VentureStar… reaping the benefits of the X-33 program

Major X-33 flight hardware has been delivered, and assembly of the vehicle is well underway in anticipation of its flight test program commencing in the summer of 1999. Attention has now turned to the operational VentureStar^TM, the first single-stage-to-orbit (SSTO) reusable launch vehicle. Activities are grouped under two broad categories: (1) vehicle development and (2) market/business planning, each of which is discussed. The mission concept is presented for direct payload delivery to the International Space Station and to low Earth orbit, as well as payload delivery with an upper stage to Geosynchronous Transfer Orbit (GTO) and other high energy orbits. System requirements include flight segment and ground segment. Vehicle system sizing and design status is provided including the application of X-33 traceability and lessons learned. Technology applications to the VentureStar^TM are described including the structure, propellant tanks, thermal protection system, aerodynamics, subsystems, payload bay and propulsion. Developing a market driven low cost launch services system for the 21st Century requires traditional and non-traditional ways of being able to forecast the evolution of the potential market. The challenge is balancing both the technical and financial assumptions of the market. This involves the need to provide a capability to meet market segments that in some cases are very speculative, while at the same time providing the financial community with a credible revenue stream. Furthermore, the market derived requirements need to be assessed so as not to impose unnecessary requirements on the vehicle design that add unreasonable cost to the development of the system, yet provides the right capabilities for new markets that could be triggered by dramatically lower space transportation prices.     

应用联合变换相关器的成像制导系统

提出了一种光电混合的成像制导系统，它采用光学联合变换相关器作为其主要的图像识别单元，利用计算机对识别结果进行判决和显示，并发出跟踪信号给导引头，从而实现制导。联合变换相关器是对光学图像信号进行并行处理的器件，实时识别性能强，精度高。此成像制导系统克服了传统的红外制导系统易受外界因素影响，实时处理能力差，误判率较高的缺点，具有并行处理速度快、信息吞吐量大、体积小等优点，应用前景广阔。     

基于AT89C52的离散信号测量电路设计

介绍了离散信号测量与控制在反舰导弹雷达导引头自动测控系统中的重要性 ,给出了基于AT89C5 2单片机控制的离散信号测量电路的具体构成和工作原理     

2000年行星际南向磁场事件及相关CME的若干分析

根据WIND飞船的观测资料，讨论了2000年发生的南向磁场（BS）事件，分析了它们的源，发现12次事件中11次的源是日冕物质抛射（CME）。运用从地球向太阳时间倒推的方法和LASCO，EIT195A的观测资料，确定了这些CME。它们都是快速CME，伴有行星际激波，都具有晕状（Halo)形态，它们在日面上发生的位置是在一个不对称的区域内。还分析了5个强南向磁场（BS≥20nT)事件，发现它们的CME源，或者具有很高的能量，或者抛射方向正对地球，或者是具有叠加效应的CME系列，分析表明，在我们所讨论的太阳活动高年，大的行星际扰动和强地磁暴与高速流的联系并不密切。     

微波衰减测量过程失控的原因分析及解决方案

针对高频串联替代法微波衰减测量标准装置测量过程所出现的失控现象 ,从测量标准仪器、被测仪器、测量方法、人为因素等方面分析了失控的原因 ,制定并实施了相应的解决方案 ,使测量过程恢复到统计受控状态     

76°/40°双三角翼前缘涡破裂及其控制实验研究

流动显示结果表明,喷流能有效地推迟双三角翼前缘涡的破裂,且随着攻角的增大,前缘涡破裂位置逐渐推后,喷流极大地改善了大攻角情况下前缘涡的非对称破裂特性,能有效地克服可能出现的机翼的"摇滚"现象.另外,后缘喷流可以减弱乃至消除前缘涡混掺现象的发生,进而有利于飞行器的操纵.     

KuaFu Mission

The KuaFu mission-Space Storms, Aurora and Space Weather Explorer-is an "L1+Polar" triple satellite project composed of three spacecraft: KuaFu-A will be located at L1 and have instruments to observe solar EUV and FUV emissions, and white-light Coronal Mass Ejections (CMEs), and to measure radio waves, the local plasma and magnetic field,and high-energy particles. KuaFuB1 and KuaFu- B2 will bein polar orbits chosen to facilitate continuous 24 hours a day observation of the north polar Aurora Oval. The KuaFu mission is designed to observe the complete chain of disturbances from the solar atmosphere to geospace, including solar flares, CMEs, interplanetary clouds, shock waves, and their geo-effects, such as magnetospheric sub-storms and magnetic storms, and auroral activities. The mission may start at the next solar maximum (launch in about 2012), and with an initial mission lifetime of two to three years. KuaFu data will be used for the scientific study of space weather phenomena, and will be used for space weather monitoring and forecast purposes. The overall mission design, instrument complement, and incorporation of recent technologies will target new fundamental science, advance our understanding of the physical processes underlying space weather, and raise the standard of end-to-end monitoring of the Sun-Earth system.     

轻便风速表检定装置不确定度的测试与评定

根据GJB/J2 74 9《建立测量标准技术报告的编写要求》 ,结合气象计量的实际情况 ,给出了轻便风速表检定装置不确定度的测试与评定方法。     

锯齿型扰流片对壁面压力分布的影响

在风洞用电子扫描阀进行测压,研究了绕平板扰流片和锯齿扰流片分离流动的壁面压力分布.结果表明平板扰流片和锯齿扰流片均在上游x/h=-6处剪切层开始分离,并再附于下游x/h≈20的位置.锯齿扰流片横向位置的变化对壁面平均压力分布几乎没有影响,但通过锯齿槽流向的压力脉动一般大于通过锯齿尖点流向的脉动.从平均压力分布看,锯齿高度可以增加扰流片阻流效果,采用锯齿扰流片可以减小下游壁面压力的脉动.     

掺磷纳米硅薄膜的微结构

采用喇曼(Raman)散射谱、高分辨率电子显微镜(HRTEM)和原子力显微镜(AFM)对掺磷纳米硅薄膜的微结构进行了分析,并对纳米硅薄膜的传导机制进行了探讨.结果表明:掺磷纳米硅薄膜由尺寸为2～4*#nm的晶粒和2～3个原子层厚的非晶界面构成,计算得到薄膜的晶态比为40%～55%.与本征纳米硅薄膜相比,掺磷纳米硅薄膜晶粒尺寸和晶态比没有明显变化,电导率却提高了2个数量级.随着掺磷浓度增加,纳米硅薄膜的晶粒尺寸、晶态比及电导率逐渐增大.AFM观察表明掺磷纳米硅薄膜由尺寸介于15～20*#nm的团簇构成,团簇排列具有带状特征.