双模态超燃燃烧室计算

选择了固定几何流通截面的双模态超燃燃烧室模型,采用气动热力调节的方法（即调节燃料喷射方式和燃烧速率）来实现双模态、宽马赫范围工作。在计算中用一维、定比热容方法分析了相关参数对燃烧室模态转变、性能的影响和隔离段与燃烧室的相互作用。计算结果表明,气动热力调节实现燃烧室内燃烧模态的转变是可行的。     

微型飞行器航时优化

 针对微型飞行器(MAV)低雷诺数条件下续航时间不足的问题,推导了适用于电动推进飞行器的航时计算公式,并提出为实现航时优化的动力系统规划方法。通过初步实验,验证了航时优化理论的正确性,通过规划延长了航时。     

Multi-Wavelength Observations of CMEs and Associated Phenomena

This chapter reviews how our knowledge of CMEs and CME-associated phenomena has been improved, since the launch of the SOHO mission, thanks to multi-wavelength analysis. The combination of data obtained from space-based experiments and ground based instruments allows us to follow the space-time development of an event from the bottom of the corona to large distances in the interplanetary medium. Since CMEs originate in the low solar corona, understanding the physical processes that generate them is strongly dependant on coordinated multi-wavelength observations. CMEs display a large diversity in morphology and kinematic properties, but there is presently no statistical evidence that those properties may serve to group them into different classes. When a CME takes place, the coronal magnetic field undergoes restructuring. Much of the current research is focused on understanding how the corona sustains the stresses that allow the magnetic energy to build up and how, later on, this magnetic energy is released during eruptive flares and CMEs. Multi-wavelength observations have confirmed that reconnection plays a key role during the development of CMEs. Frequently, CMEs display a rather simple shape, exhibiting a well known three-part structure (bright leading edge, dark cavity and bright knot). These types of events have led to the proposal of the ‘`standard model’' of the development of a CME, a model which predicts the formation of current sheets. A few recent coronal observations provide some evidence for such sheets. Other more complex events correspond to multiple eruptions taking place on a time scale much shorter than the cadence of coronagraph instruments. They are often associated with large-scale dimming and coronal waves. The exact nature of these waves and the physical link between these different manifestations are not yet elucidated. We also discuss what kind of shocks are produced during a flare or a CME. Several questions remain unanswered. What is the nature of the shocks in the corona (blast-wave or piston-driven?) How they are related to Moreton waves seen in Hα? How they are related to interplanetary shocks? The last section discusses the origin of energetic electrons detected in the corona and in the interplanetary medium. “Complex type III-like events,”which are detected at hectometric wavelengths, high in the corona, and are associated with CMEs, appear to originate from electrons that have been accelerated lower in the corona and not at the bow shock of CMEs. Similarly, impulsive energetic electrons observed in the interplanetary medium are not the exclusive result of electron acceleration at the bow shocks of CMEs; rather they have a coronal origin.     

激光熔覆制备金属间化合物抗冲蚀涂层

采用同轴送粉方法,激光熔覆制备了WC增强Ni3Al金属间化合物基复合涂层,通过试验,优化了工艺参数,对激光熔覆涂层的成分、组织和硬度进行了测试和分析.结果表明,激光熔覆涂层无裂纹和气孔,与基体形成良好的冶金结合,WC颗粒的添加显著提高了涂层硬度.     

基于遗传算法的起降航班动态排序模型的研究

讨论了空中交通流量管理中终端区航班的排序规划问题。目的是在终端区空中交通繁忙的情况下有效地为到达航班安排合理的着陆次序，并在不违反飞机间隔要求的情况下给出各飞机经过优化的着陆时间，提高机场跑道的利用率。引入离场起飞的航班问题，建立了航班排序的动态模型和基于遗传算法的终端区动态排序算法。并对一个算例采用冬文方法进行验证计算，结果表明，所提出的方法计算效率高，实用可行。     

基于支持向量机改进SMO算法的直升机旋翼自转着陆过程建模

 为了建立高精度的直升机仿真模型,把支持向量机(SVM)引入到直升机智能化建模领域,建立了直升机自转着陆过程的旋翼转速模型。根据凸二次优化问题在对偶间隙为零时取得最优解的性质,对序列最小优化算法的停机准则进行改进,并用于所建模型的训练。仿真结果表明：与神经网络模型比较,这种SVM模型具有结构简单、运算速度快和泛化能力强等优点。     

P2P环境下基于推荐的信誉计算方法

通过节点间信誉评价的相似度和信息熵的计算,提高了推荐信誉的可用性,降低了共谋推荐行为对间接信誉合成的消极影响.通过Einstein算子将多个推荐信誉合成间接信誉,体现了信誉评估的模糊性的特点.实验结果表明,该方法可以增强推荐信誉的可用性,在一定程度上减少共谋推荐对信誉真实性造成的影响.     

Numerical Investigation of the Effects of Wind Tunnel Model Vibrations on the Measured Aerodynamic Properties of Airfoils and Wings

This paper presents a numerical prediction of the unsteady flow field around oscillating airfoils at high angles of attack by solving unsteady Reynolds-averaged Navier-Stokes equations with SST turbulence model in order to simulate the effects of wind tunnel model vibrations on the aerodynamic properties of airfoils,especially high-aspect-ratio wings in a wind tunnel.The effects of the phase lagging between different modes of oscillations,i.e.,the airfoil plunging oscillation mode,the pitching oscillation mode,and the forward-backward oscillation mode,are also studied.It is shown that the vibrations (oscillations) of airfoils can cause the unsteady shedding of large-size separated vortex to precede the stationary stall incidence,hence lead to a stall onset at some earlier (lower) incidence than that in the steady sense.The different phase lagging has different effect on the flow field.When the pitching oscillation mode has small phase lagging behind the plunging oscillation mode,the effect of vibrations is large.Besides,if the amplitude of the oscillations is large enough,and the different modes of vibrations match or combine appropriately,the unsteady stall may occur 2° earlier in angle of attack than the case where airfoils keep stationary.     

小型无人飞行器风场扰动自适应控制方法

针对小型无人飞行器在执行任务时传感器测量精度低、受风场扰动影响大的问题,提出了一种利用矢量域与滑模控制相结合的复合控制方式,有效地实现了对小型无人飞行器的轨迹与航向的自适应跟踪。将复杂航迹分解为直线段与圆弧段分别构建矢量域,从而确定基于位置误差的航迹信息,并通过机载传感器获得状态和位置信息,利用滑模控制方法抑制风场扰动对小型无人飞行器的影响。试验结果表明,本文提出的控制算法能够保证阵风干扰情况下小型无人飞行器的航迹控制精度,同时具有良好的动态响应。