基于ANSYS的同面多电极电容传感器仿真研究

同面多电极电容传感器是一种新的飞机复合材料构件损伤检测技术,该检测技术的正问题中敏感场分布函数的计算要涉及到静电场中电容计算问题。在仿真研究中,电容要通过场的数值计算方法来求得。本文介绍了如何使用ANSYS有限元分析计算同面多电极电容传感器中的各电极对之间的电容,对检测材料发生异常及传感器参数改变时电容的变化进行了分析,为损伤检测的特征提取和逆问题图像重构提供了仿真数据。     

二维三轴编织复合材料压缩失效行为的细观有限元模拟

为研究典型二维三轴编织复合材料（2DTBC）的压缩破坏机理，建立了细观有限元模拟方法体系。提出了反映编织复合材料真实几何特性的单胞模型建模策略，根据Murakami-Ohno损伤理论建立了各向异性损伤模型来模拟纤维束中的损伤起始和扩展行为，通过引入波动系数描述了纤维束的起伏状态，并采用内聚力单元来模拟界面分层。在此基础上，分析得到了二维三轴编织复合材料在压缩载荷下的破坏过程，研究了压缩载荷下纤维束和界面层的损伤演化，探讨了纤维束波动对压缩性能的影响规律。通过与相关试验结果对比，该模型能够准确预测二维三轴编织复合材料在面内压缩载荷下的力学响应和主要失效行为，以及自由边效应。细观失效过程分析结果表明，二维三轴编织复合材料轴向压缩的破坏是由轴向纤维束的纤维压缩失效主导的；横向压缩破坏则是由偏轴纤维束的纤维压缩失效引起的。     

压气机叶片外物损伤模拟的撞击能量当量法

在分析外物与叶片间的运动态势后，提出压气机叶片外物员伤模拟的撞击能当量法，即使得摆锤的势能与外物摘击叶片时可能达到的功能相等。据此，设计并制作了摆锤装置，并实验观察到钛制压气机叶片损伤形态与撞击能量间的变化关系，即随着撞击能量的增加，损伤形态产生的顺序为，压痕→突缘→裂纹→突缘呈４５°剪切破坏，这与外场收集到的叶片的前缘损伤形态一致，同时，采用了ＴＣ４压气机叶片进行了相应的高周疲劳试验，验证了方法     

基于线性二次型的飞控参数故障渐近调节

 研究了含有参数故障的线性系统,提出了一种基于线性二次型的控制策略。采用该渐近调节反馈控制律,可以减小系统由于容错控制算法时延所致的性能下降。针对某飞机模型进行了仿真,结果验证了所提出策略的有效性。     

A theoretical model of semi-elliptic surface crack growth

A theoretical model of semi-elliptic surface crack growth based on the low cycle strain damage accumulation near the crack tip along the cracking direction and the Newman–Raju formula is developed. The crack is regarded as a sharp notch with a small curvature radius and the process zone is assumed to be the size of cyclic plastic zone. The modified Hutchinson, Rice and Rosengren(HRR) formulations are used in the presented study. Assuming that the shape of surface crack front is controlled by two critical points: the deepest point and the surface point.The theoretical model is applied to semi-elliptic surface cracked Al 7075-T6 alloy plate under cyclic loading, and five different initial crack shapes are discussed in present study. Good agreement between experimental and theoretical results is obtained.     

Coupling damage and reliability model of low-cycle fatigue and high energy impact based on the local stress–strain approach

Fatigue induced products generally bear fatigue loads accompanied by impact processes,which reduces their reliable life rapidly. This paper introduces a reliability assessment model based on a local stress–strain approach considering both low-cycle fatigue and high energy impact loads.Two coupling relationships between fatigue and impact are given with effects of an impact process on fatigue damage and effects of fatigue damage on impact performance. The analysis of the former modifies the fatigue parameters and the Manson–Coffin equation for fatigue life based on material theories. On the other hand, the latter proposes the coupling variables and the difference of fracture toughness caused by accumulative fatigue damage. To form an overall reliability model including both fatigue failure and impact failure, a competing risk model is developed. A case study of an actuator cylinder is given to validate this method.     

结合损伤力学与有限元方法预估铆接结构疲劳寿命

利用飞机铆接试验件疲劳试验数据,结合损伤力学与有限元方法,通过MATLAB调用ABAQUS进行损伤演化方程参数的遗传优化反演。将反演得到的损伤演化方程用于飞机结构疲劳寿命预估中,对机翼蒙皮锪窝形式的铆接结构进行了寿命计算和分析,并与试验数据作对比,证明了方法的可行性。     

舰载直升机金属动部件寿命控制技术研究

在分析现役老龄化舰载直升机动部件载荷特点的基础上,结合直升机所处的海洋腐蚀环境,讨论了舰载直升机的损伤类型和损伤容限寿命管理方法在其寿命分析中的应用,比较了损伤容限法应用于舰载直升机动部件与应用于固定翼飞机的不同点,重点讨论了损伤容限方法应用于工程实践亟待解决的关键技术。     

基于损伤力学预估点蚀疲劳寿命有限元法

飞机使用环境谱的不断变化会对机体结构造成腐蚀损伤,工程上难以在外场环境下进行实时损伤检测与疲劳性能试验。点蚀作为腐蚀的初始阶段,危害性大,部位也难以预测。采用损伤力学和有限元相结合的方法,以材料疲劳S-N数据为基础,将点蚀损伤认为是一种初始缺陷,建立基于损伤力学假设的点蚀损伤疲劳寿命预估方法,并提出一种改进型损伤参数反演方法。对点蚀疲劳失效过程进行数值模拟,模拟结果与试验结果吻合,证明该方法应用于金属材料点蚀疲劳问题中是合理的、可行的,为后续实际预腐蚀损伤疲劳研究奠定了基础。     

Diversity of Comets: Formation Zones and Dynamical Paths

The past dozen years have produced a new paradigm with regard to the source regions of comets in the early solar system. It is now widely recognized that the likely source of the Jupiter-family short-period comets (those with Tisserand parameters, T > 2 and periods, P, generally < 20 years) is the Kuiper belt in the ecliptic plane beyond Neptune. In contrast, the source of the Halley-type and long-period comets (those with T < 2 and P > 20 years) appears to be the Oort cloud. However, the comets in the Oort cloud almost certainly originated elsewhere, since accretion is very inefficient at such large heliocentric distances. New dynamical studies now suggest that the source of the Oort cloud comets is the entire giant planets region from Jupiter to Neptune, rather than primarily the Uranus-Neptune region, as previously thought. Some fraction of the Oort cloud population may even be asteroidal bodies formed inside the orbit of Jupiter. These comets and asteroids underwent a complex dynamical random walk among the giant planets before they were ejected to distant orbits in the Oort cloud, with possible interesting consequences for their thermal and collisional histories. Observational evidence for diversity in cometary compositions is limited, at best. This revised version was published online in June 2006 with corrections to the Cover Date.