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。     

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.     

Dynamical evolution of high area-to-mass ratio debris released into GPS orbits

A large set of simulations, including all the relevant perturbations, was carried out to investigate the long-term dynamical evolution of fictitious high area-to-mass ratio (A/M) objects released, with a negligible velocity variation, in each of the six orbital planes used by Global Positioning System (GPS) satellites. As with similar objects discovered in near synchronous trajectories, long lifetime orbits, with mean motions of about 2 revolutions per day, were found possible for debris characterized by extremely high area-to-mass ratios. Often the lifetime exceeds 100 years up to A/M ∼ 45 m²/kg, decreasing rapidly to a few months above such a threshold. However, the details of the evolution, which are conditioned by the complex interplay of solar radiation pressure and geopotential plus luni-solar resonances, depend on the initial conditions. Different behaviors are thus possible. In any case, objects like those discovered in synchronous orbits, with A/M as high as 20–40 m²/kg, could also survive in this orbital regime, with semi-major axes close to the semi-synchronous values, with maximum eccentricities between 0.3 and 0.7, and with significant orbit pole precessions (faster and wider for increasing values of A/M), leading to inclinations between 30° and more than 90°.     

论航空产品质量改进

航空产品质量改进针对旧的质量标准．建立新的质量标准，可以不断提高产品技术水平，克服存在的缺陷,改善使用性能。为保证质量改进取得预期效果，应从程序、方法和管理控制等多方面着手。     

中小型企业建立生产计划优化线性规划模型的通用模式

本文提出了建立企业生产计划优化线性规划模型中约束方程的通用方法。简化了建模过程。并经多个企业的实际应用证明了其普遍适用性。为中小型企业建立生产计划优化线性规划模型提供了一个通用模式。     

基于自适应Kalman滤波的改进PSO算法

针对基于Kalman滤波的PSO算法在设计与应用过程中存在的不足,提出了基于自适应Kalman滤波的改进PSO算法。利用粒子群状态空间Markov链模型,建立粒子群系统状态方程;采用粒子的速度和位置作为观测量,构建观测方程;引入记忆衰减因子动态调整Kalman滤波模型参数及噪声方差阵,降低模型误差,提高粒子的位置估计精度。仿真实验表明:改进的PSO算法无论在优化精度、收敛速度,还是在稳定性方面都有很大的改进和提高,这就有效避免了粒子的"早熟"收敛问题;尤其在处理复杂多峰问题上,改进算法表现出很明显的优越性。     

通用连锁药店管理信息系统的设计与实现

本文结合实例阐述了基于PSTN的通用连锁药店管理信息系统的设计实现，并介绍了该系统的网络拓扑结构．功能模块设计和数据存储模式等。     

关于文件类产品价格管理模式的探讨

文件类产品价格管理是总体设计部管理的重要组成部分,应予以关注和规范化。文章对此问题进行了分析和讨论。首先,以宏观经济学中有关价格的概念为理论基础,介绍了价格的职能和作用,并分析了价格管理应用于文件类产品管理的意义。在此基础上,对总体设计单位文件类产品价格管理的权利和义务进行了讨论。最后,结合航天产品价格管理特点,对文件类产品价格管理模式进行了总结,并提出了如何进一步完善的建议。     

Neutron stars: Classification and evolution

The general aproach is considered which describs the evolution of neutron stars in terms of their interaction with surrounding matter. All possible states of neutron stars are classified from this point of view. Classification and evolution of binaries contaning neutron stars are also considered.