Understanding Galaxy Formation with ISO Deep Surveys

We present the results obtained through the various ISO extragalactic deep surveys. Although IRAS revealed the existence of galaxies forming stars at a rate of a few tens (LIRGs) or even hundreds (ULIRGs) solar masses in the local universe, ISO not only discovered that these galaxies were already in place at redshift one, but also that they are not the extreme objects that we once believed them to be. Instead they appear to play a dominant role in shaping present-day galaxies as reflected by their role in the cosmic history of star formation and in producing the cosmic infrared background detected by the COBE satellite in the far infrared to sub-millimeter range. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

Molecular Hydrogen

Observations of H₂ line emission in galactic and extragalactic environments obtained with the Infrared Space Observatory (ISO) are reviewed. The diagnostic capability of H₂ observations is illustrated. We discuss what one has learned about such diverse astrophysical sources as photon-dominated regions, shocks, young stellar objects, planetary nebulae and starburst galaxies from ISO observations of H₂ emission. In this context, we emphasise use of measured H₂ line intensities to infer important physical quantities such as the gas temperature, gas density and radiation field and we discuss the different possible excitation mechanisms of H₂. We also briefly consider future prospects for observation of H₂ from space and from the ground. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

高精度光纤色散测试技术

主要介绍了一套高精度光纤色散测试系统，系统采用频域相移法测量光纤的零色散波长以减小系统误差的影响，其零色散波长测量不确定度达到了0．11nm(k=2)。     

卫星间光通讯系统中比特率等主要参量对最大通讯距离的影响

文中讨论了在保证卫星间光通讯系统的通讯质量前提下，系统的各个主要参量之间的相互制约关系，最大通讯距离受各参量影响的情况。通过分析各个参量对通讯距离影响的大小，找出了增大通讯距离的较好途径。     

边界层综合诊断技术研究

给出了对二元翼型模型和三元三角翼模型表面边界层转捩用表面热膜技术、红外热像仪技术和液晶显示技术在同一风洞中同时进行显示和测量并进行比较的结果。对二元NACA-0012翼型表面边界层转捩点位置测量，三种方法都给出了相吻合的结果。三元的60°三角翼模型经过多次实验，测量结果表明表面热膜技术能够给出三角翼模型表面边界层转捩位置的定量侧量结果。红外热像仪技术和液晶显示技术研究在应用时受到环境条件的影响，在合适的条件下也能给出模型表面边界层转捩位置的定量结果。     

Coherent optical array receiver for PPM signals under atmospheric turbulence

Adaptive combining of experimentally obtained heterodyned pulse position modulated (PPM) signals with pulse-to-pulse coherence, in the presence of simulated spatial distortions resembling atmospheric turbulence, is demonstrated. The adaptively combined PPM signals are phased up via an least-mean-square algorithm suitably optimized to operate with PPM in the presence of additive shot noise. A convergence analysis of the algorithm is presented, and results with both computer simulated and experimentally obtained PPM signals are analyzed.     

空间光学遥感器扫描运动部件运动学与动力学分析方法研究

利用CAE的建模及仿真技术并应用运动学和多体动力学分析软件 (RecurDyn)与结构力学分析软件 (Nastran)相结合的分析研究方法为解决某类带扫描运动部件的空间光学遥感器的运动特性分析及设计提供了参考 ,对该运动机构设计的合理性进行了初步分析评估     

具有双功能的电子式转速表的原理设计与应用

本文较详细地论述了双功能电子式转速表的原理，并将转速测量和超速保护两个系统有机地统一起来，成为即能测量发凡轴转速、双能监测发动机超速，并同时给出控制信号，推动执行机构，保护发动机，最后给出实用的电路图。     

聚硫橡胶研制与工艺方法的研究

介绍了聚硫橡胶配方的选择、技术性能的测试、工艺方法的确定和要求，以及在使用中应注意的几个问题。该胶已在航天产品的红外光学系统和电子电气系统中得到应用。应用表明，该胶性能稳定，质量可靠。     

远红外加热制备预浸带及其对复合材料性能的影响

以远红外加热方式制备了连续芳纶纤维浸胶带，并与工艺成熟的电加热方式制备的预浸带及相应的复合材料性能作比较，确定了远红外加热预浸胶工艺参数。研究结果表明，远红外加热所制备的预浸带性能及相应复合材料压力容器性能与现行工艺成熟的电加热制品性能相当。