Driving major solar flares and eruptions: A review

This review focuses on the processes that energize and trigger M- and X-class solar flares and associated flux-rope destabilizations. Numerical modeling of specific solar regions is hampered by uncertain coronal-field reconstructions and by poorly understood magnetic reconnection; these limitations result in uncertain estimates of field topology, energy, and helicity. The primary advances in understanding field destabilizations therefore come from the combination of generic numerical experiments with interpretation of sets of observations. These suggest a critical role for the emergence of twisted flux ropes into pre-existing strong field for many, if not all, of the active regions that produce M- or X-class flares. The flux and internal twist of the emerging ropes appear to play as important a role in determining whether an eruption will develop predominantly as flare, confined eruption, or CME, as do the properties of the embedding field. Based on reviewed literature, I outline a scenario for major flares and eruptions that combines flux-rope emergence, mass draining, near-surface reconnection, and the interaction with the surrounding field. Whether deterministic forecasting is in principle possible remains to be seen: to date no reliable such forecasts can be made. Large-sample studies based on long-duration, comprehensive observations of active regions from their emergence through their flaring phase are needed to help us better understand these complex phenomena.     

基于非线性摩擦模型参数观测器的自适应摩擦补偿方法的研究

通过摩擦补偿的分析提出了一种基于非线性摩擦模型参数观测器的自适应摩擦补偿方法,从工程实用角度出发采用的是库仑加粘滞的摩擦模型,设计了两个观测器实现对库仑摩擦系数和粘滞摩擦系数的估计,并用MATLAB软件对转台工作状态进行了仿真,结果表明此观测器有良好的自适应补偿性能。     

转动帆板红外热流计算及等效方法研究

目前的空间外热流分析软件和在航天器稳态热平衡试验中模拟的外热流都不包括帆板对航天器表面的红外加热,而有时帆板的红外加热并不小,应该叠加到模拟的外热流中.文章针对一种低轨道航天器,计算了帆板红外加热的强度,给出了在热平衡试验中叠加的方法,并讨论了在固定帆板方位的同时保持其红外热流等效的可能性.结果表明,可以精确计算帆板红外加热,对任意的帆板方位均可以保持其红外加热的等效.     

切向结构永磁同步电机中磁钢厚度对性能的影响

提出了切向结构永磁同步电机中磁钢厚度的约束条件;依据电机学理论并结合有限元计算方法,研究了气隙长度恒定时不同极对数下气隙磁密、每极磁通与磁钢厚度的关系,探讨了磁钢厚度对电机的过载能力、铁耗等性能的影响;在气隙长度发生变化时,为了保证漏磁大小不变,讨论了气隙与非导磁衬套厚度、磁钢厚度的关系。并指出:(1)气隙恒定时,随着磁钢厚度的增加,不同极对数时磁钢体积增大所提供的磁势对每极磁通的影响有所不同;铁耗和过载能力随磁钢厚度的增加而增大。(2)气隙增大时,为了保证气隙磁密和漏磁不变,必须增加非导磁衬套的厚度。(3)极对数增加时,减小磁钢厚度能提高电机的性价比。     

基于反电势形状函数法的无刷直流电动机直接转矩控制

采用两相导通模式时通过逆变器开关状态不能确定电压空间矢量,现有方案是通过实时测量3个相电压来解决这一问题,但系统变得复杂;此外现有方案在转矩观测中包含的微分项会降低控制精度,增大计算量,影响系统实时性。针对这两点不足,提出反电势形状函数法,在软件中实现了相电压的实时计算,使转矩观测变得简洁,更易于工程实用。最后给出的仿真与实验结果证明了反电势形状函数法用于无刷直流电机直接转矩控制中的可行性与有效性。     

Investigation of Hypervelocity Impacts on Retrieved Surfaces by Direct Simulation Monte Carlo

Hypervelocity impacts on the retrieved Hubble Space Telescope (HST) solar array was investigated by our extended Direct Simulation Monte Carlo (DSMC) model and the result matches well with the measured data in most of the particle mass range. The revelation of the altitude dependence of particles flux onto the retrieved surfaces provides some insight in understanding the observed higher flux onto Mir space station relative to that onto Long Duration Exposure Facility (LDEF). Our analysis suggests that a slightly higher primary flux onto Mir space station would be possible even without taking into account the secondary impacts, as a result of the existence of the highly eccentric orbits of small-sized debris. It is, furthermore, predicted that 43% of the measured impact flux onto Mir station in PIE experiment may be from secondary impacts, and a corresponding 7% for the detectors in Echantillions experiment.     

基于扰动观测器的无人机固定时间编队协同控制

针对无人机的编队控制问题,基于虚拟领航者编队方法,提出了 1种基于固定时间超螺旋干扰观测器的反步控制策略。首先,设计了 1种固定时间超螺旋扰动观测器,以保证在固定时间内,对无人机编队机动所受扰动的快速观测;其次,针对编队控制问题,设计了基于超螺旋扰动观测器的反步控制策略,该控制器显著降低了抖振效应;然后,使用李雅普诺夫理论和固定时间理论,分析了控制策略的固定时间稳定性;最后,通过仿真算例验证了所提出的控制策略的有效性与可行性。     

基于快速模糊干扰观测器的UASV再入Terminal滑模控制

针对无人空天飞行器再人大气层过程中气动参数变化剧烈、控制精度要求高的特点，设计了基于快速模糊干扰观测器的Terminal滑模控制方案。通过改进传统模糊干扰观测器的学习律，提出一种快速模糊干扰观测器，增强了其在线逼近干扰及系统不确定的能力。Terminal滑模的有限时间收敛特性提高了系统跟踪速度，同时采用快速模糊干扰观测器消除全部扰动的影响，从而保证了飞行品质。最后，仿真结果表明了快速模糊干扰观测器的优越性及闭环控制方案的有效性。     

机载单站无源定位三维模型及其仿真

针对在空间作匀速直线运动的目标，建立了机载单站无源定位的三维模型。给出了其中的预处理过程和系统状态方程，并采用UKF算法进行滤波处理以提高定位精度。仿真结果表明，模型和算法有效。与扩展卡尔曼滤波(EKF)相比，在初始误差较大时UKF也能快速收敛。     

关于鲁棒Kx观测器设计的几个问题

对于具有结构不确定性的线性系统,本文研究了与Kx观测器设计有关的几个问题。文中建立了观测器应满足的条件,并对控制器设计时的分离原理和闭环系统的鲁棒性进行了讨论。