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。     

电离层顶部电子含量对GNSS电离层层析的影响分析

卫星信号射线上的总电子含量(slant total electron content, STEC)是像素基全球卫星导航系统电离层层析(computerized ionospheric tomography, CIT)建模的必要数据来源，但电离层层析通常忽略1 000 km以上的顶部电子含量，为弄清这部分电子含量对层析结果的影响，利用NeQuick2模型计算站星视线上的STEC与其在电离层区域内的STEC比值来改正原始数据，并分别利用改正前后的STEC进行电离层层析。结果显示，电离层顶部电子含量占比约为10%，白天占比略大于黑夜，与测高仪站的数据相比，改正后的均方根值比改正前提高了20%以上；与Swarm卫星提供的电子剖面数据对比，改正后的层析结果精度较改正前提升了19.6%左右，且该方法受地磁扰动影响较为明显。总的来说，利用CIT进行小尺度电离层探测，可较直观地看出，顶部电子含量对层析结果的影响较大，需要采取相应手段予以剔除。     

Numerical Simulation of a Swept Wing Hot-air Anti-icing System

对后掠翼热气防冰系统的表面温度进行了数值仿真研究.用欧拉方法计算局部水收集系数,外部对流换热系数用附面层积分法计算,蒙皮导热和内部换热用计算流体力学(CFD)方法计算,用基于FLUENT的用户自定义函数(UDF)方法将外部换热、蒙皮导热和内部换热三者耦合求解,实现了热流边界条件的自动加载和温度的自动更新.通过对ARJ21-700机翼防冰系统性能的计算,说明所研究的计算方法能对三维后掠翼热气防冰系统作出总体性能的评估和局部性能的评价,为自然结冰条件下飞机的飞行试验提供依据,从而大大降低飞行试验风险.     

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。     

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).     

高亚声速近壁流场模拟装置研究

采用计算流体力学方法对用于激光辐照热效应实验研究的高亚声速流场模拟装置的近壁流场进行了数值计算,分别针对靶材固壁为平面和弧面的情况比较了实验区无侧板和有侧板时的流场品质,结果表明侧板与靶材固壁构成的半开放槽道能够形成更大范围的均匀流实验区。根据数值计算优化的实验区结构参数研制了流场模拟装置,流场校测结果与数值计算符合良好,流场品质能够满足激光辐照热效应实验研究的要求。     

英语学习策略与大学英语四级通过情况的相关性研究——以桂林航天工业高等专科学校为例

论文通过对桂林航天工业高等专科学校部分学生的英语学习策略调查问卷及相关数据进行SPSS数据分析,分析通过大学英语四级的学生英语学习策略使用情况,及通过分析调查对象的英语学习策略使用情况,是否知道学习策略对于学习策略的选择的影响,各学习策略之间的关系等提出,指导学生,提高大学英语四级通过率。