飞机封闭腔室减重降噪优化方法

噪声水平是现代飞机封闭腔室设计的重要指标,设计中单纯地对壁板进行加肋处理虽能显著降低噪声但会大大增加结构质量,为此对由封闭腔室构成的结构-声耦合系统进行了减重降噪优化研究。基于结构-声耦合有限元模型,利用有限元软件ACTRAN计算了频谱加载时舱内的声压响应。通过试验对简化处理及数值计算进行了验证,并修正了相关模型参数。为了降低结构质量,以加强肋为边界对舱门壁板进行了分区,通过对各个区域壁板厚度及肋条截面积的优化设计,使系统动刚度分配更趋合理,降低了声辐射能量以及结构-声腔的耦合性,从而实现了在满足噪声约束条件下减轻结构质量的目标。本文的工作对实际工程中由加肋壁板所构成的类似结构的减重降噪设计有着较好的工程指导价值。     

基于EM‑EKF的深空光学自主导航系统光轴偏差补偿算法

在深空探测任务中,光学自主导航的精度受导航敏感器件安装精度的影响较大。提出了一种基于期望最大化-扩展卡尔曼滤波(EM-EKF)的光学自主导航系统光轴偏差补偿算法。算法基于条件概率的思想,预先设定状态变量和观测量的统计特性参数,通过不断地最大化条件期望,得到出现概率最大的状态变量估值和光轴偏差参数估值。该算法可分为4步:EKF、固定区间平滑、求解条件期望和期望最大化,不断迭代即可得到光轴偏差估计值。以火星探测近火段为例进行仿真验证,经光轴偏差补偿后,导航精度由100 km提升至20 km以内。     

大型空间环境模拟器热沉气氮调温系统设计与实现

文章结合某型号航天器对调温热沉试验需求,对国内外气氮调温系统进行分析调研,对某空间环境模拟器进行了气氮调温系统流程设计,对影响系统的关键参数如气氮流量、液氮体积流量及有关供气供热管径等进行分析研究和设计实施,并进行了系统调试。调试结果表明,热沉温度均匀性达到±5℃,升/降温速率均达到或超过1℃/min,满足相应的型号试验要求。     

复杂电磁环境下无线接收机电磁兼容快速测试技术应用CSCD

复杂射频电磁环境下,无线接收机作为主要的敏感设备,其电磁兼容性直接影响着整个武器装备的电磁兼容特性. 本文针对GJB 151B中对于接收机非线性测试方法的局限性,引入了一种利用自动双频测试系统对接收机干扰响应的快速测试方法;并搭建了实验室半实物仿真测试平台,检测了某接收机在（ 4-6 ） GHz组合频率干扰下的所有非线性的干扰响应通道. 测试结果对于评估接收机及其所在系统的外部电磁环境适应性具有重要参考价值.     

Coupled Stress-Electricity Model for Electromagnetic Emission Induced by Concrete Fracture

Electromagnetic emission induced during concrete fracturing is of great significance to health monitoring of concrete structures.A coupled stress-electricity model is established by analyzing the interaction between stress and electricity during concrete fracturing.And based on this model,the electromagnetic radiation parameters are calculated.The theoretical calculation is well coincident with experimental results.This work provides theoretical support for concrete testing system.     

Prediction of shock-layer ultraviolet radiation for hypersonic vehicles in near space

A systemic and validated model was developed to predict ultraviolet spectra features from the shock layer of near-space hypersonic vehicles in the ‘‘solar blind" band region. Computational procedures were performed with 7-species thermal non-equilibrium fluid mechanics, finite rate chemistry, and radiation calculations. The thermal non-equilibrium flow field was calculated with a two-temperature model by the finite volume technique and verified against the bow-shock ultra-violet(BSUV) flight experiments. The absorption coefficient of the mixture gases was evaluated with a line-by-line method and validated through laboratory shock tube measurements. Using the line of sight(LOS) method, radiation was calculated from three BSUV flights at altitudes of 38,53.5 and 71 km. The investigation focused on the level and structure of ultraviolet spectra radiated from a NO band system in wavelengths of 200–400 nm. Results predicted by the current model show qualitative spatial agreement with the measured data. At a velocity of 3.5 km/s(about Mach11), the peak absolute intensity at an altitude of 38 km is two orders of magnitude higher than that at 53.5 km. Under the same flight conditions, the spectra structures have quite a similar distribution at different viewing angles. The present computational model performs well in the prediction of the ultraviolet spectra emitted from the shock layer and will contribute to the investigation and analysis of radiative features of hypersonic vehicles in near space.     

Numerical simulations of water spray on flame deflector during the four-engine rocket launching

This paper aims to study on the cooling effect with two types of water spray nozzle on the flame deflector during the four-engine launch vehicle take-off. To accurately simulate the two-phase flow of the rocket gas with multispecies and the water spray, the three-dimensional compressible Navier-Stokes equations, discrete ordinates methods and realizable k-Ɛ turbulence model are used to establish the rocket supersonic plumes impact model. The Eulerian dispersed phase (EDP) model was used to simulate the water spray into the exhaust gas. The accuracy and effectiveness of the gas-liquid flow model are verified by a good agreement between simulation results and experimental data. On this basis, a series of numerical simulation studies under different water injection position are performed. The results show that the high temperature regions, along the axis of engines on the deflector plate, have no significant temperature decreasing effect by water spray from the nozzles mounted on the apex of the deflector, and the high temperature converts a large quantity of water into vapor near the plume boundary, which would decrease the flow conductivity. With the cooling spray nozzle fixed directly to the deflector plate, the temperature decrease effect is obvious and the effect of thermal shock on deflector plate induced by exhaust plume is reduced, so that it can prevent the flame deflector from thermal ablation. The study results provide indepth information and engineering guidance for designing the water spray systems and increasing the safety of the launch process.     

基于TEC的空间站末端回路温控系统建模及其热力学性能分析

针对空间站中间回路温度波动过大,高温时导致科学载荷工作温度超出允许范围的问题,设计了一种基于热电制冷器(TEC)的末端单向流体回路温控系统。该系统包含一个TEC温控模块,当中间回路温度过高,末端回路冷却功率不足时,该模块可提供额外的制冷量,降低流入冷板的工质温度,形成针对科学载荷的相对低温区域,恢复回路的冷却能力。分别建立了温控系统数学模型与数值仿真模型,并完成了热负载扰动、中间回路温度扰动、末端回路流量扰动和并联支路热扰动等4种扰动对系统热力学特性影响的仿真分析,验证了TEC模块的温控性能。结果表明:在科学载荷发热功率增加30%、中间回路的温度升高5K、末端回路流量减小至0.0015kg/s等多种工况下,所设计的温控系统能够将载荷温度控制在1K以内,实现科学载荷精确温控。      

火星表面热环境对航天器热控影响分析

火星大气对太阳辐射产生吸收和散射作用，同时还将与火星表面航天器发生对流换热。热设计时难以直接评估对流、辐射和导热三种换热对航天器的影响，从而确定主要的控温途径。在调研火星表面辐射、大气等热环境的基础上，从线性化传热系数和对流辐射比的角度对比分析了辐射、对流和导热对航天器的影响。器表辐射传热系数随光学属性和温度的变化范围为0.3～1.4W/(m2·℃)，对流传热系数随风速变化为0.2～1.5W/(m2·℃)，器内导热传热系数可控制在0.25W/(m2·℃)以下。结果表明，太阳辐射较火星表面和天空辐射而言是主要外热源，航天器表面的辐射和对流换热为两条并联换热途径，两者均可成为主要换热途径，器内导热传热是控制航天器内外隔热的主要可控因素。     

多状态空间信息网络拓扑生成优化算法

依据空间信息网络（SIN）高动态性的特点，并考虑卫星工作的多状态特性，兼顾星间通信时延和拓扑抗毁性的要求，研究了多状态下空间信息网络拓扑生成及动态优化的问题。根据卫星星座的周期性，建立了一种卫星网络的拓扑周期表。综合卫星的可视性和连接度等约束条件，以网络平均和最大时延作为通信性能的优化目标，建立拓扑的多目标优化模型。提出一种改进的多目标模拟退火（IMOSA）算法，求解全局时延最优的卫星拓扑，并在考虑多状态情况下对链路进行优化，以满足网络高动态性。最后基于具有66颗低轨（LEO）的铱星星座进行仿真，研究表明：针对多状态条件下的铱星星座，该算法最大化减小了通信时延，得到抗毁性良好的拓扑结构，通信性能较之原有静态拓扑明显得到改善。