Analysis of the Micrometeoroid and Debris Hazard Posed to an Orbiting Parabolic Mirror

Many concepts of future space systems involve the use of parabolic mirrors for optical applications. The need for a highly reflective finish means that performance of such systems will be particularly vulnerable to space debris and micrometeoroids. A case study was performed to examine the micrometeoroid and debris hazard posed to an orbiting parabolic mirror. The mirror considered was nominally Earth-pointed in a circular orbit with two candidate altitudes in low Earth orbit (LEO), well within the region inhabited by man-made debris. The timeframes of interest for the two missions were 2002–2004 and 2005–2015. Microgram and larger particles were considered.To perform this study, it was necessary to determine the debris and meteoroid flux across the parabolic surface. To assess sensitivity of results to uncertainity in available data, two approaches were taken. The first approach was an analytical procedure based on use of long duration exposure facility (LDEF) data and published theoretical results. The second approach used two readily available computer models: the ESA MASTER model and NASA's ORDEM96. In addition, an in-house implementation of the Grün meteoroid model was used. While multiple results were available for the total flux and flux distributed over azimuth, only the MASTER model was available for generating the desired elevation data to obtain the flux distribution over the parabolic mirror. In an attempt to bound the uncertainty in the knowledge of the elevation distribution, the results from both the MASTER and ORDEM96 models were processed together to form a separate, hybrid prediction. In addition, results were used in the preliminary design of a protective skirt.This case study elucidated the practical obstacles and considerations in performing a sufficiently accurate debris and meteoroid analysis using data and tools that are readily available to the broad space sector. The resulting procedures are useful in the assessment of the risk posed to optics by the meteoroid and debris environment and in the design of protection.     

变极性等离子弧焊电源的研制

本文介绍了变极性等离子弧焊电源的工作原理，试验研究了方波交流频率和电流极性比对电弧稳定性、阴极清理作用和热输入的影响。研制的电源不仅频率、电流极性比以及正负半波电流幅值分别可以调节，而且还具有交流载波焊接功能，是一种焊接铝合金的理想电源。     

8m×6m低速风洞技术改造研究

8m× 6m风洞是亚洲最大的低速风洞 ,为了不断满足国民经济发展对风洞试验的要求 ,为了解决本身存在的问题 ,8m× 6m风洞运行 2 0年来首次进行了大规模技术改造。采用了自行研制和引进改进相结合的方式 ,圆满地完成了改造 ,使该风洞的试验能力提高到了一个新的水平。     

光栅的衍射在高分辨力测长仪器中的应用研究

选用高密度光栅产生衍射条纹 ,研究其信号合成、采集及处理的方法以实现在长度计量中 ,纳米分辨力的计数。     

太阳电池阵深空探测适应性设计概论

随着近年来月球探测的推进,深空探测的论证,针对深空探测对太阳电池阵低温度、低光强、强辐射等环境的技术需求,以火星探测和木星探测太阳电池阵设计分析为例,通过任务环境特点分析,给出了特殊服役环境下太阳电池选型方法,方阵设计与验证建议,对国内深空探测太阳电池阵设计具有一定参考意义。     

HY-750开口回流低速风洞

介绍了HY 75 0风洞的结构、动力系统和测试系统的组成及特点。对风洞流场进行了校测 ,结果表明 ,风洞流场品质较好 ,主要指标优于××标准规定 ,标模实验精度也达到了标准规定的合格指标。从风洞使用情况看 ,交流变频矢量控制技术在风洞中使用是可行的 ,软件平台Labview在风洞测试系统的应用也是成功的。该风洞不仅能满足测力、测压、流场演示等教学需要 ,还将在科学研究和型号研制、实验中发挥一定作用     

单边带电台高效率线性发送系统的实现

为了提高某单边带电台的功率性能指标，采用了高效率线性放大系统。文中讨论了宽带、线性和调正等主要问题，尤其是说明了在系统中使用了宽带Ｅ类高效率功率放大器，并给出了试验结果。试验结果表明，Ｅ类功率放大器的效率在１．６－－６ＭＨｚ范围内超过了９０％，整机效率大于５０％，提高了输出功率，增大了通信距离，延长了电池使用寿命，反映了应用高效率线性功率放大系统的优越性。     

高频功率放大器的计算机计算和分析程序(RFPACCA)

本文介绍了高频功率放大器的计算机计算和分析程序,详细说明了高频功率放大器过压工作子程序的编制原理,同时给出了计算实例。     

磁暴期间中低纬电离层暴形态和物理机制分析

本文利用东亚地区１２个低纬电离层台站的测高仪观测数据，对１９７８年８月２７日发生的一次曲型磁暴期间电离层峰值高度和密度的变化进行了分析。采用滑动平均区分开电离层中不同时间尺度的扰动，分析了影响中低纬度电离层暴的几种扰动形态特征，并对其物理机制进行了讨论。结果表明：伴随磁暴急始的磁层压缩，电离层中表现出峰值密度增加和峰值高度下降；磁暴主相期间热层大气暴环流及其所引起的中性大气成分变化控制着电离层的大     

星载L波段宽带低噪声放大器芯片设计

基于0.25μm 砷化镓赝品高电子迁移率晶体管（GaAs pHEMT）工艺，设计了一款应用于星载微波接收机的L波段单片微波集成电路（MMIC）低噪声放大器（LNA）。该低噪声放大器采用电流复用拓扑结构，降低了芯片的工作电流，节省了宝贵的卫星能量资源；通过两级负反馈方式优化了器件的稳定性和增益平坦度，提高了卫星通信质量；恒流源的偏置结构使得工作电流随工艺波动较小，芯片维持在稳定的工作状态下。测试结果表明：该放大器工作电流为35mA，在频率范围0.9~1.8GHz内，增益大于33dB，噪声系数小于0.6dB，增益平坦度小于0.5dB；芯片尺寸为2.0mm×1.3mm，满足航天产品的高性能小型化应用需求。