基于机器人的自动激光焊接系统的开发

激光焊接作为一种高质量、高效率的焊接方法近年来得到了广泛的应用.机器人作为自动化技术与先进制造技术的典型代表和主要技术手段,在自动化焊接中发挥着重要的作用.本文介绍了在原有设备基础上,针对原有激光焊接设备存在的参数更改困难、时序控制精度低以及浪费人力、工作效率低等问题,利用激光器与机器人现有接口,进行了系统集成的软硬件设计,从而开发出一套基于机器人的自动激光焊接系统.实践表明,该系统操作方便,极大地提高了工作效率;完全可以控制机器人与激光器联动以及焊接过程中功率的调整,为激光焊接工艺的改进提供了有利的条件.     

The Cassini Visual And Infrared Mapping Spectrometer (Vims) Investigation

The Cassini visual and infrared mapping spectrometer (VIMS) investigation is a multidisciplinary study of the Saturnian system. Visual and near-infrared imaging spectroscopy and high-speed spectrophotometry are the observational techniques. The scope of the investigation includes the rings, the surfaces of the icy satellites and Titan, and the atmospheres of Saturn and Titan. In this paper, we will elucidate the major scientific and measurement goals of the investigation, the major characteristics of the Cassini VIMS instrument, the instrument calibration, and operation, and the results of the recent Cassini flybys of Venus and the Earth–Moon system.This revised version was published online in July 2005 with a corrected cover date.     

子午扩张流道中叶片积叠线形式对损失的影响

采用全三维粘性流N－S方程程序，对具有大扩张角中间机匣的某型涡轮 低压导向器叶栅中的流场进行了数值模拟。在子午面型线不变的条件下，导向器叶栅采用了10种不同变曲和倾斜形式的叶片。计算结果表明：导向器叶栅采用不同积叠线形式的叶片，对导向器叶栅出口截面上通道涡的位置，强度和尺度以及能量损失的影响是显著的，采用适度的正弯或正倾斜叶片可降低导向器叶栅的能量损失。     

纤维单向缠绕制备C/C扩张段成型技术

在"锥形体纤维单向缠绕技术"的基础上进行了碳纤维单向缠绕制备C/C扩张段成型工艺的探索,制备出了Φ180 mm C/C扩张段试验件,并对其进行了性能测试及整体探伤.测试结果为:超声探伤分贝差为15 dB的缺陷面积小于5%;沿母线方向层间剪切强度大于10 MPa,大端环向层间剪切强度偏小;内压爆破压强为0.6 MPa,破裂模式较好.试验结果表明,采用碳纤维单向缠绕技术制备C/C扩张段工艺可行.     

利用多普勒原理测量微机电系统中微结构的动态特性

介绍了将显微扫描激光多普勒测振仪与基础激振法相结合的微结构动态特性的非接触无损测量方法、扫描激光多普勒测振仪的工作原理、设计的基础激振器及其驱动信号.并给出典型微结构--微悬臂梁的测量结果.测量结果与理论计算及有限元仿真结果相符,验证了该方法的有效性.     

昆虫翅悬停飞行中的三维空间旋涡结构

昆虫(果蝇)悬停飞行中,翅膀按照特定的拍动方式往复运动,产生非定常高升力维持身体的平衡.研究昆虫高升力机理,需要探索拍动翼运动引发的三维空间非定常流场的特性,尤其是三维空间非定常涡的发展变化过程.本文将氢气泡流动显示技术应用于动态模型实验,定性的观察拍动翼前缘涡(LEV)的发展破裂过程.并利用数字体视粒子图像测速,DSPIV(Digital Steroscopic Particle Image Velocimetry)技术,测得了拍动翼运动瞬时相位和相位平均的三维空间流场信息(速度向量场、截面涡量场、空间涡量场,以及三维空间流线),揭示了拍动翼展向流动的存在,并结合定性和定量方法多角度说明了前缘涡沿展向发展到破裂的流动结构,并说明了侧缘涡与前缘涡的相互影响.测量结果表明:在雷诺数960的情况下,拍动翼运动至相位时,翼面上前缘涡在距翼根约60%展长的位置发生破裂;翼根至破裂点之间,展向流动稳定,指向翼梢;破裂点以后,展向流改变方向,指向翼根.     

Numerical analysis and optimization of boundary layer suction on airfoils

Numerical approach of hybrid laminar flow control(HLFC) is investigated for the suction hole with a width between 0.5 mm and 7 mm. The accuracy of Menter and Langtry’s transition model applied for simulating the flow with boundary layer suction is validated. The experiment data are compared with the computational results. The solutions show that this transition model can predict the transition position with suction control accurately. A well designed laminar airfoil is selected in the present research. For suction control with a single hole, the physical mechanism of suction control, including the impact of suction coefficient and the width and position of the suction hole on control results, is analyzed. The single hole simulation results indicate that it is favorable for transition delay and drag reduction to increase the suction coefficient and set the hole position closer to the trailing edge properly. The modified radial basis function(RBF) neural network and the modified differential evolution algorithm are used to optimize the design for suction control with three holes. The design variables are suction coefficient, hole width, hole position and hole spacing. The optimization target is to obtain the minimum drag coefficient. After optimization,the transition delay can be up to 17% and the aerodynamic drag coefficient can decrease by 12.1%.     

一种临近空间升浮一体飞行器气动布局设计研究

应用理论方法和数值模拟方法开展升浮一体太阳能无人机气动布局设计研究,通过优化选形设计获得高升阻比气动布局,对比两种方法的计算结果以及分析存在差别的原因;应用张线天平支撑风洞试验测试技术,对设计布局开展实验验证研究,建立大展弦比的双机身气动布局风洞试验测试方法,分析了不同雷诺数下实验模型的纵向和横向气动特性影响。研究结果表明:风洞试验结果与设计结果吻合良好,验证了设计结果的可靠性,获得了对总体设计具有指导意义的结论和试验数据结果。     

民机飞行结冰参数的模拟与校准

结冰问题的研究对于民用飞机设计十分重要,采用结冰风洞试验是主要的方法之一,欧美国家有很多成熟的结冰风洞用于型号研究。结冰风洞中需要对很多参数进行控制,其中水雾参数精确控制的难度很大,而且一般通过间接方法来进行测试校准,往往误差较大,导致不同结冰风洞试验结果往往有所差异。文章介绍了在意大利宇航中心的IWT 结冰风洞完成的冰风洞校准试验,对结冰风洞水雾参数校准方法进行了阐述,为民机结冰风洞研究提供参考。     

Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals

Both heliophysics and planetary physics seek to understand the complex nature of the solar wind’s interaction with solar system obstacles like Earth’s magnetosphere, the ionospheres of Venus and Mars, and comets. Studies with this objective are frequently conducted with the help of single or multipoint in situ electromagnetic field and particle observations, guided by the predictions of both local and global numerical simulations, and placed in context by observations from far and extreme ultraviolet (FUV, EUV), hard X-ray, and energetic neutral atom imagers (ENA). Each proposed interaction mechanism (e.g., steady or transient magnetic reconnection, local or global magnetic reconnection, ion pick-up, or the Kelvin-Helmholtz instability) generates diagnostic plasma density structures. The significance of each mechanism to the overall interaction (as measured in terms of atmospheric/ionospheric loss at comets, Venus, and Mars or global magnetospheric/ionospheric convection at Earth) remains to be determined but can be evaluated on the basis of how often the density signatures that it generates are observed as a function of solar wind conditions. This paper reviews efforts to image the diagnostic plasma density structures in the soft (low energy, 0.1–2.0 keV) X-rays produced when high charge state solar wind ions exchange electrons with the exospheric neutrals surrounding solar system obstacles.The introduction notes that theory, local, and global simulations predict the characteristics of plasma boundaries such the bow shock and magnetopause (including location, density gradient, and motion) and regions such as the magnetosheath (including density and width) as a function of location, solar wind conditions, and the particular mechanism operating. In situ measurements confirm the existence of time- and spatial-dependent plasma density structures like the bow shock, magnetosheath, and magnetopause/ionopause at Venus, Mars, comets, and the Earth. However, in situ measurements rarely suffice to determine the global extent of these density structures or their global variation as a function of solar wind conditions, except in the form of empirical studies based on observations from many different times and solar wind conditions. Remote sensing observations provide global information about auroral ovals (FUV and hard X-ray), the terrestrial plasmasphere (EUV), and the terrestrial ring current (ENA). ENA instruments with low energy thresholds (\(\sim1~\mbox{keV}\)) have recently been used to obtain important information concerning the magnetosheaths of Venus, Mars, and the Earth. Recent technological developments make these magnetosheaths valuable potential targets for high-cadence wide-field-of-view soft X-ray imagers.Section 2 describes proposed dayside interaction mechanisms, including reconnection, the Kelvin-Helmholtz instability, and other processes in greater detail with an emphasis on the plasma density structures that they generate. It focuses upon the questions that remain as yet unanswered, such as the significance of each proposed interaction mode, which can be determined from its occurrence pattern as a function of location and solar wind conditions. Section 3 outlines the physics underlying the charge exchange generation of soft X-rays. Section 4 lists the background sources (helium focusing cone, planetary, and cosmic) of soft X-rays from which the charge exchange emissions generated by solar wind exchange must be distinguished. With the help of simulations employing state-of-the-art magnetohydrodynamic models for the solar wind-magnetosphere interaction, models for Earth’s exosphere, and knowledge concerning these background emissions, Sect. 5 demonstrates that boundaries and regions such as the bow shock, magnetosheath, magnetopause, and cusps can readily be identified in images of charge exchange emissions. Section 6 reviews observations by (generally narrow) field of view (FOV) astrophysical telescopes that confirm the presence of these emissions at the intensities predicted by the simulations. Section 7 describes the design of a notional wide FOV “lobster-eye” telescope capable of imaging the global interactions and shows how it might be used to extract information concerning the global interaction of the solar wind with solar system obstacles. The conclusion outlines prospects for missions employing such wide FOV imagers.