复合材料胶接损伤的指数监测方法

为了监测复合材料胶接损伤,基于主动Lamb波和时频分析,提出了一种复合材料损伤监测的指数法。通过对Lamb波信号进行时频分析,提取波形包络。通过计算得到损伤散射信号,选取对损伤敏感的直达波波包,将此波包在结构出现损伤后的能量变化值与损伤前的能量之比作为损伤指示。该方法不用选择特定的Lamb波模式,解决了Lamb波在复合材料结构中存在的频散、多模式及模式转换给信号分析带来的困难。同时在复合材料胶接的损伤演化试验中,对该方法进行了应用验证研究。结果表明:该方法可以用于复合材料胶接损伤的定性和定量分析。     

Broadening of Fe X (6374 Å) profiles above the limb in a coronal hole

Profiles of the visible Fe X (6374 Å) coronal emission line as a function of height above the limb were obtained out to 1.16 solar radii in a coronal hole using the NSO/Sacramento Peak Observatory Coronagraph, Universal Spectrograph and a CCD camera. These are the first coronal line profiles obtained as a function of height in a coronal hole from the ground. Analysis of the line widths suggests a large component of nonthermal broadening which increases with height ranging from 40 to 60 km/s, depending upon the assumed temperature or thermal component of the profile.     

运输飞行成本指数计算

对运输飞行成本进行了划分,提出了计算成本指数的方法,分析了成本指数对运输飞行经济性的影响。以某航空公司为例,计算了该航空公司的成本指数,并在全飞行模拟机上验证了使所计算的成本指数飞行的运输飞行成本。结果表明,使正确的成本指数飞行,将大量节约运输飞行成本。可为航空公司计算自己的成本指数,降低成本,提高运输飞行经济性提供参考。     

基于季节特性的航材备件定量订货模型

为达到降低库存费用、保障飞机持续适航的目的,建立定量订货模型,并通过对部分航材消耗数据的分析,提出利用中心移动平均法求得季节指数的方法,将其作为权系数对该模型进行修正,以提高航材采购数量的精确性。实验证明,该模型能有效地为航材备件的计划采购提供理论指导和决策支持。     

带有太阳电池阵的卫星电源系统在轨测试方法

根据带有太阳帆板的地球同步卫星在轨测试需求,分析了星上电源系统的组成及技术状态;并以光照区可调节母线为例。给出了卫星电源系统在轨测试方法及相应的计算公式;最后,通过工程验证了该方法的正确性。     

平面埋入式进气道的口面参数选择与试验验证

为了提高飞行器的隐身性能和降低其迎风阻力,采用具有平面腹部的低雷达截面外形机身与埋入式进气道的组合是一种良好的解决方案。但迄今尚未有成熟的平面埋入式进气道设计方法可供借鉴,为此对平面埋入式进气道口面参数进行了组合对比研究,旨在通过口面参数的选择来改善进气道的气动性能。在此基础上,选择一组口面参数设计了一梯形进口的平面埋入式进气道方案,并进行了高速风洞试验验证。研究结果表明:(1)进口侧棱决定了所产生的卷吸涡的强度,而前唇口导流角决定了进口段的横向压力梯度,两者均是驱动主流进入进气道内部的关键因素,为此对进气道总压恢复系数和周向畸变指数均有着重要影响;后唇口型线特征参数对进气道出口总压高低压区的分布起着调节作用,为此可以作为控制周向畸变指数的一种辅助措施。(2)合适的口面参数能明显改善平面埋入式进气道的性能。选取23°导流角、4°侧棱角以及30°后唇口型线特征参数组合进行了方案设计和风洞试验验证,在Ma₀=0.7,α＝-2°~8°,β＝0°~2°的范围内,进气道的总压恢复系数在0.920~0.952之间,周向畸变指数在1.142%~2.237%之间,达到了实用水平。(3)研究范围内,攻角的增加有利于改善平面埋入式进气道的总压恢复系数和周向畸变指数,而小角度侧滑时对出口流场畸变的影响不大,不仅未下降,反而稍有增加。     

军用飞机效费综合特性研究

从目前军用飞机效费比概念在实际应用中存在的问题出发,以军用飞机效费综合特性为研究对象,阐述了其产生的背景、定义、内涵、度量方法、控制规律、参数体系和全寿命管理与控制的工作流程,建立了军用飞机效费综合特性及其全寿命管理与控制的基本理论、方法和技术框架。基于目前型号工程中的应用实践,对其应用前景作了进一步的展望。     

基于支持向量机的航空发动机性能衰退指标预测

针对航空发动机性能衰退状态的趋势预测问题,基于非线性支持向量机回归建立了发动机性能衰退指标的预测模型,给出了反映其性能衰退的综合指标。利用该模型对发动机的性能衰退指标进行了预测分析,并与神经网络模型预测结果进行了比较。结果表明:支持向量机回归预测模型能更准确地对发动机的未来状况进行预测。     

飞机外场维修性数据计算与分析方法

迄今为止,飞机的维修性分析工作从理论上说已经比较完善了,但在实际的工程应用中,由于缺乏外场使用过程中对维修性数据的科学正确积累,使得飞机维修性分析工作的开展仍然较为困难.通过对某型机系统及整机外场维修性数据的平均修复时间(MTTR)分析,根据当前外场故障数据实际统计,探索一种工程上可行的维修性数据分析方法.     

A Comparative Study of the Influence of the Active Young Sun on the Early Atmospheres of Earth, Venus, and Mars

Because the solar radiation and particle environment plays a major role in all atmospheric processes such as ionization, dissociation, heating of the upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect of solar induced X-ray and EUV (XUV) heating on the upper atmospheres of Earth, Venus and Mars since the time when the Sun arrived at the Zero-Age-Main-Sequence (ZAMS) about 4.6 Gyr ago. We apply a diffusive-gravitational equilibrium and thermal balance model for studying heating of the early thermospheres by photodissociation and ionization processes, due to exothermic chemical reactions and cooling by IR-radiating molecules like CO₂, NO, OH, etc. Our model simulations result in extended thermospheres for early Earth, Venus and Mars. The exospheric temperatures obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen and high Jeans’ escape rates for heavier species like H₂, He, C, N, O, etc. The duration of this blow-off phase for atomic hydrogen depends essentially on the mixing ratios of CO₂, N₂ and H₂O in the atmospheres and could last from ∼100 to several hundred million years. Furthermore, we study the efficiency of various non-thermal atmospheric loss processes on Venus and Mars and investigate the possible protecting effect of the early martian magnetosphere against solar wind induced ion pick up erosion. We find that the early martian magnetic field could decrease the ion-related non-thermal escape rates by a great amount. It is possible that non-magnetized early Mars could have lost its whole atmosphere due to the combined effect of its extended upper atmosphere and a dense solar wind plasma flow of the young Sun during about 200 Myr after the Sun arrived at the ZAMS. Depending on the solar wind parameters, our model simulations for early Venus show that ion pick up by strong solar wind from a non-magnetized planet could erode up to an equivalent amount of ∼250 bar of O⁺ ions during the first several hundred million years. This accumulated loss corresponds to an equivalent mass of ∼1 terrestrial ocean (TO (1 TO ∼1.39×10²⁴ g or expressed as partial pressure, about 265 bar, which corresponds to ∼2900 m average depth)). Finally, we discuss and compare our findings with the results of preceding studies.