复杂凸凹曲率飞机蒙皮充液成形技术研究与应用

随着飞机气动、隐身等性能要求的提高,飞机外形曲率更加异形化,大量应用复杂凸凹曲率蒙皮,传统的拉伸成形方法已经不能完全满足新一代飞机蒙皮加工的要求。基于生产某型号飞机复杂凸凹曲率蒙皮这一背景,介绍了充液成形基本原理及关键技术,利用有限元数值模拟方法,分析板材充液成形过程中液室压力、厚度减薄率、板材失稳及贴胎度的变化规律,优化工艺参数,并且根据数值模拟结果指导工业生产。理论分析和现场实践证明:充液成形技术为复杂凸凹曲率蒙皮零件的制造提供了新的工艺方法,满足新一代飞机的凸凹曲率外形蒙皮的制造要求。     

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.     

基于连续损伤力学的轮盘超转破裂行为预测与验证

为有效预测轮盘的超转破裂行为,建立了1种基于连续损伤力学的预测方法。给出了该方法下基于光滑拉伸试验数据的直接时效GH4169合金弹塑性本构模型参数与损伤模型参数确定方法。对缺口半径分别为0.5、2和5 mm的3种缺口圆棒试样的拉伸响应曲线进行了有限元计算,并与试验结果进行了对比。结果表明:该模型可以较准确地预测缺口试样的极限拉伸载荷和拉伸断裂变形。采用弧长法对模拟盘的超转破裂过程进行了非线性有限元计算,使用模拟盘超转破裂试验进行了验证。该模型不仅可以较准确地预测模拟盘的破裂转速,还能有效预测模拟盘的超转破裂模式。对于实际轮盘破裂转速预测具有一定的指导意义。     

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。     

轮缘封严气流与转子干涉损失机理的数值研究

为了研究涡轮转静盘腔中轮缘封严气流与下游转子的干涉机理和损失机制,在不同封严流量下,针对轮缘封严气流对下游转子气动性能和流场分布的影响进行了数值模拟。结果表明,随着封严流量增加,涡轮级效率不断降低。在轮毂到10%叶高和30%～60%叶高,流量系数增加。封严气流主要通过在转子进口封严出流不同的分布和在通道输运过程中与转子通道二次流的交互作用对转子的气动性能产生影响。同时,封严气流引起下游转子气动性能的降低,存在三个损失机制:一是封严腔体摩擦泵效应减弱,增加了封严出流与主流之间周向速度差所引起的粘性剪切损失;二是不同分布的封严出流造成进气负攻角和堵塞效应,降低了转子的做功能力;三是不同分布的封严出流在输运过程中与转子通道二次流的交互作用,导致了二次流损失加剧。     

三角翼大幅度俯仰运动非定常测压实验洞壁干扰研究

用两个几何相似大小不同的前缘后掠角 70°三角翼模型在闭口风洞中进行正弦俯仰振荡实验 ,测量三角翼模型吸力面动态压力以及风洞洞壁上最佳测压点的非定常压力。实验表明 ,三角翼模型在正弦俯仰振荡时 ,其吸力面动态压力以及洞壁上最佳测压点的非定常压力与三角翼模型上的法向力一样呈现迟滞环现象。模型展宽比 (翼展 /洞宽 )增大 ,迟滞环幅度增大 ,动态压力绝对值增大。无论上仰或下俯 ,模型展宽比 (翼展 /洞宽 )增大 ,三角翼模型吸力面涡破碎位置离前缘较远。风洞顶壁上最佳测压点非定常压力迟滞环方向与风洞底壁上对应最佳测压点非定常压力迟滞方向相反。风洞洞壁上最佳测压点非定常压力变化频率与模型正弦俯仰振荡频率一致 ,各最佳测压点间呈现时间延迟现象。     

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。     

GNSS超快速产品在全球标准时间复现中的应用

为满足大跨度空间范围内的时间同步需求,对基于共视时间比对原理的标准时间复现系统进行改进,采用全视时间比对方法解决原系统应用基线受限的问题.考虑实时性的要求,使用全球卫星导航系统(GNSS)超快速产品(预测部分)提供卫星位置和卫星钟差,以尽可能消除广播星历和钟差对复现结果的影响.分析了常用的几家机构发布的GNSS超快速产...     

双重失效模式下民用航空发动机高压涡轮叶片报废特性与可靠性分析

基于某型民用航空发动机下发后观测涡轮叶片报废状态的双重失效模式,计算了高压涡轮(HPT)叶片由自新使用循环数(CSN)引起的报废率.并结合疲劳损伤累积理论,探究了叶片报废率与失效分布函数之间的关系,得到了涡轮叶片失效分布与寿命期望的计算方法.基于大量涡轮叶片的观测数据,拟合出涡轮叶片按CSN计的失效分布,研究发现:某型...     

磨削表面粗糙度在线实时测量的研究

在试验研究的基础上,研制了一种新的光纤表面粗糙度在线测量系统。以光散射法为理论基础,用光纤束作为传感器,并用单片机进行数据处理和实时显示。针对外圆磨削在线检测中存在的冷却液、工件尺寸变化、环境干扰以及仪器的装夹与对中等问题进行了研究,找到了改进或解决的办法,从而更利于该测试技术的实施与推广。