磁暴期间甚低纬哨声的导管传播

对磁暴期间甚低纬哨声导管传播的机理进行了初步的讨论，根据暴时低纬哨声的特点，认为暴时出现的扩展哨、多跳回波是沿东向扰动电场导致的场列电离增强路径传播的。对在东向电场影响下低纬Ｆ层的数值模拟表明，东向电场导致的场列电离增强结构有利于哨声的捕获和传播。     

平台压强指数附加物“TCA”与配方组分粒度和含量的关系

较详细地叙述了平台推进剂压强指数附加物“ＴＣＡ”与推进剂组与的粒度、含量的关系。     

MHD structures, waves and turbulence in the solar wind: Observations and theories

A comprehensive overview is presented of recent observational and theoretical results on solar wind structures and fluctuations and magnetohydrodynamic waves and turbulence, with preference given to phenomena in the inner heliosphere. Emphasis is placed on the progress made in the past decade in the understanding of the nature and origin of especially small-scale, compressible and incompressible fluctuations. Turbulence models to describe the spatial transport and spectral transfer of the fluctuations in the inner heliosphere are discussed, and results from direct numerical simulations are dealt with. Intermittency of solar wind fluctuations and their statistical distributions are briefly investigated. Studies of the heating and acceleration effects of the turbulence on the background wind are critically surveyed. Finally, open questions concerning the origin, nature and evolution of the fluctuations are listed, and possible avenues and perspectives for future research are outlined.     

Augmented Empirical Models of Plasmaspheric Density and Electric Field Using IMAGE and CLUSTER Data

Empirical models for the plasma densities in the inner magnetosphere, including plasmasphere and polar magnetosphere, have been in the past derived from in situ measurements. Such empirical models, however, are still in their initial phase compared to magnetospheric magnetic field models. Recent studies using data from CRRES, Polar, and Image have significantly improved empirical models for inner-magnetospheric plasma and mass densities. Comprehensive electric field models in the magnetosphere have been developed using radar and in situ observations at low altitude orbits. To use these models at high altitudes one needs to rely strongly on the assumption of equipotential magnetic field lines. Direct measurements of the electric field by the Cluster mission have been used to derive an equatorial electric field model in which reliance on the equipotential assumption is less. In this paper we review the recent progress in developing empirical models of plasma densities and electric fields in the inner magnetosphere with emphasis on the achievements from the Image and Cluster missions. Recent results from other satellites are also discussed when they are relevant.     

影响模压成型碳/环氧复合材料制件性能的因素分析

文章简述了碳/环氧复合材料模压成型工艺特性,从模压成型模具基本要求、模压成型温度、压力和保温时间等工艺参数对制件性能的影响作了较为详细分析。文中还提出将复合材料基础理论分析应用于生产过程中,对有效控制制件工艺状态稳定及其性能具有一定的现实意义。     

碳／环氧复合材料薄壁细长管件的研制与试验

文章简要介绍了碳／环氧复合材料薄壁细长管件的研制情况，着重介绍了工艺方案选定、选材和材料特性试验、成型工艺及解决主要技术难点等内容。制品经地面环模和飞行试验考验，取得了满意效果。     

集中涡法在计算旋成体大迎角气动特性中的应用

本文用集中涡法计算了尖头旋成体在大迎角时的气动特性。基于实验数据,选取了一组比较合适的自由积分参数,建立了初始分离角和雷诺数之间的经验关系式,从而在计算中较好地考虑了雷诺数的影响。马赫数的影响是通过Gthert法则进行修正予以考虑的。旋涡运动的微分方程组是用变步长的四阶龙格-库塔法来求解的。根据不同的积分位置分别选择三种不同的积分初始步长,以提高计算速度。本文对F_3A16和F3.5A7两种模型作了计算,计算结果和实验结果吻合得较好。     

Emission heights of coronal bright points on Fe XII radiance map

The study of coronal bright points (BPs) is important for understanding coronal heating and the origin of the solar wind. Previous studies indicated that coronal BPs have a highly significant tendency to coincide with magnetic neutral lines in the photosphere. Here we further studied the emission heights of the BPs above the photosphere in the bipolar magnetic loops that are apparently associated with them. As BPs are seen in projection against the disk their true emission heights are unknown. The correlation of the BP locations on the Fe XII radiance map from EIT with the magnetic field features (in particular neutral lines) was investigated in detail. The coronal magnetic field was determined by an extrapolation of the photospheric field (derived from 2-D magnetograms obtained from the Kitt Peak observatory) to different altitudes above the disk. It was found that most BPs sit on or near a photospheric neutral line, but that the emission occurs at a height of about 5 Mm. Some BPs, while being seen in projection, still seem to coincide with neutral lines, although their emission takes place at heights of more than 10 Mm. Such coincidences almost disappear for emissions above 20 Mm. We also projected the upper segments of the 3-D magnetic field lines above different heights, respectively, on to the tangent x–y plane, where x is in the east–west and y in the south–north direction. The shape of each BP was compared with the respective field-line segment nearby. This comparison suggests that most coronal BPs are actually located on the top of their associated magnetic loops. Finally, we calculated for each selected BP region the correlation coefficient between the Fe XII intensity enhancement and the horizontal component of the extrapolated magnetic field vector at the same x–y position in planes of different heights, respectively. We found that for almost all the BP regions we studied the correlation coefficient, with increasing height, increases to a maximal value and then decreases again. The height corresponding to this maximum was defined as the correlation height, which for most bright points was found to range below 20 Mm.     

气动补偿空速管的研究与发展

气动补偿空速管是与飞行安全性和飞机飞行的高度分层密切相关的重要器件,在改进现役飞机和设计新机空速系统中起着重要作用。本文依据多年来大量的气动计算和风洞实验所得到的结果,叙述了气动补偿空速管的原理、分类、设计思想、特点、风洞校准、气动计算、使用和发展等情况。     

极低湍流度下翼型边界层及近场尾流的雷诺应力测量试验研究

在西北工业大学低湍流度风洞中，用热线风速仪在对称翼型边界层及近场尾流中，于２０多处剖面上移测速度型、湍流强度、雷诺正应力及切应力等湍流参量。着重讨论了各雷诺应力分量的分布。结果表明，在边界屋和尾流宽度方向及流动方向上均有明显的规律性，其有关特征值明显低于常规风洞湍流度下的结果。