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.     

一座柔壁低湍流度风洞收缩段设计及主要工作特性

本文介绍了一座“柔壁低湍流度风洞”收缩段气动设计中的几个关键问題:合理选用较大的收缩比,恰当选定变湍流度网格位置和采用五次方壁型曲线。试验结果表明,这座雷诺数较大的、具有柔壁功能的低(变)湍流度风洞有优良的流场品质,尤其是湍流度可低达0.01%～0.02%,并具有大范围的变湍流度能力。     

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。     

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。     

液体推进剂对ATR发动机性能影响的研究

为了研究液体推进剂对ATR发动机的燃烧室进口油气比、排气温度、比冲等重要性能参数的影响,针对两套不同的ATR发动机热力循环参数,选择目前国内常用的液体推进剂作为燃料,对上述参数进行了数值模拟。计算结果与理论分析表明：做功能力强的推进剂有利于减小燃烧室进口的油气比,提高ATR发动机比冲;选择合适的推进剂与ATR发动机设计参数相匹配有利于提高二次燃温,进而从油气比和排气温度两个方面改善二次燃烧性能,提高ATR发动机比冲;即使在设计状态推进剂与设计参数两者之间做到了很好的匹配,但是在非设计状态,由于油气比的变化仍然表现出推进剂与工作参数的失配性。     

对单脉冲雷达的遮盖性干扰效果评估

振幅和差法是单脉冲雷达常见的测角定向体制。在分析振幅和差式单脉冲雷达工作原理及遮盖性干扰原理的基础上,建立了基于振幅和差式单脉冲雷达的遮盖性干扰评估模型,并对建立的干扰模型进行了计算机仿真。仿真结果表明:在造成足够大的角度跟踪误差时,遮盖性干扰对振幅和差式单脉冲雷达具有较好的干扰效果。     

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.     

新型整星隔振平台的被动隔振性能及星箭耦合特性分析

针对卫星的隔振要求,提出一种新型半主动整星隔振平台,采用磁流变(MR)阻尼器作为半主动作动器。为增加平台的横向转动刚度,提出一种套筒式防摇结构。建立新型整星隔振系统的详细有限元(FE)模型,对隔振系统进行基础随机激励下的响应分析和隔振平台的振级落差分析,并建立星箭系统的详细有限元模型,分析星箭结合后对整星隔振性能的影响情况,以及加入新型隔振平台后对火箭动态特性的影响。结果表明:新型整星隔振平台具有优良的被动隔振性能;火箭的动态特性对新型隔振系统的性能有一定影响,但当火箭和隔振平台结合处的刚度较大时,影响较小;加入新型隔振平台后,在火箭点火时到一级分离时,火箭整体的动态特性无明显变化。     

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。