大面积覆铜多层印制板通孔焊接温度场仿真

为了提高型号产品中连接大面积覆铜的通孔元器件焊点的过锡率,进而提高焊点的可靠性,本文建立了四层大面积覆铜通孔焊焊接三维模型,研究添加温度补偿后的四层覆铜的印制板通孔焊接过程中的温度场分布,得出焊接温度对过锡率的影响规律。发现焊接温度350 ℃时通孔过锡量达到100%,这与实际焊接所有焊点过锡量均达到100%的结果一致。有限元温度仿真结果与热电偶测温结果吻合较好,表明该模型可以准确地模拟焊接过程中温度演化,可为大面积覆铜通孔焊点的手工焊接过程和焊接参数优化提供理论指导。     

不同增长机制下航空网络自愈特性

结合复杂网络理论,从能量的角度分析了航空网络的功能自愈机理,并研究了航空网络在不同增长机制下的自愈特性。首先,将网络结构划分为自愈结构与耦合结构,并针对航空网络3种增长机制进行了分析和抽象建模;然后,从网络全局角度出发研究了美国航空网络在遭受蓄意攻击造成全网功能瘫痪的情况下,网络功能的恢复鲁棒性和网络增长对网络自愈能力的影响。研究表明,美国航空网络具有较好的恢复鲁棒性,接近80%的机场在受到能量冲击造成的短暂失效后具有功能自愈能力。航空网络不同的增长机制对网络的自愈能力有着不同的影响。结果证实,为完善航空网络而建立的机场群,由于其较大的连接需求,加大了网络区域密度,复杂了网络拓扑结构,降低了网络的自愈能力;而小型机场的增加不会影响网络整体的自愈能力。      

Applications of tuned mass dampers to improve performance of large space mirrors

In order for future imaging spacecraft to meet higher resolution imaging capability, it will be necessary to build large space telescopes with primary mirror diameters that range from 10 m to 20 m and do so with nanometer surface accuracy. Due to launch vehicle mass and volume constraints, these mirrors have to be deployable and lightweight, such as segmented mirrors using active optics to correct mirror surfaces with closed loop control. As a part of this work, system identification tests revealed that dynamic disturbances inherent in a laboratory environment are significant enough to degrade the optical performance of the telescope. Research was performed at the Naval Postgraduate School to identify the vibration modes most affecting the optical performance and evaluate different techniques to increase damping of those modes. Based on this work, tuned mass dampers (TMDs) were selected because of their simplicity in implementation and effectiveness in targeting specific modes. The selected damping mechanism was an eddy current damper where the damping and frequency of the damper could be easily changed. System identification of segments was performed to derive TMD specifications. Several configurations of the damper were evaluated, including the number and placement of TMDs, damping constant, and targeted structural modes. The final configuration consisted of two dampers located at the edge of each segment and resulted in 80% reduction in vibrations. The WFE for the system without dampers was 1.5 waves, with one TMD the WFE was 0.9 waves, and with two TMDs the WFE was 0.25 waves. This paper provides details of some of the work done in this area and includes theoretical predictions for optimum damping which were experimentally verified on a large aperture segmented system.     

Effects of uncertainties and flexible dynamic contributions on the control of a spacecraft full-coupled model

One of the most important problems for performing a good design of the spacecraft attitude control law is connected to its robustness when some uncertainty parameters are present on the inertial and/or on the elastic characteristics of a satellite. These uncertainties are generally intrinsic on the modeling of complex structures and in the case of large flexible structures they can be also attributed to secondary effects associated to the elasticity. One of the most interesting issues in modeling large flexible space structures is associated to the evaluation of the inertia tensor which in general depends not only on the geometric ‘fixed’ characteristic of the satellite but also on its elastic displacements which of course in turn modify the ‘shape’ of the satellite. Usually these terms can be considered of a second order of magnitude if compared with the ones associated to the rigid part of a structure. However the increasing demand on the dimension of satellites due to the presence for instance of very large solar arrays (necessary to generate power) and/or large antennas has the necessity to investigate their effects on their global dynamic behavior in more details as a consequence. In the present paper a methodology based on classical Lagrangian approach coupled with a standard Finite Element tool has been used to derive the full dynamic equations of an orbiting flexible satellite under the actions of gravity, gravity gradient forces and attitude control. A particular attention has been paid to the study of the effects of flexibility on the inertial terms of the spacecraft which, as well known, influence its attitude dynamic behavior. Furthermore the effects of the attitude control authority and its robustness to the uncertainties on inertial and elastic parameters has been investigated and discussed.     

某大型低温运载火箭无人值守加注发射技术研究

针对提升和保障航天发射人员安全问题,提出了低温运载火箭无人值守加注发射(CLVUFL)的理念和内涵.通过国内外代表性CLVUFL的技术对比,发现国内低温火箭加注发射应用CLVUFL技术存在箭地接口复杂、加注发射时间较长、关键设备可靠性有待提高、智能化自动化程度不高等主要问题.针对某大型低温运载火箭加注发射流程,通过分析...     

运载火箭大容量CPCI集成数据采集与测试系统设计

介绍了一种用于运载火箭测试的CPCI数据采集系统设计方案,该测试系统针对某运载火箭测试需求,从顶层设计出发,以龙芯2F处理器为基础平台,对测试系统组成构架、硬件平台设计和软件系统设计等各个层面进行了优化设计,该系统实现了高流量、高速度的多种信号连续采集处理和发送,测试系统具有体积小、集成度高、可扩展和便于维修的特点.     

大飞机发动机自主研制影响因素分析

研制拥有自主知识产权的大飞机是国家的既定战略,发动机是大飞机的心脏,发动机的自主研制关系到具有自主知识产权大飞机的实现。通过对飞机企业、发动机企业的调查和相关文献的搜集,找出大飞机发动机自主研制的影响因素,利用解释结构模型法建立发动机自主研制影响因素的解释结构模型,再利用层次分析法计算出各个影响因素的权重,在此基础上分析了各因素的重要作用,并提出了提高这些制约因素的对策。     

采用信标的大型可展开天线指向控制方法

为提高大型可展开天线的指向控制精度,并适应喷气卸载等在轨工况,基于Craig-Bampton法建立了表征柔性天线指向的动力学模型,在此基础上提出了一种采用信标的大天线指向控制方法.该方法先基于卡尔曼滤波,对大天线的振动状态进行检测,若天线未出现明显振动,则通过信标敏感器修正天线指向偏差,同时引入星本体姿态敏感器以保证稳定性;若天线振动超过阈值,则仅引入星本体敏感器以衰减振动,直至天线未出现明显振动.最后利用瑟拉亚(Thuraya)卫星的在轨实测热变形数据进行了仿真验证.结果表明,在未受到喷气扰动时,大天线指向精度优于±0.02°,在受到喷气扰动后,系统可正确检测并切换跟踪输入.这说明,该指向控制方法在保证稳定性的同时,可以有效修正大天线指向偏差,并能适应在轨位保、卸载喷气工况.     

大挠性空间桁架结构的动力学建模与仿真研究

对航天器结构中常用的一字型空间桁架,基于建立的普通式和拉索式空间桁架结构简化模型,用有限元法建立空间桁架结构模型,分别对两种空间桁架结构的模态特性、谐响应和瞬时激励响应等动力学特性进行了仿真研究,分析了拉索式空间桁架结构的弦张力对桁架结构振动特性的影响。研究较好地模拟了大挠性空间桁架结构的动力学特性及其在外太空的真实工况,有一定的参考意义。