行星际空间MHD模拟激波跃变关系分析

分析了模拟得到的可以传播到1AU以远的日地空间磁流体力学激波与Rankine-Hugnoniot跃变关系的符合程度．通过对模拟激波的结构及其在传播过程中的演化进行的分析，提出了模拟激波的定位方法；基于所提出的定位方法，利用向长青提出的确定MHD激波局地参数的方法计算了模拟得到的激波与Rankine-Hugnoniot跃变关系的偏差．结果表明在激波传播到100Rs以后，激波对中前向快激波与Rankine-Hugnoniot关系的符合达到很高的程度，相对误差在10^-2数量级以内；并且在激波传播到150 Rs以后，相对误差在10^-3数量级以内．这个结果说明文中所使用的有限差分数值格式能较好地模拟激波．     

应用分力合成方法提高系统性能指标的研究

提出了将柔性结构的分力合成主动振动抑制方法和反馈控制律结合使用来提高柔性结构控制系统性能指标的方法。应用该方法仅需要知道闭环系统及柔性振动的频率及阻尼，而且可以同时抑制任意多个振动模态（包括控制器引起的振动，柔性振动及其他形式的振动），分力合成方法对频率及阻尼的不确定性具有较强的鲁棒性，使该方法易于工程实现，文章针对单柔性杆，将分力合成主动振动抑制方法和反馈控制相结合，设计了不同形式的大角度机动控制律，数值仿真和试验结果充分验证了方法的有效性。     

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。     

基于多体分析的对接机构结构锁动力学仿真研究

分析了周边式空间对接机构结构锁的执行机构的特点，以及运用现有动力学分析软件解决此问题的困难；继而采用多体动力学建模方法，建立了结构锁执行机构的动力学模型，并针对本模型的特殊性采用了变步长的广义坐标分块求解算法；最后通过求解模型得到了机构的动力学特性曲线，证明了滚珠丝杆和弹簧复合机构作为结构锁执行部件是可行的．     

研究用现场数据估计系统可靠性参数置信区间

研究用元部件现场信息估计系统可靠性参数,如系统可靠度、可靠寿命等区间估计问题。文中提出了一种新的估计方法——替换百分点法,并运用Monte Carlo数字仿真对估计的置信度和精度进行了分析,研究结果表明此方法具有工程应用价值。     

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.     

微重力下管肋式空间辐射器的整体优化分析

建立了向一重力环境下管肋式空间辐射器传热过程的数学模型，并以单质量散热量最大和热载体驱动功率最小为优化目标，对管式空间辐射器进行了优化分析。     

MATLAB在飞机环境控制系统仿真中的应用

介绍了在MATLAB环境下,对飞机环境控制系统的建模方法,开发了飞机环控系统综合仿真的MATLAB工具箱.简单介绍了所开发的仿真工具箱,并且用此工具箱对某型飞机的环控系统进行了仿真研究,与实验结果的对比表明,所开发的工具箱,具有很高的仿真精度.