空间真空环境下密封电磁继电器的触点失效研究

密封电磁继电器有其固有的漏率,在应用于空间真空环境下由于气体泄漏使得其内部气体压力逐渐降低,导致继电器的触点在低气压环境下工作失效（负载切换时）。文章选择国产继电器样品对上述机理进行了试验验证,并对继电器内部气体压力与触点电弧失效的规律进行了研究。     

高原航线飞机颠簸出现规律的对比分析——以青藏高原与云贵高原为例

不同的高原产生大气湍流的条件不尽相同,因此航线上飞机颠簸的出现规律也不一样。分析青藏高原和云贵高原的地形差异和气候区别,并根据四川航空公司的机载QAR数据,对青藏高原和云贵高原的飞机颠簸出现次数、出现概率和颠簸强度进行统计,对比分析了青藏高原和云贵高原航线上飞机颠簸的出现和分布规律,为高原航线飞机颠簸的预报和航行签派工作提供重要参考。     

综合模块化航电软件仿真测试环境研究

 伴随着综合模块化航空电子(IMA)软件在新一代飞机上的应用,其高复杂性、高度综合的特点以及分层的健康监控和故障管理模式给软件测试提出了挑战。传统的仿真测试环境在应对IMA软件测试中难以满足RTCA DO-178B中规定的对验证过程结果的验证的要求。本文在分析IMA软件特点的基础上,根据DO-178B的要求,综合国外的发展情况和国内的研究进展情况,研究综合模块化航电软件仿真测试环境需求,提出了基于软件故障注入的综合模块化航电软件灰盒仿真测试环境方案,并给出优势分析。该仿真测试环境方案以IMA软件为测试对象,应用软件故障注入技术和代码插装技术满足测试规范文件的要求。其具有通用灵活、适配性强、强实时性等特点,为中国新一代航电软件的系统验证和测试奠定了基础。     

基于Eclipse的航天嵌入式软件集成 开发环境设计与实现

针对当前航天器软件研制过程中需要使用多种开发工具的问题,设计实现了集工程管理、代码编辑、语法检查、编译链接和调试测试于一体的航天嵌入式软件集成开发环境.研究成果已应用于航天器嵌入式软件的研发,缩短了软件研发周期并提高了软件质量,同时也为软件集成开发环境的研发提供借鉴.     

大型民用飞机应急撤离模型与仿真方法研究

在元胞自动机模型和行人流模型基础上,解决了飞机疏散模型中的元胞严重冲突问题,实现了模型元胞速度动态可变和对不同出口的流量控制,针对多出口状态下准确地模拟绕过复杂障碍物等要求,建立了基于大型飞机环境特点约束的网格吸引力概率模型,并通过应用某型飞机客舱布局作为算例进行了乘客应急疏散的过程模拟。最后在DELMIA平台下对人员的疏散行为进行建模并实现三维演示验证,模型的仿真过程接近真实情况,仿真结果和现有疏散实验结果相吻合。     

铝电解电容在湿热环境下的贮存可靠性

针对电子设备中的铝电解电容在贮存环境下的失效问题,通过对铝电解电容进行湿热贮存试验,考察了湿热环境引起的铝电解电容外观状态和电性能的变化,并对试验中出现的失效现象进行了分析.结果表明,铝电解电容在湿热环境下出现了引脚腐蚀和橡胶塞长霉的失效现象;环境温度对铝电解电容贮存可靠性有重要影响,温度超过40℃引脚腐蚀速度会大大加快.温度在30℃适宜霉菌生长,温度超过30℃后没有长霉现象.阳极箔上的阳极氧化膜被腐蚀是铝电解电容在湿热环境下出现电容量和漏电流增大的原因.     

海洋环境对吊放声纳作战使用影响研究

作战海域海洋环境对航空吊放声纳工作深度、探潜能力有重要影响。文中以声纳方程为基础,分析了作战海域海况、深度等海洋环境因素对吊放声纳作战使用及探测能力的影响,为合理使用吊放声纳提供了依据。     

战斗机综合热能管理系统稳态仿真

建立综合热管理系统稳态仿真数学模型,在SIMULINK软件平台上搭建仿真模块,对系统同一高度不同马赫数及同一马赫数不同高度进行了稳态仿真,得到系统中关键部件的进出口温度和流量,并分析了马赫数以及高度变化对各状态点温度的影响。分析得出马赫数增加各状态点的温度基本是增加的,只有燃油冷却出口温度先减后增;各状态点的温度随高度的增高基本是减小的,只有燃油冷却出口温度是增加的。     

Charging of dust grains by anisotropic solar wind multi-component plasma

In this paper we study the charging process of small grain particles by anisotropic multi-component solar wind plasmas (electrons, protons and heavy ions), versus two-component (electron/proton) plasmas. We are focusing attention on the important characteristics of the charging process, namely the charging time, floating potential and current content as functions of plasma parameters such as He⁺⁺/H⁺ (α/p) number density and T_α/T_p temperature ratios of alpha particles to protons, as well as plasma streaming velocity v₀. Measured statistical properties of solar wind plasma parameters at 1 AU show considerable variations in α/p-temperature ratios from 1 to 10, in α/p-number density ratio from 0.01 to 0.35, as well as in values of streaming velocity v₀ from 200 km/s to 1000 km/s and more. Periods of these variations could last for several days each, leading to significant variability in the charging process, according to newly derived general analytical expressions. Numerical calculations performed for protons/alphas plasmas showed large disparity in the charging characteristics. For example, in anisotropic plasma, grain charging time varies up to 90% depending on α/p-particles temperature and number density ratios, whereas changes in floating potential are up to 40%. In contrast, in isotropic plasma, charging characteristic for grains do not change very much for the same plasma parameters variations, with charging time varying about 12% and floating potential only varying about 4%. It is also shown that in highly anisotropic plasma, with all ballistic electrons and ions, dust grains could not hold their charges, and characteristic discharged time is calculated. We note that the analysis is equally applicable to any sized body immersed in solar wind plasma.     

Kinetic theory of sheath formation in solar wind plasma

We present a general self-consistent kinetic theory for plasma sheath formation in solar wind plasma. The theory could be applied to anisotropic, as well as to isotropic collisionless plasma without resorting to any simplifications, limitations, or assumptions, such as the necessary existence of a ‘pre-sheath’ region of ions acceleration to ensure the Bohm criterion. The kinetic framework is first applied to sheath formation around an arbitrary oriented planar absorbing surface, charged by solar wind anisotropic plasma, under the condition of negligible photoelectric effect. We then make use of our kinetic approach for the plane geometry in isotropic collisionless plasma, as a particular case of a planar electrode orientation parallel to plasma streaming velocity, also analyzing the sheath structure around spherical and cylindrical absorbing electrodes submerged in isotropic collisionless plasma. Obtained results demonstrate principal differences in spatial charge distributions in sheath regions between spherical or cylindrical electrodes of large size and an unbound planar surface submerged in isotropic plasma. In the case of a planar electrode, we directly compare results obtained in our kinetic and hydrodynamic theories and conventional hydrodynamic theory of plasma sheath formation. The outcome from the present study have direct implications to the analysis of plasma sheath structure and associated distribution in space of charged dust grains, which is relevant to the moon exploration near the optical terminator region or in shadowed craters in the moon.