用集成功放组成的精密功率放大器

介绍了一种用厚膜集成功放加上稳幅电路组成的精密功率放大器，其稳定度、频率响应和波形失真都达到了很高的指标。     

带人工雨线的斜拉桥拉索模型测压试验研究

斜拉桥拉索风雨激振是当今国际风工程和桥梁工程研究人员非常关注的问题.为了掌握风雨激振时拉索的气动力特性,研究人员对风向角为0°时带人工雨线的拉索模型进行了测力试验.但至今人们尚未测量过风向角不为0°时带人工雨线的拉索模型上的气动力.本文设计、制作了可方便调节拉索模型倾角和风向角的试验装置以及用于测压试验的带人工雨线的拉索模型,并在风洞中进行了细致的试验.试验得到了具有典型倾角的拉索在不同风向角下,拉索模型上的平均风压和脉动风压系数,以及气动力系数.这些结果为建立精细的理论模型提供了基础.     

基于模糊模式识别的电力远动通道监控系统

分析了电力远动通道监控系统的现状,为解决其不足之处提出了一种电力远动通道监控的新方案.采用了一种基于模糊模式识别的综合评判远动通道通信质量的方法来实现对远动通道的监控,并详细论述了方案中模糊模式识别模型的建立,同时给出了系统的实现方案.在实际应用中表明,该系统能够有效地解决目前监控系统存在的不足,为电力远动通道监控开辟了新途径.     

飞机风洞实验动力模拟器的设计研究

在飞机的飞行中，动力装置与飞机机体间的干扰是复杂的，因此在进行实际飞机设计的过程中，风洞实验是不可缺少的。本文重点介绍了进排气动力装置的引射器模拟器的设计。     

用于航空高压直流电源系统的笼型异步发电机控制策略的研究

 现代电力电子技术的发展使得笼型异步发电机能够适用于航空高压直流系统中。着重对笼型异步电机与电力电子变换器结合构成的发电系统进行了研究,说明了采用直接转矩控制策略可使这种发电系统具有很好的动态特性。介绍了异步发电机直接转矩控制的原理与实现方法,并给出了仿真与实验结果。     

中国航改燃气轮机的现状及发展

综合论述了中国航空发动机改装燃气轮机的基本现状和应用前景,总结了航改燃气轮机的发展历程和技术经验,探讨了中国自主开发燃气轮机的发展趋势和途径。     

直升机动力传动系统扭转振动整体传递矩阵分析

研究了复杂多轴齿轮传动系统整体传递矩阵方法及在直升机动力传动系统扭转振动分析中的应用.首先说明了直升机传动系统传递矩阵方法力学模型,推导了传动系统中典型齿轮副啮合传递矩阵、并车级和行星级齿轮啮合传递矩阵,说明了这种具有多种齿轮副啮合的复杂多轴系统整体传递矩阵模型组集方法,最后用这种方法进行了典型直升机动力传动系统扭转振动特性分析,讨论了这种直升机动力系统振动特性的特点.      

低功率激光-TIG电弧复合焊接不锈钢熔深研究

建立了一套低功率YAG脉冲激光-TIG电弧复合热源焊接系统,并用本系统对不锈钢1Cr18Ni9Ti进行焊接.研究了3种热源作用下不锈钢的焊缝熔深.通过引入焊缝有效热输入概念,对复合热源影响熔深的机理进行了分析.     

大气紊流环境下的纵向飞行参数响应分析

介绍了大气紊流环境下飞机纵向飞行参数的计算与匹配方法.由于紊流的随机性特征,飞行参数响应分析采用时域与频域相结合的方式,对某型飞机紊流环境下的纵向飞行参数进行了计算分析.采用所介绍的方法,可以获得比较合理的飞行情况来指导型号设计工作.     

A Comparative Study of the Influence of the Active Young Sun on the Early Atmospheres of Earth, Venus, and Mars

Because the solar radiation and particle environment plays a major role in all atmospheric processes such as ionization, dissociation, heating of the upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect of solar induced X-ray and EUV (XUV) heating on the upper atmospheres of Earth, Venus and Mars since the time when the Sun arrived at the Zero-Age-Main-Sequence (ZAMS) about 4.6 Gyr ago. We apply a diffusive-gravitational equilibrium and thermal balance model for studying heating of the early thermospheres by photodissociation and ionization processes, due to exothermic chemical reactions and cooling by IR-radiating molecules like CO₂, NO, OH, etc. Our model simulations result in extended thermospheres for early Earth, Venus and Mars. The exospheric temperatures obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen and high Jeans’ escape rates for heavier species like H₂, He, C, N, O, etc. The duration of this blow-off phase for atomic hydrogen depends essentially on the mixing ratios of CO₂, N₂ and H₂O in the atmospheres and could last from ∼100 to several hundred million years. Furthermore, we study the efficiency of various non-thermal atmospheric loss processes on Venus and Mars and investigate the possible protecting effect of the early martian magnetosphere against solar wind induced ion pick up erosion. We find that the early martian magnetic field could decrease the ion-related non-thermal escape rates by a great amount. It is possible that non-magnetized early Mars could have lost its whole atmosphere due to the combined effect of its extended upper atmosphere and a dense solar wind plasma flow of the young Sun during about 200 Myr after the Sun arrived at the ZAMS. Depending on the solar wind parameters, our model simulations for early Venus show that ion pick up by strong solar wind from a non-magnetized planet could erode up to an equivalent amount of ∼250 bar of O⁺ ions during the first several hundred million years. This accumulated loss corresponds to an equivalent mass of ∼1 terrestrial ocean (TO (1 TO ∼1.39×10²⁴ g or expressed as partial pressure, about 265 bar, which corresponds to ∼2900 m average depth)). Finally, we discuss and compare our findings with the results of preceding studies.