A 2-D comparison of ionospheric convection derived from SuperDARN and DMSP measurements

Ion drift vectors measured by the DMSP satellites are compared with plasma convection vectors obtained by the SuperDARN HF radars through the standard Map Potential algorithm of Ruohoniemi and Baker [Ruohoniemi, M., Baker, K.B. Large-scale imaging of high-latitude convection with super dual auroral radar network HF radar observations. J. Geophys. Res. 103, 20797–20811, 1998]. Despite significant data spread, the agreement can be qualified as reasonable for a data set comprising of 149 satellite passes over the Northern Hemisphere at high latitudes. The slope of the best-fit line relating SuperDARN and DMSP velocity magnitudes is of the order of 0.3 with a tendency for the SuperDARN velocities to be smaller. The agreement between the azimuths of the ion drift and convection is better with the slope of the best-fit line being close to 1. It is shown that consistency between the radar and satellite measurements is much better if the SuperDARN line-of-sight velocities are compared with the DMSP cross-track ion drifts for events showing slow spatial and temporal variations of the convection. If areas of strong convection changes are included into comparison, the degree of agreement deteriorates drastically. This result implies that differences in the spatial and temporal resolutions of DMSP and SuperDARN measurements are crucial factors contributing to the observed discrepancies. In addition, some differences are introduced when the SuperDARN line-of-sight velocities are filtered and reprocessed into vectors with the application of a background convection model.     

用MultiGen建模与Performer类库实现实时窗外视景

介绍了如何利用MultiGenCreator建造适合Performer高效运行的模型,以及在SGI图形工作站上用Performer实现塔台模拟机的视景系统。重点介绍了如何改进模型使其能在程序中方便的组织和控制,并提出了运动目标的模拟。     

Development of TY-3 Microgravity Rocket System

TY-3微重力火箭总长 6 0 0 0 mm,起飞质量 1 1 0 0 kg,有效载荷 5 0 kg,最大飞行高度 2 2 0 km,能提供 1 0 - 4 g约 36 0 s时间的微重力试验条件 ,该火箭已于 2 0 0 0年 1 0月飞行试验成功 ,而且一种更先进的微重力火箭系统正在设计中。     

连接压力在Ti/Ni/Ti复合层TLP扩散连接Si3N4陶瓷中的作用机制

研究了Ｔｉ／Ｎｉ／Ｔｉ复合层ＴＬＰ扩散连接Ｓｉ３Ｎ４陶瓷时压力对接头形成的作用机制。结果表明,ＴＬＰ来不及与陶瓷发生充分反应并形成高强度结合界面就已完全凝固,为形成高强度的结合界面,必须进一步发生固态扩散反应。只有当连接过程中施加足够的压力,才能保证ＴＬＰ在其存在期间充分铺展陶瓷,并在ＴＬＰ完全凝固后形成大量扩散通道,为固态扩散反应提供必要条件。     

Ti-24Al-15Nb-1Mo合金氩弧焊

研究用Ti-Al-Nb基(高Nb)合金作填充材料氩弧焊(充氩箱中)Ti-24Al-15Nb-1Mo合金时的焊缝成形及其接头显微结构和力学性能特点.结果表明,固溶处理状态下母材氩弧焊时具有较低的冷裂纹敏感性.焊态下,接头抗拉强度912～927MPa,延伸率2.5%～3.7%,焊缝冲击韧性4.7J/cm2～10.4J/cm2,近热影响区是接头力学性能的薄弱区域.     

地面效应对火箭橇发动机尾喷管流场特性的影响研究

摘要：基于火箭撬地面试验的需要，设计了大载荷高加速的短轨火箭橇动力系统，并对地面效应对火箭发动机尾喷管流场的影响进行了理论和试验研究。文中采用FLUENT计算软件对不同条件下的火箭发动机尾喷管外流场进行了三维数值仿真，分析了单枚火箭以及双枚火箭工作时，地面效应对发动机尾喷管流场特性的影响。针对本文研究的大载荷高加速的短轨火箭撬动力系统，地面效应的影响和双尾喷管之间的相互作用都是在1.5ms时开始显现，在2ms~3ms时比较明显，在5ms~20ms开始减小，最后形成稳定的尾部流场。对于喷管出口直径275mm、轴线距离地面不小于472mm和双喷管轴线距离不小于680mm的火箭橇动力系统，在火箭橇运动起来20ms之后，地面效应影响和双火箭发动机之间相互作用变得非常小。     

浅析光学测量方法在修理企业零件制造方面的应用

介绍了应用光学测量方法还原无图零件、铸造件、磨损件以及测绘零件三维模型的方法，运用数控加工、增材制造等加工方法，实现了无图样零件的制造和检测。     

Temporal evolution of the EIA along 95°E as obtained from GNSS TEC measurements and SAMI3 model

The total electron content (TEC) derived from GNSS measurements at a trans-hemispheric meridional chain of ground stations around 95°E longitude are used to study the quiet time inter-hemispheric structure and dynamics of the equatorial ionization anomaly (EIA) during the period March 2015 to February 2016. The stations are Dibrugarh (27.5°N, 95°E, 43° dip), Kohima (25.6°N, 94.1°E, 39° dip), Aizawl (23.7°N, 92.8°E, 36° dip), Port Blair (11.63°N, 92.71°E, 9° dip) and Cocos Islands (12.2°S, 96.8°E, 43° dip). The observation shows that the northern crest of the EIA lies in the south of 23°N (Aizawl) in all seasons but recedes further south towards the equator during December solstice. The largest poleward expansion of the northern (southern) EIA is observed in the March equinox (December solstice). The equinoctial and hemispherical asymmetry of TEC is noted. The winter anomaly is observed in the northern hemisphere but not in the southern hemisphere. The highest midday TEC over any station is observed in the March equinox. The TEC in southern summer (December solstice) is significantly higher than that in the northern summer (June solstice). The observed northern EIA contracts equatorward in the postsunset period of solstice but the southern EIA persists late into the midnight in the December solstice. The asymmetry may be attributed to the different geographic location of the magnetically conjugate stations. The SAMI3 simulations broadly capture the EIA structure and the inter-hemispheric asymmetry during solstices. The difference between observations and the SAMI3 is higher in March equinox and December solstice. The higher E?×?B vertical drift in the 90–100°E sector and the large geographic-geomagnetic offset in observing stations may have contributed to the observed differences.     

基于三维激光成像系统的相机标定方法

三维激光成像系统中点云数据与影像数据的融合可以对被扫描物体赋予真彩色.为了获得点云数据与影像数据良好的融合效果,就需要精确的确定载体坐标系与相机坐标系之间的关系.本文针对三维激光成像系统点云模型真彩色处理方法进行研究,提出了一种基于三维激光成像系统的相机标定方法.通过对相机坐标系的标定,建立点云数据与影像数据之间的数学模型.实验结果显示,采用所提出的方法,能够使得三维立体点云数据与影像数据精确融合.最终得到被扫描目标的真彩色3D模型.