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。     

Re对Ni3Al屈服强度及断裂强度影响的第一原理研究

为了满足航空发动机热端部件材料力学性能的不断提高,应用基于密度泛函理论的第一原理方法,研究了Re对Ni_3Al金属间化合物力学强度的影响。通过建立掺杂Re前后Ni_3Al的滑移模型和断裂模型,计算了晶胞的不稳定堆垛层错能γ_(US)和断裂能γ_C,进而判断Re对Ni_3Al屈服强度和断裂强度的影响。另外根据经验判据,γ_C/γ_(US)值可表征材料的韧脆性。计算结果表明,Re的掺杂增大了Ni_3Al [11■](111)和[1■0](111)两个滑移系下的γ_(US),使得滑移系不易开动,不易使Ni_3Al发生塑性变形,增大了Ni_3Al的屈服强度。Re增大了Ni_3Al在密排面处的断裂能,使得其不易在密排面发生断裂,增大了断裂强度。关于改善Ni_3Al的韧性,Re的掺杂对于密排面上不同滑移方向的影响具有一定的差别。此研究工作可为改善航空发动机单晶叶片的力学性能提供理论基础。     

升降平台跌落对起落架过载的影响

建立了升降平台跌落时起落架动力学模型,给出了描述缓冲支柱和轮胎力性能的数学公式,使之适用于起落架严重受载的情况;通过数值仿真研究了升降平台跌落时的直升机起落架过载。分析了升降平台跌落时起落架产生大过载的力学机理。升降平台从不同高度自由跌落时,机轮系留引起的起落架正过载相对增加量不超过10%,而系留情况下起落架回弹行程中的负过载比压缩行程中的正过载高得多。     

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.     

空气压强对激光推进器冲量耦合系数影响

设计并加工了激光推进器实验模型,以空气为推进工质,利用脉冲式CO2激光器,研究了空气压强对激光推进器冲量耦合系数影响。实验结果表明,空气压强对激光推进器性能有显著影响。在文中实验条件下,当空气压强大于6 kPa时,激光推进器冲量耦合系数随压强减小而减少较慢;当空气压强小于6 kPa时,激光推进器冲量耦合系数随压强减小而减少很快。     

超燃冲压发动机燃烧室亚/超燃模态数值研究

采用Mac Cormack格式、B-L湍流模型及氢/空气两步化学反应模型,计算了双模态冲压发动机燃烧室在不同来流条件和供油规律下的二维燃烧流场。计算结果表明,在相同来流条件下,供油规律对燃烧室的工作模态有着重大影响;在不同来流条件下,可通过调节供油规律,使燃烧室分别实现亚燃模态和超燃模态。     

水反应金属燃料发动机的性能调节

在水反应金属燃料发动机性能分析研究基础上,分析了壅塞式和非壅塞式发动机构型优缺点及性能调节特性,着重探讨了非壅塞式水反应金属燃料发动机燃气流量自适应调节规律和特点。计算结果分析表明,非壅塞式发动机具有水燃比自适应调节特性,且高压强指数水反应金属燃料调节效果显著。     

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.