载人月面着陆及起飞技术初步研究

载人登月任务中最具特色的就是载人月面着陆及起飞过程,其技术体系丰富,是影响载人登月任务成败的关键环节。文章详细分析了载人月面着陆及起飞阶段的飞行方案,阐述了载人任务与无人任务设计准则上的区别,剖析了载人月面着陆及起飞技术的内涵。此外重点分析了低温推进剂蒸发量控制技术、10∶1深度变推力液体发动机技术、发动机推力矢量控制技术、大承载着陆缓冲技术、发动机羽流导流与防护技术、月尘清除及防护技术等六项与载人登月舱推进系统和结构系统相关的关键技术,分析提出了相应的技术途径和解决方案,对深入认识载人登月飞行器系统的技术体系及技术难度具有重要意义。     

新型浮动式收敛袋型密封自适应同心性能数值与实验研究

提出了新型浮动式收敛袋型密封结构，建立了新型收敛袋型密封数值求解模型，研究新型收敛袋型密封周向压力分布规律，分析进出口压比和偏心率对新型收敛袋型密封泄漏量及浮动同心力的影响。设计搭建了浮动式自同心密封实验台，在数值计算结果与实验测试结果相互验证的基础上，研究进出口压比和偏心率对新型浮动式收敛袋型密封泄漏量及自适应同心性能的影响。研究结果表明：在本文研究工况下，新型收敛袋型密封所产生的浮动同心力是传统迷宫密封的8.9~10.9倍。在不同进出口压比和偏心率下，传统浮动式迷宫密封均始终处于初始偏心位置，自适应同心性能较差。新型浮动式收敛袋型密封均向转子轴心方向移动，且随着进出口压比和偏心率的增大，浮动响应时间缩短，自适应同心性能增强。新型浮动式收敛袋型密封具有良好的浮动响应特性和自适应同心性能。     

高温热源羽流流场及伴生粉尘控制特性

采用CFD数值模拟软件对高温热源上部接受罩的羽流温度场和速度场进行分析,比较不同工况下上部伞形接受罩对高温烟气的控制特性,同时提出合理设置排风罩位置和风量的措施。     

封闭圆柱形粉尘爆炸罐内扬尘诱导湍流特性的确定

采用热线风速仪和系综平均法测定和研究了封闭圆柱形粉尘爆炸罐内扬尘湍流的瞬态特性，并与球形爆炸容器内已测定的扬尘湍流瞬态特性进行了比较，对系综平均法用于扬尘湍流的测量误差与测量次数的关系进行了探讨。     

静电效应及其防护

静电放电是两个具有不同电位的物体,由于直接接触或静电场感应而引起的两物体间电荷的转移,静电放电产生宽带干扰。本文分析了静电干扰的机理,并介绍了飞机及机上的燃油、电爆装置、信息技术设备的静电防护措施和电子产品静电放电敏感度测试方法。     

静电悬浮微加速度计高灵敏度电容检测通道设计

高灵敏度电容式位移检测是实现静电悬浮微加速度计闭环测控的关键技术之一.针对微加速度计径向悬浮检测的特点及指标要求,设计了高灵敏度、高精度电容式微位移检测通道.该通道主要由前置RC隔离网络与C/V转换、高共模抑制比差动放大器、二级运放、二阶压控电压源有源带通滤波、相敏解调(含模拟乘法器与四阶Butterworth低通滤波...     

粉尘爆炸与爆炸危险度评价

分析了粉尘爆炸的分类、条件、特性、因素、爆炸极限和最小点火能,重点介绍了粉尘爆炸的机理。在此基础上,采用Fuzzy评价的方法,建立了发生粉尘爆炸的危险度评价模型。     

GEMS at the Galactic Cosmic-Ray Source

Galactic cosmic rays probably predominantly originate from shock-accelerated gas and dust in superbubbles. It is usually assumed that the shock-accelerated dust is quickly destroyed by sputtering. However, it may be that some of the dust can survive bombardment by the high-metallicity gas in the superbubble interior, and that some of that dust has been incorporated into solar system materials. Interplanetary dust particles (IDPs) contain enigmatic submicron components called GEMS (Glass with Embedded Metal and Sulfides). These GEMS have properties that closely match those expected of a population of surviving shock-accelerated dust at the GCR source (Westphal and Bradley in Astrophys. J. 617:1131, 2004). In order to test the hypothesis that GEMS are synthesized from shock-accelerated dust in superbubbles, we plan to measure the relative abundances of Fe, Zr, and Mo isotopes in GEMS using the new Resonance Ionization Mass Spectrometer at Argonne National Laboratory. If GEMS are synthesized from shock-accelerated dust in superbubbles, they should exhibit isotopic anomalies in Fe, Zr and Mo: specificially, enhancements in the r-only isotopes ⁹⁶Zr and ¹⁰⁰Mo, and separately in ⁵⁸Fe, should be observed. We review also recent developments in observations of GEMS, laboratory synthesis of GEMS-like materials, and implications of observations of GEMS-like materials in Stardust samples.     

Spatial distribution and orbital properties of interplanetary dust at high latitudes

Although the interplanetary dust cloud is assumed to be mainly concentrated in the ecliptic plane, there is a component of dust particles on highly inclined orbits that forms the out-of-ecliptic distribution. The ULYSSES mission for the first time makes this component accessible to in-situ, detection. Evidence for this dust component is also provided from the analysis of the Zodiacal light brightness and especially from the spherical shape of the solar F — corona. An obvious source for an out-of-ecliptic dust population is the activity of comets on high eccentric, highly inclined orbits. We discuss the dynamical conditions of particles under the influence of the radiation pressure when released from the comet and discuss their input to the dust cloud based on brightness analysis and in-situ results.     

某型飞机发电机供电系统一起典型故障的分析

分析了在维修过程中某型飞机发电机供电系统的一起典型故障的原因,详述该故障排除的过程,以及通过此故障的排除获得的两点启示。