辐射温度计标定误差分析

本文通过理论分析和实验,建立了标准辐射温度计和被检辐射温度计因工作波长不同而产生的标定误差公式,通过几种典型黑体空腹温度分布的测量及有效发射率的计算,讨论了分别以标准辐射温度计和接触温度计校准被检辐射温度计时误差及其走向。     

快速加热恒应力试验方法的初步研究

短时高温试验是适应现代高速飞行器的发展而建立起来的一种新型的力学性能试验方法。目前已有多种试验方案, 其中快速加热恒应力拉伸试验是在某恒定应力下, 以一定的速率加热试件, 测定合金的应变与温度的关系, 并从而求得材料在试验条件下的屈服温度(通常以引起0.2%的残余应变为准)。本文简要地评述了短时高温试验方法的现状; 介绍了为进行快速加热恒应力拉伸试验而建立的试验装置, 并提供了国产Д16AT及B95AT合金的初步试验数据;最后还对所得数据进行处理和分析。     

冲击作用下弹塑性接触的耗能套筒结构的减震性能分析

求解了导弹发射筒内耗能套筒结构在冲击作用下的弹塑性接触问题。依据弹塑性有限元法,应用Lagrange乘子法引入接触区域上的位移协调约束条件,通过迭代修正使每个接触单元满足库仑摩擦律的要求,再按照Newmark β逐步积分法进行计算,求得结构的冲击响应。所得计算结果和相关实验结果吻合良好,表明所提出的计算模型和方法是正确合理的。最后将套筒结构所受的冲量和对应的位移增量进行多项式拟合,得到的拟合公式为耗能套筒结构的设计计算提供了理论依据。     

飞机复杂蒙皮拉形数值模拟系统开发及关键技术研究

针对飞机复杂蒙皮拉伸成形特点,基于静态隐式算法开发了复杂蒙皮拉形数值模拟系统STRETCH FORM。系统分为前置处理、核心求解和后置处理3个模块。介绍了系统各模块的主要功能以及机构运动、静态隐式有限元算法和接触搜索算法等关键技术理论。利用商业软件MARC和PAM STAMP进行了S形蒙皮拉形的模拟计算对比,并对某型号机的进气道蒙皮零件进行了生产验证,结果表明系统具有较高的可靠性和计算精度。     

空间站梦天载荷舱结构设计与验证

针对天宫空间站梦天载荷舱提出了采用一种含大开口的半硬壳铆接结构,实现了结构承载、载荷进出舱及载荷试验平台一体化设计。采用数值仿真的方法,考虑主动段飞行及地面整器起吊载荷等因素的影响,进行了结构强度迭代分析,识别结构的潜在薄弱环节,并开展针对性的局部结构验证试验。最后,设计并建立大开口结构的全工况静力试验平台,开展载荷舱整舱静力试验。数值计算与试验所得结果吻合较好,验证了载荷舱大开口结构设计的正确性。载荷舱结构的设计方法及验证思路可为其他飞行器结构提供参考。     

尺度效应下大功率伺服电机再生冷却通道超临界态甲烷传热特性研究

针对飞行器电动执行机构的大功率伺服电机强化散热问题,建立了不同尺度的电机缠绕式螺旋管再生冷却通道数值模型,对超临界态甲烷在尺度效应影响下的传热特性和机理进行研究,探讨了不同尺度冷却通道中超临界态甲烷所受重力浮升力和离心浮升力对传热性能的影响.结果表明,离心浮升力及重力浮升力均受到超临界态甲烷热物性剧烈变化的影响;在相同...     

密集型空气雾化流场破碎特征数学模型研究

低速液体射流在高速湍流气体作用下的气液同轴射流雾化流场是瞬态密集型喷雾场,高速湍流中影响和控制雾化的因素很多。针对空气雾化流场液核分布与特征进行分析,开发了模拟液核的随机浸入体模型,结合大涡模拟方法对同轴射流空气雾化喷嘴下游流场进行数值模拟。模拟结果与实验结果对比表明：随机浸入体模型可快速捕捉液核的长度和位置信息。当气液动量比M为3~10000时,能够较准确地预测液核长度,当M>10时,其预测结果远优于唯象模型;该模型能够捕捉回流区、大尺度涡等流场结构。同时,可以准确地预测喷嘴附近的液滴粒径,特别是在气流速度较大（>60m/s）时,液滴平均直径预测误差<10%。     

Kalman弹道滤波器的快速收敛性研究

在弹道修正过程中,需根据一段实测弹道参数,准确地估算常规弹箭的飞行弹道。工程中,常应用Kalman滤波方法,结合质点弹道模型建立六状态滤波弹道模型。速度初值估计的准确性,是对滤波过程造成影响的主要因素。为改善这一状况,采用多项式拟合用以对速度状态进行估计并以此作为滤波初始值。在此种估计下滤波,速度滤波过程可快速收敛,位置滤波过程收敛速度大幅度提高,可使最优弹道诸元参数获取时间缩短30%。     

A self-similar solution of a curved shock wave and its time-dependent force variation for a starting flat plate airfoil in supersonic flow

The problem of aeroelasticity and maneuvering of command surface and gust wing interaction involves a starting flow period which can be seen as the flow of an airfoil attaining suddenly an angle of attack. In the linear or nonlinear case, compressive Mach or shock waves are generated on the windward side and expansive Mach or rarefaction waves are generated on the leeward side. On each side, these waves are composed of an oblique steady state wave, a vertically-moving one-dimensional unsteady wave, and a secondary wave resulting from the interaction between the steady and unsteady ones. An analytical solution in the secondary wave has been obtained by Heaslet and Lomax in the linear case, and this linear solution has been borrowed to give an approximate solution by Bai and Wu for the nonlinear case. The structure of the secondary shock wave and the appearance of various force stages are two issues not yet considered in previous studies and has been studied in the present paper. A self-similar solution is obtained for the secondary shock wave, and the reason to have an initial force plateau as observed numerically is identified. Moreover, six theoretical characteristic time scales for pressure load variation are determined which explain the slope changes of the time-dependent force curve.     

Space Weather Service for Chinese Space Science Satellites

Strategic Priority Research Program on Space Science has gained remarkable achievements. Space Environment Prediction Center (SEPC) affiliated with the National Space Science Center (NSSC) has been providing space weather services and helps secure space missions. Presently, SEPC is capable to offer a variety of space weather services covering many phases of space science missions including planning, design, launch, and orbital operation. The service packages consist of space weather forecasts, warnings, and effect analysis that can be utilized to avoid potential space weather hazard or reduce the damage caused by space storms, space radiation exposure for example. Extensive solar storms that occurred over Chinese Ghost Festival (CGF) in September 2017 led to a large enhancement of the solar energetic particle flux at 1 AU, which affected the near Earth radiation environment and brought great threat to orbiting satellites. Based on the space weather service by SEPC, satellite ground support groups collaborating with the space Tracking, Telemetering and Command system (TT&C) team were able to take immediate measures to react to the CGF solar storm event.