A deformation model of flexible,HAMR objects for accurate propagation under perturbations and the self-shadowing effects

A new type of space debris in near geosynchronous orbit (GEO) was recently discovered and later identified as exhibiting unique characteristics associated with high area-to-mass ratio (HAMR) objects, such as high rotation rates and high reflection properties. Observations have shown that this debris type is very sensitive to environmental disturbances, particularly solar radiation pressure, due to the fact that its motion depends on the actual effective area, orientation of that effective area, reflection properties and the area-to-mass ratio of the object is not stable over time. Previous investigations have modelled this type of debris as rigid bodies (constant area-to-mass ratios) or discrete deformed body; however, these simplifications will lead to inaccurate long term orbital predictions. This paper proposes a simple yet reliable model of a thin, deformable membrane based on multibody dynamics. The membrane is modelled as a series of flat plates, connected through joints, representing the flexibility of the membrane itself. The mass of the membrane, albeit low, is taken into account through lump masses at the joints. The attitude and orbital motion of this flexible membrane model is then propagated near GEO to predict its orbital evolution under the perturbations of solar radiation pressure, Earth’s gravity field (J₂), third body gravitational fields (the Sun and Moon) and self-shadowing. These results are then compared to those obtained for two rigid body models (cannonball and flat rigid plate). In addition, Monte Carlo simulations of the flexible model by varying initial attitude and deformation angle (different shape) are investigated and compared with the two rigid models (cannonball and flat rigid plate) over a period of 100?days. The numerical results demonstrate that cannonball and rigid flat plate are not appropriate to capture the true dynamical evolution of these objects, at the cost of increased computational time.     

基于MBSE的飞机大部件智能装配能力建设方法

飞机大部件智能装配能力建设涉及领域多、范围广,多学科、多专业交叉融合特点显著,是一项复杂的系统工程。近年来,飞机智能装配能力建设已实现相当程度的单点技术突破与应用,但并未达到全局最优,亟需采用科学的方法对智能装配体系能力建设进行整体规划与全局优化。提出采用基于模型的系统工程(Model-Based Systems Engineering,MBSE),科学开展飞机大部件智能装配体系能力建设的方法研究,逐级明确、细化智能装配能力建设需求与技术方案,构建相对应的数字模型并采用仿真技术进行不断验证、迭代优化,最终实现智能装配能力效能的最大化。     

Uncertain multiobjective redundancy allocation problem of repairable systems based on artificial bee colony algorithm

Based on the uncertainty theory, this paper is devoted to the redundancy allocation problem in repairable parallel-series systems with uncertain factors, where the failure rate, repair rate and other relative coefficients involved are considered as uncertain variables. The availability of the system and the corresponding designing cost are considered as two optimization objectives. A crisp multiobjective optimization formulation is presented on the basis of uncertainty theory to solve this resultant problem. For solving this problem efficiently, a new multiobjective artificial bee colony algorithm is proposed to search the Pareto efficient set, which introduces rank value and crowding distance in the greedy selection strategy, applies fast non-dominated sort procedure in the exploitation search and inserts tournament selection in the onlooker bee phase. It shows that the proposed algorithm outperforms NSGA-II greatly and can solve multiobjective redundancy allocation problem efficiently. Finally, a numerical example is provided to illustrate this approach.     

多层隔热组件的制作工艺

介绍了多层隔热组件及影响其隔热性能的主要因素,包括反射屏与间隔层的选材、多层组件的层密度、放气孔等.结合实际工程应用,对于多层隔热组件的材料选择和制作工艺进行了着重说明.     

迎接航空工业新一轮技术革命

以波音787和F-35为代表的高复杂性与高风险并存的大型飞机项目,虽然严格按照系统工程进行管理,却屡屡出现延迟交付和成本超支等问题,由此引发了业界的深刻反思.传统的系统工程方法只适用于过去各个组成部分可分解的结构性复杂项目,而今天的大型项目由于大量采用了软件、供应链发生了重大改变,使得由此形成的整体复杂性用传统的系统工...     

HELIO: The Heliophysics Integrated Observatory

Heliophysics is a new research field that explores the Sun–Solar System Connection; it requires the joint exploitation of solar, heliospheric, magnetospheric and ionospheric observations.     

Debris Discs Around Stars: The 2004 ISO Legacy

Debris discs around stars were first discovered by the Infrared Astronomical Satellite (IRAS) in 1983. For the first time material orbiting another star than the Sun, but distinct from a circumstellar envelope, was observed through its far infrared emission. This major discovery motivated astronomers to investigate those discs by further analyzing the IRAS data, using ground-based telescopes for the hunting of exoplanets, developing several projects using the Infrared Space Observatory (ISO), and now exploiting the ISO Data Archive (IDA). This review presents the main ISO results, statistical as well as individual, on debris discs in orbit around pre-main-sequence and main-sequence stars. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

对称性惩罚贴近度在等级划分中的应用

本文在分析了等级划分中的最大值法、贴近度分析方法的基础上,提出了一种改进型的等级划分方法;对称性惩罚贴近度方法。该方法运用对称性惩罚因子使等级划分中的信息得到比较充分的利用,最终的决策结果也更趋于合理。     

带滑移滞变系统的三阶段逐步收敛的识别方法

针对非线性带滑移滞变系统模型复杂，参数多，识别时收敛困难等问题，提出了一种三阶段逐步收敛的识别方法对Baber与Noori提出的带滑移滞变模型进行了参数识别。计算实例表明，该方法具有收敛速度快、且容易收敛的特点，对于参数较多、模型复杂的系统，是一种非常有效的参数识别方法。     

基于CSCW的分布式多媒体会议系统

CSCW是今后人们利用计算机进行工作的发展趋势，本文介绍了CSCW的背景、概念及其体系结构，重点讲述了目前技术较为完善的基于CSCW的分布式多媒体会议系统，包括其关键技术、系统结构模型以及工作流程等，进一步说明了CSCW在未来多学科领域的广阔前景。