起落架落震试验测试系统的现状及其发展

能动地我国起落架落震试验测试系统发展的现状进行分析，指出了落震试验测试系统所存在的问题，说明了未来的发展重点及方向。     

欠发达地区招商引资过程中政府、企业与居民互动关系研究——以苏北X县Y镇为例

目前,苏北各地相继实施了招商引资政策。招商引资政策的实施是在现行财政和行政体制背景下进行的,该过程中政府、企业及居民三者的互动关系主要表现为:政府与企业相互交换资源,通过利益共谋形成利益共同体,并通过政府权力运作形成制度化、规范化的利益交换关系;与此同时,该过程中居民从政府、企业方获益甚少或从未获益,因而居民与政府、企业形成利益对抗体,并最终形成了"二对一"的三方关系。这一不和谐的三方关系不利于当前乡村建设与发展,必须主要从政府层面来规范招商引资行为,改善三方不和谐的关系现状。     

"公安学基础理论"教学法探讨

“公安学基础理论”是一门理论性较强的课程，其中涉及的内容大多较为抽象、枯燥，传统单一的教学方法不利于学生的理解和掌握。文章仅就“公安学基础理论”课堂教学的几种有效方法作简单探讨。     

模拟地球同步轨道辐照环境对光学太阳反射镜性能的影响

研究了模拟地球同步轨道辐照环境对卫星用温控涂层-光学太阳反射镜(OSR)性能的影响。对所研制的两类OSR 片进行的辐照试验项目有,真空紫外辐照、低能电子和两种能量的质子辐照。此外还进行了等离子体环境条件下的表面充/放电效应试验。经过相当于安装在地球同步轨道卫星南北极位置处,在空间七年所受到的电子、质子和紫外辐照总剂量的辐照后,导电型OSR 的太阳光谱吸收率α_s 由0.068增加到0.078,法向发射率ε_n 由0.83降低到0.72;而非导电型OSR的α_s 由0.066增加到0.085,ε_n 由0.82降低到0.76。表面充/放电试验的结果表明:导电型OSR 的充电电位仅在15～40V 之间,而非导电型OSR 的充电电位则可高达13kV。因此导电型OSR能有效地控制表面的充/放电现象。     

SPR生物传感器在生命科学及在航天医学中的应用

表面等离子体共振生物传感器在分析生物分子相互作用方面，具有灵敏度高、实时在线、简单快捷和抗干扰能力强等优点，被广泛应用于临床检验、药物筛选等研究领域；因其能满足空间特殊环境下的使用要求，在航天医学领域具有广阔的应用前景．本文综述了表面等离子体共振生物传感器的原理、特点、在生命科学研究中的应用及在航天医学中的应用前景．     

防静电白色热控涂层的空间环境性能试验

通过在氧化锌晶格中掺入重金属离子，得到具有防静电功能的白色颜料，再以丙烯酸树脂为粘合剂制备出空间飞行器外表面用的ACR－1防静电白色热控涂层；研究了空间环境效应（包括紫外辐照，电子和质子辐照）对该热控涂层太阳吸收率的影响并与有机硅白色热控涂层进行了比较，地面模拟空间环境试验研究结果证明，ACR－1防静电白色热控涂层具有良好的空间稳定性。     

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.     

柱面菲涅耳太阳聚光透镜的光学设计和光学效率

研究了柱面线聚焦菲涅耳太阳聚光透镜的光学设计和光学效率。依据理论分析，对透镜参数进行了优化设计，成功地研制出了柱面线聚焦菲涅耳聚光透镜。还分析了透镜相对孔径（F数）和成型模具等因素对透镜光学效率的影响。     

精密GPS卫星钟差的改正和应用

分析了GPS卫生钟差的变化特性，探讨了利用GPS地面跟踪站的观测数据估算GPS卫星钟差的可行性，建立了相应的算法和软件系统，并把由地面跟踪站的实测数据估算的卫星钟差用于星载GPS定轨计算，得到优于1m的定轨精度。     

Noise in wireless systems from solar radio bursts

Solar radio bursts were first discovered as result of their interference in early defensive radar systems during the Second World War (1942). Such bursts can still affect radar systems, as well as new wireless technologies. We have investigated a forty-year record of solar radio burst data (1960–1999) as well as several individual radio events in the 23rd solar cycle. This paper reviews the results of a portion of this research. Statistically, for frequencies f  1 GHz (near current wireless bands), there can be a burst with amplitudes >10³ solar flux units (SFU; 1 SFU = 10⁻²² W/m²) every few days during solar maximum conditions, and such burst levels can produce problems in contemporary wireless systems.