实现问题,采用三维工艺模型设计、铺层工艺仿真、铺层样片排版与数控下料、激光投影铺层定位等数字化技术,不但从根本上改变了传统的复合材料构件生产方式,解决了工艺技术难题,而且在缩短研制周期、提高产品质量,降低研制成本等方面都取得了显著的应用效果。     

3D-Cf / Mg 复合材料的热残余应力研究

采用随动硬化有限元模型,研究了三维碳纤维增强镁基复合材料(3D-Cf/Mg)基体热残余应力的大小、分布以及不同工艺处理对热残余应力的影响。同时,对复合材料进行了高、低温处理,利用XRD定性分析了处理前后复合材料基体热残余应力的变化。计算结果表明:经过-196℃低温处理后,复合材料基体的平均Mises热残余应力由169.06 MPa减小至55.29 MPa;高温处理后,基体平均热残余应力几乎不变。该结果与实验结果吻合,证明了低温处理能明显降低复合材料基体的热残余应力。     

基于数字孪生的设备加工过程监测技术研究

针对典型航空产品装配生产线的生产过程中缺乏有效的人机交互手段,设备实时运行状态可视化监控程度低等问题,提出了一种基于数字孪生的加工设备运行状态监测方法,包括模型构建与优化处理、NC程序解析与加工仿真、软硬件通信与数据传输和实时仿真与数据分析。最后在某航空发动机外涵机匣装配生产线验证了该方案,可以实现NC程序加工仿真分析、设备运行过程中状态的在线监测和实时三维仿真。     

飞机起落架全方位移动装配机器人设计与研究

起落架作为支撑飞机重量、吸收撞击能量的重要部件,在装配和试验过程中面临着装配空间狭小、装配精度高等特殊要求,急需研制一款具备可移动、多自由度调节功能的柔性装配平台。通过对起落架装配需求进行分析,设计出基于Mecanum轮的全方位移动和基于3–RPS的并联机构组成的6自由度装配机器人,详细介绍了装配机器人的结构组成、控制方法,对机器人运动学特性进行分析获得运动学模型,并进行运动学参数设置及精度分析。通过对起落架装配机器人精度测试以及实物装配,验证该机器人的功能和性能满足使用要求。     

三元整体叶轮的曲面造型及其计算机辅助制造技术

针对一种三元整体叶轮,采用B样条方法对叶片中性面上顶部和根部的两组数据点进行了插值曲线的反算,进而构造出直纹面形式的叶片中性面和叶片曲面;研究了在五坐标机床上采用球头棒铣刀侧铣加工叶轮时的刀位计算方法,给出了在UG环境下的叶轮曲面建模方法及其数控加工仿真步骤。     

CVD Al2O3-SiO2涂层的莫来石化行为

采用CVD工艺,以AlCl3-SiCl4-H2-CO2为先驱体气相体系,在石墨纸上于550℃制备出Al2O3-SiO2复合氧化物涂层,通过DTA和XRD分析了该涂层的莫来石化过程.该涂层由γ-Al2O3和非晶SiO2组成,其DTA曲线有四个典型峰,793℃弱的放热峰为开始莫来石化峰;984℃尖锐的放热峰为γ-Al2O3向δ-Al2O3转化峰;1240℃弱的吸热峰为δ-Al2O3向α-Al2O3转化峰,该过程比较缓慢;1337℃强的放热峰为莫来石形成峰,发生在δ-Al2O3与SiO2之间.结果表明,该CVD过程不具氧化性,对C不腐蚀,制备的Al2O3-SiO2涂层经1350℃热处理2h可转化为莫来石结合α-Al2O3.     

防老剂D纯度对天然橡胶(NR)热氧老化性能的影响

为了改善天然橡胶的热氧老化性能,试验了防老剂D提纯品和工业品对天然橡胶(NR)热氧老化性能的影响,测试了其热氧化诱导期、热失重、热老化的性能变化。结果表明：含杂少纯度高的防老剂D使天然橡胶的抗热氧老化得到改善。     

Observations of non-migrating tides and ionospheric perturbations of O(D) airglow by ISUAL instrument

In this paper, we present the spatial variations of O(¹D) airglow observed by the ISUAL (Imager of Sprites and Upper Atmospheric Lightning) instrument on board the FORMOSAT-2 satellite. With a CCD camera and a 630 nm filter, ISUAL can measure global atmospheric emissions lying between the heights of 80 and 300 km. In days of 3–6 September 2008 and 25–27 February 2009, ISUAL has measured the emissions of O(¹D) airglow with results showing strong longitudinal peak-3 and peak-4 structures. The Lomb-Scargle analyses for these two cases show periods of longitudes of 120° and 90° supporting the DE2 and DE3 non-migrating tides. The 630 nm emissions are enhanced in equatorial regions and are lying along the equator. Over Africa its intensity can sometimes increase up to 80% relative to other longitudes. The perturbation is so strong that non-migrating tides are erased. A case of bimodal distribution with strong emissions at latitudes in equator and mid-latitude in geographic coordinates was observed.     

Analytic and numerical treatment of motion of dust grain particle around triangular equilibrium points with post-AGB binary star and disc

This paper investigates the motion around the triangular equilibrium points, of a passively gravitating dust particle in the gravitational field of a low-mass post-AGB binary system, surrounded by circumbinary disc. The two bodies of the binary are modeled as a triaxial star and a radiating-oblate star. Due to small deviation of disc stars on circular orbits, we have assumed that the Coriolis and centrifugal forces of the stars are slightly perturbed. The triangular equilibrium points of the particle are found. These points are defined by, triaxiality of the primary star, oblateness and radiation of the secondary one and the gravitational potential from the disc mass. Further, when the disc mass increases, the particle moves nearer to the stars and farther away from the disc. In general, these equilibrium points are linearly stable when μ < μ_C; where μ is the mass ratio and μ_C is the critical mass function, defined by the parameters of the system. The effects of each of these parameters on the size of the stability region are stated, and the periodic motion around the stable points is examined. It is seen that the orbits are ellipses, and the orientation, eccentricities, lengths of the semi-major and semi-minor axes are influenced by the parameters of the problem. In particular, for our numerical linear stability analysis, we have taken an extremely depleted pulsating star, IRAS 11472-0800 as the post-AGB triaxial star, with a weakly-radiating young white dwarf star; G29-38 as the secondary. For this system, the stability result of the triangular points comes out different. Here, μ_C < μ throughout the entire range of the mass ratio and the critical mass function. Hence, the triangular equilibrium points are unstable. The stability of the orbits is tested using the Poincaré surfaces of section (Pss). The region of stability is controlled by the introduced parameters and the Jacobi constant.     

基于纹理的活动轮廓三维图像分割研究

对具高噪声和低对比度三维图像的识别和分割算法进行了研究。基于活动轮廓模型,用Gabor变换提取图像的纹理特征,根据统计学信息假设,通过偏微分方程水平集和窄带方法求解,获得较基本活动轮廓的算法分割更光滑精确的物体轮廓。实验结果表明:改进模型算法的效率和准确度达到预期效果。