空天机复合循环推进技术新概念研究——液化空气循环在其中的应用

研究了空天机复合循环推进技术中的一个新概念——以液化空气循环为基础的SERJ组合发动机性能。计算了空气液化后分离为液氧和液氮后组合发动机在不同高度、不同飞行马赫数下的性能曲线,并考虑了液化空气量对组合发动机性能的影响。对计算结果的分析表明,液化空气循环虽然使组合发动机推力下降,但能使比冲有较大幅度的上升;液化空气量过大与过小均不利于进一步提高比冲性能,而是存在一个最佳值。     

原子谱线参数的辨识方法

在一种原子谱线参数测量的辨识方法基础上编制了一套原子港线参数辨识的标准软件。用此软件对纯氩和氩、氮混合非平衡电弧等离子体射流的原子谱线进行了处理，获得了射流的电子温度、气体平动温度、电子和原子数密度。状态诊断表明；实验条件下的等离子体射流除中心点为ＬＴＥ外非平衡效应是非常显著的。     

航空发动机钛火试验技术研究新进展

钛火是现代航空发动机典型的灾难性故障.针对高推重比发动机对钛火试验技术的迫切需求,系统开展了摩擦氧浓度法钛合金燃烧技术及理论研究,建立了阻燃性能评价方法和摩擦着火模型,阐明了阻燃钛合金的阻燃机理.在总结近期研究进展基础上,从钛火的演化规律、机理和防控三个层次,提出钛火试验技术及应用研究的思路和方向,即接近发动机气流环境的阻燃性能综合评价、发动机气流环境的阻燃性能预测模型和阻燃技术的试验验证.未来实现发动机钛火防控体系的科学构建,助推压气机“全钛化”和发动机推重比不断提高.     

液氧/甲烷发动机评述

简要介绍了国外液氧/甲烷发动机的研究情况。重点论述了甲烷的特点及它用作液体燃料的优缺点。液氧/甲烷发动机具有较高的性能,甲烷有好的再生冷却性能,是一个可供选择的推进剂组合。但由于其密度比冲比液氧/煤油发动机低,使用安全性也不如煤油;性能又比液氧/液氢发动机低,这些都限制了液氧/甲烷发动机的发展和应用。迄今为止,还没有一个液氧/甲烷发动机型号开展研制工作,因而也就不可能有其使用的历史。     

玻璃纤维复合材料的原子氧剥蚀效应试验研究

对两种玻璃纤维复合材料开展了原子氧效应的地面模拟试验研究。总结了试验前后试样质量及表面形貌的变化规律，计算得到了材料的剥蚀率。试验结果表明，随着原子氧累积通量的增大，玻璃纤维复合材料的质量和体积损失减慢。经分析认为，在原子氧与复合材料的作用过程中，树脂优先被剥蚀，而将纤维暴露在外，由于玻璃纤维对底层树脂基体的遮挡作用，导致在原子氧效应试验后期，玻璃纤维复合材料的剥蚀速度减缓。     

研究原子氧对空间材料效应的氧等离子体试验装置

介绍我所研制成的一台评价原子氧对空间材料效应的高频放电氧等离子体试验装置的结构和性能.对Kapton试样的测试表明:用这种装置试验的结果与美国洛克希德公司装置的测试结果相当.其作用强度相当于200km高度轨道中原子氧作用强度的4倍以上.     

IIR滤波器在芯片原子钟中的应用

芯片原子钟是具有小体积,低功耗特点的原子钟。本文采用了IIR滤波器方案对芯片原子钟物理系统输出信号进行处理,该方案有利于减小芯片原子钟的体积、提高芯片原子钟短期频率稳定度。实验结果表明,与FIR滤波方案相比,IIR滤波器使用的FPGA资源减小了约58%;与现有模拟滤波方案相比,使用IIR滤波器方案的芯片原子钟频率稳定度提高了1.4×10~(-10)τ~(-1/2)(τ=1s-100s),电路面积减小了10%。     

多元高温合金固溶极限预测

综合考虑了溶质元素与基体元素的原子半径、电负性以及外层电子数的立方根对溶质元素固溶度的影响，推导出二元合金的固溶度定量方程，提出了多元高温合金固溶极限曲线的预测新方法，并将其应用于计算镍基和钴基三元合金相图的γ／（γ＋σ）相界和γ（γ＋μ）相界。结果表明，计算的固溶极限曲线与已知相图的固溶极限曲线较吻合，与Ｍｄ值法计算的相界比较，该方法具有较高的精度。     

Experimental comparison between aircraft fuel tank inerting processes using NEA and MIG

Fuel tank inerting technologies are able to reduce the fire risk by injection of inert gas into the ullage or fuel, the former called ullage washing and the latter fuel scrubbing. The Green On-Board Inert Gas Generation System (GOBIGGS) is a novel technology based on flameless catalytic combustion, and owning to its simple structure and high inerting efficiency, it has received a lot of attentions. The inert gas in the GOBIGGS is mainly comprised of CO₂, N₂, and O₂ (hereinafter, Mixed Inert Gas (MIG)), while that in the On-Board Inert Gas Generation System (OBIGGS), which is one of the most widely used fuel tank inerting technologies, is Nitrogen-Enriched Air (NEA). The solubility of CO₂ is nearly 20 times higher than that of N₂ in jet fuels, so the inerting capability and performance are definitely disparate if the inert gas is selected as NEA or MIG. An inerting test bench was constructed to compare the inerting capabilities between NEA and MIG. Experimental results reveal that, if ullage washing is adopted, the variations of oxygen concentrations on the ullage and in the fuel are nearly identical no matter the inert gas is NEA or MIG. However, the ullage and dissolved oxygen concentrations of MIG scrubbing are always higher than those of NEA scrubbing.     

Loop Models from SOHO Observations

The Coronal Diagnostic Spectrometer (CDS) on SOHO is a grazing/normal incidence spectrograph, aimed to produce stigmatic spectra of selected regions of the solar surface in six spectral windows of the extreme ultraviolet from 150 Å to 785 Å (Harrison et al. 1995). In the present work, CDS, EIT, MDI and Yohkoh observations of active region lops have been analyzed. These observations are part of JOP 54. CDS monochromatic images from lines at different temperatures have been co-aligned with EIT and MDI images, and loop structures have been clearly identified using Fe XVI emission lines. Density sensitive lines and lines from adjacent stages of ionization of Fe ions have been used to measure electron density and temperature along the loop length; these measurements have been used to determine the electron pressure along the loop and test the constant pressure assumption commonly used in loop modeling. The observations have been compared with a static, isobaric loop model (Landini and Monsignori Fossi 1975) assuming a temperature-constant heating function in the energy balance equation. Good agreement is found for the temperature distribution along the loop at the coronal level. The model pressure is somewhat higher than obtained from density sensitive line ratios.