基于变结构控制器的敏捷卫星姿态机动方法

随着遥感卫星观测能力的逐步提升,对卫星敏捷机动能力提出了更高的要求。针对敏捷卫星大角度姿态机动问题,以6个单框架控制力矩陀螺(SGCMG)组成五棱锥构型的姿态控制系统执行机构,在构建敏捷卫星姿态运动数学模型以及设计SGCMG系统操纵律的基础上,对卫星绕Euler轴进行姿态机动的角轨迹进行规划,并设计了一种基于误差四元数与误差角速度的变结构控制器。仿真及在轨验证结果表明,该控制器能够完成规划轨迹的良好跟踪且具有较强的鲁棒性,研究成果对敏捷卫星姿态控制系统的设计具有重要的参考意义。     

载波相位差分GPS/惯性组合导航

载波相位测量是目前测量精度最高的测量方法,所以载波相位差分ＧＰＳ同惯导组合能获得高精度的导航系统。但载波相位测量需要确定整周模糊度,现在已探索出多种算整周模糊度的方法,但这些方法而且需要一定的解算时间。文中提出了把模糊度作为状态变量进行组合的方法,用整周模糊度的浮点解同样可得到较高精度的导航系统。仿真结果表明,该方法是行之有效的,扩大了组合系统的应用范围,对航空、航天、铁路、航海等载体的高精度导航     

对象状态测试

阐述了面向对象软件测试中对象状态测试的重要性，提出了对象状态测试模型，介绍了从Ｃ＋＋源程序构造模型的方法，最后给出了基于ＯＳＤ的面向对象状态测试的测试策略，测试标准和测试用例的生成方法。     

非接触动静结合型机械密封的主动可控性及其脱开机理

针对非接触动静结合型机械密封运行中的脱开现象和泄漏量控制要求,研究基于改变闭合力的机械密封主动可控方法.在原有基础上完善了动静结合型机械密封主动可控的原理,包括控制策略、控制元件及控制流程;结合高速涡轮泵轴端机械密封,给出了主动控制的设计过程,并理论和试验研究了其可控性和受可控元件影响的性能规律.完善了现有的机械密封脱开理论,并结合试验结果对可控型机械密封的脱开转速进行了机理分析.研究结果表明:提出的基于闭合力调控的密封可控性策略及控制敏感性参数范围[1,3.19],可满足对涡轮泵轴端机械密封泄漏量的动态主动控制;完善的脱开转速理论能合理地解释机械密封起飞阶段的端面非接触状态向接触状态转变过程.研究结果对于特殊工况下特种机械密封的设计、运行监测及动态控制具有参考价值.     

细长体大迎角绕流的滚转角特性

尖拱和钝拱细长体的截面侧向力分布呈现明显的滚转角效应。不同滚转角下尖拱侧向力沿轴向分布曲线(CC～x/D)的相位和半周期各不相同,截面侧向力随滚转角变化(CC～)呈现一定的无规律性;而钝拱CC～x/D曲线的相位和半周期基本相同,但振幅值大小依赖于滚转角,CC～分布呈完全的无规律性。尖拱模型头部的加工精度导致的微扰动使得尖拱CC～x/D分布变成型式基本一致的两簇曲线,其特征点和半周期分别对应相同,CC～分布呈现典型的双周期方波。     

飞机增稳系统的耗散控制问题研究

讨论了飞机增稳系统的耗散控制问题．首先将增稳系统的运动方程简化为定常线性系统;其次,研究系统的耗散性分析;再次,设计状态反馈控制器使得系统的闭环系统耗散;最后,通过数值仿真验证了方法的可行性。     

带挤压油膜阻尼器的盘式拉杆转子双稳态振动特性

建立了带挤压油膜阻尼器的盘式拉杆转子动力学模型,利用非线性微分方程多周期解求解方法,对不同系统参数组合下的动力学方程进行求解,研究了带挤压油膜阻尼器的盘式拉杆转子双稳态振动特性的影响规律,比较了带与不带挤压油膜阻尼器系统稳定周期解的动力学特性.通过频谱分析得出:忽略挤压油膜阻尼器时双稳态区主要为基频振动,考虑挤压油膜阻尼器的盘式拉杆转子在双稳态区除了基频振动外,还有倍频的出现.      

On the Composition of the Solar Interior Rapporteur Paper I

Standard solar models, although they are free from the influence of much of the fluid motion that is bound to be present in the Sun, have been shown by helioseismology to represent the spherically averaged structure of the Sun amazingly well. This state of affairs has come about after painstaking refinements by a great many people of the pertinent microphysics, including that which controls the equation of state, the opacity, the nuclear reaction rates and the diffusion that inhibits gravitational segregation of chemical elements. It has instilled confidence in the modellers in being able to predict the composition of the solar interior. But there are consequences of the flow, related particularly to redistribution of chemical species, that can be difficult to identify observationally, yet which may degrade any inferences we might make. Their potential presence must at least be acknowledged by anyone who tries to asses the reliability of the models. This report summarizes the discussions in the preceding pages of this volume of the current theoretical and observational status of the subject, pointing to many of the caveats that have been raised, and attempting at the same time to put them into a seemingly coherent discourse in the context of our present understanding of the workings of the solar interior. This revised version was published online in June 2006 with corrections to the Cover Date.     

Microphysics: Equation of State

The equation of state is one of the three fundamental ingredients used to construct stellar models. The plasma of the interiors of stars such as the Sun is only slightly non-ideal. However, the extraordinary accuracy of the helioseismological data requires refined equations of state. It turned out to be necessary to include a Coulomb correction, commonly evaluated in the Debye-Hückel approximation. Higher-order non-ideal effects have implications as well, both for plasma physics and for solar physics. As a typical example, the recently studied thermodynamic consequence of excited states in compound particles is discussed. This effect is of considerable relevance in the helioseismic determination of the helium abundance in the solar convection zone. This revised version was published online in June 2006 with corrections to the Cover Date.