自适应飞机驾驶员最优控制模型研究及应用

针对驾驶员最优控制模型(OCM)无法反映飞行员在未知环境下渐进适应过程这一缺点,采用自适应状态估计理论对OCM进行改进,建立了基于自适应状态估计的驾驶员最优控制模型(MOCM-AE),给出了算法流程。通过对比飞行试验数据和未知扰动下的着舰应用,对模型进行了评估。通过人机闭环仿真进行了飞行试验再现,得到了人机闭环频域曲线。对比结果表明,与OCM相比MOCM-AE的频域特性曲线与试验更为吻合。在着舰应用中,引入低空紊流作为未知扰动进行着舰仿真,结果表明OCM强烈依赖于先验经验,而MOCM-AE无论是否具有先验经验,无论是否存在未知扰动,均能取得良好着舰效果。在未知扰动和舰尾流影响下,MOCM-AE比传统OCM着舰精度提高59%,着舰点分布范围缩小29%,这体现了飞行员对未知环境的适应能力。     

一种超薄反作用飞轮的大面积磁悬浮结构分析

为提高轴向磁通反作用飞轮的轴向刚度和寿命,结合轴向磁通飞轮的结构,提出一种超薄、大面积磁悬浮的反作用飞轮。重点分析该飞轮的大面积磁悬浮结构,从磁环的宽度、磁环的充磁方向、磁环间距、铁芯厚度和磁悬浮刚度五个方面展开研究。通过有限元仿真可以发现：随磁环宽度的增加,定子对转子的斥力是先增大后减小;定子内外环磁化方向相反时比相同时能得到更大的斥力;在内外环磁化方向相反时,内外环磁钢间距越小,定子对转子斥力越大;磁悬浮部分铁芯厚度的减小对定转子间的斥力的影响极其有限,但对降低飞轮重量具有重要意义;磁悬浮的刚度与转子偏离中心的距离近似成正比。     

基于改进差分进化算法的飞行控制律评估方法

 针对基本差分进化(DE)算法收敛慢、易陷入局部最优的问题,提出了基于混沌理论(CT)与高斯扰动的DE算法,进而通过典型测试函数仿真证明了该方法在收敛速度与全局搜索能力方面均优于基本型和其他改进型DE算法。在此基础上构建了基于DE算法的飞行控制律评估流程与实施步骤。实例表明,该方法克服了传统评估方法的缺陷,可在全飞行包线范围内及所有可预测参数摄动情况下对飞行控制律进行快速、准确的评估。     

基于非奇异终端滑模的复合控制导弹反演设计

针对轨控式复合控制导弹制导末端的姿态控制问题,结合反演控制、二阶非奇异终端滑模和非线性干扰观测器技术,设计了一种新的反演滑模姿态控制方法.在反演设计的第一步采用动态面法,避免了传统反演设计存在的“计算膨胀”问题,并使姿态角跟踪误差收敛至原点附近任意小的邻域内;第二步设计引入了二阶非奇异终端滑模,使得角速率跟踪误差在有限时间内收敛至零,同时消除控制量的抖振现象.采用非线性干扰观测器补偿系统不确定性,并基于Lyapunov稳定性理论证明了闭环系统所有误差信号最终有界.仿真结果表明了所设计的轨控式复合控制导弹制导末端姿态控制方案的正确性与有效性.     

Magnetic reconnection on the Sun: ESPD Senior Prize Lecture

Magnetic reconnection is a fundamental process for changing the magnetic topology and converting magnetic energy into other forms on the Sun, such as heat, flow energy and fast particle energy. In two dimensions it is fairly well understood, although some aspects still need to be developed. In three dimensions, it behaves very differently and a substantial body of theory and numerical experiment has now been built up, including reconnection at null points, separators and quasi-separators.Some aspects of solar flares can be understood with 2D reconnection models, but other aspects such as the shapes of flare ribbons, the acceleration of particles and the creation of twist in erupting flux ropes need a 3D understanding. A paradigm shift in our understanding of coronal heating by reconnection has been stimulated by dramatic new observations of photospheric flux cancellation from SUNRISE and from SST together with the realisation that it may well be driving nanoflare heating events and possibly campfires.     

Variations in cosmic ray cutoff rigidities during the great geomagnetic storm of November 2004

A very strong interplanetary and magnetospheric disturbance observed on 7–13 November 2004 can be regarded as one of the strongest events during the entire period of space observations. In this paper we report on the studies of cosmic ray cutoff rigidity variations during 7–13 November 2004 showing how storm conditions can affect the direct cosmic ray access to the inner magnetosphere. Effective cutoff rigidities have been calculated for selected points on the ground by tracing trajectories of cosmic ray particles through the magnetospheric magnetic field of the “storm-oriented” Tsyganenko 2003 model. Cutoff rigidity variations have also been determined by the spectrographic global survey method on the basis of experimental data of the neutron monitor network. Relations between the calculated and experimental cutoff rigidities and the geomagnetic Dst-index and interplanetary parameters have been investigated. Correlation coefficients between the cutoff rigidities obtained by the trajectory tracing method and the spectrographic global survey method have been found to be in the limits 0.76–0.89 for all stations except the low-latitude station Tokyo (0.35). The most pronounced correlation has been revealed between the cutoff rigidities that exhibited a very large variation of ∼1–1.5 GV during the magnetic storm and the Dst index.     

Symmetry and asymmetry of ionospheric weather at magnetic conjugate points for two midlatitude observatories

Variations of the ionospheric weather W-index for two midlatitude observatories, namely, Grahamstown and Hermanus, and their conjugate counterpart locations in Africa are studied for a period from October 2010 to December 2011. The observatories are located in the longitude sector, which has consistent magnetic equator and geographic equator so that geomagnetic latitudes of the line of force are very close to the corresponding geographic latitudes providing opportunity to ignore the impact of the difference of the gravitational field and the geomagnetic field at the conjugate points on the ionosphere structure and dynamics. The ionosondes of Grahamstown and Hermanus provide data of the critical frequency (foF2), and Global Ionospheric Maps (GIM) provide the total electron content (TECgps) along the magnetic field line up to the conjugate point in the opposite hemisphere. The global model of the ionosphere, International Reference Ionosphere, extended to the plasmasphere altitude of 20,200 km (IRI-Plas) is used to deliver the F2 layer peak parameters from TECgps at the magnetic conjugate area. The evidence is obtained that the electron gas heated by day and cooled by night at the summer hemisphere as compared with the opposite features in the conjugate winter hemisphere testifies on a reversal of plasma fluxes along the magnetic field line by the solar terminator. The ionospheric weather W-index is derived from NmF2 (related with foF2) and TECgps data. It is found that symmetry of W-index behavior in the magnetic conjugate hemispheres is dominant for the equinoxes when plasma movement along the magnetic line of force is imposed on symmetrical background electron density and electron content. Asymmetry of the ionospheric storm effects is observed for solstices when the plasma diffuse down more slowly into the colder winter hemisphere than into the warmer summer hemisphere inducing either plasma increase (positive phase) or decrease (negative phase of W-index) in the ionospheric and plasmaspheric plasma density.     

基于SMDO的滑模控制器设计及其在导弹上的应用

提出了一种基于滑模干扰观测器(SMDO)的滑模控制器(SMC)设计方法.针对一类级联多输入多输出(MI-MO)非线性系统,根据奇异摄动原理将其分为内、外回路分别进行控制器设计.以外回路为例,分析了传统基于饱和函数的滑模控制的鲁棒性,针对其在面I临干扰时鲁棒性较差的问题,在名义滑模控制律的基础上设计了基于超扭曲算法的SM...     

水下重力辅助惯性导航关键技术研究及实现

重力辅助惯性导航已渐成水下导航领域的研究热点,其实现是一项复杂的工程,涉及多项的关键技术.文章首先介绍了重力辅助导航的基本原理;之后详细阐述了在真实海洋环境下,重力辅助导航所需解决的若干关键技术问题,并给出了相应的研究成果;最后总结了我国水下重力辅助导航的发展趋势及研究的若干建议.     

高超声速飞行器自抗扰分数阶PID控制器设计(英文)

自抗扰控制器利用跟踪微分器可解决超调量及快速性之间的矛盾,分数阶PID控制器在提高控制品质的同时扩大了被控系统参数的稳定域。结合自抗扰技术及分数阶PID控制器设计了自抗扰分数阶PID控制器,并应用于高超声速飞行器再入姿态控制。仿真结果表明,自抗扰分数阶PID控制器对于高超声速飞行器非线性模型及强外干扰的影响下具有很好的控制效果,并且有较大的稳定域,即针对被控系统参数变化具有更强的鲁棒性。