Optimal network topology of relative navigation and communication for navigation sharing in fractionated spacecraft cluster

Navigation sharing as a key technology provides orbit and attitude information broadcasting for the whole fractionated spacecraft cluster (FSC). The navigation sharing concept has already been proposed for some years. However, the problem of achieving the optimal navigation sharing by designing the proper network topology is still unsolved, especially in the case that some members of the cluster have absolute navigation devices, some just have relative navigation devices and some only have communication devices. In this paper, a comprehensive model of describing the navigation sharing problem in FSC is proposed. The model of network topology constructing by relative navigation links and communication links is established. By using the graph theory and genetic algorithm as the tool, the conditions for navigation sharing in FSC with different sharing degrees are obtained. Finally, some examples are presented to test the methods, and it has been found that, the absolute positions and attitudes of all the members can still be determined even some members in FSC have no absolute navigation devices.     

Indicators of black-hole mass and Eddington accretion ratio from QSO X-ray and UV spectra

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra.     

一种用于光传飞控系统的光纤温度传感器研究

利用半导体光吸收原理，设计出一种光纤温度传感器，它可实现强电磁干扰下高空无人机内的环境温度测量，具有体积小，结构简单的特点。该测试仪用GaAs晶片作为温度敏感元件，采用透射式结构，利用双光束补偿原理消除了光路扰动产生的误差。实验结果表明该传感器在-20-85℃的范围内有良好的温度响应。     

夜气辉对天基光学碎片探测的影响分析

设计并完成了夜气辉背景下的天基碎片观测试验，获取了综合谱段的观测数据。基于观测数据进行夜气辉的辐射特性及其对天基碎片探测的影响分析。结果表明，夜气辉辐射随纬度和高度呈现一定的分布特点，这些特点均符合夜气辉的理论分布规律。在约90 km处辐射最强，亮度可达到单位积分时间每平方角秒近15星等，这对恒星及碎片提取概率影响较大，其中，13等星的提取概率仅为40.5%。     

Multiscale eigenelement method for periodical composites: A review

Based on the eigenvector expansion idea, the Multiscale Eigenelement Method (MEM) was proposed by the author and co-workers. MEM satisfies two equivalent conditions, one condition is the equivalence of strain energy, and the other is the deformation similarity. These two equivalent conditions character the structure-preserving property of a multiscale analysis method. The equivalence of strain energy is necessary for achieving accurate macro behaviors such as lower order frequencies, while the deformation similarity is essential for predicting accurate micro behaviors such as stresses. The MEM has become a powerful multiscale method for the analysis of composite structures because of its high accuracy and efficiency. In this paper, the research advances of MEM are reviewed and all types of eigenelement methods are compared, focusing on superiorities and deficiencies from practical viewpoint. It is concluded that the eigenelement methods with smooth shape functions are more suitable for the analysis of macro behaviors such as lower order frequencies, and the eigenelement methods with piecewise shape functions are suitable for the analysis of both macro and micro behaviors.     

机载系统NANDFlash存储技术

为了发挥NANDFlash在机载环境中非易失性、体积小、固态性、重量轻、低功耗、抗震动等特点,介绍了NANDFlash的存储特性,对NANDFlash存储的关键技术进行了改进,提出了基于域机制的地址映射方式和基于阈值的损耗均衡方法,为机载系统能够更加可靠、实时和安全地进行数据存储提供了选择。     

第3代新型低碳高合金钢弧齿锥齿轮失效分析

在中央传动调试试验中发生主动弧齿锥齿轮轮齿断裂故障,并连带其他部件产生不同程度损伤。主动弧齿锥齿轮整个圆周的接触印痕偏向小端一侧、靠近齿底,从动弧齿锥齿轮接触印痕分布在小端齿顶部位,印痕已不完整、局部超出工作面。为了排除15Cr₁₄Co₁₂Mo₅Ni₂钢弧齿锥齿轮试验中发生的断裂故障,对齿轮进行宏观检查、断口分析、组织检查、硬度测试、成分分析、啮合印痕仿真分析与验证,确定了故障齿轮断裂的性质和产生原因。结果表明：主动弧齿锥齿轮为高周疲劳断裂,疲劳起源于小端面与齿凸面根部转接棱角部位,与材质与冶金缺陷无关;在工作过程中存在异常咬合是导致该齿轮产生早期疲劳开裂的主要原因。建议优化齿面加工参数,提高齿轮工作过程中的咬合质量,从而避免此类故障再次发生。     

不同流速比超声速混合层气动光学效应研究

针对不同流速比混合层流场气动光学效应问题,首先采用大涡模拟数值方法进行了数值仿真,其次用光线追迹方法进行了气动光学效应仿真,最后对混合层的气动光学效应进行了评价。结果表明,混合层流场涡结构与光程差极小值存在一一对应关系,并且其流速比低的混合层气动光学效应更加严重。同时,研究了不同光学参数对斯特列尔比的影响,得到了相应的规律。     

单颗磨粒磨削仿真研究进展

概述了传统磨削仿真的基本方法及发展过程,总结了磨粒模型和工件模型的研究现状,具体分析了有限元法、光滑流体粒子动力学法、分子动力学法以及综合仿真方法等应用于单颗磨粒磨削材料的去除机理、成屑机理、工件表面质量以及磨粒磨损等仿真中的研究现状,最后阐述了各类仿真方法的局限性,并提出了单颗磨粒磨削仿真进一步的发展前景。     

一种带有过渡因子的下压指令设计方法

针对高超声速飞行器由滑翔段转入下压段的过程中运动状态无法快速与制导律进行匹配,从而引起弹道震荡的问题,设计了一种带有过渡因子的下压指令,改善了飞行器的过渡品质。首先,分析了高超声速飞行器平衡滑翔弹道,提出了平滑过渡的基本条件,并引入了一次函数、多项式、正弦、指数形式的过渡因子;然后,设计了3种带有过渡因子的下压指令;最后,通过仿真验证了下压指令的合理性。结果表明,该算法设计出的下压指令计算量小、制导精度高,且具有一定工程应用价值。