铌掺杂ITO镀膜玻璃电磁散射特性试验

座舱玻璃镀膜是实现飞行器隐身技术的重要途径之一。利用雷达散射截面(RCS)均值增益研究铌掺杂ITO镀膜玻璃隐身性能;针对不同方块电阻的铌掺杂ITO镀膜玻璃,进行系列化RCS暗室测试,分析不同入射频率、极化方式的电磁散射特性。结果表明:方块电阻增大时电磁散射减弱,合适的方块电阻(小于40Ω/m~2)有利于实现座舱外形隐身,散射特性与金属接近,频率较高时,镜面散射波峰较窄。     

Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals

Both heliophysics and planetary physics seek to understand the complex nature of the solar wind’s interaction with solar system obstacles like Earth’s magnetosphere, the ionospheres of Venus and Mars, and comets. Studies with this objective are frequently conducted with the help of single or multipoint in situ electromagnetic field and particle observations, guided by the predictions of both local and global numerical simulations, and placed in context by observations from far and extreme ultraviolet (FUV, EUV), hard X-ray, and energetic neutral atom imagers (ENA). Each proposed interaction mechanism (e.g., steady or transient magnetic reconnection, local or global magnetic reconnection, ion pick-up, or the Kelvin-Helmholtz instability) generates diagnostic plasma density structures. The significance of each mechanism to the overall interaction (as measured in terms of atmospheric/ionospheric loss at comets, Venus, and Mars or global magnetospheric/ionospheric convection at Earth) remains to be determined but can be evaluated on the basis of how often the density signatures that it generates are observed as a function of solar wind conditions. This paper reviews efforts to image the diagnostic plasma density structures in the soft (low energy, 0.1–2.0 keV) X-rays produced when high charge state solar wind ions exchange electrons with the exospheric neutrals surrounding solar system obstacles.The introduction notes that theory, local, and global simulations predict the characteristics of plasma boundaries such the bow shock and magnetopause (including location, density gradient, and motion) and regions such as the magnetosheath (including density and width) as a function of location, solar wind conditions, and the particular mechanism operating. In situ measurements confirm the existence of time- and spatial-dependent plasma density structures like the bow shock, magnetosheath, and magnetopause/ionopause at Venus, Mars, comets, and the Earth. However, in situ measurements rarely suffice to determine the global extent of these density structures or their global variation as a function of solar wind conditions, except in the form of empirical studies based on observations from many different times and solar wind conditions. Remote sensing observations provide global information about auroral ovals (FUV and hard X-ray), the terrestrial plasmasphere (EUV), and the terrestrial ring current (ENA). ENA instruments with low energy thresholds (\(\sim1~\mbox{keV}\)) have recently been used to obtain important information concerning the magnetosheaths of Venus, Mars, and the Earth. Recent technological developments make these magnetosheaths valuable potential targets for high-cadence wide-field-of-view soft X-ray imagers.Section 2 describes proposed dayside interaction mechanisms, including reconnection, the Kelvin-Helmholtz instability, and other processes in greater detail with an emphasis on the plasma density structures that they generate. It focuses upon the questions that remain as yet unanswered, such as the significance of each proposed interaction mode, which can be determined from its occurrence pattern as a function of location and solar wind conditions. Section 3 outlines the physics underlying the charge exchange generation of soft X-rays. Section 4 lists the background sources (helium focusing cone, planetary, and cosmic) of soft X-rays from which the charge exchange emissions generated by solar wind exchange must be distinguished. With the help of simulations employing state-of-the-art magnetohydrodynamic models for the solar wind-magnetosphere interaction, models for Earth’s exosphere, and knowledge concerning these background emissions, Sect. 5 demonstrates that boundaries and regions such as the bow shock, magnetosheath, magnetopause, and cusps can readily be identified in images of charge exchange emissions. Section 6 reviews observations by (generally narrow) field of view (FOV) astrophysical telescopes that confirm the presence of these emissions at the intensities predicted by the simulations. Section 7 describes the design of a notional wide FOV “lobster-eye” telescope capable of imaging the global interactions and shows how it might be used to extract information concerning the global interaction of the solar wind with solar system obstacles. The conclusion outlines prospects for missions employing such wide FOV imagers.     

嵌入式大气数据传感系统研究进展

大气数据的精确测量对飞行器的导航与控制至关重要。相较于传统的探针式大气数据测量系统,嵌入式大气数据传感系统更适用于隐身性能要求、大迎角飞行要求的飞行器或高超声速飞行器。回顾了嵌入式大气数据传感系统的发展历程,介绍了该系统完整的组成部分及其工作原理,并指出该系统在应用时的四项关键技术(测压孔布局、气动模型及求解算法、校正算法、故障检测及管理技术),结合国外多种飞行器上该系统不同的应用方案,分别对比分析四项关键技术不同应用方式的优缺点;指出了该系统的四项关键技术均会影响系统精度及可靠性,实际应用中需综合考虑选择其应用方式;最后展望了该系统在未来航空航天领域的应用。     

航空齿轮磨削加工安装偏心误差补偿研究

磨齿加工时齿坯几何中心与回转工作台轴心存在安装偏心误差,降低了磨齿加工精度。以数控成型砂轮磨齿机工作原理为基础,建立偏心误差磨削加工几何模型;提出安装偏心误差补偿法,建立偏心误差补偿数学模型,通过数学模型求出磨削砂轮在X、Y两个方向的进给补偿增量;以YK73125数控成型砂轮磨齿机为例,进行安装偏心误差补偿实验,齿轮的左右齿面单个齿距极限偏差绝对值分别减小了0.9μm和1.6μm,齿距累积总偏差绝对值分别减小了49.6μm和43.3μm。结果表明:安装偏心误差与单个齿距偏差和齿距累积总偏差成正比;采用安装偏心误差补偿进行磨齿加工,有效地减小了单个齿距偏差和齿距累积总偏差,齿轮的精度有所提高。     

电缆故障在线检测定位装置研究

电缆作为飞机电源系统的重要组成部分,实现电缆故障的在线诊断,可以提高其可靠性。采用扩展频谱时域反射法(SSTDR),基于FPGA技术,设计一种板级速率为500 MHz的飞机电缆故障在线检测和定位装置,并进行实验验证。结果表明:该装置能够实现电缆开路、短路以及间歇性电弧的在线检测和定位,具有定位精度高、实时性好等优点;利用该装置在线监测电缆的健康状态,实现难以复现的间歇性故障的检测,能够提高地面运营、维护效率,节省人力物力,具有较高的工程应用价值。     

临近空间动能拦截器神经反演姿态控制器设计

为满足临近空间动能拦截器姿态控制快速性、准确性和鲁棒性的要求,设计了一种自适应神经反演姿态控制器。首先,建立了姿控发动机侧喷干扰模型,并推导了包含质心漂移、参数摄动和外界干扰的三通道强耦合模型;其次,设计了自适应神经反演姿态控制器,为提高控制精度,采用径向基函数（RBF）神经网络对各个通道的不确定项进行估计和补偿,并基于最小学习参数的思想,将神经网络学习参数拟合为一个参数,提高了RBF计算效率,保证了估计的实时性。最后,采用伪速率（PSR）脉冲调制器将设计的连续控制律转化为脉冲控制律,实现了拦截器的变推力控制,并克服了脉冲脉宽调制（PWPF）调制器相位滞后问题。数字仿真表明,所设计的控制器收敛速度快,控制精度高,对强扰动具有鲁棒性。     

变循环发动机模态转换建模及控制规律设计方法研究

为了实现变循环发动机快速可靠的模态转换,本文发展了变循环发动机模态转换过渡态模型及控制规律设计方法。在变循环发动机动态数值仿真程序的基础上,针对模态选择阀与涵道引射器这两个模态转换过程中的关键变几何部件,建立了高精度的气流突扩局部损失模型。首次提出了可考虑模态选择阀堵塞对发动机性能影响的模态选择阀堵塞模型,消除了由于模型不精确造成的模态转换参数波动。在建立的变循环发动机数学模型的基础上,提出了基于直接推力控制技术的模态转换控制规律设计方法,考虑了变循环发动机的8个可调参数,采用差分进化算法对模态转换过程进行了优化。结果表明,本文提出的模态转换控制规律设计方法可以实现变循环发动机快速平稳的模态转换,双外涵转单外涵的参数变化规律与单外涵转双外涵的参数变化规律基本类似,推力在0.6秒就稳定在目标推力值,其余参数大多在1.4秒之后才趋于稳定。本文提出的变循环发动机模态转换控制规律设计方法还可应用于常规航空发动机的加/减速过渡态控制规律设计中。     

待机状态下机翼结冰的快速计算方法

飞机在飞行过程中遭遇结冰气象,尤其是过冷大水滴结冰条件所导致的机翼结冰,将严重影响飞机的气动性能与操纵品质,从而导致飞行故障或飞行事故,是飞机飞行安全的重要影响因素,是飞机研制中必须重点解决的难题。虽然针对结冰已建立有多种计算仿真程序,但快速获得结冰模拟冰形,包括过冷大水滴条件下的结冰模型是工程师们一直追求的解决方案。利用前向多层神经网络,尝试建立了一种针对待机状态下的机翼结冰模型。此方法基于坐标转换原理,将获取的采用直角坐标表达的标准翼型的机翼结冰数据转换为对应的极坐标表达的数据,以飞行参数、气象参数和极坐标角度作为输入,极坐标模值作为输出训练构建出此种机翼结冰模型。使用所建立的模型,仿真预测结果表明该计算方法具备快速性和精确性,其计算精度可满足实际要求。     

机翼结冰生命周期的数字孪生软件系统

飞机巡航中的机翼结冰情况是关系到飞行安全的重大实际问题之一,如果能够实时监测甚至根据环境提前预测机翼结冰过程和状况,对改进机翼防除冰设计、规避飞行危险都具有重大意义。数字孪生技术作为5G信息时代中新兴的技术,为物理过程的虚拟呈现提供了新的思路与解决方案、同时数字孪生技术结合人工智能等技术,同样可以应用于飞机巡航中机翼结冰物理过程,对实时监测与预测提供了新的技术保证。从数字孪生的角度出发,以机翼结冰神经网络模型为切入点,设计实现了一款基于数字孪生和人工智能技术的巡航中机翼结冰二维过程快速呈现软件系统。软件获取飞机巡航结冰参数与飞行参数,运行结果能够利用动态显示方式,呈现飞机巡航中机翼结冰全生命周期。     

内混音速空气雾化重油喷嘴的试验研究

在横向气流中直射喷嘴雾化研究及超音速气流中喷嘴雾化研究的基础上,针对工业窑炉中烧嘴以重油(通常为油渣)工作的问题,设计和试验研究了内混音速气流两次空气雾化重油喷嘴,从原理上解决了喷嘴雾化细度(燃烧完全)和火焰长度(刚性)之间的矛盾。文中得出合理选择这种喷嘴的结构形式、几何尺寸以及混合腔压力,同时得出很好的雾化细度以及要求的火焰长度。结果表明,混合腔压力与供气压力之比应在0.60～0.70之间,所需压缩空气的压力为0.4MPa,所设计的喷嘴已投入使用。