室温贮存对树脂粘度和加压点的影响

讨论了５４０５改性双马来酰亚胺树脂基体在室温下，贮存时间对粘度以及对固化过程中加压点的影响，给出了相应的计算方法。     

在《机械设计基础》课程教改中加强学生实践能力的培养

为加强学生实践能力的培养,切实提高教学质量,针对《机械设计基础》课程教学中存在的几个现实问题,提出了课程教学改革的意见。     

基于多传感器信息融合的自主移动机器人导航算法研究

本文介绍了一种基于微控制器控制，以GPS为主要导航手段，且基于多传感器信息融合的自主移动机器人导航系统的软硬件设计思想及实现方法。重点讨论了基于栅格法的导航算法在微控制器系统中的实现。最后给出了该导航系统在比较典型的环境中实现导航与避障的实验结果。     

灰色系统理论中二维数据序列均值生成的讨论

灰色系统理论中非等时序序列或含有空穴的序列,通常可以用均值生成方法来填补,生成等时序序列。本文研究发现,用非紧邻均值生成方法生成的内点与实际存在有明显的误差,为此讨论了均值生成和有偏生成算法。利用数据序列点的局部凹凸特性来表示数据序列点的特征,提出了采用数据序列点连线的状态选取生成系数的方法。通过对一维数据序列传统均值生成方法的比较,给出了二维数据序列的定义,讨论了在二维数据序列下的均值生成方法,提出了有偏生成算法中生成系数分解的选取方法。     

深层搅拌法技术及其工程应用

深层搅拌技术是对软土地基进行处理的较常用技术 ,它具有加固效果显著、形式灵活多样、环境无污染、施工机具简单、施工速度快、节省投资等优点 ,目前在地基处理和基坑工程中广泛采用。本文主要阐述该技术特点及在地基处理工程中的应用 ,对同类工程设计具有重要的参考价值。     

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。     

直接不交化方法在故障树定量分析中的应用

在布尔集合运算方法和不交化方法基础上，提出了单调关联故障树系统定量分析优化方法，通过故障树定量分析优化方法，可以方便地得到系统的可靠度、不可靠度、最小割集、最小路集、关键重要度等指标。     

Ada软件的动态测试技术研究

为改善软件质量，对Ａｄａ软件的动态测试技术进行了研究，并且就以下内容着重进行了讨论；Ａｄａ软件的分析与理解；Ａｄａ软件的动态测试原则与方法；Ａｄａ软件的动态测试工具ＡＳＤＴ。     

神舟2号大气密度探测器的探测结果(Ⅰ)日照和阴影区域热层大气密度变化

选用了神舟2号（SZ-2）大气密度探测器在2001年2—4月间的探测数据,进行日照和阴影区域热层大气密度变化的探讨.结果表明:在高度410km附近,日照和阴影区域大气密度变幅为2—3倍,变幅的大小与地磁活动程度呈负相关关系.日照面大气密度峰区位于星下点地方时1400—1500LT的纬度处,峰值大小与太阳活动程度呈正相关关系.阴影面大气密度谷区位于星下点地方时0400-0500的纬度处,同时在±10°纬度区域中还出现了阴影面峰区.     

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.