固体火箭发动机推力振荡特性数值研究

为了揭示固体火箭发动机推力振荡特性,以大型助推器P230的缩比发动机为基础,使用大涡模拟方法,对障碍物旋涡脱落诱发的振荡流场开展数值模拟,通过对比燃烧室压力、推力的振频和振幅,总结了推力振幅的估算方法.研究结果表明,推力振幅对压力振幅放大机理的关键参数是喉通比,放大比例与喉通比成反比;奇数阶声振型对推力振幅的贡献最大,偶数阶声振型对推力振幅的影响可以忽略,旋涡脱落对推力振幅的作用小于奇数阶声振型,且随涡/声耦合程度的增大而增强.     

Study of Micrometeoroid and Orbital Debris Effects on the Solar Panels Retrieved from the Space Station “MIR”

A study of micrometeoroid and orbital debris (MMOD) long-term effects on solar cell samples of solar panels returned from the space station MIR has been carried out. Five samples from the solar array, which spent over 10 years in space, have been studied with the help of optical microscopes with magnification up to 1000. Craters with dimensions as small as 1m were registered. Additional large impact features were investigated by observing a large number of cells (150) with an optical microscope of small magnification. The aim of the study was to define morphological and statistical characteristics of samples surface damages as well as the extent of surface erosion caused by MMOD impacts. The results of statistical analysis of the data obtained in this study are shown to correlate with the experimental data obtained in the Hubble Telescope solar panel return experiment, and MMOD flux estimations are in good agreement with modern MMOD models. The relative surface area damaged by impacts of small size (1–100m) MMOD particles is estimated to be 0.01%, while the relative surface area of large impact features (greater than 0.1mm) is estimated to be 0.045%.     

温度相依固体推进剂的蠕变损伤模型

针对复合固体推进剂材料,建立了与温度相耦合的蠕变损伤演变模型,进行了单轴和双轴条件下蠕变破断试验,确定了材料参数.该模型对复合固体推进剂的应力分析、寿命预估具有应用价值.     

固体发动机O形橡胶圈密封性能试验研究

分析了O形橡胶圈自然贮存、热空气加速老化、相容性及全尺寸发动机密封结构自然贮存等一系列单项试验结果,得到了O形橡胶圈在压缩状态下的密封贮存性能及其使用期,这些结果可供发动机设计使用.     

NEPE推进剂用中性聚合物键合剂的分子设计

中性聚合物键合剂(NPBA)是美国Kim C.S.发明的一种新助剂。这种键合剂可显著提高NEPE推进剂的力学性能。本文根据Kim C.S.发表的专利和论文,介绍了降温相分离沉积包覆的原理,归纳提出了NPBA的分子设计方法,并且举例说明。     

IR radiation characteristics of rocket exhaust plumes under varying motor operating conditions

The infrared(IR) irradiance signature from rocket motor exhaust plumes is closely related to motor type,propellant composition,burn time,rocket geometry,chamber parameters and flight conditions.In this paper,an infrared signature analysis tool(IRSAT) was developed to understand the spectral characteristics of exhaust plumes in detail.Through a finite volume technique,flow field properties were obtained through the solution of axisymmetric Navier-Stokes equations with the Reynolds-averaged approach.A refined 13-species,30-reaction chemistry scheme was used for combustion effects and a k-e-Rtturbulence model for entrainment effects.Using flowfield properties as input data,the spectrum was integrated with a line of sight(LOS) method based on a single line group(SLG) model with Curtis-Godson approximation.The model correctly predicted spectral distribution in the wavelengths of 1.50–5.50 lm and had good agreement for its location with imaging spectrometer data.The IRSAT was then applied to discuss the effects of three operating conditions on IR signatures:(a) afterburning;(b) chamber pressure from ignition to cutoff;and(c) minor changes in the ratio of hydroxyl-terminated polybutadiene(HTPB) binder to ammonium perchlorate(AP) oxidizer in propellant.Results show that afterburning effects can increase the size and shape of radiance images with enhancement of radiation intensity up to 40%.Also,the total IR irradiance in different bands can be characterized by a non-dimensional chamber pressure trace in which the maximum discrepancy is less than 13% during ignition and engine cutoff.An increase of chamber pressure can lead to more distinct diamonds,whose distance intervals are extended,and the position of the first diamond moving backwards.In addition,an increase in HTPB/AP causes a significant jump in spectral intensity.The incremental rates of radiance intensity integrated in each band are linear with the increase of HTPB,and the growth rates of radiance intensities in some bands reach up to 50% as HTPB weight increases by 3%.     

波音737飞机垂尾高频天线前缘风蚀的预防与修理

波音737飞机垂直尾翼前缘高频天线风蚀是该机型日常维护中的常见故障,本文分析了风蚀的预防以及修理的原理和方法,通过安装聚亚安酯防风蚀膜和喷涂FP-200防风蚀涂层,可有效避免飞机AOG停场,减少运行维护成本以及保障高频天线的通信正常。     

Numerical study on similarity of plume infrared radiation between reduced-scale solid rocket motors

This study seeks to determine the similarities in plume radiation between reduced and full-scale solid rocket models in ground test conditions through investigation of flow and radiation for a series of scale ratios ranging from 0.1 to 1. The radiative transfer equation(RTE) considering gas and particle radiation in a non-uniform plume has been adopted and solved by the finite volume method(FVM) to compute the three dimensional, spectral and directional radiation of a plume in the infrared waveband 2–6 μm. Conditions at wavelengths 2.7 μm and 4.3 μm are discussed in detail, and ratios of plume radiation for reduced-scale through full-scale models are examined. This work shows that, with increasing scale ratio of a computed rocket motor, area of the hightemperature core increases as a 2 power function of the scale ratio, and the radiation intensity of the plume increases with 2–2.5 power of the scale ratio. The infrared radiation of plume gases shows a strong spectral dependency, while that of Al_2O_3 particles shows spectral continuity of gray media.Spectral radiation intensity of a computed solid rocket plume's high temperature core increases significantly in peak radiation spectra of plume gases CO and CO_2. Al_2O_3 particles are the major radiation component in a rocket plume. There is good similarity between contours of plume spectral radiance from different scale models of computed rockets, and there are two peak spectra of radiation intensity at wavebands 2.7–3.0 μm and 4.2–4.6 μm. Directed radiation intensity of the entire plume volume will rise with increasing elevation angle.     

双补燃室固冲凝聚相颗粒分布对比试验研究

针对固冲发动机燃烧效率较低以及凝相粒子分布规律不清楚的现状,本文建立了一套评价固冲发动机燃烧效率的双补燃室试验装置和研究凝相颗粒分布的取样装置。对比研究了结构相同的补燃室内的参数,其误差小于0.5%,说明该装置可以用于精确对比不同补燃室的燃烧效率。然后应用该装置完成了补燃室长度分别为600mm、800mm、1000mm,进气角度分别为30°、45°、60°的对比试验,分析了粒子的粒度分布规律和化学成分变化规律,该规律与数值分析的规律相同。试验结果表明：在进气角度不变情况下,补燃室长度增加有利于提高燃烧效率,燃烧室压强提高,凝相粒子直径明显减小,B粒子燃烧更充分;在补燃室长度为1000mm的情况下,进气角度增加有利于燃烧效率增加,燃烧室压强提高,粒子直径减小,B粒子燃烧更充分。双补燃室发动机是评价补燃室燃烧效率的有效装置,粒度分布和燃烧产物的化学成分有助于补燃室结构设计。     

固体火箭点火超压形成机理与影响因子研究

为研究固体火箭点火超压的形成机理和影响因子,以Ariane 5火箭固体助推器1/35缩比模型为研究对象,〖JP+1〗基于可压缩气体三维Navier-Stokes方程建立固体火箭尾焰流场的数学模型。同时,使用有限速率/涡耗散模型表征尾焰复燃反应,采用有限体积法求解火箭尾焰流场控制方程,得到箭体尾部近场的点火超压幅值与分布情况。与试验数据比较,数值结果较好的反映了点火超压的过程特性。进而,采用该数学模型和求解方法,研究了点火超压的影响因子。计算结果表明,尾焰复燃反应对点火超压的影响较小,与无复燃反应的计算结果比较,点火超压的峰值相对变化幅度不大于1.85%,点火超压的波形与分布特性的变化可以忽略;建压速率越快,点火超压峰值越大,且呈非线性比例关系增长;喷管膨胀比主要影响点火超压的波形,对其峰值影响较小。