大膨胀比跨声速涡轮流动结构及损失的数值研究

为了揭示跨声速大膨胀比涡轮损失的主要特点和两种不同尾缘冷却方式对损失的影响,以典型大膨胀比跨声速涡轮和跨声速叶栅为研究对象开展了数值研究。研究发现大膨胀比跨声速涡轮的主要损失是叶型损失,占到总损失的65%左右,尾缘激波损失是叶型损失的主要来源。尾缘全劈缝冷气入射通过提高尾缘基压区基压来减少尾缘膨胀波对气流的加速程度,从而降低最高马赫数和激波损失,尾缘压力面劈缝冷气入射通过改变叶片尾缘压力面激波波系结构,使原来的一道激波变成两道或者两道以上的弱激波,从而减少激波损失。两种尾缘冷气方式都有利于降低大膨胀比跨声速涡轮激波损失,但压力面劈缝冷气入射方式效果更为明显。     

飞机液压管路支撑的有限元建模方式对应力分析的影响

在飞机典型液压导管不同构型和负载模式下,做了应力试验测量,得到应力试验的数据,并在有限元环境MSC.PATRAN中,针对导管的不同构型建立有限元分析模型,对每种构型下支架与卡箍采用八种不同的简化方式,得到仿真结果。然后将不同简化方式的仿真结果与试验结果作对比分析,考虑不同因素(如支架刚度、卡箍橡胶刚度、导管与橡胶间的摩擦与滑动等)对分析结果的影响,找到了在工程上简单易行,精度上可以接受的支撑简化方法。     

Ⅲ—Ⅴ族四元固溶体中原子近邻及次近邻的键长表达方式

基于ＦＤＵＣ模型和Ⅲ－Ⅴ族元素共价半径不变的假设，本文出了Ⅲ－Ⅴ族固溶体中原子近邻和次近邻的键长表达式。这套键长表达式除依赖于四个Ⅲ－Ⅴ族元素的含量（ｘ，ｙ）外，只与四个纯化合物的晶胞参数或这四个Ⅲ－Ⅴ族元素的共价半径有关。而且也含盖了相应的伪二元固溶体的情况。本文还对其他的理论模型作了进一步的比较和讨论。     

一种用于液晶曝光中的激光检测系统

介绍了一种非接触式激光检测系统，可用于检测液晶曝光中液晶模板与基板之间的间隙，给出了该种系统的测量原理、硬件系统、信号处理方法、测量结果、分辨力和误差分析，并指出了这种测量系统的应用。     

积木式方法与试验金字塔的历史沿革与发展趋势

采用积木式方法构建试验金字塔是目前已经被广泛接受的用来完成大型飞机结构强度验证的基本手段。本文概述了积木式方法和试验金字塔的发展历程和趋势，介绍了不同型号的美军机在研制过程中所建立的强度验证试验金字塔的统计结果，并且从试验层级、对象、目的和类型等四个方面比较了试验内容的数量与经费占比，由此来说明基础层级试验验证工作在强度验证试验金字塔中重要性和经济性。通过对虚拟试验在强度验证工作中的发展趋势、应用和限制的介绍，为顺利完成相关的全尺寸部件和整机的强度验证提供可靠的保障手段。     

电机瞬态转速测试

介绍了一种利用单片机和光电转速传感器来测量电机瞬态转速及电机转速变化过程的方法。该方法简单、反应时间快、准确度高。     

Filament Thread-like Structures and Their?Small-amplitude Oscillations

Thanks to gradually improving observational capabilities, both from space and ground-based observatories, it is now generally accepted that thin threads (width ??200 km) constitute the building blocks of solar filaments and prominences. At ultra-small scales, high quality image sequences show a non-static picture of filaments and reveal that their oscillatory behavior is an important dynamic feature of these structures. Filament seismology sheds light on the internal magnetic structures of filaments and their interactions with surrounding solar regions. Understanding the overall magnetic topology of solar filaments and prominences including their small-scale thread-like structures is essential in interpretation and understanding of their oscillations. For this reason we aim here to present an update of the dynamic and spatial structures of prominences and filaments as inferred from high resolution observations in the past decennia. Some constraints in high resolution observations are addressed. Our review focuses mainly on the observational aspects and aims to summarize recent oscillation studies of individual filament threads and groups of threads. Finally, some theoretical interpretations of oscillations of filament threads and the inferred physical conditions of filament plasma are also discussed.     

Energy Release and Particle Acceleration in Flares: Summary and Future Prospects

RHESSI measurements relevant to the fundamental processes of energy release and particle acceleration in flares are summarized. RHESSI??s precise measurements of hard X-ray continuum spectra enable model-independent deconvolution to obtain the parent electron spectrum. Taking into account the effects of albedo, these show that the low energy cut-off to the electron power-law spectrum is typically ?tens of keV, confirming that the accelerated electrons contain a large fraction of the energy released in flares. RHESSI has detected a high coronal hard X-ray source that is filled with accelerated electrons whose energy density is comparable to the magnetic-field energy density. This suggests an efficient conversion of energy, previously stored in the magnetic field, into the bulk acceleration of electrons. A new, collisionless (Hall) magnetic reconnection process has been identified through theory and simulations, and directly observed in space and in the laboratory; it should occur in the solar corona as well, with a reconnection rate fast enough for the energy release in flares. The reconnection process could result in the formation of multiple elongated magnetic islands, that then collapse to bulk-accelerate the electrons, rapidly enough to produce the observed hard X-ray emissions. RHESSI??s pioneering ??-ray line imaging of energetic ions, revealing footpoints straddling a flare loop arcade, has provided strong evidence that ion acceleration is also related to magnetic reconnection. Flare particle acceleration is shown to have a close relationship to impulsive Solar Energetic Particle (SEP) events observed in the interplanetary medium, and also to both fast coronal mass ejections and gradual SEP events. New instrumentation to provide the high sensitivity and wide dynamic range hard X-ray and ??-ray measurements, plus energetic neutral atom (ENA) imaging of SEPs above ??2 R_??, will enable the next great leap forward in understanding particle acceleration and energy release is large solar eruptions??solar flares and associated fast coronal mass ejections (CMEs).     

航天器总装过程特种车辆运输问题的研究

文章针对航天器总装过程所涉及的特种车辆转运问题进行研究。通过对特种车辆种类和航天器各平台总装涉及特种车辆数量分析,提出集装箱运输方案并对集装箱进行设计、实施,取得了良好效果,同时指出集装箱化运输也是航天器工装运输的趋势。