TC11焊接接头高周疲劳分形损伤模型

根据金属疲劳断口具有几何分形特征,将Chaboche高周疲劳损伤模型推广到分数维空间,建立了综合考虑断口细观特征的高周疲劳分形损伤演化模型.针对TC11钛合金电子束焊接接头,以载荷控制的疲劳试验为基础研究其高周疲劳性能;采用扫描电镜法(SEM)对断口微观特征进行定量分析,计算得到了各级载荷下疲劳断口的分形维数;通过对试...     

基于低可探测性的参考航迹规划

根据分层规划思想,确定参考航迹是进行航迹规划时首先要解决的问题。在充分考虑雷达探测的各种环境因素及飞行器RCS方位分布特性的基础上,将雷达对目标发现概率作为参考航迹的一个重要评价指标,基于自适应进化算法,采用新的遗传算子,最终生成综合考虑雷达威胁和飞行距离的参考航迹。结果表明,该航迹规划模型能根据对低可探测性和航程的不...     

C/SiC材料在模拟空天往返条件下的可重复使用性能评估

针对飞行器空天往返、多次使用的发展需求,以2D C/SiC材料为对象,选择开放大气模拟环境、800 ℃温度条件开展了常/高温拉伸试验、以及常温→高温→降温循环变化历程下拉-拉疲劳的耦合试验,得到不同的力学性能规律,分析了影响材料表面涂层完整性的控制因素及转化点。表明C/SiC材料具有优良的高温静态持续强度性能,但在常-高温循环变化历程下的疲劳性能明显衰减。采用剩余刚度衰减模型,提出了力-热-氧耦合时考虑常-高温循环历程影响因素、以及氧化尺寸效应影响的疲劳剩余性能评估方法。     

基于雷达散射截面约束的气动优化设计

采用拉格朗日乘子法优化设计了雷达散射截面约束条件下的锥形融合气动外形.拉格朗日乘子法中的极小化问题采用动态演化的优化设计方法求解.该方法是一种基于非定常演化的优化设计方法,即在求解非定常流动支配方程的时候同时履行优化过程,较其它基于定常解的优化方法具有高得多的计算效率.其中的雷达散射截面通过求解非结构的笛卡儿网格上的时域麦克斯韦方程来得到,而升阻比则通过求解锥形流方程来计算.通过优化设计,得到了M∞=8.0时,升阻比为4.98,雷达散射截面只有1.66m2的锥形融合气动外形.     

Semi-analytical investigations of high area-to-mass ratio geosynchronous space debris including Earth’s shadowing effects

This paper investigates the long-term perturbations of the orbits of geosynchronous space debris influenced by direct radiation pressure including the Earth’s shadowing effects. For this purpose, we propose an extension of our homemade semi-analytical theory [Valk, S., Lemaître, A., Deleflie, F. Semi-analytical theory of mean orbital motion for geosynchronous space debris under gravitational influence. Adv. Space Res., submitted for publication], based on the method developed by Aksnes [Aksnes, K. Short-period and long-period perturbations of a spherical satellite due to direct solar radiation. Celest. Mech. Dyn. Astron. 13, 89–104, 1976] and generalized into a more convenient non-singular formalism. The perturbations accounting for the direct radiation pressure with the Earth’s shadow are computed on a revolution-by-revolution basis, retaining the original osculating Hamiltonian disturbing function. In this framework, we compute the non-singular mean longitude at shadow entry and shadow exit at every orbital revolution in opposition to classical approaches where the singular eccentric anomalies at shadow entry and shadow exit are computed. This new algorithm is developed using non-singular variables. Consequently, it is particularly suitable for both near-circular and near-equatorial orbits as well as orbits which transit periodically around null eccentricities and null inclinations.The algorithm is tested by means of numerical integrations of the equations, averaged over the short periods, including radiation pressure, J₂, the combined Moon and Sun third body attraction as well as the long-term effects of the 1:1 resonance occurring for geosynchronous objects. As an extension of [Valk, S., Lemaître, A., Anselmo, L. Analytical and semi-analytical investigations of geosynchronous space debris with high area-to-mass ratios influenced by solar radiation pressure. Adv. Space Res., doi:10.1016/j.asr.2007.10.025, 2007b], we especially apply our analysis to space debris with area-to-mass as high as 20 m²/kg. This paper provides numerical and semi-analytical investigations leading to a deep understanding of the long-term evolution of the semi-major axis. Finally, these semi-analytical investigations are compared with accurate numerical integrations of the osculating equations of motion over time scales as high as 25 years.     

基于用户自定义变更的本体进化

提出一种基于用户自定义变更的本体进化方法。首先给出了该方法的形式化描述,建立了本体一致性模型和原子变更及冲突消解方法,然后对用户自定义变更模型进行语义描述,将用户自定义变更转换成原子变更,并对其进行了优化。最后给出了用户自定义变更及优化的实例。结果表明:本方法可以很好地满足本体进化过程中用户的复杂需求,并实现了本体变更的形式化描述,解决了各种变更中的冲突问题。     

7075-T6铝合金厚板FSW焊缝沿厚度方向上的显微组织演变规律

采用金相显微镜（OM）、扫描电镜（SEM）和背散射电子衍射（EBSD）技术表征7075铝合金厚板搅拌摩擦焊（FSW）焊核中心区的微观结构，研究沿焊缝厚度方向上的显微组织演变规律。结果表明，焊核中心区发生了明显的动态再结晶，由原始粗大的板条状组织转变成了细小的等轴晶；随着距焊缝上表面距离的增加，中心区等轴晶晶粒尺寸呈现逐渐增大的趋势。其中，中心区上部4 mm处的晶粒尺寸最小，仅为7.8 μm；底部19 mm处的晶粒尺寸最大，达18.6 μm。中心区动态再结晶分数随距离的增大而逐渐减小，从中心区顶部1 mm处最大值90.4%减小至底部19 mm处最小值57.5%。受动态再结晶影响，焊核中心区主要以大角度晶界（HAGB）分布为主，且中心区大角度晶界随距离的增加呈逐渐降低的趋势；但每一个典型位置处的大角度晶界分布呈现先增大后减小的趋势，且在45°左右时达到最大值；此外，中心区并没有强取向组织产生。同时，焊核中心区主要以细小、弥散的二次析出强化相η相为主，且二次析出强化相颗粒尺寸随距离的增加而呈逐渐增大的趋势，但二次析出强化相颗粒总体数量却呈相反的趋势变化。     

Asteroid and comet hazard: Identification problem of observed space objects with the parental bodies

This article focuses on the genetic identification of observed small cosmic bodies with alleged parental bodies; namely, comets, asteroids and meteoroid swarms. There is a problem of the upper D-value limit as a measure of proximity between the orbits of the bodies in the five-dimensional phase space (Southworth and Hawkins, 1963). In the study of genetic relationships of the comet and meteor complexes, the D value is usually taken as equal to 0.2 for all meteor showers. However, the upper D limit should be investigated for each meteoroid complex. For example, such investigation was performed for the Taurid meteor complex (Porub?an et al., 2006). In this paper, the upper D-criterion limit value was investigated for the Perseid meteor shower. The 1862 III Swift–Tuttle comet is its parental comet.     

Assessing and minimizing collisions in satellite mega-constellations

We aim to provide satellite operators and researchers with an efficient means for evaluating and mitigating collision risk during the design process of mega-constellations. We first introduce a novel algorithm for conjunction prediction that relies on large-scale numerical simulations and uses a sequence of filters to greatly reduce its computational expense. We then use this brute-force algorithm to establish baselines of endogenous (intra-constellation), or self-induced, conjunction events for the FCC-reported designs of the OneWeb LEO and SpaceX Starlink mega-constellations. We demonstrate how these deterministic results can be used to validate more computationally efficient, stochastic techniques for close-encounter prediction by adopting a new probabilistic approach from Solar-System dynamics as a simple test case. Finally, we show how our methodology can be applied during the design phase of large constellations by investigating Minimum Space Occupancy (MiSO) orbits, a generalization of classical frozen orbits that holistically account for the perturbed-Keplerian dynamics of the Earth-satellite-Moon-Sun system. The results indicate that the adoption of MiSO orbital configurations of the proposed mega-constellations can significantly reduce the risk of endogenous collisions with nearly indistinguishable adjustments to the nominal orbital elements of the constellation satellites.     

基于微分进化算法的二自由度PID控制器参数优化

针对二自由度PID控制器参数多、调节困难等问题,提出了一种基于微分进化算法参数调节优化方法。证明了微分进化算法能够收敛到平稳点,并具有概率全局收敛性。研究了二自由度PID控制器参数与抑制特性、跟踪特性的关系,并将微分算法与遗传算法、粒子群算法的参数优化结果进行了比较。仿真验证表明,微分算法能够更好地实现二自由度PID控制器参数的调节,具有优异的跟踪特性和抑制特性。