纯镁和镁锂合金在中性3.5%NaCl溶液中的腐蚀行为

采用电化学方法研究了纯Mg和Mg-Li合金在中性3.5%NaCl溶液中的腐蚀行为,采用扫描电镜观察了腐蚀后的表面形貌,利用XRD测试了腐蚀前后纯Mg和Mg-Li合金表面的组成成分,并用失重法测试了腐蚀速率。结果表明:腐蚀初期,纯Mg的腐蚀电流小于Mg-Li合金,纯Mg的腐蚀电位高于Mg-Li合金,纯Mg的电化学反应电阻大于Mg-Li合金。经过24h腐蚀后,纯Mg的腐蚀速率大于Mg-Li合金,且两者腐蚀形貌不同,纯Mg的腐蚀坑大而深,蚀坑数量少;Mg-Li合金的腐蚀坑小而浅,蚀坑数量多并且表面变黑。纯Mg的腐蚀产物主要为Mg(OH)2,Mg-Li合金的腐蚀产物主要为Mg(OH)2,LiOH,MgLi,Mg3Li7,Al2O3。     

溅射靶对离子推力器的热辐射影响研究

为了研究真空环境设备内溅射靶温度升高后对30 cm离子推力器的热辐射影响,采用有限元分析的方法,首先对真空舱内的离子推力器羽流分布进行了模拟,在获得羽流对溅射靶造成的温度变化后,进一步分析了溅射靶温度升高对离子推力器温度以及栅极热形变位移所造成的影响.仿真结果显示,推力器羽流可采用定向分子流模型进行描述,羽流在真空舱内...     

数值模拟喷焰2.7微米红外辐射特性

以固体火箭发动机尾喷焰的红外探测为主要应用背景,利用反向蒙特卡罗法和有限体积法计算了火箭尾喷焰红外辐射特性,获得了尾喷焰在探测波长为2.7μm下的红外辐射的空间、光谱分布特性,两种方法的计算结果也非常接近,具有重要的理论意义和实际应用背景。     

Investigation on plume interference effect of solid propellant micro-thruster

The three-dimensional numerical simulation of two-phase plume flow of solid propellant micro-thrusters was developed. Then it was used to investigate the plume interference effect by combining the direct simulation Monte Carlo (DSMC) method for multi-component gas flow with the two-way coupling model for two-phase rarefied flow. At different space between the two micro-thrusters and different wall temperature,the plume interference effect was analyzed specifically. The results show that under the plume interference effect the gas is compressed and the flow direction is changed,which resulted in the increasing of gas pressure and temperature; solid phase made no significant effect on the flow parameters of gas phase; with the rising of the space between the two micro-thrusters,the maximum pressure decreased and the maximum temperature increased in the domain under the plume interference effect; the wall temperature could influence the temperature of the gas which is extremely close to the wall,but not the gas pressure.      

轻型飞机纵向静稳定性试验的估算

推导出了在试飞试验前对轻型飞机纵向静稳定性进行估算的公式,分别给出了握杆和松杆状态下静稳定性的估算方法。在此估算的基础上推导出了试飞试验时所要测的驾驶杆位移和杆力等估算式,进而提出了从试验数据到飞机中性点和实际纵向静稳定裕度的分析处理方法。     

一种快速求解Orr-Sommerfeld方程中性稳定性曲线的方法

提出一种快速准确求解 Orr- Som merfeld(O- S)方程的中性曲线和临界雷诺数 Recr的方法。在求解过程中 ,先分析 a0 ,cr0 的范围 ,利用网格自适应自动搜索 a0 ,cr0 ,采用三次样条函数计算并迭代到一定精度从而获得雷诺数 Re与波数 a及波速 cr 的关系曲线 ,克服了通常求解中性曲线时 ,要预估每一点的 a,cr的不足。算例表明 ,本方法计算速度快 ,结果准确 ,花较少的机时就能计算出与谱方法精度相当的临界 Recr。     

对流辐射板抑制涡扇发动机热喷流红外辐射的实验

用对流辐射换热板来降低混合排气涡扇发动机热喷流的红外辐射,并在涡扇发动机热喷流模拟实验台上进行了实验研究.测量了安装对流辐射换热板前后,轴对称喷管的热喷流的温度分布,轴对称喷管和二元喷管的热喷流在3～5 μm波段的红外辐射强度.结果表明:对流辐射换热板可以降低热喷流高温核心区的温度约10%,降低涡扇发动机热喷流的红外辐射强度约20%～30%.      

基于BP神经网络的装备备件重要度评估

针对装备备件重要度的评估问题,构建了相应的评估指标体系,建立了用于备件重要度评估的三层BP神经网络.然后,构造样本对BP神经网络进行训练,利用训练好的网络对备件重要度进行评估.结果表明,该方法能够较好地克服人为因素和模糊随机性的影响,取得了较好的评估效果.     

Neutral Atmospheres of the Giant Planets: An Overview of Composition Measurements

Measurements of the chemical composition of the giant planets provide clues of their formation and evolution processes. According to the currently accepted nucleation model, giant planets formed from the initial accretion of an icy core and the capture of the protosolar gas, mosly composed of hydrogen and helium. In the case of Jupiter and Saturn (the gaseous giants), this gaseous component dominates the composition of the planet, while for Uranus and Neptune (the icy giants) it is only a small fraction of the total mass. The measurement of elemental and isotopic ratios in the giant planets provides key diagnostics of this model, as it implies an enrichment in heavy elements (as well as deuterium) with respect to the cosmic composition. Neutral atmospheric constituents in the giant planets have three possible sources: (1) internal (fromthe bulk composition of the planet), (2) photochemical (fromthe photolysis ofmethane) and(3) external (from meteoritic impacts, of local or interplanetary origin). This paper reviews our present knowledge about the atmospheric composition in the giant planets, and their elemental and istopic composition. Measurements concerning key parameters, like C/H, D/H or rare gases in Jupiter, are analysed in detail. The conclusion addresses open questions and observations to be performed in the future.