刚体卫星姿态的有限时间控制

针对刚体卫星的姿态控制问题,设计了不存在和存在扰动力矩两种条件下的有限时间状态反馈控制律.对于无扰动力矩情形,基于非线性齐次系统性质,设计了一种便于工程实践性的连续、非奇异的比例微分形式控制算法,保证姿态闭环系统有限时间收敛到零点,而且此算法能直接推广到卫星姿态跟踪问题.对于存在扰动力矩的情形,基于有限时间Lyapunov定理设计的连续、非奇异的控制力矩保证卫星姿态和角速度在有限时间内收敛到原点附近的邻域.当外扰力矩为零时,此控制律使闭环系统状态有限时间收敛到平衡点.数学仿真结果说明了提出的控制算法有效.     

Ionospheric F-region response to geomagnetic disturbances

The F2-region reaction to geomagnetic storms usually called as an ionospheric storm is a rather complicated event. It consists of so called positive and negative phases, which have very complicated spatial and temporal behavior. The main morphological features of ionospheric storms and the main processes governing their behavior were understood at the end of the 1900s and described in a series of review papers. During the recent decade there were many publications dedicated to the problem of ionospheric storms. In this paper a concept of ionospheric storm morphology and physics formulated at the end of the 1990s is briefly summarized and the most interesting results obtained in the 2000s are described. It is shown that the main features of the studies of the previous decade were: the use of GPS TEC data for analyzing the ionospheric storm morphology, attraction of sophisticated theoretical models for studying the processes governing ionospheric behavior in disturbed conditions, and accent to analysis of ionospheric behavior during prominent events (very strong and great geomagnetic storms). Also a special attention was paid to the pre-storm enhancements in foF2 and TEC.     

The impact of large solar events on the total electron content of the ionosphere at mid latitudes

Ionospheric disturbances associated with solar activity may occur via two basic mechanisms. The first is related to the direct impact on the ionosphere of EUV photons from a flare, and the second by prompt electric field penetration into the magnetosphere during geomagnetic storms. In this paper we examine the possibility that these two mechanisms may have an impact at mid latitudes by calculating the total electron content (TEC) from GPS stations in Mexico during several large X-ray flares. We have found that indeed large, complex flares, which are well located, may affect the mid latitude ionosphere. In fact, in the solar events of July 14, 2000 and April 2001 storms, ionospheric disturbances were observed to increase up to 138 and 150 TECu, respectively, due to the influence of EUV photons. Also, during the solar events of July 2000, April 2001, Halloween 2003, January 2005 and December 2006, there are large ionospheric disturbances (up to 393 TECu in the Halloween Storms), due to prompt penetration electric field, associated with CME producing geomagnetic storm.     

交互式棱柱网格生成中翘曲现象形成机制及消除算法

在基于径向基函数插值的交互式棱柱网格生成中,当物面网格单元空间法矢变化范围较大或变化剧烈时,棱柱网格生成会发生翘曲问题,降低棱柱网格质量。针对该问题,首先采用DLR-F6机翼外形算例对翘曲现象进行了介绍和初步分析,并结合平板外形棱柱网格生成,通过不同波长推进位移扰动模拟法矢变化对推进位移的影响,研究棱柱网格翘曲现象的形成机制。不同位移扰动下平板棱柱网格生成结果证实边界棱线网格点推进位移不光滑会通过空间插值放大,引起棱柱网格发生翘曲,且网格翘曲的表现形式与推进位移的分布有关。从而间接表明棱柱网格生成中翘曲现象是由法矢变化带来推进位移分布不光滑引起的。然后从翘曲现象的形成机制出发,基于拉普拉斯方法发展了推进位移光顺技术,并通过DLR-F6机翼算例进行了验证。测试结果表明,光顺技术能够完全消除棱柱网格的翘曲,获得光顺的高质量棱柱网格。最后通过DLR-F6翼身组合体外形棱柱网格生成,展示了添加光顺技术的棱柱网格生成算法的应用潜力。     

高精度舰载惯性导航系统的重力影响研究

舰载的高精度惯性导航系统中,重力误差补偿的精度与导航的精度息息相关。长航时舰载导航系统,与短航时惯性导航系统相比,重力扰动随时间积累对导航精度的影响更加明显,因此不能再用简单的重力模型对重力进行近似,而需要对重力扰动误差进行补偿。本文针对舰载高精度惯性导航,理论上推导了重力扰动误差对惯性导航精度的影响,并以北向单通道模型对重力扰动误差与水平定位精度的解析关系式进行验证;进而用simulink仿真验证解析关系式的正确性,并在不同条件下进行了仿真。仿真结果表明：静态条件下,20小时以上的长航时导航中,北向或东向重力扰动分量每增加10mgal时,对应位置误差范围约增加130m。     

仿真转台周期性干扰抑制的研究

提出采用加速度反馈方案,在无需加大系统带宽的情况下提高系统的动态刚度,从而提高了系统对周期性干扰的抑制能力。仿真结果表明,与传统PID控制相比,采用加速度反馈确实能够较好地抑制系统中的周期性干扰。     

电静液作动器自调节积分鲁棒运动控制

针对电静液作动器系统中存在的匹配干扰及不匹配干扰,基于扩张状态观测器,设计了一种自调节积分鲁棒控制方法。首先设计扩张状态观测器估计系统的匹配不确定性并且进行前馈补偿;然后设计自调节积分鲁棒控制器分别处理系统的不匹配干扰和状态估计误差,实现了电静液作动器的渐近跟踪控制;最后通过仿真验证了该控制方案的有效性。结果表明：相较于传统的PID控制器,该控制器的跟踪误差约为0.2mm,控制精度达到0.4%左右。     

基于扩张状态观测器的永磁同步电机自抗扰无源控制

针对传统永磁同步电机滑模控制存在的抖振以及系统抗扰动鲁棒性差问题,提出一种基于扩张状态观测器的永磁同步电机自抗扰无源控制方法。转速外环设计自适应滑模控制器,采用扩张状态观测器对系统干扰项进行观测,用其进行前馈补偿。电流内环将无源控制与自抗扰控制相融合,得到dq旋转坐标系下的电压给定。新型控制方法可有效抑制系统抖振,增强系统鲁棒性。试验结果验证了所提控制方法的有效性和实用性。     

基于自适应方法的多无人机编队队形控制

针对"长机-僚机"近距编队队形因风场扰动而不能保持期望队形的问题,首先,提出了一种自适应队形保持控制的方法,该方法可用于抵消因风场不确定性对无人机的横侧向和前行方向所产生的距离误差,同时能够保持无人机编队稳定飞行。其次,由于风场的不确定性会引起"长机-僚机"之间的动力学发生变化,因此设计了一种基于"长机-僚机"相对运动模型的自适应控制律用以估计风场在3个方向的大小,进而控制无人机之间的相对运动以消除风场不确定性所产生的距离误差并保持速度的一致性,最终实现保持期望的队形。再次,通过构建合理的李雅普诺夫函数,证明无人机编队在风场干扰下能够保持编队稳定飞行,同时"长机-僚机"之间相对横向、横侧向以及纵向的距离误差均接近零。最后,通过仿真验证：所提出的自适应控制方法具有良好的鲁棒性,这为工程实践提供理论依据。     

Global characteristics of ionospheric electric fields and disturbances during the first hours of magnetic storms

The ionospheric plasma density can be significantly disturbed during magnetic storms. In the conventional scenario of ionospheric storms, the negative storm phases with plasma density decreases are caused by neutral composition changes, and the positive storm phases with plasma density increases are often related to atmospheric gravity waves. However, recent studies show that the global redistribution of the ionospheric plasma is dominated primarily by electric fields during the first hours of magnetic storms. In this paper, we present the measurements of ionospheric disturbances by the DMSP satellites and GPS network during the magnetic storm on 6 April 2000. The DMSP measurements include the F region ion velocity and density at the altitude of ∼840 km, and the GPS receiver network provides total electron content (TEC) measurements. The storm-time ionospheric disturbances show the following characteristics. The plasma density is deeply depleted in a latitudinal range of ∼20° over the equatorial region in the evening sector, and the depletions represent plasma bubbles. The ionospheric plasma density at middle latitudes (20°–40° magnetic latitudes) is significantly increased. The dayside TEC is increased simultaneously over a large latitudinal range. An enhanced TEC band forms in the afternoon sector, goes through the cusp region, and enters the polar cap. All the observed ionospheric disturbances occur within 1–5 h from the storm sudden commencement. The observations suggest that penetration electric fields play a major role in the rapid generation of equatorial plasma bubbles and the simultaneous increases of the dayside TEC within the first 2 h during the storm main phase. The ionospheric disturbances at later times may be caused by the combination of penetration electric fields and neutral wind dynamo process.