一种基于实体模型的三轴数控加工刀轨生成算法

实体模型是几何造型的高级模型，它具有完整的曲面拓扑关系，国内基本实体模型的数摈加工算法的需求日渐迫切，本文提出了一种适合实体模型的三轴数控加工刀位轨迹生成算法；首先根据加工行距作一组平行于刀轴的平面，与模型的待加工表面求交，得到一系列交线，再根据加工步长规划另一组与上述平面垂直且平行于刀轴的平面，与上述交线求交，得到一交点网格，判断刀具与数据点的位置关系从而得到刀位轨迹。     

一种新的射频仿真目标位置控制方法与软件研究

针对射频目标仿真系统中目标位置的控制，本文通过对国内外目标位置控制的常用方法进行研究，提出一种新的通用目标位置控制方法，该方法适用于任何天线分布的面阵。利用这种新的方法编写了基于三元阵天线阵面的射频仿真目标位置控制软件，实现对多目标在天线阵面上多种轨迹运动下的高速准确的定位，并能实时监视目标的运动状态和运动轨迹。     

惩罚函数法在发动机性能计算中的应用

按照涡喷发动机工作时遵守的气动热力学定律，建立了发动机的稳定数学模型，并针对双轴涡轮发动机性能计算的非线性数学模型，利用优化和最优控制理论中的惩罚函数法，对发动机性能进行了基于约束的最优求解程序设计，利用程序对某型发动机的稳定飞行特性进行了计算，计算结果表明，使用惩罚函数法求出的特性曲线变化规律正确，发动机平衡方程的解的精度更高，在此基础上得出的发动机飞行特性也更准确。另外惩罚函数法对初值的要求很低，迭代运算不易发散。     

基于LabVIEW平台的数字抽取滤波器的设计与应用

介绍了基于LabVIEW平台的数字抽取滤波器的设计。该方法是对高采样率的数据进行低通数字滤波，然后对结果用1／K倍重新采样，将数字信号频带压缩K倍，从而实现动态测试较大的动态范围要求和划分频带要求，数字抽取滤波器的设计包含调制，数字滤波和抽取三方面，LabVIEW是一种基于图形编程语言（G语言）的开发环境，采用交互界面设计，模块化编程，该滤波器也是作者正在研制的动态测试分析虚拟仪器的一个重要组成部分。本文给出了在LabVIEW平台上所进行数字抽取滤波器的设计原理，仿真结果和在动态数字信号分析中的应用。     

星光折射航天器自主定轨方案比较

当星光透射大气发生折射时 ,用星光折射角精确地反映星光在大气中离地球表面的高度 ,并建立高度、航天器与地球的几何关系。通过对折射角进行观测 ,间接测得地平 ,从而改善了用地平仪直接测地平所造成的航天器自主导航精度低的不足。本文提出了几种利用星光折射的航天器自主定轨方案 ,并作了细致的仿真实验 ,对直接和间接两种测量地平方法以及几种星光折射自主定轨方案进行了分析比较。     

Ariane transfer vehicle in service of man in orbit

The Ariane transfer vehicle (ATV), an Ariane 5 borne, unmanned propulsion vehicle, is designed to transport the logistics needed to resupply the International Space Station (ISS) and the man tended free flyer (MTFF) step 2 with pressurized and unpressurized cargo and to dispose the waste. The ATV is an expendable vehicle and is disposed of by a safe atmospheric burn up. In accordance with the AR5 schedule it should be operational in 1996 for missions toward ISS and beyond the year 2000 for MTFF 2 missions. The main constituents of the proposed ATV are the modified AR5 third stage L5, an upgraded VEB steering the launcher as well as the ATV and the P/L-adaptor providing mechanical and umbilical links to the payload. The mechanical part of the RVD-kit will be placed on the payload-module, the main RVD sensors are located on the adaptor and the needed computer intelligence will be integrated on the VEB. To minimize the development, and recurring costs, the ATV concept fully complies to the idea of maximum use of existing hardware and software, mainly from the AR5, Hermes and Columbus programs thus minimizing development and recurring costs. The ATV is compatible to ISS, MTFF and OMV and is able to transport logistic modules compatible with NSTS and U.S.-expendable launchers.     

复合材料(结构)粘接质量检测的错位散斑技术

系统地分析了错位散斑条纹的形成机制,并在多种条件(真空荷载、热流荷载、音频扫描荷载等)下对各种复合材料结构粘接质量进行了检测及评估,可检测出厚1mm层合板内直径>5mm的缺陷,夹芯结构内直径>10mm的缺陷;对于包覆层结构可检测出深度在12mm以内、直径>5mm的空隙脱粘缺陷,而零粘接力缺陷也能检测出厚度为2mm、直径>30mm的缺陷。同时引入相移技术使错位散斑检测方法不仅具备非接触、高精度和全场实时观测等特点,而且也实现了复合材料结构粘接质量的定量无损检测。     

结构局部刚度变化对小卫星动特性影响

首先针对模块式小卫星动特性进行灵敏度理论分析，分析目标是寻找提高结构动特性的局部位置和参数。然后基于有限元法分析改变局部刚度对结构动特性的影响。小卫星结构动特性分析计算的主要问题是建立计算成本可控的有限元模型，本文详细讨论了小卫星有限元模型建模方法和简化途径，并通过7个算例考察改变模块底板局部刚度、改变适配器支撑刚度、模块问设置弹簧模拟阻尼器等对小卫星结构动特性的影响。灵敏度分析和计算表明，影响动特性的主要因素是模块盒底板刚度和星箭适配器的支撑刚度；增加模块局部刚度以及适配器支撑刚度可以屏蔽星体摆动和包带联结部位的某些频率，同时可以减缓部分中间模块的振幅；在部分模块间设置弹簧可以模拟阻尼器或减振器的效果。另一方面，降低适配器刚度可以增加隔振作用。因而优化模块刚度分布和支撑刚度分布是改进动力学性能的有效途径。本文分析为模块式小卫星动力学修改以及多功能结构设计和主动振动设计提供依据。     

航天飞行器防热部件烧蚀行为的数值模拟

对航天飞行器防热部件在氧－煤油发动机火焰喷吹下的烧蚀行为进行了有限元数值模拟。利用“杀死”单元的方法建立防热部件瞬态温度场的有限元模型，实现了烧蚀边界的退缩，从而完成了对烧蚀尺寸变化的定量描述。烧蚀开始于4．59s，到12s时线烧蚀量为1．47mm。计算结果与试验的实测结果一致。     

LISA — a study of the ESA cornerstone mission for observing gravitational waves

The primary objective of the Laser Interferometer Space Antenna (LISA) mission is to detect and observe gravitational waves from massive black holes and galactic binaries in the frequency range 10⁻⁴ to 10⁻¹ Hz. This low-frequency range is inaccessible to ground-based interferometers because of the unshieldable background of local gravitational noise and because ground-based interferometers are limited in length to a few km. LISA is an ESA cornerstone mission and recently had a system study (Ref. 1) carried out by a consortium led by Astrium, which confirmed the basic configuration for the payload with only minor changes, and provided detailed concepts for the spacecraft and mission design. The study confirmed the need for a drag-free technology demonstration mission to develop the inertial sensors for LISA, before embarking on the build of the flight sensors. With a technology demonstration flight in 2005, it would be possible to carry out LISA as a joint ESA-NASA mission with a launch by 2010 subject to the funding programmatics. The baseline for LISA is three disc-like spacecraft each of which consist of a science module which carries the laser interferometer payload (two in each science module) and a propulsion module containing an ion drive and the hydrazine thrusters of the AOCS. The propulsion module is used for the transfer from earth escape trajectory provided by the Delta II launch to the operational orbit. Once there the propulsion module is jettisoned to reduce disturbances on the payload. Detailed analysis of thermal and gravitational disturbances, a model of the drag-free control and of the interferometer operation confirm that the strain sensitivity of the interferometer will be achieved.