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。     

Exact multisensor dynamic bias estimation with local tracks

An exact solution is provided for the multiple sensor bias estimation problem based on local tracks. It is shown that the sensor bias estimates can be obtained dynamically using the outputs of the local (biased) state estimators. This is accomplished by manipulating the local state estimates such that they yield pseudomeasurements of the sensor biases with additive noises that are zero-mean, white, and with easily calculated covariances. These results allow evaluation of the Cramer-Rao lower bound (CRLB) on the covariance of the sensor bias estimates, i.e., a quantification of the available information about the sensor biases in any scenario. Monte Carlo simulations show that this method has significant improvement in performance with reduced rms errors of 70% compared with commonly used decoupled Kalman filter. Furthermore, the new method is shown to be statistically efficient, i.e., it meets the CRLB. The extension of the new technique for dynamically varying sensor biases is also presented.     

两级运载火箭回收方案设想

文章通过对K—1运载火箭的回收方案进行分析研究,提出回收质量分别为10t和20t的两级运载火箭的回收方案设想。文章指出,根据现有的回收技术水平,对运载火箭的回收是完全可行的。     

跨声速风洞斜孔壁非线性流动试验

为分析跨声速风洞斜孔壁近壁区域的流动特性，评估气流偏角-压力系数的非线性关联，在0.6 m跨超声速风洞中开展了基于七孔探针的流动特性测量试验。通过气流偏角和压力系数分布分析了斜孔壁流动的差阻特性，以及马赫数、模型升力对斜孔壁流动的影响，最后基于试验结果发展了计算斜孔壁特性参数的微分法，并与经验方法结果进行对比。结果表明，斜孔壁流动呈现出明显的差阻性和非线性，在负压差范围内，近壁流动仍以出流为主；高亚声速时，空风洞模型区孔壁流动特性趋于实壁；安装模型后，随着升力的增大，升力面对应的孔壁区域流动向入流发展，孔壁流动特性趋于开口边界。