一类完整性控制系统的设计及其在挠性航天器中的应用

本文利用变形Riccati方程的性质,提出一种多变量控制系统设计法。所设计的系统动态特性好,具有最优性,且在执行器失效时具有完整性。文中就挠性航天器动力学控制问题进行了应用研究。     

星载SAR性能与T／R组件不一致性的关系

本文分析了T／R组件幅相不一致性对星载SAR雷达系统性能的影响，T／R组件不一致性对星载SAR雷达天线副瓣电平有一定的影响。由于天钱的融瓣电平是不同频率信号贡献的平均值，所以天线的副瓣电平的大小依赖平均T／R组件不一致性。     

大丰模式与复合生态系统理论的应用

农村县域现代化建设是一个整体性、动态性开放系统，与社会、经济、自然三个子系统有关。该文采用复合生态系统原理，研究了大丰县生态模式发育过程、试验效果、架内结构、目标评价体系和社会调控。按其“整体、协调、再生”的原则，分析了三个子系统错综复杂的相互关联和制约关系，物质、能量、信息流动关系及其运动规律，提出一条合理配置产业、合理利用资源、保护生态环境实现农村社会持续发展的路子。旨在尽快把这项研究成果转化为生产力。     

某型无人机碳纤维尾撑钻孔组合夹具设计与应用

结合设计图样及材料特性,研究了一种用于加工碳纤维尾撑的工艺及钻孔组合夹具,并阐述了其设计要点。     

空间陀螺仪显式标定与隐式标定方法

针对航天器陀螺仪误差系数的标定问题,提出了显式与隐式两种标定方法。建立了显式标定与隐式标定方法的状态方程与测量方程,利用扩展Kalman滤波获得了陀螺仪误差系数的高精度估计,同时比较了显式标定与隐式标定的不同,仿真结果表明,在当前参数设置下,显式标定与隐式标定精度基本相同,两种方法得到的误差系数估计相对误差在10%以内,而隐式标定方法实现较为容易,但对航天器姿态测量精度较为敏感。     

Direct dark matter searches with CDMS and XENON

The cryogenic dark matter search (CDMS) and XENON experiments aim to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering on the target nuclei. The experiments use different techniques to suppress background event rates to the minimum, and at the same time, to achieve a high WIMP detection rate. The operation of cryogenic Ge and Si crystals of the CDMS-II experiment in the Soudan mine reported spectrum-weighted exposures of 34 (12) kg-d for the Ge (Si) targets after cuts, over the recoil energies 10–100 keV for a WIMP mass of 60 GeV/c². It gives an upper limit (90% C.L.) of spin-independent WIMP-nucleon cross-section at 1.6 × 10⁻⁴³ cm² for a WIMP mass of 60 GeV/c², starting to constrain predications in supersymmetry models. The two-phase xenon detector of the XENON10 experiment is currently taking data in the Gran Sasso underground lab and promising preliminary results were recently reported. Both experiments are expected to increase their WIMP sensitivity by a one order of magnitude in the scheduled science runs for 2007.     

Prospects in the orbital and rotational dynamics of the Moon with the advent of sub-centimeter lunar laser ranging

Lunar laser ranging (LLR) measurements are crucial for advanced exploration of the laws of fundamental gravitational physics and geophysics as well as for future human and robotic missions to the Moon. The corner-cube reflectors (CCR) currently on the Moon require no power and still work perfectly since their installation during the project Apollo era. Current LLR technology allows us to measure distances to the Moon with a precision approaching 1 mm. As NASA pursues the vision of taking humans back to the Moon, new, more precise laser ranging applications will be demanded, including continuous tracking from more sites on Earth, placing new CCR arrays on the Moon, and possibly installing other devices such as transponders, etc. for multiple scientific and technical purposes. Since this effort involves humans in space, then in all situations the accuracy, fidelity, and robustness of the measurements, their adequate interpretation, and any products based on them, are of utmost importance. Successful achievement of this goal strongly demands further significant improvement of the theoretical model of the orbital and rotational dynamics of the Earth–Moon system. This model should inevitably be based on the theory of general relativity, fully incorporate the relevant geophysical processes, lunar librations, tides, and should rely upon the most recent standards and recommendations of the IAU for data analysis. This paper discusses methods and problems in developing such a mathematical model. The model will take into account all the classical and relativistic effects in the orbital and rotational motion of the Moon and Earth at the sub-centimeter level. The model is supposed to be implemented as a part of the computer code underlying NASA Goddard’s orbital analysis and geophysical parameter estimation package GEODYN and the ephemeris package PMOE 2003 of the Purple Mountain Observatory. The new model will allow us to navigate a spacecraft precisely to a location on the Moon. It will also greatly improve our understanding of the structure of the lunar interior and the nature of the physical interaction at the core–mantle interface layer. The new theory and upcoming millimeter LLR will give us the means to perform one of the most precise fundamental tests of general relativity in the solar system.     

机载可编程遥测数据采集系统

介绍一种功能很强的机载可编程遥测数据采集系统。采集数据种类多 ,数量大。系统采用双微处理器方案 ,主微处理器负责整个系统的控制管理 ,从微处理器完成众多异步数据流的接收 ,通过共享存储器方式解决双 CPU之间的数据通信问题 ;应用软硬件功能模块化设计、遥测格式可编程设计及系统并行总线设计 ,简化了系统 ,提高了系统性能和系统的通用性与可扩展性 ,可广泛应用于各种飞机多种用途的飞行试验     

基于Riccati方程解的再入飞行器制导律设计

提出一种再入飞行器纵向制导律设计方法。首先对纵向运动方程沿着实际轨道线性化,然后利用线性最优调节器原理设计制导律。在每个制导周期内求解代数R iccati方程,利用其正定解构造反馈控制律,与标准轨道的控制量叠加后形成全量控制,用于实际再入轨道的制导。仿真结果表明,所设计的制导律对再入初始偏差具有较强的鲁棒性,同时它也能较好地补偿由于气动参数和大气密度摄动造成的航程误差,从而保证落点精度。