可重构零空间控制分配算法及流程规划

针对飞机正常情况和舵面故障情况下的控制分配算法展开研究。根据控制效能矩阵的特点设计了性能指标,并给出了对应的最优逆控制。对带约束的一般控制分配问题,采用零空间横截方法进行了再分配。设计了针对舵面卡死故障的重构控制律。结合某飞机仿真平台,进行了卡死故障的重构仿真,结果表明,控制分配算法能够在故障状态下完成对指令的精确跟踪。     

基于模型的系统工程在作动器领域的应用研究

以飞机作动器产品为研究对象,通过条目化需求分析,将产品设计过程进行逐级分解。利用AMESim、AN-SYS系列软件等仿真工具,建立从部件到产品的各级仿真模型,并开展仿真分析工作,通过对仿真分析过程和结果的分析,探索了基于模型的系统工程方法的工作流程,总结了飞机液压作动器基于模型的系统工程方法的应用基础。     

Modeling Multifractality of the Solar Wind

The question of multifractality is of great importance because it allows us to investigate interplanetary hydromagnetic turbulence. The multifractal spectrum has been investigated with Voyager (magnetic field) data in the outer heliosphere and with Helios (plasma) data in the inner heliosphere. We use the Grassberger and Procaccia method that allows calculation of the generalized dimensions of the solar wind attractor in the phase space directly from the cleaned experimental signal. We analyze time series of plasma parameters of the low-speed streams of the solar wind measured in situ by Helios in the inner heliosphere. The resulting spectrum of dimensions shows a multifractal structure of the solar wind attractor. In order to quantify that multifractality, we use a simple analytical model of the dynamical system. Namely, we consider the generalized self-similar baker’s map with two parameters describing uniform compression and natural invariant measure on the attractor of the system. The action of this map exhibits stretching and folding properties leading to sensitive dependence on initial conditions. The obtained solar wind singularity spectrum is consistent with that for the multifractal measure on the weighted baker’s map.     

Shear Flow Instabilities in Low-Beta Space Plasmas

We study instabilities driven by a sheared plasma flow in the low-frequency domain. Two unstable branches are found: the ion-sound mode and the kinetic Alfvén mode. Both instabilities are aperiodic. The ion-sound instability does not depend on the plasma β (gas/magnetic pressure ratio) and has a maximum growth rate of about 0.1 of the velocity gradient dV ₀/dx. On the other hand, the kinetic Alfvén instability is stronger for larger β and dominates the ion-sound instability for β > 0.05. Possible applications for space plasmas are shortly discussed.     

Complexity,Forced and/or Self-Organized Criticality,and Topological Phase Transitions in Space Plasmas

The first definitive observation that provided convincing evidence indicating certain turbulent space plasma processes are in states of ‘complexity’ was the discovery of the apparent power-law probability distribution of solar flare intensities. Recent statistical studies of complexity in space plasmas came from the AE index, UVI auroral imagery, and in-situ measurements related to the dynamics of the plasma sheet in the Earth's magnetotail and the auroral zone. In this review, we describe a theory of dynamical ‘complexity’ for space plasma systems far from equilibrium. We demonstrate that the sporadic and localized interactions of magnetic coherent structures are the origin of ‘complexity’ in space plasmas. Such interactions generate the anomalous diffusion, transport, acceleration, and evolution of the macroscopic states of the overall dynamical systems. Several illustrative examples are considered. These include: the dynamical multi- and cross-scale interactions of the macro-and kinetic coherent structures in a sheared magnetic field geometry, the preferential acceleration of the bursty bulk flows in the plasma sheet, and the onset of ‘fluctuation induced nonlinear instabilities’ that can lead to magnetic reconfigurations. The technique of dynamical renormalization group is introduced and applied to the study of two-dimensional intermittent MHD fluctuations and an analogous modified forest-fire model exhibiting forced and/or self-organized criticality [FSOC] and other types of topological phase transitions. This revised version was published online in August 2006 with corrections to the Cover Date.     

Effect of q-nonextensive hot electrons on bifurcations of nonlinear and supernonlinear ion-acoustic periodic waves

Nonlinear and supernonlinear ion-acoustic periodic waves are investigated in a three-component unmagnetized plasma which consists of mobile fluid cold ions, Maxwellian cold electrons and q-nonextensive hot electrons employing phase plane analysis. Using the traveling wave transformation, the plasma system is reduced to a planar autonomous dynamical system. Utilizing phase plane analysis of planar dynamical systems, all possible phase portraits including nonlinear homoclinic orbit, nonlinear periodic orbit, supernonlinear homoclinic orbit and supernonlinear periodic orbit are presented depending on physical parameters $q,\alpha ,\sigma$ and V. Using numerical simulations, nonlinear and supernonlinear ion-acoustic periodic waves are shown for different conditions. It is found that the nonextensive parameter q plays a crucial role in the bifurcations of nonlinear and supernonlinear ion-acoustic periodic waves. Our study may be applicable to understand the nonlinear and supernonlinear periodic features in auroral plasma.     

面向深空探测的电磁帆推进技术研究进展

电磁帆是一类利用太阳风驱动的无工质或少工质新型推进技术,在需要推力器长时间工作的深空探测任务中具有非常广阔的应用前景。首先介绍了电磁帆的基本概念和主要分类,其次分别介绍了电帆、纯磁帆和磁等离子体帆三类推进方式的系统组成和工作原理,重点介绍了各自的研究现状,并梳理出了相关关键技术,同时介绍了等离子体磁罩技术。最后对电磁帆推进技术研究进展进行了总结,为国内开展此方面研究提供了研究方向和发展思路。     

微等离子体转化二氧化碳发射光谱诊断

火星大气层的主要成分为二氧化碳，如果能够利用低温等离子体方法高效分解二氧化碳，使其转化为氧气和一氧化碳加以利用，可以大幅降低航天员生命保障相关载荷长途运输的成本，进一步提高生命保障能力。低温等离子体放电过程中会产生大量活性组分，可以在数百度温度下实现二氧化碳的高效解离，是具有很大潜力的二氧化碳解离与转化方式。设计了一种尺度在亚毫米级、功率输入为数瓦的直流微槽等离子体反应器，可以在较低气体温度下实现二氧化碳分解。测量了反应器电流、功率等放电参数，采用发射光谱确定了体系中激发态组分，分析了激发态粒子谱线强度随输入电压、稀释气体比例等反应器工作参数变化，利用氮气分子振转谱带测量了等离子体放电区振动温度和气体温度。研究表明，添加氩、氦、氮气均可以增强二氧化碳的分解，添加氦气可以促进二氧化碳的电离过程。稀释气体激发态因具有高能量，可以通过潘宁解离通道增强二氧化碳分解。氦组分激发态的能量高于二氧化碳电离能，可以促进二氧化碳的电离反应。微等离子体内存在强烈的振动 平动非平衡现象：振动温度约为4400~4800K，而气体温度仅为450 ~600K，表明可以通过合理的放电和结构设计，定向将能量注入到振动态，从而进一步促进二氧化碳的振动解离。     

基于滑模变结构和扩张状态观测器的电动舵机复合控制方法

为提高电动舵机伺服系统的鲁棒性,同时解决实际工作中电动舵机不确定负载引起的跟踪精度低的问题,提出了一种采用指数趋近率的滑模变结构控制率结合扩张状态观测器对负载扰动进行实时估计的电动舵机的伺服控制方法,给出了控制器设计方法和试验验证。仿真和试验结果表明,与常规的滑模控制器相比,采用扩张状态观测器的变结构控制能有效提高电动舵机的跟踪性能。     

直升机后缘襟翼驱动器迟滞现象仿真与抑制

直升机后缘襟翼多采用压电驱动器作为驱动元件，但是在使用过程中压电驱动器迟滞会对其振动控制性能产生不利影响，因此针对压电驱动器迟滞开展了迟滞建模与抑制研究。通过实验研究了压电驱动器在不同驱动频率下的迟滞特性，采用Bouc-Wen模型对驱动器迟滞现象进行了建模，并采用粒子群算法（PSO）辨识模型参数，与实际测量迟滞曲线进行了对比，在10~60 Hz范围内所建立的迟滞模型能够较为精确地描述压电驱动器迟滞现象。建立了基于Bouc-Wen逆模型的前馈补偿控制与PID反馈控制相结合的复合控制策略，实验结果显示该控制策略能够在10~60 Hz较宽的频率范围内有效抑制该压电驱动器迟滞现象。建立了考虑驱动器迟滞的主动控制后缘襟翼振动控制动力学模型，并对中等速度稳态前飞条件下后缘襟翼振动控制性能进行了仿真，仿真结果显示驱动器迟滞会在一定程度上削弱振动控制性能，而采用复合控制可以提高后缘襟翼旋翼振动控制性能。