无人机编队飞行技术的研究现状与展望

无人机编队飞行是无人机及其应用技术发展研究的新热点.在分析无人机编队飞行特点的基础上,阐述了无人机编队飞行原理与方法的研究现状,并展望了其今后的主要应用前景.     

Walker星座星间链路构建准则及优化设计研究

首先通过分析Walker星座空间结构,得到星座星间链路基本几何关系;其次研究了卫星之间的相对运动规律和星座几何构型,确定了能够反映空间几何特性的Walker星座星间链路设计的基本准则,得到了星座全连通性数学解析判据,并根据星座一体化设计中的层次约束准则思想,给出了星间链路分析设计流程;最后,针对几个考虑星间链路的Walker星座的一体化优化设计问题,给出了分析设计实例。     

Formation and Composition of Planetesimals

The composition of planetesimals depends upon the epoch and the location of their formation in the solar nebula. Meteorites produced in the hot inner nebula contain refractory compounds. Volatiles were present in icy planetesimals and cometesimals produced in the cold outer nebula. However, the mechanism responsible for their trapping is still controversial. We argue for a general scenario valid in all regions of the turbulent nebula where water condensed as a crystalline ice (Hersant et al., 2004). Volatiles were trapped in the form of clathrate hydrates in the continuously cooling nebula. The epoch of clathration of a given species depends upon the temperature and the pressure required for the stability of the clathrate hydrate. The efficiency of the mechanism depends upon the local amount of ice available. This scenario is the only one so far which proposes a quantitative interpretation of the non detection of N₂ in several comets of the Oort cloud (Iro et al., 2003). It may explain the large variation of the CO abundance observed in comets and predicts an Ar/O ratio much less than the upper limit of 0.1 times the solar ratio estimated on C/2001 A2 (Weaver et al., 2002). Under the assumption that the amount of water ice present at 5 AU was higher than the value corresponding to the solar O/H ratio by a factor 2.2 at least, the clathration scenario reproduces the quasi uniform enrichment with respect to solar of the Ar, Kr, Xe, C, N and S elements measured in Jupiter by the Galileo probe. The interpretation of the non-uniform enrichment in C, N and S in Saturn requires that ice was less abundant at 10 AU than at 5 AU so that CO and N₂ were not clathrated in the feeding zone of the planet while CH₄, NH₃ and H₂S were. As a result, the 14N/15N ratio in Saturn should be intermediate between that in Jupiter and the terrestrial ratio. Ar and Kr should be solar while Xe should be enriched by a factor 17. The enrichments in C, N and S in Uranus and Neptune suggest that available ice was able to form clathrates of CH₄, CO and the NH₃ hydrate, but not the clathrate of N₂. The enrichment of oxygen by a factor 440 in Neptune inferred by Lodders and Fegley (1994) from the detection of CO in the troposphere of the planet is higher by at least a factor 2.5 than the lower limit of O/H required for the clathration of CO and CH4 and for the hydration of NH₃. If CO detected by Encrenaz et al. (2004) in Uranus originates from the interior of the planet, the O/H ratio in the envelope must be around of order of 260 times the solar ratio, then also consistent with the trapping of detected volatiles by clathration. It is predicted that Ar and Kr are solar in the two planets while Xe would be enriched by a factor 30 to 70. Observational tests of the validity of the clathration scenario are proposed.     

原位钛基复合材料中TiB的生成热力学及动力学

采用自蔓延高温合成（SHS）、感应熔炼和熔模精铸相结合的方法，利用Ti—B—Al体系制备出了原位自生TiB增强的钛基复合材料。借助XRD、SEM和TEM分析了复合材料的物相和增强体的形态。结果表明：在复合材料中只存在TiB增强体和Ti，无TiAl3杂质相形成，TiB增强体呈柱状短纤维，这与其B27晶体结构有关，且增强体／基体界面清洁无杂质污染，并从热力学和动力学两方面论述了在Ti—B—Al体系中制备TiB增强体的生成机制：在Ti-B—Al体系中，Al首先受热熔化使得Ti和B相继溶解于Al液中；Ti与Al之间先行发生化学反应形成Ti—Al金属间化合物，放出的热量进一步引发了溶解于液相中的B和Ti产生高温自蔓延形成Ti—B化合物。以热力学理论分析，应最终形成TiB2，但实际上由于动力学影响，最终形成了TiB。     

L10-TiAl金属间化合物Mn,Nb合金化电子结构的计算

采用第一原理赝势平面波方法计算了L10型TiAl金属间化合物中掺入Mn,Nb后的电子结构和价键结构.通过合金原子形成热得出Mn优先占据Al点阵位置,Nb优先占据Ti点阵位置.Mulliken聚居数分析发现Mn或Nb合金化后,分别降低了(001)和(002)面内的原子间键合强度,掺入Nb还降低了层间的原子间键合强度,而掺入Mn,则使层间原子间键合强度增加.整体上来讲,掺入Mn有利于改善TiAl的室温脆性,而掺入Nb,不利于改善TiAl的室温脆性.     

PPT小卫星轨道转移任务分析

针对CAST968小卫星平台,结合HY-1卫星,分析了该卫星轨道转移任务的应用需求;对比HY-1卫星采用的单组元肼推力器,指出了脉冲等离子体推力器（Pulsed Plasma Thruster,PPT）的应用特点;根据该卫星平台的外形和结构参数,对星上轨道转移PPT的数量和工作方式进行了初步设计;基于PPT的研究现状和推进能力,对PPT的轨道转移方案进行了论证分析,计算了相关的轨道转移参数。研究表明,PPT可以适用于微小卫星小能量轨道转移任务,与传统的化学轨道转移推进系统相比,优势较明显。     

基于自适应连续蚁群算法的卫星星座设计(英文)

蚁群算法是一种解决多变量问题的新型启发式仿生算法。本文分析了卫星对地面的覆盖条件,提出用——/(n 1)重覆盖率来评价星座的覆盖性能,建立了以覆盖性能为目标函数的卫星星座参数优化模型。采用蚁群算法对卫星星座参数进行优化,为星座优化问题提供了一种新方法。在连续蚁群算法的基础上对算法进行改进,提出蚂蚁种群数量的自适应准则,有效的提高了搜索范围与收敛速度。通过仿真表明,与其他方法相比,蚁群算法在星座参数优化有着明显的效率。     

考虑执行机构误差的编队卫星姿态分布式时延滑模自适应协同控制

针对编队卫星姿态协同控制问题,在考虑到执行机构误差的前提下,提出一种将时延控制与滑模自适应控制相结合的鲁棒控制方法.该方法通过引入自适应更新律实现对执行机构小角度安装误差的在线估计,同时通过滑模控制完成对外界干扰和执行机构随机幅值误差等随机扰动的抑制.由于引入了时延环节,只需对上一时刻控制力矩进行单位时延,达到大大简化...     

过驱动轮控卫星的动态控制分配方法

反作用飞轮在卫星姿态控制中具有重要作用,配置3个以上飞轮的卫星构成一类过驱动系统,能够提高姿态控制系统的可靠性.针对期望控制力矩到冗余飞轮的指令分配问题,提出了一种基于伪逆法的动态控制分配方法,并针对传统伪逆法难以考虑飞轮最大力矩等物理约束问题,采用零空间方法对传统伪逆法给出的分配结果进行了修正.基于稳定控制模式下姿态...     

基于模糊专家系统的编队防空辅助决策系统

应用模糊推理理论的思想和方法设计和实现了编队防空辅助决策专家系统.文章详细介绍了系统的基本结构、知识表示和推理机制.系统采用模糊关系矩阵和基于框架的模糊推理相结合的推理方法,具有较高的准确性.最后给出了一个应用实例.