直升机机动飞行逆仿真技术研究进展

回顾了直升机机动飞行逆仿真技术国内外发展概况，借鉴国内外的研究成果，针对逆仿真核心技术的发展现状进行了分析和讨论，在此基础上，对直升机机动飞行逆仿真技术的进一步发展趋势进行了分析。     

错频转子系统动力特性研究

根据某级压气机叶／盘转子的实际结构，建立了叶／盘带短轴的有限元模型。采用NASTRAN结构分析软件，得到了模化协调转子所需的数据，构建了多自由度叶／盘转子系统动力学模型，并在此基础上通过改变多自由度模型中叶片刚度实现错频。采用基尔法求解错频转子系统的运动方程。获得了此多自由度系统的动态响应，并对不同错频方案进行了对比分析。     

直升机旋翼运动参数试飞技术

旋翼挥舞角、摆振角是直升机的关键参数。介绍了一种非接触式激光测试系统．对直升机旋翼挥舞角和摆振角进行试飞测试，并在Z11上得到了成功的应用，其结果真实可信，测量精度高。     

一种分析轮式起落架直升机“舰面共振”的方法

 针对轮式起落架直升机，提供了一种“舰面共振”动力稳定性分析方法。首先，针对直升机在舰面上随舰船一起摇晃时左右起落架受载不对称的状况，近似采用受对称载荷产生对称变形、受非对称载荷产生非对称变形的方法计算了直升机的平衡状态；其次，根据轮式起落架轮胎和缓冲支柱刚度和阻尼共同作用的特点，结合轮式起落架的几何关系，采用复刚度的方法得出起落架作用于机体的刚度与阻尼；最后，用桨叶振动模态法对轮式起落架的直升机进行了不同旋翼升力卸载以及鱼叉系留与否的“舰面共振”动力稳定性计算分析，并通过算例得到验证。     

气动/推力矢量控制面融合方式研究

针对在过失速机动中气动/推力矢量控制面协调问题,分析了最小控制能量和链式递增两种典型控制面融合方式的特点.结合实际应用上存在的问题,提出了一种新的融合控制方式.通过仿真计算和分析,并与典型的链式递增融合方式进行比较后可知,这种新的控制方式改善了采用链式递增融合控制方式中气动舵面的振荡现象.并且与最小控制能量融合方式相比更具有实用性.     

一个基于WINDOWS环境的网络连接服务

该文介绍了在校园网环境及WINDOWS平台，采用TCP/IP协议设计并开发PING网络连接服务和客户机/服务器功能的VC^ 程序。     

Evolution of the Protosolar Nebula and Formation of the Giant Planets

The formation of planetary systems is intimately tied to the question of the evolution of the gas and solid material in the early nebula. Current models of evolution of circumstellar disks are reviewed here with emphasis on the so-called “alpha models” in which angular momentum is transported outward by turbulent viscosity, parameterized by an dimensionless parameter α. A simple 1D model of protoplanetary disks that includes gas and embedded particles is used to introduce key questions on planetesimal formation. This model includes the aerodynamic properties of solid ice and rock grains to calculate their migration and growth. We show that the evolution of the nebula and migration and growth of its solids proceed on timescales that are generally not much longer than the timescale necessary to fully form the star-disk system from the molecular cloud. Contrary to a widely used approach, planet formation therefore can neither be studied in a static nebula nor in a nebula evolving from an arbitrary initial condition. We propose a simple approach to both account for sedimentation from the molecular cloud onto the disk, disk evolution and migration of solids. Giant planets have key roles in the history of the forming Solar System: they formed relatively early, when a significant amount of hydrogen and helium were still present in the nebula, and have a mass that is a sizable fraction of the disk mass at any given time. Their composition is also of interest because when compared to the solar composition, their enrichment in elements other than hydrogen and helium is a witness of sorting processes that occured in the protosolar nebula. We review likely scenarios capable of explaining both the presence of central dense cores in Jupiter, Saturn, Uranus and Neptune and their global composition. This revised version was published online in August 2006 with corrections to the Cover Date.     

基于DCOM技术构建分布式数控故障诊断系统

简要介绍DCOM技术的特点,对利用DCOM技术构建分布式数控故障诊断系统进行了研究,并提出了系统的组件模型结构。     

热结构动力优化设计

 考虑温度沿飞行器表面的分布及材料物性系数随温度的变化,按Ｋｕｈｎ－Ｔｕｃｋｅｒ条件建立迭代式,研究具有频率约束、振型节点约束以及变量上、下限约束的热结构动力优化设计。算例讨论了前３阶固有特性及最小目标随温度场的变化规律,证实本方法有效、可行。     

起落架落震试验的数字模拟方法

 <正> 在计算飞机起飞、着陆和滑行等地面运动的静、动态载荷时,除了需要飞机结构和气动参数外,起落架减震器的性能参数更占有重要地位。而这些性能参数中尤以决定油液阻尼力的流最系数为重要。长期以来,国内主要靠查手册、凭经验确定这个系数,如果能较准确地确定流量系数,对载荷计算是很有意义的事。