用FoxBase实现超文本多媒体技术飞机主客仓空调故障诊断系统

本文通过一个应用系统的编制过程，阐述了用数据库技术实现超文本多媒体技术的方法。     

仿真与响应曲面法的结合及其在综合生产计划中的应用

 论述响应曲面法与仿真相结合的优化结构,着重讨论了一阶和二阶响应曲面的仿真拟合原理和寻优过程,从而可在仿真环境下给出最优决策参数。利用所开发的GASPRSM仿真优化软件,对飞机工厂生产计划安排进行了仿真运行,证明可以取得显著的经济效果。     

流变铸造法制备Al_2O_（3P）／ZA4－3复合材料的研究

为提高模用锌合金ＺＡ４－３的性能，扩大其应用范围，本项工作采用流变铸造法成功地制备了性能稳定的Ａｌ２Ｏ３Ｐ／ＺＡ４－３复合材料。对该材料进行了弯曲强度、冲击韧性、压缩强度、硬度及耐磨性等性能试验，结果表明：Ａｌ２Ｏ３ｐ的加入，使锌合金的压缩强度、室温和高温硬度以及耐磨性明显提高，其弯曲强度略有降低，而其冲击韧性下降了　。最后还讨论了成形工艺参数、颗粒含量和颗粒直径对该复合材料性能的影响。     

铸造SiCp／ZL101复合材料的组织与性能

本文利用半固态搅拌铸造法制备了ＳｉＣｐ／ＺＬ１０１复合材料，对其组织和某些性能进行了研究，结果表明：ＳｉＣｐ在基体中分布均匀，无严重团聚现象，与基体结合良好，与基体合金相比，耐磨性，硬度有显著提高。     

三维有限元网格的自动划分

本文作者从研究结构的数学模型入手,讨论了建立三维结构有限元计算模型的方法。成功地获得了一些具有应用代表性的三维板壳和块体结构有限元计算网格的自动划分原理和算法。     

CARDC 2.4m引射式跨声速风洞设计与运行调试

中国空气动力研究与发展中心研制了可更换喷嘴的中压气体引射器 ,利用现有中压气源驱动 ,建成一座增压回流引射式跨声速风洞。试验段截面尺寸 2 .4m×2 .4m ,M =0 .3～ 1 .2。稳定段最高工作压力为 0 .45MPa ,最高模型试验雷诺数Rec=1 5× 1 0 6(M =0 .90 ,C =0 .2 4m) ,稳定吹风时间≥ 1 5s。风洞气动回路上分别配置有多喷管引射器、栅指扩散段、跨声速试验段驻室抽气系统及特殊的主排气系统等装置。采用智能自适应解耦控制技术 ,实现总压和M数独立、快速、精确地控制。该气动布局与部段配置及其功能设计 ,在国内跨声速风洞中均是首次采用。     

用电离层特性参量提取等效风场信息

导出了利用中低纬电离层特性参量获取电离层F层峰区高度上等效风场（包含电场和风场信息在内）的基本方程，并尝试用该方法从电离层特性参量（峰高和临频）提取等效风场信息，利用武汉站DGS-256电离层数字测高仪数据及由美国Massachusetts Lowell大学最新版的剖面反演程序换算得到F层峰高，获得了武汉地区夏季至日点附近，冬季至日点附近，冬季地磁特别宁静的九天和冬季平均等效风场的初步特征，并利用Fejer经验电场模式计算冬季电场引起的垂直漂移，估计电场和风场对武汉地区的垂直等效风场的贡献大小，结果表明：等效风场呈现出白天与夜晚幅度和方向的差异。至日点附近冬季与夏季白天的幅度差异以及明显的凌晨凹陷现象；平均情况下，垂直等效风场幅度和方向的变化主要是由中性风引起，受电场的影响不大。     

GPS定时校频应用技术的基础研究

针对利用GPS进行定时校频技术开展了一系列的应用基础研究,包括GPS定时校频的方法及其不确定度、定时校频数据的处理等。在给出实验结果的同时,对影响GPS定时精度的各种因素(包括SA影响)进行了讨论;同时对提高GPS定时精度的途径作了初步探讨。     

MONITORING OF ENERGETIC PARTICLE ENVIRONMENT INSIDE THE CHINA-BRAZIL EARTH RESOURCE SATELLITE

On 14 October 1999, the Chinese-Brazil earth resource satellite (CBERS-1) was launched in China. On board of the satellite there was an instrument designed at Peking University to detect the energetic particle radiation inside the satellite so the radiation fluxes of energetic particles in the cabin can be monitored continuously. Inside a satellite cabin, radiation environment consists of ether penetrated energetic particles or secondary radiation from satellite materials due to the interactions with primary cosmic rays.Purpose of the detectors are twofold, to monitor the particle radiation in the cabin and also to study the space radiation environment The data can be used to study the radiation environment and their effects on the electronics inside the satelhte cabin. On the other hand, the data are useful in study of geo-space energetic particle events such as solar proton events, particle precipitation and variations of the radiation belt since there should be some correlation between the radiation situation inside and outside the satellite.The instrument consists of two semi-conductor detectors for protons and electrons respectively. Each detector has two channels of energy ranges. They are 0.5-2MeV and ≥2MeV for electrons and 5-30MeV and 30-60MeV for protons. Counting rate for all channels are up to 104/(cm2@s)and power consumption is about 2.5 W. There are also the additional functions of CMOS TID (total integrated dose) effect and direct SEU monitoring. The data of CBMC was first sent back on Oct. 17 1999 and it's almost three years from then on. The detector has been working normally and the quality of data is good.The preliminary results of data analysis of CBMC not only reveal the effects of polar particle precipitation and radiation belt on radiation environment inside a satellite, but also show some important features of the geo-space energetic particle radiation.As one of the most important parameters of space weather, the energetic charged particles have great influences on space activities and ground tech nology. CBMC is perhaps the first long-term on-board special equipment to monitor the energetic particle radiation environment inside the satellite and the data it accnmulated are very useful in both satellite designing and space research.     

Acceleration of interplanetary pick-up ions and anomalous cosmic rays

It may not be doubted anymore that anomalous cosmic rays (ACRs) are produced in the heliosphere from interplanetary pick-up ions through their acceleration at the solar wind termination shock. However, there is no general agreement in the community of heliospheric researchers concerning the mechanism of injection of the pick-up ions into the shock acceleration. We discuss here three possible ways for pick-up ions to be involved into the acceleration process at the termination shock: (1) preacceleration of pick-up ions in the whole region from the Sun up to the termination shock by solar wind turbulences and interplanetary shock waves, (2) local preacceleration of pick-up ions in a vicinity of the termination shock by shock surfing, and (3) formation of high-velocity tails in pick-up ion spectra consisting of secondary pick-up ions which are produced in the supersonic solar wind due to ionization of energetic neutral atoms entering from the inner heliosheath.