刻纹光纤用于复合材料内应变与损伤探测的可行性研究

提出了一种新颖的、采用刻纹多模光纤组成的光纤强度型应变／应力传感器，并将其埋入复合材料结构内组成传感阵列，探索了将其用于结构内应力、应变等的状态探测或损伤估计的可行性。     

Inflatable shape changing colonies assembling versatile smart space structures

Various plants have the ability to follow the sun with their flowers or leaves during the course of a day via a mechanism known as heliotropism. This mechanism is characterised by the introduction of pressure gradients between neighbouring motor cells in the plant?s stem, enabling the stem to bend. By adapting this bio-inspired mechanism to mechanical systems, a new class of smart structures can be created. The developed overall structure is made up of a number of cellular colonies, each consisting of a central pressure source surrounded by multiple cells. After launch, the cellular arrays are deployed in space and are either preassembled or alternatively are attached together during their release or afterwards. A central pressure source is provided by a high-pressure storage unit with an integrated valve, which provides ingress gas flow to the system; the gas is then routed through the system via a sequence of valve operations and cellular actuations, allowing for any desired shape to be achieved within the constraints of the deployed array geometry. This smart structure consists of a three dimensional adaptable cellular array with fluid controlling Micro Electromechanical Systems (MEMS) components enabling the structure to change its global shape. The proposed MEMS components include microvalves, pressure sensors, mechanical interconnect structures, and electrical routing. This paper will also give an overview of the system architecture and shows the feasibility and shape changing capabilities of the proposed design with multibody dynamic simulations. Example applications of this lightweight shape changing structure include concentrators, mirrors, and communications antennas that are able to dynamically change their focal point, as well as substructures for solar sails that are capable of steering through solar winds by altering the sails? subjected area.     

宽频带垂直极化天线的研究

为适应跳频通信等宽频带系统的要求 ,设计一种仙人掌式的宽频带天线。用多端口网络理论分析该天线的阻抗特性 ,阐明该天线能够实现宽频带工作的原理。利用 Ansoft公司的 HFSS仿真工具对天线进行仿真设计 ,并对天线进行了测试 ,实测结果与仿真结果相吻合。研究了地对天线性能的影响。地的直径分别为 3 0 mm、2 0 0 mm、3 0 0 mm时 ,该天线 VSWR小于 2的相对阻抗带宽超过 3 4%。地对天线辐射方向图有着显著影响 ,通过选择地的大小可以获得所需的方向图     

空时接收并行干扰消除器的性能分析及优化

提出一种新的用于DS-CDMA系统上行链路阵列接收加部分并行干扰消除的联合处理方案。在接收端多径信号的阵列处理方面,将传统的RAKE接收改为LS-DRMTA算法,能大大降低基站处理的运算量。在波束形成器之后引入干扰对消器,对传统的并行干扰消除器“硬判决”的缺陷进行优化,改为部分并行干扰消除器,可以更好地检测出期望用户信号,而且避免了消除串行干扰中存在延时问题,仿真结果表明,该联合处理方案简单有效,适合工程应用。     

构架式可展天线机构自由度分析——拆杆等效法

针对四面体构架式可展天线机构的多环耦合特性,提出了一种空间多环耦合机构的自由度分析方法——拆杆等效法。首先拆除四面体基本可展单元机构的耦合约束链,将剩余部分视为一个并联机构,然后应用螺旋理论分析各输出节点的自由度数目及性质,进而构造各输出节点与定节点之间的等效串联运动链,最后复原拆除的耦合约束链得到四面体基本可展单元的等效机构,应用修正的G-K公式计算等效机构的自由度数目,并基于反螺旋理论分析等效机构的自由度性质,从而获得四面体基本可展单元的运动特性。根据四面体基本可展单元的等效机构及其组合方式对最小组合单元及大尺寸构架式可展天线机构的结构进行了化简,并根据其几何特征约束方程推导了最小组合单元及大尺寸构架式可展天线机构的自由度。建立了由27个四面体基本可展单元组成的构架式可展天线机构的仿真模型,对该机构的自由度进行了验证,结果表明提出的拆杆等效法求得的自由度正确,为进一步分析此类天线机构的运动学和动力学奠定了基础,同时为其他类型的空间多环耦合机构的自由度分析提供了一种新的思路。     

航空航天智能材料与智能结构研究进展

智能材料作为新兴多功能材料,能够实现结构功能化、功能多样化。智能结构是在结构中集成智能材料作为传感器和驱动器,使结构除了具有承载、传力、连接等功能外,还具有自感知、自诊断、自驱动、自修复等能力,以更好地适应外界环境的变化,可显著提升航空航天架构的性能。目前智能材料与智能结构已成为航空航天架构减重增效研究的重点。根据国内外智能材料和结构的研究进展,综述了压电材料、铁磁材料、形状记忆材料、智能复合材料等智能材料的发展;讨论了智能结构的研究及应用前景,包括自诊断智能结构、自修复智能结构和减振降噪智能结构;最后,指出了智能材料与结构当前面临的一些挑战性问题,展望了其在航空航天领域的应用前景。     

一种新型双线极化BD2 B3抗干扰天线设计

设计了一种双线极化BD2B3抗干扰天线单元,采用2个幅度相等相位相差90°的馈电点,产生幅度相等相位正交的2个线极化波实现双线极化,用该天线单元进行抗干扰阵列组合,能够有效减小天线阵列的体积。     

基于频域分析的ROSAR成像算法

在现有的ROSAR(Synthetic Aperture Radar with Rotating antennas)成像算法中,基于斜距泰勒级数展开的算法存在方位向失配问题,时域相关卷积算法不能快速校正距离弯曲.频域ROSAR成像算法采用驻相点原理,直接对ROSAR回波信号进行二维频域变换,保留回波信号的频谱特征,进而构造相应的频域去耦函数和频域匹配函数,实现频域距离弯曲校正和目标场景重构.仿真结果表明,该算法能够快速校正距离弯曲及有效克服方位向失配问题.     

卫星天线双轴定位机构建模与仿真

卫星天线定位机构对控制天线的运动精确具有重要的意义。本文介绍了卫星点波束天线双轴定位机构的基本组成,建立了刚体动力学模型、仿真模型,并开发了仿真软件,对系统进行了仿真。     

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.