Old tail lobes effect on the solar-wind – Magnetosphere energy transport for the 27 August 2001 substorm

The magnetic flux of tail lobes Ψ is divided in two parts of comparable values Ψ₁ and Ψ₀₂, with the first that appears during substorm and the second, observed before substorm start. The first was named “new magnetic flux”, the second – “old magnetic flux”. The first, Ψ₁, is known to play a definitive role in the energy transport from the solar wind into the magnetosphere-ionosphere-atmosphere system, but the role of Ψ₀₂ in this transport is not well known. From the 27 August 2001 substorm data we study the involvement in the above transport process of the old flux Ψ₀₂. This involvement is observed in the polar cap (PC) area, which existed prior to the substorm and is called respectively “the old PC”. In this study, as distinct from earlier works, we use the balance equation of the energy stored in magnetosphere and energy consumed. Activation of the old PC magnetic flux Ψ₀₂ was found to increase the energy input by ∼85% in the event under consideration.     

基于分布式自适应的多智能体容错一致性控制

针对"领航者-跟随者"的多智能体编队，由于领航者系统出现故障引起编队通讯中断而不能完成任务的问题，提出了一种基于一致性理论的分布式自适应控制方法，用于解决该问题。首先，以一个位于顶点的智能体作为领航者，其余3个位于同一条线上的智能体作为跟随者，由此所构成的三角形编队作为被控对象。其中，领航者速度方向作为编队的前行方向，跟随者位于领航者之后。其次，基于图论，对智能体局部信息参数进行分布式自适应更新，并设计分布式自适应控制律，用于弥补多智能体编队中领航者故障所造成的影响。同时，根据相邻智能体的局部信息，设计整体分布式自适应容错控制律，进一步通过构建合理的Lyapunov函数，证明所设计控制器的稳定性，以及"领航者-跟随者"之间相对横向以及相对纵向的距离误差均收敛于固定常数。最后，仿真验证表明：所提出的自适应控制方法具有良好的鲁棒性，这也为工程实践提供了理论依据。     

运载火箭加速度计反馈主动减载实施效果评价

针对运载火箭加速度计反馈主动减载实施效果评价,提出一种基于主动减载姿态动力学稳态分析的评价方法,在传统的“载荷侧滑角”评价指标基础上增加了“姿态偏差”、“摆角需求”和“弹道偏离”评价。稳态分析中考虑了结构干扰的偏置效应以及质心运动对风的抵消效应,重点推导了风切变对于火箭姿态动力学特征参数的影响机理。某型号案例分析结果表明,在典型“平稳风+切变风”风场作用下,主动减载技术在4项评价指标上均取得理想实施效果,并且显著缓解风切变导致的姿态参数快变现象。     

航空发动机压气机静子通道压力信号时频特征

进行发动机整机试验,获取了压气机第一级静子通道内的压力信号.通过时频分析,从压力信号中辨识出了以550 Hz和2200 Hz为中心的时频结构;辨识出了压气机前3级转子叶片通过频率信号及它们的一些和频、差频信号.同时,还观察到在试验发动机减速过程中,放气带打开前,压气机前3级转子的叶片通过频率信号及它们的一些和频、差频信号幅度显著增强,这表明减速过程中压气机第一级转子尖区的流动分离逐渐趋于严重.因此,监控压气机静子通道压力信号时频特征的变化,可以获得特定的压气机转子的流场信息,从而为压气机稳定性控制提供重要依据.      

空天飞行器多源容错鲁棒组合导航系统设计

空天飞行器具有机动灵活、高速飞行和实时打击等特点,为保证空天飞行器在各种复杂飞行工况下导航系统的精度、可靠性与鲁棒性,构建了包含惯性导航、卫星导航与天文导航的多源容错鲁棒组合导航系统。针对空间复杂电磁环境造成的在非线性系统中量测噪声非高斯分布的问题,设计了一种基于Huber定则的鲁棒多传感器信息融合方法;针对高动态与GNSS信号受干扰及欺骗等情况下,卫导信号异常、失锁与星图拖尾等问题,设计了故障诊断与滤波器重构策略。仿真结果表明,所设计的多源容错鲁棒组合导航系统在复杂动态环境下能够有效提高导航系统的精度与容错能力,为空天飞行器导航系统设计提供了有效参考。     

等离子体激励抑制翼型失速分离的实验研究

进行了低速、低雷诺数条件下等离子体激励抑制NACA0015翼型失速分离的实验研究,研究了等离子体激励电压、激励电极数目和激励位置对流动分离抑制效果的影响.在翼型吸力面敷设不对称电极布局的等离子体激励器.在来流速度为4.27m/s,雷诺数为4.96×104的情况下,未施加等离子体激励时,从攻角为9°起翼型吸力面发生显著的前缘流动分离;施加等离子体激励后,流动分离在攻角小于26°的情况下均能很好地重附到翼型吸力面表面.实验表明,流动分离越严重,对等离子体激励的强度要求也越高,等离子体激励的电压和电极组数也必须相应增大;给定的流动分离状态下,等离子体激励的电压和电极组数存在一个阈值;等离子体激励的最佳位置在流动分离起始点的前缘;雷诺数增大后,流动分离更难抑制.     

轴流式压气机近失速状态端壁流动时频分析

为准确辨识某型单轴涡喷发动机压气机近失速点的流动特征,对其端壁静压信号进行了时频分析。时频分析结果表明,近失速点的工况下,与其它各级相比,压气机第一级静子机匣壁面流动变化最为显著;随着发动机工作点沿共同工作线趋近喘振边界,压气机第一级静子机匣壁面静压信号中以550Hz为中心的宽带信号开始出现并逐步增强。所发现的压气机端壁流态特征可用于发动机节流过程中工作点接近失速边界的程度的判定,具有一定的工程应用价值。      

Critical Issues on Magnetic Reconnection in Space Plasmas

The idea of expedient energy transformation by magnetic reconnection (MR) has generated much enthusiasm in the space plasma community. The early concept of MR, which was envisioned for the solar flare phenomenon in a simple two-dimensional (2D) steady-state situation, is in dire need for extension to encompass three-dimensional (3D) non-steady-state phenomena prevalent in space plasmas in nature like in the magnetosphere. A workshop was organized to address this and related critical issues on MR. The essential outcome of this workshop is summarized in this review. After a brief evaluation on the pros and cons of existing definitions of MR, we propose essentially a working definition that can be used to identify MR in transient and spatially localized phenomena. The word “essentially” reflects a slight diversity in the opinion on how transient and localized 3D MR process might be defined. MR is defined here as a process with the following characteristics: (1) there is a plasma bulk flow across a boundary separating regions with topologically different magnetic field lines if projected on the plane of MR, thereby converting magnetic energy into kinetic particle energy, (2) there can be an out-of-the-plane magnetic field component (the so-called guide field) present such that the reconnected magnetic flux tubes are twisted to form flux ropes, and (3) the region exhibiting non-ideal MHD conditions should be localized to a scale comparable to the ion inertial length in the direction of the plasma inflow velocity. This definition captures the most important 3D aspects and preserves many essential characteristics of the 2D case. It may be considered as the first step in the generalization of the traditional 2D concept. As a demonstration on the utility of this definition, we apply it to identify MR associated with plasma phenomena in the dayside magnetopause and nightside magnetotail of the Earth’s magnetosphere. How MR may be distinguished from other competing mechanisms for these magnetospheric phenomena are then discussed.This revised version was published online in July 2005 with a corrected cover date.