子母弹抛壳过程非定常流动的数值模拟

利用弹簧近似和网格重构相结合的非结构动网格技术,耦合求解Euler方程及弹道方程,模拟飞行在46千米高空、0°攻角、马赫数6.5、壳片分离初速分别为6m/s,12m/s、壳片分离角速度分别为0°/s,50°/s,150°/s的子母弹抛壳动态过程。研究表明,抛壳初期,壳片与母弹周围形成复杂流动,在壳片内表面存在激波的生成、发展、减弱等非定常过程,导致壳片受到气动力随着分离距离增加表现为很强的非线性特征;壳片分离初始角速度对壳片姿态的影响不是线性的,尽管分离初始角速度增加到150°/s,由于转动惯量小、俯仰力矩大,壳片实际飞行姿态达不到设计要求,壳片攻角较小,气动阻力小,导致壳片伴随母弹较长时间飞行;增大分离初速是实现快速分离的有效措施。     

舰载飞机纵向着舰自抗扰导引系统设计

为使舰载飞机沿着理想的下滑轨迹安全着舰,自动着舰系统必须具备跟踪甲板运动和抑制气流扰动的性能。因此,采用自抗扰控制器(ADRC)设计了纵向着舰导引系统。仿真结果表明,自抗扰导引系统不但对典型输入的跟踪性能令人满意,而且抑制突风扰动的能力较强;和PID导引律相比,系统响应的品质有较大的改善。     

P70霍尔推力器新型缓冲腔磁路对预电离及放电的影响

为有效利用从P70霍尔推力器放电通道进入缓冲腔的快电子能量,考虑两个磁场特征以提高缓冲腔预电离率。一是提高磁感应强度,二是缓冲腔内从气体分配器到放电通道方向的负梯度。采用FEMM有限元磁场计算软件,在不改变推力器电离和加速通道内优化磁场特征的前提下,设计的新型缓冲腔磁路满足上述磁场特征。放电实验结果表明,在新型缓冲腔磁路下放电电流低频振荡幅值更小。新型磁路有助于延长推力器寿命,有助于电离和加速通道内电离与加速区的分离。     

基于DSP无速度传感器的永磁同步电机控制技术

提出一种新型无速度传感器的永磁同步电机控制策略。电机的位置信号通过位置扰动算法获得,并使用矢量控制技术实现PMSM的高性能控制,DSP56005用于实现位置估计和矢量控制算法,通过实验结果证明该方法的正确性。     

基于QPSO算法的自抗扰控制器设计及参数整定

提出了一种基于量子粒子群(QPSO)的自抗扰控制器(ADRC)设计及参数整定方法.利用自抗扰控制器抗于扰能力强、鲁棒性好、对模型参数变化适应能力强的特点,设计了自抗扰纵向飞行控制器以提高飞行控制性能.针对所设计的自抗扰控制器参数多,需要依靠专家经验或试凑进行整定的问题,应用QPSO算法进行控制器参数整定.仿真结果表明,...     

Model Development and Adaptive Imbalance Vibration Control of Magnetic Suspended System

对星载磁悬浮单框架控制力矩陀螺,建立其转子的平动与转动的动力学方程。所建模型反映了转子的动、静不平衡特性,以及转子运动与框架、星体运动的耦合关系。模型是主动磁悬浮控制与动框架效应分析的基础。对动、静不平衡量未知的转子,设计了自适应对中控制器。在分散PD、比例交叉反馈控制器与高低通滤波器的基础上,通过动、静不平衡量的辨识与补偿控制,使转子绕其惯量主轴旋转,衰减角动量交换执行机构高速转子因不平衡而对基座产生的干扰力,消除星上主要颤振源,达到降低卫星姿态抖动的目的。     

Evolution of coronal mass ejection/shock system in interplanetary space

The evolution of coronal mass ejection/shock system is investigated by numerically solving the usual set of two-dimensional single-fluid polytropic magnetohydrodynamic equations from 1 R_s to 1 AU in the meridian plane. The simulation result reveals that the coronal mass ejection/shock system formed near the sun evolves into the magnetic cloud/shock system near the earth’s orbit through the following three phases: the initial formation, the dominant latitudinal expansion and the similar expansion.     

Relativistic solar protons in the ground level event of 23 February 1956: New study

In this study we applied again to the outstanding solar particle event of 23 February 1956, the largest one in the entire history of observations of solar cosmic rays. Due to significant improvement of the analysis/modeling techniques and new understanding of physical processes in the solar atmosphere and interplanetary space, a possibility arises to interpret the old data in the light of modern concept of multiple particle acceleration at/near the Sun. In our new analysis the data of available then neutron monitors and muon telescopes are used. The technique of the analysis includes: (a) calculation of asymptotic cones of ground-based detectors; (b) modeling of cosmic ray detector responses at variable parameters of the flux of solar relativistic protons; (c) determination of primary solar proton parameters outside magnetosphere by comparison of computed responses with observations. Certain evidence was obtained that the flux of relativistic solar protons consisted of two distinct components: prompt and delayed ones. The prompt component with exponential energy spectrum caused a giant impulse-like increase at a number of European cosmic ray stations. The delayed component had a power-law spectrum and was a cause of gradual increase at cosmic ray stations in the North American region. A numerical simulation of the proton acceleration in the vicinity of the magnetic reconnection region brings to the proton spectrum with exponential dependence on energy. This agrees with observational data for the prompt component. It is also shown that the huge increase in ∼5000% on neutron monitors was due to the prompt component only with the exponential proton spectrum. The power-law spectrum of comparable intensity gave considerably smaller effect.     

磁尾等离子体片对流对亚暴的影响

采用2(1/2)维全粒子电磁模拟方法研究了等离子体片中稳态对流及局地爆发高速流对磁层亚暴触发过程的影响.研究发现,地向瞬时局地高速流可触发磁场重联,导致储存于磁尾磁场能量的快速释放.但是,等离子体片稳态对流可抑制磁尾磁场重联过程.此项研究结果表明,局地爆发高速流能够触发磁层亚暴;而行星际磁场(IMF)持续南向时的稳态磁层对流期间,不易发生亚暴.      

基于角加速度的陀螺框架伺服系统干扰观测器

磁悬浮控制力矩陀螺(MSCMG,Magnetically Suspended Control Moment Gyro)是大型航天器姿态控制的关键执行机构,影响MSCMG输出力矩准确度的一个关键因素是其框架伺服系统的控制精度.为提高MSCMG框架伺服系统的抗干扰能力和控制精度,提出了一种基于角加速度的干扰观测器.其设计思想是:卡尔曼滤波器利用角位置估计出角速度并送往状态观测器以获取准确的角加速度,角加速度和电流作为干扰观测器的输入以获得补偿电流,补偿电流加到电流环的输入端以补偿各种干扰.干扰观测器结构简单,抗干扰能力强.实验表明:该方法有效地提高了MSCMG框架伺服系统的角速度精度与稳定度.