An experimental study of the dual-loop control of electro-hydraulic load simulator （EHLS）

This paper investigates motion coupling disturbance（the so called surplus torque）in the hardware-in-the-loop（HIL）experiments.The＇＇velocity synchronization scheme＇＇was proposed by Jiao for an electro-hydraulic load simulator（EHLS）in 2004.In some situations,however,the scheme is limited in the implementation for certain reasons,as is the case when the actuator＇s valve signal is not available or it is seriously polluted by noise.To solve these problems,a＇＇dual-loop scheme＇＇is developed for EHLS.The dual-loop scheme is a combination of a torque loop and a position synchronization loop.The role of the position synchronization loop is to decouple the motion disturbance caused by the actuator system.To verify the feasibility and effectiveness of the proposed scheme,extensive simulations are performed using AMESim.Then,the performance of the developed method is validated by experiments.     

Formation control using μ-synthesis for Inner-Formation Gravity Measurement Satellite System

Inner-Formation Gravity Measurement Satellite System (IFGMSS) is used to map the gravity field of Earth. The IFGMSS consists of two satellites in which one is called “inner satellite” and the other one is named as “outer satellite”. To measure the pure Earth gravity, the inner satellite is located in the cavity of the outer satellite. Because of the shield effect of the cavity, the inner satellite is affected only by the gravitational force, so it can sense Earth gravity precisely. To avoid the collision between the inner satellite and the outer satellite, it is best to perform a real-time control on the outer satellite. In orbit, the mass of the outer satellite decreases with the consumption of its propellant. The orbit angular rate of the inner satellite varies with time due to various disturbing forces. These two parameters’ uncertainties make the C–W function be not so accurate to describe the formation behavior of these two satellites. Furthermore, the thrusters also have some uncertainties due to the unmodelled dynamics. To cancel the effects caused by the above uncertainties, we have studied the robust control method based on the μ-synthesis. This μ-synthesis eliminates the conservativeness and improves the control efficiency comparing with the H_∞ method. Finally, to test the control method, we simulate an IFGMSS mission in which the satellite runs in a sun synchronous circular orbit with an altitude of 300 km. The simulation results show the effectiveness of the robust control method. The performances of the closed-loop system with the μ-controller are tested by the μ-analysis. It has found that the nominal performance, the robust stability and the robust performance are all achieved. The transient simulation results further prove the control response is fast and the accuracy of the relative position meets the demand of the gravity measurement.     

航天器控制软件可靠性工程方法研究

当前航天器控制软件的复杂度越来越高,软件的规模十分庞大,对软件可靠性安全性要求极高,因此对航天器控制软件的可靠性设计和度量具有重要意义.介绍和分析适用于航天器控制软件的可靠性设计方法,并结合某型号给出实际的软件设计以及可靠性度量的具体实例.     

基于增量谐波平衡法的流量调节器非线性频率特性

针对多个状态变量、非线性关系复杂、方程刚性强的流量调节器系统,应用增量谐波平衡法研究了调节器在入口压力扰动下的强迫振荡问题,得到了系统周期解的解析表达式。通过与龙格库塔数值仿真结果相比较,验证了增量谐波平衡法应用于该系统的有效性,且计算量相对较小。进而在频域内探讨了流量调节器系统的非线性频响特性,结果表明,随着扰动振幅的增大,幅频响应在整个频率范围上都有所增大。计算结果可以用于评估线性化方法的误差范围。通过分析周期解的时均值与稳态值的差别,揭示了调节器受上游压力周期扰动时,其出口流量的时均值略低于稳态值的非线性特性。     

Effect of the Interplanetary Electric Field on the Magnetopause From Global MHD Simulations

The north-south component B_z of the Interplanetary Magnetic Field (IMF) and solar wind dynamic pressure P_d are generally treated as the two main factors in the solar wind that determine the geometry of the magnetosphere. By using the 3D global MHD simulations, we investigate the effect of the Interplanetary Electric Field (IEF) on the size and shape of magnetopause quantitatively. Our numerical experiments confirm that the geometry of the magnetopause are mainly determined by P_dB_z, as expected. However, the dawn-dusk IEFs have great impact on the magnetopause erosion because of the magnetic reconnection, thus affecting the size and shape of the magnetopause. Higher solar wind speed with the same B_z will lead to bigger dawn-dusk IEFs, which means the higher reconnection rate, and then results in more magnetic flux removal from the dayside. Consequently, the dayside magnetopause moves inward and flank magnetopause moves outward.      

极端太阳风条件下的磁层顶位形

基于极端太阳风条件下的三维MHD数值模拟数据, 构建了一种极端太阳风条件下的三维非对称磁层顶位形模型. 所提出的模型考虑了行星际南向磁场(IMF) B_z日下点距离侵蚀的饱和效应, 太阳风动压B_d对磁层顶张角影响的饱和效应, 赤道面、昼夜子午面磁层顶的不对称性以及极尖区的内凹结构和内凹中心的移动, 并利用Levenberg-Marquart多参量非线性拟合方法拟合了模型参数. 数值模拟研究表明, 在极端太阳风条件下, 随B_d增大, 磁层顶日下点距离减小, 磁层顶磁尾张角几乎不变; 随南向(IMF)B_z增大, 磁层顶日下点距离略有减小, 磁层顶磁尾张角减小, 极尖区内凹中心向低纬移动. 通过对2010年8月1日太阳风暴事件验证发现, 本文所建立的模型能够描述极端太阳风条件下的三维磁层顶位形.      

面向星敏感器测试的数字星模系统设计

分析星敏感器和数字星模系统的功能,描述数字星模系统的功能需求,提出数字星模系统的设计方法．数字星模系统由星图组件和通信组件组成,基于该系统,针对星敏感器进行静态和动态星图测试试验,并对试验的方法和结果进行分析说明．试验表明数字星模系统及其设计方法的正确性、有效性．     

考虑管路的飞机液压刹车系统压力振荡分析

飞机液压刹车系统通常采用压力伺服阀控制刹车压力,由于布局限制,压力伺服阀和刹车作动器之间往往存在较长的液压管路.管路会给系统引入欠阻尼的频率特性,而且该特性会与压力伺服阀固有的局部压力闭环结构相耦合,使得压力伺服阀的输出压力容易出现振荡、失稳现象.因此通过在飞机液压刹车系统建模中考虑管路模型,在频域上分析了压力伺服阀与管路、容腔耦合的现象和原因,具体给出了管路参数和油液参数变化对压力闭环的影响,并通过时域仿真进一步验证了频域分析的结论.同时分析了匹配设计管路、增加系统阻尼和降低系统增益3种避免压力闭环控制振荡失稳的方法.为飞机液压刹车系统的设计与优化提供了理论参考依据.      

一种舰载反导的复合干扰模式

在质心干扰的基础上,提出关于"距拖干扰+箔条干扰"的复合型干扰模式。通过提前布放箔条陷阱,利用距离门拖引干扰技术,完善原有质心干扰的性能,并将其运用于多目标导弹来袭的态势中。通过运筹学中排队论等相关知识的推论、证明,验证了这种舰载反导策略具有较高的可行性和实践性。     

一种月球样品容器承力结构的改进设计

月球取样是我国探月工程三期的核心计划内容,月球样品容器是获取样品的关键部件之一,月球样品容器在整个飞行过程中要经受各种复杂动力学环境,它的承力结构是保证样品容器不会因力学环境而失效。为了减轻重量,样品容器采用了一种框架式承力结构,本文对这种承力结构的设计进行了改进,通过理论分析和仿真验证,证明了这种改进后的承力结构的合理性。