高校体育课21世纪人才素质的训练场

正确的生存价值观，较强的竞争能力，良好的合作精神，坚实的身体基础，是未来社会对人才素质的基本要求，体育课应作为培养这些素质的训练场。     

点缀你的主页

随着因特网的发展，主页不在只是网络服务商可以做的事情，那么主页内容以及它的可观赏性就成了它吸引读者的中心。本文简述图形及动画制作方法。运用这些图形及动画来修饰主页，以启到画龙点睛的作用。     

复合固体丁羟推进剂药柱表面防湿涂层研制

介绍了一种丁羟推进剂药柱表面防湿保护涂层,它可以涂敷在药柱表面形成一层薄膜,其透湿系数小于3.0×10~(-13)g·cm/(m~2·s·Pa),能有效阻止湿气扩散到推进剂内部,这种保护涂层有效地降低了湿气对推进剂性能的影响,延缓推进剂的老化,而对推进剂点火性能无明显影响。     

“集体参与法”在“毛论课”中的实践特色

毛泽东思想概论课的开设对大学生素质的培育极具深远意义。“集体参与法”，是我们在“毛论课”初期开设中，根据课程内容特点与学生实际，服从素质培养的准则与目标，探索试行的一种新教学方法。此法从课堂组织结构、教学运行方式、课堂活动主体等各方面，都力寻面对传统教学法主要弊端的根本突破，追求一种动态、多向沟通、多向转化的新风格。初期实践表明：此法在转变学生学习姿态，增强学生政治素养，培塑学生主体意识、团队意识与创新能力上功效显著。     

影响高校德育工作的几个消极因素

本文市场经济、社会消极现象、应试教育、高等教育及德育教育自身缺陷等方面对高校德育工作的消极影响加以分析，立足现实，提出问题，与高等教育工作者，德育工作者共同探讨，以求改进完善高校德育工作。作者坚信，真正找到了问题所在，也就找到了解决问题的切入点。     

CCSDS中LDPC码编码器的FPGA设计与实现

CCSDS标准推荐了一组适用于深空通信的LDPC码。为了满足在一个系统中使用多种码率LDPC码的需要,设计了一个能够实现标准中4种码率码编码的通用编码器,该编码器合理安排了生成矩阵存储单元,充分复用了硬件资源,用一种码编码需要的资源消耗实现了4种码的编码,大大节省了资源;用VHDL语言在FPGA上实现了该编码器,通过仿真验证,表明该编码器在占用硬件资源不大的条件下,能够正确完成4种码率码的编码。     

Dy对EB-PVDβ-NiAl涂层高温瞬态氧化行为的影响(英文)

β-NiAl是一种有前景的应用于1150°C以上的抗氧化涂层材料。本文利用电子束物理气相沉积(EB-PVD)方法制备了0~0.5at%Dy含量的β-NiAl涂层,研究了涂层的瞬态氧化行为。1200°C时,在0.05at%Dy掺杂的涂层中只观察到了稳态α-Al2O3相,而在0.5at%Dy掺杂的涂层中,1h氧化过程中,发生了θ-Al2O3到α-Al2O3的相变。1100°C时,在最初的15min所有涂层均发生了θ-α相变。0.05at%Dy掺杂的涂层在45min的时候相变已经完成,这比0.5at%Dy掺杂涂层要早得多。过量Dy的掺杂能够延缓θ-α相变。未掺杂和过量掺杂涂层在20h氧化之后仍存在针状相θ-Al2O3,而0.05at%Dy掺杂的涂层中则为经典的颗粒状α-Al2O3形貌。     

Airfoil Aeroelastic Flutter Analysis Based on Modified Leishman-Beddoes Model at Low Mach Number

Based on modified Leishman-Beddoes (L-B) state space model at low Mach number (lower than 0.3), the airfoil aeroelastic system is presented in this paper. The main modifications for L-B model include a new dynamic stall criterion and revisions of normal force and pitching moment coefficient. The bifurcation diagrams, the limit cycle oscillation (LCO) phase plane plots and the time domain response figures are applied to investigating the stall flutter bifurcation behavior of airfoil aeroelastic systems with symmetry or asymmetry. It is shown that the symmetric periodical oscillation happens after subcritical bifurcation caused by dynamic stall, and the asymmetric periodical oscillation, which is caused by the interaction of dynamic stall and static divergence, only happens in the airfoil aeroelastic system with asymmetry. Validations of the modified L-B model and the airfoil aeroelastic system are presented with the experimental airload data of NACA0012 and OA207 and experimental stall flutter data of NACA0012 respectively. Results demonstrate that the airfoil aeroelastic system presented in this paper is effective and accurate, which can be applied to the investigation of airfoil stall flutter at low Mach number.     

复杂系统体系结构设计方法研究

体系结构研究是认识复杂系统、控制系统复杂度的首要问题。复杂系统通常由多个具有交联关系的功能模块组成,各个模块之间通过相互作用组织起来,使系统具备特定的整体属性。随着系统复杂程度的增加,整个系统的组成结构、联结关系以及各个组成部分的规格说明显得越来越重要。与具体部件功能的实现技术相比,系统总体结构设计和组件规格描述相对重...     

WMAP extragalactic point sources as potential Space VLBI calibrators

The point source list of the Wilkinson Microwave Anisotropy Probe (WMAP) is a uniform, all-sky catalogue of bright sources with flux density measurements at high (up to 94 GHz) radio frequencies. We investigated the five-year WMAP list to compile a new catalogue of bright and compact extragalactic radio sources to be potentially studied with Very Long Baseline Interferometry at millimeter wavelengths (mm-VLBI) and Space VLBI (SVLBI). After comparing the WMAP data with the existing mm-VLBI catalogues, we sorted out the yet unexplored sources. Using the 41, 61 and 94 GHz WMAP flux densities, we calculated the spectral indices. By collecting optical identifications, lower-frequency radio flux densities and VLBI images from the literature, we created a list of objects which have not been investigated with VLBI at 86 GHz before. With total flux density at least 1 Jy and declination above −40°, we found 37 suitable new targets. It is a nearly 25% addition to the known mm-VLBI sources. Such objects are also potentially useful as phase-reference calibrators for the future Japanese SVLBI mission ASTRO-G at its highest observing frequency (43 GHz). The phase-referencing capability of ASTRO-G would allow long integrations and hence better sensitivity for observing faint target sources close to suitable phase calibrators in the sky.