J7L飞机纵向电传系统控制律设计研究

提出了采用现代最优控制理论与经典控制理论协调配合的方法，按ＭＵＬ－Ｆ－８７８５Ｃ品质规范要求，设计了Ｊ７Ｌ飞机纵向电传系统控制律。文中针对原型机某些缺陷采用陷模型跟踪最优二次型方法，设计ＦＢＷ纵向基本控制律，并用常规方法设计动态补偿器，指令通道等环节，从对该机主要飞行状态的评价来看，均达到了ＭＩＬ－Ｆ－８７８５Ｃ规范的一级飞行品质要求，由此可见，这种协调设计方法，对飞行控制系统的设计具有较大的潜力     

Investigation of hot jet on active control of oblique detonation waves

The hot jet injection is utilized to actively control the oblique detonation wave, such as initiating and stabilizing an oblique detonation wave at a desired position that is shorter than the length of induction zone, and adjust the height of the oblique detonation wave at the exit of combustor when the oblique detonation wave engine is working on off-design flight conditions. The fifth order Weighted Essentially Non-Oscillatory (WENO) scheme and a two-step reversible reaction mechanism of the stoichiometric H₂/Air are adopted in the simulations. With the help of hot jet injection, the transition from inert oblique shock wave to the oblique detonation wave immediately occurs near the position of hot jet injection, and consequently the length of combustor can be reduced. The angle of oblique detonation wave also decreases as the hot jet injection approaches the nose of wedge. Additionally, the height of the oblique detonation wave at the exit of combustor can be flexibly adjusted, and also depends on the injection position and the strength of the hot jet. If the velocity of the hot jet is too weak to directly trigger the overall oblique detonation wave at the position of injection, increasing the injection pressure will improve the strength of the hot jet and results in a successful transition.     

What are the physical mechanisms of eruptions and CMEs?

CMEs are due to physical phenomena that drive both, eruptions and flares in active regions. Eruptions/CMEs must be driven from initially force-free current-carrying magnetic field. Twisted flux ropes, sigmoids, current lanes and pattern in photospheric current maps show a clear evidence of currents parallel to the magnetic field. Eruptions occur starting from equilibria which have reached some instability threshold. Revisiting several data sets of CME observations we identified different mechanisms leading to this unstable state from a force free field. Boundary motions related to magnetic flux emergence and shearing favor the increase of coronal currents leading to the large flares of November 2003. On the other hand, we demonstrated by numerical simulations that magnetic flux emergence is not a sufficient condition for eruptions. Filament eruptions are interpreted either by a torus instability for an event occurring during the minimum of solar activity either by the diffusion of the magnetic flux reducing the tension of the restraining arcade. We concluded that CME models (tether cutting, break out, loss of equilibrium models) are based on these basic mechanisms for the onset of CMEs.     

Bolometric luminosities and brightness temperatures of BL Lac Objects and FR I radio galaxies

To understand the connection among the subclasses of BL Lac Objects, FR I radio galaxies and Flat spectrum radio quasars (FSRQs), here the correlations of the bolometric luminosities with redshifts and brightness temperatures of these objects are studied. The bolometric luminosities vary linearly with redshifts, but few objects are scattered at high redshift. The bolometric luminosity versus brightness temperature distribution shows a correlation between these two components, except a few scattered objects, mostly RBLs. The bolometric luminosities and brightness temperatures of FR I radio galaxies with low redshift (<0.1) and low spectral index (α_rx < 0.75) are comparable to those of XBLs and those characteristics of FR I radio galaxies, with relatively high redshift (>0.2) and high spectral index, can be comparable with RBLs with low redshift (z < 0.5) and low bolometric luminosity. Those scattered RBLs with high redshifts (z > 0.5) are believed to be in complex environment with companion galaxies, most of these RBLs are still unresolved. The bolometric luminosity and brightness temperature of these scattered RBLs are comparable to those of quasars. The FSRQs are at high redshifts and bolometric luminosities and the brightness temperatures are also high relative to BL Lac Objects. These results support the FRI/BL Lac unification scheme. It suggests that, the FR I radio galaxies may be the parent populations of the BL Lac Objects, but it needs more investigation to confirm the unification of FR I radio galaxies, XBLs and RBLs.     

The role of ultraviolet imaging in studies of resolved and unresolved young stellar populations. M31 and M33

We discuss the relevance of UV data in the detection and characterization of hot massive stars and young stellar populations in galaxies. We show results from recent extensive surveys in M31 and M33 with Hubble Space Telescope (HST) multi-wavelength data including UV filters, which imaged several regions at a linear resolution (projected) of less than half a pc in these galaxies, and from GALEX far-UV and near-UV wide-field, low-resolution imaging of the entire galaxies. Both datasets allow us to study the hierarchical structure of star formation: the youngest stellar groups are the most compact, and are often arranged within broader, sparser structures. The derived recent star-formation rates are rather similar for the two galaxies, when scaled for the respective areas. We show how uncertainties in metallicity and type of selective extinction for the internal reddening may affect the results, and how an appropriate complement of UV filters could reduce such uncertainties, and significantly alleviate some parameter degeneracies.     

基于神经网络的拖靶高度自抗扰控制研究

为了解决建立拖靶数学模型的难点以及高度测量误差的影响,提出了基于神经网络的拖靶高度自抗扰控制方法。自抗扰控制降低了模型的不准确对飞行控制造成的影响。以垂向加速度信号和高度信号作为神经网络的输入信号,得到自抗扰控制器的补偿因子系数,既降低了高度表测量误差的影响,又使得自抗扰控制的补偿因子得到实时更正。仿真表明,该方法使得拖靶的控制性能更加精确,有效抑制了外界的干扰,达到了恒高飞行的目标。     

Evaluation of a satellite constellation for active debris removal

This paper analyzes an example of a three-dimensional constellation of debris removal satellites and proposes an effective constellation using a delta-V analysis that discusses the advisability of rendezvousing satellites with space debris. Lambert?s Equation was used to establish a means of analysis to construct a constellation of debris removal satellites, which has a limit of delta-V injection by evaluating the amount of space debris that can be rendezvoused by a certain number of removal satellite. Consequently, we determine a constellation of up to 38 removal satellites for debris removal, where the number of space debris rendezvoused by a single removal satellite is not more than 25, removing up to 584 pieces of debris total. Even if we prepare 38 removal satellites in their respective orbits, it is impossible to remove all of the space debris. Although many removal satellites, over 100 for example, can remove most of the space debris, this method is economically disproportionate. However, we can also see the removal satellites are distributed nearly evenly. Accordingly, we propose a practical two-stage strategy. The first stage is to implement emergent debris removal with the 38 removal satellites. When we find a very high probability of collision between a working satellite and space debris, one of the removal satellites in the constellation previously constructed in orbit initiates a maneuver of emergent debris removal. The second stage is a long-term space debris removal strategy to suppress the increase of space debris derived from collisions among the pieces of space debris. The constellation analyzed in this paper, which consists of the first 38 removal satellites, can remove half of the over 1000 dangerous space debris among others, and then the constellation increases the number of the following removal satellites in steps. At any rate, an adequate orbital configuration and constellation form is very important for both space debris removal and economic efficiency. Though the size of constellation of debris removal satellites would be small originally, such a constellation of satellites should be one of the initial constellations of removal satellites to ensure the safety of the future orbital environment.     

模糊线性/非线性自抗扰切换控制及其应用

针对干扰弹在作战过程中所遇到的强非线性的干扰、模型不确定性的影响等特性,提出了一种模糊线性/非线性自抗扰切换控制器。首先,以干扰弹滚转运动模拟装置为研究对象,分别建立了以飞轮角速度为被控量、滚转角为被控量的数学模型;提出了用模糊规则改进线性/非线性自抗扰切换控制条件,进而实现更为平稳的模糊软切换;然后选择采用飞轮角速度线性自抗扰控制内环和滚转角模糊线性/非线性自抗扰切换控制外环的双闭环控制策略;最后,搭建了系统的仿真模型与实验平台。仿真与实验结果都表明该控制器兼具了线性自抗扰与非线性自抗扰的优势,具有较高的实际应用价值。     

空间挠性结构的Stewart平台主动基座振动控制

研究基于Stewart平台主动基座的挠性结构振动控制。首先,建立含Stewart平台主动基座的柔性梁刚柔耦合动力学模型;随后,在模态空间上分别针对挠性结构的一阶和二阶模态设计由线性扩张状态观测器(LESO)和PD控制器组成的自抗扰控制器(ADRC);最后,基于独立模态控制(IMSC)中的模态滤波器从物理坐标中提取模态坐标,建立振动主动控制实验系统,基于模态空间的自抗扰控制方法完成挠性结构的前两阶模态振动主动控制实验。研究结果表明,利用Stewart平台作为主动基座,采用自抗扰控制方法实现挠性结构的振动抑制是一种高效的振动主动控制方法,在空间振动主动控制领域具有广阔的应用前景。