脉冲等离子体推力器羽流预测计算研究

为了能够将脉冲等离子体推力器成功地运用于空间,需对其羽流进行研究。将一维 MHD双温放电模型的计算结果作为入口条件,运用DSMC（Direct Simulation Monte\|Carlo ）／PIC（Particle in Cell）流体混合算法一体化模拟实验室PPT羽流。验证计算显示该模 型具有一体化模拟脉冲等离子体推力器羽流的能力。对不同初始放电能量下的羽流场进行模 拟,给出了离子、中性粒子、电子温度、轴线上质量流率和出口平面返流质量流率的变化情 况。计算结果显示高放电能量下返流量更大,同时中性粒子在返流中所占比例也越大。
     

遥测伪周期时间序列子序列异常检测算法

针对现有异常检测算法用于伪周期时间序列异常序列检测时易造成误差累积,导致序列周期与特征值上显著差异的不足,文章以卫星遥测伪周期时序数据为对象,综合两种常规分段方法的优势,提出了最大周期窗宽内基于极值的模式子序列分段算法。在此基础上,给出了一种基于均序列动态生成模型的子序列异常检测方法（AnomalySubsequenceDetectionmethodbasedonOptimizedSequenceModel,ASD_OSM）,并采用2次四分位距准则（DoubleQuantilerangescriterion,2Q准则）设置距离检测门限阈值,将超出阈值的序列判定为异常序列。某航天器传感器遥测子序列异常检测试验结果表明,提出的检测方法能够有效减少漏判,提高卫星遥测伪周期数据异常序列检测的准确性。     

基于编队控制的自适应HELLO更新算法

在无人机(UAVs)编队自组织网络中,针对无人机之间位置信息更新周期不合理,从而导致编队控制不稳定和控制开销过大的问题,提出一种基于无人机编队控制的自适应HELLO更新算法。该算法应用编队控制稳定性理论推导出无人机组成期望编队的控制延时上限,结合该延时上限和编队运动状态自适应地设定HELLO更新周期。仿真结果表明,本文提出的算法与固定HELLO更新周期算法相比,既能保证在组编控制过程的稳定性,又能实时维护稳定阶段的链路,并且显著减少网络中不必要的控制开销。      

GEO编队空间机器人系统交会方法

针对地球静止轨道（GEO）上被服务航天器的远距离和非合作特点,提出一种高自主、高协同、多任务的编队空间机器人在轨服务系统方案,实现对非合作目标的自主交会接近。首先,分析GEO卫星轨道约束力小的轨道特征和非合作的信息交互特征,给出由操作空间机器人和监视空间机器人组成的编队在轨服务系统,设计交会接近相对测量分系统以及在轨服务飞行任务;接着,给出典型远距离交会接近的多视线相对导航方法与多冲量相对制导律;最后,进行远距离交会任务仿真校验,结果表明编队空间机器人交会接近方法是有效的。     

考虑气膜冷却的涡轮静叶三维优化

为研究气冷涡轮叶片设计的特点,搭建了一个可以对采用气膜冷却的气冷涡轮叶片进行全三维优化的平台,该平台可在有冷气喷射的条件下对叶片进行多目标优化.优化平台中采用11参数法对叶片进行造型.针对该造型方法和优化设计的要求对优化变量的选取和优化策略以及优化目标的设定进行了一定的探讨,采用多岛遗传算法对优化问题进行寻优.采用该平台对某航空涡轮第一级静叶进行了优化.由于对不同目标进行了加权处理,所以随着优化目标侧重点的不同,优化方案的叶型呈现出不同特点,其气动效率和冷却效果均有所改善.     

Preparation of the Biochip experiment on the EXPOSE-R2 mission outside the International Space Station

Biochips might be suited for planetary exploration. Indeed, they present great potential for the search for biomarkers – molecules that are the sign of past or present life in space – thanks to their size (miniaturized devices) and sensitivity. Their detection principle is based on the recognition of a target molecule by affinity receptors fixed on a solid surface. Consequently, one of the main concerns when developing such a system is the behavior of the biological receptors in a space environment. In this paper, we describe the preparation of an experiment planned to be part of the EXPOSE-R2 mission, which will be conducted on the EXPOSE-R facility, outside the International Space Station (ISS), in order to study the resistance of biochip models to space constraints (especially cosmic radiation and thermal cycling). This experiment overcomes the limits of ground tests which do not reproduce exactly the space parameters. Indeed, contrary to ground experiments where constraints are applied individually and in a limited time, the biochip models on the ISS will be exposed to cumulated constraints during several months. Finally, this ISS experiment is a necessary step towards planetary exploration as it will help assessing whether a biochip can be used for future exploration missions.     

Prebiotic significance of extraterrestrial ice photochemistry: detection of hydantoin in organic residues

The delivery of extraterrestrial organic materials to primitive Earth from meteorites or micrometeorites has long been postulated to be one of the origins of the prebiotic molecules involved in the subsequent apparition of life. Here, we report on experiments in which vacuum UV photo-irradiation of interstellar/circumstellar ice analogues containing H(2)O, CH(3)OH, and NH(3) led to the production of several molecules of prebiotic interest. These were recovered at room temperature in the semi-refractory, water-soluble residues after evaporation of the ice. In particular, we detected small quantities of hydantoin (2,4-imidazolidinedione), a species suspected to play an important role in the formation of poly- and oligopeptides. In addition, hydantoin is known to form under extraterrestrial, abiotic conditions, since it has been detected, along with various other derivatives, in the soluble part of organic matter of primitive carbonaceous meteorites. This result, together with other related experiments reported recently, points to the potential importance of the photochemistry of interstellar "dirty" ices in the formation of organics in Solar System materials. Such molecules could then have been delivered to the surface of primitive Earth, as well as other telluric (exo-) planets, to help trigger first prebiotic reactions with the capacity to lead to some form of primitive biomolecular activity.     

双层金属平板模拟机匣抗冲击性研究

采用LS-Dyna软件分析了双层平板模拟机匣的抗冲击性能,讨论了层间距和厚度分配对双层平板模拟机匣抗冲击性能的影响。研究结果表明：在叶片正撞击时,双层模拟机匣的损伤为局部剪切和整体塑性变形的混合型。层间距只影响外层板吸收的能量,随着层间距的变化,双层平板吸收能量没有一定规律。厚度分配比小于1时,双层板的抗冲击性能随着厚度分配比的减小而增强;厚度分配比大于1时,双层板的抗冲击性能随着厚度分配比的增大而增强。     

基于相控阵天线的大尺寸微波基板与连接器一体化精密装焊技术研究

相控阵天线集成化、小型化的发展趋势要求其收发组件具备更高系统的集成度、更小的成本及体积.收发组件中功率分配与合成网络的小型化需要微波基板电路与机壳大面积接地互联,并使用规格更小的SMP连接器,实现电气连接和信号传输.针对某型号相控阵天线收发组件,使用的尺寸为145 mm×160 mm的RO4350B微波基板和39个SMP连接器焊接至铝镀银机壳上工艺进行研究.通过分析工艺指标难点,对基板焊接、SMP连接器焊接以及组合后一体化焊接中的各难点研究并给出相应措施,解决了焊接工艺中存在的空洞率、装焊精度、温度传输等问题,成功将基板与连接器进行一体化精密焊接,使基板与SMP连接器焊接指标均满足要求,有效焊接面积均可达85％,SMP连接器孔缝表面均填满95％以上,同轴度偏差<0.05 mm,且平面度落差<0.05 mm,装配精度和质量满足型号需求.     

高速圆柱滚子轴承工作温度研究

将滚子与套圈滚道摩擦生热视为移动热源,建立了高速圆柱滚子轴承温度场计算模型;使用ANSYS的APDL语言发展了轴承工作温度分析的参数化程序,输入热流密度等边界条件,程序能够自动建模精确的分析高速圆柱滚子轴承工作温度.以一个型号轴承为例,分析了不同工况参数对轴承工作温度的影响,结果显示轴承内圈转速、径向载荷和润滑油入口油温对轴承工作温度影响显著.