均布压力作用各向异性矩形薄板大挠度问题

基于冯·卡门模型，选择中心挠度为摄动参数，利用摄动方法将正交异性矩形薄板大挠问题的非线性偏微分方程组逐级线性化，导出了各级摄动对应的几个线性偏微分方程组，然后再借助变分法求解，得到了均布载荷作用下正交异性矩形薄板的载荷-挠度曲线。     

干式变压器数据采集与控制系统的设计

介绍了一种基于V/F变换的高精度干式变压器数据采集与控制系统 ,采用LM2 3 1A/F变换芯片和89C5 2单片机实现工业现场测量对象的A/D转换。V/F变换器具有高精度 ,高线形度 ,且外围电路简单的特点。采用单片机直接与V/F变换器连接进行A/D转换 ,不需要额外的硬件电路 ,充分利用硬件资源 ,精心设计软件 ,系统分辨率可达 12位 ,转换精度可达 0 .0 2 %。当传感器与上位机距离较远时 ,可以采用RS -4 85接口或无线数据发送 /接收模块实现远距离的数据通信     

尾支杆干扰非线性修正方法的初步研究

利用CFD方法 ,采用两套网格重叠的形式 ,研究了一种对尾支杆干扰进行修正的非线性方法。运用本方法 ,研究了尾支杆等直段长度、直径和锥角对模型气动特性的影响 ,研究了四个模型有攻角时的尾支杆干扰 ,并对GBM 0 4A模型的零阻进行了尾支杆干扰的修正。     

GDBMS中图形数据的表示与存贮

GDBMS是作者设计并实现的一个实验性的工程图形数据库管理系统。它基于扩充关系数据模型,成功地完成了对工程图形数据的描述。 本文从图形的数据库表示出发,对几何实体的建模方法进行了分析,介绍了GDBMS中的图形数据模型及其实现方法。该数据模型吸取图元枚举法(PI方法),结构实体几何表示法(CSG法)和边界表示法(BR方法)的优点,在进行交互式图形编辑以及图形显示时,采用CSG结构,在数据库的存贮和处理时,采用扩充的BR方法。     

大客车局部优化造型对其使用性能的影响

随着车速的提高,汽车在行驶中受到的空气阻力便成为不可忽视的问题,因此与减阻节能相关的汽车优化造型也就显得越来越重要了。由于运动物体所受到的空气阻力系数的大小主要取决于它的头部的形状,因而我们对厢式大客车驾驶室前风窗区的几种不同造型在低速风洞中进行了测力的实验研究。实验结果表明,驾驶室前围不同形式的过渡是影响厢式客车空气阻力的重要因素。其中在适当的风窗倾角下,经过良好的圆化处理后,可使厢式大客车的空气阻力减小27%左右。这不仅节省了燃料的消耗,还可以提高汽车的最大行驶速度,改善其加速和爬坡能力。     

水上飞机自由飞模型起飞与降落性能的综合试验

本文综述了用4台发动机为动力的水上飞机自由飞模型起飞与降落性能的综合试验,这些性能包括稳定性、操纵性、飞溅、水阻力、着水撞击、起飞砰击、失速及耐波性等。模型与真实飞机保持几何、质量、运动状态、拉力、升降舵效率及其波浪谱的相似,故模型试验与真实飞机的试飞结果比较符合。同时着重介绍了模型试验的机载测试系统与地面测试系统。     

航天雷达高度表

介绍几种航天雷达高度表，其中包括弹载雷达高度表、“土星”雷达高度表和“天空实验室”雷达高度表，最后介绍一种卫星雷达高度表的设计方法。     

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。     

Remote sensing of planetary properties and biosignatures on extrasolar terrestrial planets

The major goals of NASA's Terrestrial Planet Finder (TPF) and the European Space Agency's Darwin missions are to detect terrestrial-sized extrasolar planets directly and to seek spectroscopic evidence of habitable conditions and life. Here we recommend wavelength ranges and spectral features for these missions. We assess known spectroscopic molecular band features of Earth, Venus, and Mars in the context of putative extrasolar analogs. The preferred wavelength ranges are 7-25 microns in the mid-IR and 0.5 to approximately 1.1 microns in the visible to near-IR. Detection of O2 or its photolytic product O3 merits highest priority. Liquid H2O is not a bioindicator, but it is considered essential to life. Substantial CO2 indicates an atmosphere and oxidation state typical of a terrestrial planet. Abundant CH4 might require a biological source, yet abundant CH4 also can arise from a crust and upper mantle more reduced than that of Earth. The range of characteristics of extrasolar rocky planets might far exceed that of the Solar System. Planetary size and mass are very important indicators of habitability and can be estimated in the mid-IR and potentially also in the visible to near-IR. Additional spectroscopic features merit study, for example, features created by other biosignature compounds in the atmosphere or on the surface and features due to Rayleigh scattering. In summary, we find that both the mid-IR and the visible to near-IR wavelength ranges offer valuable information regarding biosignatures and planetary properties; therefore both merit serious scientific consideration for TPF and Darwin.     

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.