Gd2SiO5纳米粉体的并流化学共沉淀法合成

以Gd₂O₃和正硅酸乙酯(TEOS)为原材料,采用并流化学共沉淀法合成Gd₂SiO₅粉体材料。研究Gd₂SiO₅前驱体的热响应特征、Gd₂SiO₅粉体的物相组成和微观形貌,并对Gd₂SiO₅粉体的合成机理进行初步探讨。结果表明:前驱体的低Gd/Si摩尔比和反应体系的高pH值会导致Gd₂SiO₅粉体生成Gd_9.33(SiO₄)₆O₂杂质相,相反则会导致生成Gd2O3杂质相。当Gd/Si摩尔比为20∶11、pH值为9~10、合成温度为1000~1300℃时,合成的粉体纯度较高,Gd₂SiO₅颗粒呈不规则形貌特征,平均粒度为100~200 nm。Gd₂SiO₅合成过程中,前驱体以一种—[Si—O—Gd]—网络结构存在,在煅烧过程中逐渐转化为Gd₂SiO₅晶体以及Gd_9.33(SiO₄)₆O₂和Gd₂O₃杂相。     

整级环境下涡轮叶片型面加工几何偏差影响的不确定性分析

加工等过程中产生的几何偏差会导致涡轮叶片气动性能及工作状态发生显著变化,对该影响的准确评估与合理分析具有重要意义.本文提出了一种考虑三维型面几何偏差对气动性能影响的不确定性计算分析方法,包括随机叶型几何建模、不确定性量化计算和敏感性分析等,并结合某一单级高压涡轮进行分析.基于随机过程理论和主成分分析法,参考现有叶片加工...     

单幅图像的三维重构视觉系统特征点提取算法的研究与实现

实现基于单幅二维图像不标定欧氏重构三维场景的关键技术之一是有效提取彩色伪随机编码图像特征角点。为给图像特征点匹配提供更多的样本信息,采用定位于彩色图像Harris算子探测特征角点,并动态给出角点响应的自适应阈值条件。特征点提取实验及三维欧氏重构结果证实了该方法的适用性和有效性。     

面向多种复杂零件的高精度人机协同装配系统

实现复杂三维结构体及小刚度零件的自动装配是极其困难的,为了解决此类零件难以夹持以及夹持变形的难题,分别设计了针对复杂结构的本体件快换夹持器和针对小刚度零件的气囊柔性夹持器以及针对微小平板类零件真空吸附式夹持器,并融合高精度调整技术以及合理的检测技术,设计了一台面向多种复杂零件的高精度人机协同装配系统。使用Abaqus仿真计算了气囊柔性夹持器对小刚度零件夹持变形的影响,零件特征面的弹性变形仅为1μm。通过装配间隙仅为32μm的轴孔对位装配实验,证明了该装配系统能完成零件间2μm~3μm高精度装配。该装配系统能够解放劳动力,提高生产装配的自动化。     

数字样机在飞机数字化协同研制中的发展

飞机数字样机是飞机产品的数字化表述,是与飞机相关的所有三维数字信息构成的产品模型集合,可用于工程设计、工程分析(空间分析、运动分析、拆装模拟、加工制造和维护检测)、工程仿真等活动。飞机数字样机的出现从根本上革新了传统飞机协同研制方式,开创了飞机数字化协同研制的新阶段,随着数字化技术、计算机网络技术的不断发展,数字样机在飞机数字化协同研制中的作用和地位也不断发展。从飞机数字化协同研制的发展历程出发总结论述了数字样机的发展历程。     

2.5维机织复杂结构件的静强度

采用宏细观结合方法,针对经纱和纬纱等材料组分可能发生的多种失效模式,分别建立了基于改进的Hashin准则的系统性的材料失效准则及不同失效模式下的刚度退化模型.引入逐渐损伤的思想,建立了2.5维机织复杂结构件静强度系统性分析方法.模拟并分析了材料经向拉伸和纬向拉伸的应力-应变曲线,与实验得到的材料应力-应变曲线相比,相同应变下应力误差不超过6.5%,具有较好的重合度;对2.5维机织压气机静子连接结构模拟件开展了逐渐损伤模拟,结果表明:结构损伤主要集中在叶根倒角附近,其中吸力面叶根处的基体压缩失效形式会引起结构大幅变形,是结构破坏的主要原因.      

Portfolios of promise: A review of R&D investment techniques and how they apply to technology development in space agencies

Despite a rich legacy of impressive technological accomplishments, the government acquisition of advanced space systems is increasingly synonymous with schedule slips and cost overruns. Program reviews have suggested that investing more in centralized and strategic research and development outside particular programs will reduce technical uncertainties and improve cost and schedule outcomes. This paper suggests roles for a centralized technology office by examining the methods available in the literature for managing portfolios of research projects.     

Observations of non-migrating tides and ionospheric perturbations of O(D) airglow by ISUAL instrument

In this paper, we present the spatial variations of O(¹D) airglow observed by the ISUAL (Imager of Sprites and Upper Atmospheric Lightning) instrument on board the FORMOSAT-2 satellite. With a CCD camera and a 630 nm filter, ISUAL can measure global atmospheric emissions lying between the heights of 80 and 300 km. In days of 3–6 September 2008 and 25–27 February 2009, ISUAL has measured the emissions of O(¹D) airglow with results showing strong longitudinal peak-3 and peak-4 structures. The Lomb-Scargle analyses for these two cases show periods of longitudes of 120° and 90° supporting the DE2 and DE3 non-migrating tides. The 630 nm emissions are enhanced in equatorial regions and are lying along the equator. Over Africa its intensity can sometimes increase up to 80% relative to other longitudes. The perturbation is so strong that non-migrating tides are erased. A case of bimodal distribution with strong emissions at latitudes in equator and mid-latitude in geographic coordinates was observed.     

Alternative transfer to the Earth–Moon Lagrangian points L4 and L5 using lunar gravity assist

Lagrangian points L4 and L5 lie at 60° ahead of and behind the Moon in its orbit with respect to the Earth. Each one of them is a third point of an equilateral triangle with the base of the line defined by those two bodies. These Lagrangian points are stable for the Earth–Moon mass ratio. As so, these Lagrangian points represent remarkable positions to host astronomical observatories or space stations. However, this same distance characteristic may be a challenge for periodic servicing mission. This paper studies elliptic trajectories from an Earth circular parking orbit to reach the Moon’s sphere of influence and apply a swing-by maneuver in order to re-direct the path of a spacecraft to a vicinity of the Lagrangian points L4 and L5. Once the geocentric transfer orbit and the initial impulsive thrust have been determined, the goal is to establish the angle at which the geocentric trajectory crosses the lunar sphere of influence in such a way that when the spacecraft leaves the Moon’s gravitational field, its trajectory and velocity with respect to the Earth change in order to the spacecraft arrives at L4 and L5. In this work, the planar Circular Restricted Three Body Problem approximation is used and in order to avoid solving a two boundary problem, the patched-conic approximation is considered.