大功率无电极高密度等离子体电磁推进概述

无电极高密度等离子体电磁推进技术已成为未来深空探测、载人航天和货运、太阳能电站以及航天器在轨服务与维护等空间任务中极具竞争力的核心推进技术之一。在梳理不同无电极等离子体电磁加速机制基础上,开展大功率无电极高密度等离子体电磁推进技术性能对比,给出新概念无电极场反构型电磁推进技术向未来超大功率拓展的优势和发展潜力,同步分析了该技术亟需解决的关键基础问题,旨在为中国新概念场反构型电磁推进技术的研发提供理论基础。     

2 AU以内的“渐进型”太阳高能粒子事件模拟

太阳高能粒子（Solar Energetic Particle,SEP）事件是影响地球空间以及深空辐射环境的主要因素之一。“渐进型”太阳高能粒子事件中的高能粒子主要来自于日冕物质抛射（Coronal Mass Ejection,CME）所驱动的激波扩散加速（Diffusive Shock Acceleration,DSA）过程。CME驱动的激波在行星际的传播过程中,其结构不断演化,进而影响到高能粒子的加速过程。本文利用二维太阳高能粒子加速和传播模型,对发生于2014年4月18日的太阳高能粒子事件实例进行了数值模拟。模型考察了黄道面上2 AU的距离以内包含地球所在位置的4个不同点,分别计算了每个点上高能粒子的通量。数值模拟的结果表明：黄道面内不同位置的观察点,与激波波前的磁力线连接不同,从而导致观察点处高能粒子的通量有着显著的差异。该模型的计算结果可以为深空探测计划开展辐射环境研究提供必要的输入。     

Modelling ignition probability with pairwise mixing-reaction model for flame particle tracking

Reduced order models for ignition analysis can offer insights into ignition processes and facilitate the combustor optimization. In this study, a Pairwise Mixing-Reaction (PMR) model is formulated to model the interaction between the flame particle and the surrounding cell mixture during Lagrangian flame particle tracking. Specifically, the model accounts for the two-way coupling of mass and energy between the flame particle and the surrounding shell layer by modelling the corresponding turbulent mixing, chemical reaction and evaporation process if present. The state of a flame particle, e.g., burnt, hot gas or extinguished, is determined based on particle temperature. This model can properly describe the ignition process with a spark kernel being initiated in a nonflammable region, which is of practical importance in certain turbine engines and has not been rigorously accounted for by the existing models based on the estimation of local Karlovitz number. The model is integrated into an ignition probability analysis platform and is demonstrated for a methane/air bluff-body flame with the flow and fuel/air mixing characteristics being extracted from a non-reacting simulation. The results show that for the spark location being at the extreme fuel-lean outer shear layer of the recirculation zone, PMR can yield ignition events with a significant number of active flame particles. The mechanisms for the survival of the initial flame particles and the entrainment of the survived flame particles into the recirculation zone are analyzed. The results also show that the ignition probability map from PMR agrees well with the experimental observation: a high ignition probability in the shear layer of the recirculation zone near the mean stoichiometric surface, and low ignition probabilities inside the recirculation zone and the top stagnation region of the recirculation zone. The parametric study shows that the predicted shape of the ignition progress factor and ignition probability is in general insensitive to the model parameters and the model is adequate for quantifying the regions with high ignition probabilities.     

Sliding mode control design for oblique wing aircraft in wing skewing process

When the wing of Oblique Wing Aircraft (OWA) is skewed, the center of gravity, inertia and aerodynamic characteristics of the aircraft all significantly change, causing an undesirable flight dynamic response, affecting the flying qualities, and even endangering the flight safety. In this study, the dynamic response of an OWA in the wing skewing process is simulated, showing that the three-axis movements of the OWA are highly coupled and present nonlinear characteristics during the wing skewing. As the roll control efficiency of the aileron decreases due to the shortened control arm in an oblique configuration, the all-moving horizontal tail is used for additional roll and the control allocation is performed based on minimum control energy. Given the properties of pitch-roll-yaw coupling and control input and state coupling, and the difficulty of establishing an accurate aerodynamic model in the wing skewing process due to unsteady aerodynamic force, a multi-loop sliding mode controller is formulated by the time-scale separation method. The closed-loop simulation results show that the asymmetric aerodynamics can be balanced and that the velocity and altitude of the aircraft maintain stable, which means that a smooth transition is obtained during the OWA’s wing skewing.     

三维五向编织复合材料的冲击压缩特性及破坏机制

利用分离式霍普金森压杆(split Hopkinson pressure bar,SHPB)实验系统和高速摄像技术对三维五向碳/环氧编织复合材料的动态压缩特性进行研究。通过对编织角为22.3°的试样分别进行沿纵向和横向方向的冲击压缩实验,得到材料在200~1200 s^-1应变率范围内的应力应变曲线,并结合高速摄像记录的动态压缩过程,对不同应变率下材料在高速变形下的渐进破坏规律进行分析。同时,综合试样的宏观破坏特征和微观断口形貌特征,进一步分析材料的破坏模式及破坏机理。结果表明:随着应变率的增加,材料在纵向和横向均具有一定的应变率强化效应,在横向方向的应变率强化效应更为显著;不同加载方向下材料的渐进破坏过程、应力应变曲线特征以及破坏方式均具有明显差异,且随着应变率的增加而发生改变。     

二氧化碳（CO2）气硬树脂砂用促硬剂的研究

本文介绍了一种对碱性甲阶酚醛树脂有促硬作用的盐,在树脂中加入强碱和该促硬剂后,形成了稳定液态粘结剂,吹ＣＯ２气体硬化后可得到较高的即时抗压强度和２４小时抗压终强度。     

高频噪声场中薄壁结构响应的预估

本文用统计能量分析(StatisticalEnergyAnalysis简称SEA)法研究了在高频宽带随机噪声场中板及加筋板(航空航天器用蒙皮)的加速度响应。发现,在高频段同样外场激励情况下,加筋板的响应大于光板的。本文解释了这一用质量定理无法解释的现象,并用叠加法确定了复杂结构加筋板的模态密度、辐射阻抗和输入功率。     

太阳纯电子事件和质子-电子事件的电子能谱的机制

本文计算、分析了太阳耀斑加速电子在日冕中传输时激发的等离子体尾场的效应,认为耀斑电子的高能成份激发的尾场,能够加速低能耀斑电子,低能耀斑电子的能量增值可达几十keV至上百keV,这种尾场加速将软化约100keV以下的能量范围内(探测阈之上)的耀斑电子能谱。结合考虑尾场效应,本文提出了太阳耀斑加速电子从加速区到形成电子事件之间的能谱演化模式,说明了太阳纯电子事件的双幂律电子能谱和太阳质子-电子事件的单幂律电子能谱的形成,认为两类事件的电子能谱差异为耀斑电子日冕传输中不同程度的尾场效应所致,前者尾场效应弱,电子能谱呈双幂律,后者尾场效应较强,电子能谱为单幂律谱。      

变幅加载下疲劳可靠性分析

分别对疲劳载荷、寿命与强度的随机性进行了分类。基于二维概率Miner准则,建立了在变幅载荷谱或随机时间历程载荷谱给定的条件下,对结构构件进行疲劳可靠性分析的新方法,并由此推导出统计Miner准则中α的分布。最后,分别给出了实验数据验证结果和工程应用实例,显示出该方法具有简便性和实用性。      

迎角过载边界限制器的设计方法

介绍了迎角过载边界限制器的意义、设计要求和一些有代表性的国内外飞机的边界限制器设计方法。边界限制经历了硬限制、软限制、反馈限制和比较逻辑反馈限制几个阶段。分析了这些设计方法的优缺点,并对比较逻辑反馈限制器的设计方法进了理论推导,提出了这类边界限制器重要参数的确定方法。