钣金制件表面的相贯线求作方法

本文提出钣金制件表面相贯线求作的新方法。     

Astrophysics in 2006

The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006. We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the Universe) and others of which there are always many, like meteors and molecules, black holes and binaries.     

The double-pulsar binary J0737–3039

A recent multibeam pulsar survey of the outer Galactic plane at Parkes has discovered the first-known double-pulsar binary, a very compact double neutron star system in which both stars are observable as radio pulsars. In this review, we briefly describe the discovery and the studies which have been enabled by the unique properties of the system. These range from the most precise confirmation yet of the theory of general relativity, with the possibility of even more new tests and the measurement of second-order post-Newtonian effects, to studies of the magnetospheres and emission properties of the two pulsars. The discovery also results in a significant increase in the expected rate of occurrence of the mergers of double neutron star systems, and hence the rate of detection of such events by the new ground-based gravitational wave detectors.     

The Local Bubble and Interstellar Material Near the Sun

The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun appears to be located in one of these flows of low density material. This nearby interstellar matter, dubbed the Local Fluff, has a bulk velocity of ∼19 km s⁻¹ in the local standard of rest. The flow is coming from the direction of the gas and dust ring formed where the Loop I supernova remnant merges into the LB. Optical polarization data suggest that the local interstellar magnetic field lines are draped over the heliosphere. A longstanding discrepancy between the high thermal pressure of plasma filling the LB and low thermal pressures in the embedded Local Fluff cloudlets is partially mitigated when the ram pressure component parallel to the cloudlet flow direction is included.     

WSO-UV project

During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan.     

基于超螺旋二阶滑模的双馈风力发电机控制策略

传统双馈风力发电机(DFIG)控制存在抖振现象,容易造成系统的不稳定。为了减轻控制抖振现象,提高控制的稳定性,在分析了DFIG动态特性的基础上,建立了DFIG的数学模型,设计了超螺旋二阶滑模控制器,并研究了突变风的情况下滑模控制器的控制性能。通过MATLAB/Simulink工具进行了仿真验证。仿真结果证明:滑模控制器具有良好的最优转矩跟踪能力和无功调节能力,与一般的控制方法相比鲁棒性较强,转子控制电压连续,控制产生的抖振可以大幅减轻,系统的稳定性大大提升。     

通用加速计算在环幕失真校正中的应用研究

大规模场景的沉浸式投影系统大都以环幕作为显示设备,而由环幕造成的几何失真使系统真实感大大降低。从环幕产生失真的几何原理出发,通过建立投影平面和成像面之间的坐标映射关系,生成了一种几何失真校正的理论模型。同时,研究了一种适于通用加速计算的图形硬件架构CUDA,基于其多线程的硬件执行机制,通过将几何失真的校正矩阵组织成纹理进行多重纹理贴图映射,设计了预失真校正的硬件加速算法,该算法还利用基于权值的超采样技术对加速中的走样进行了设计。最后,对该方法的校正效率和效果进行了实验验证,证明该方法具有更高的场景交互速度和很好的校正效果。     

变循环发动机总体结构和模式转换机构研究

根据1种涡扇发动机的总体结构设计方案,围绕变循环特征的适应性进行了改进设计,给出了变循环发动机的总体结构初步方案,设计了模式转换原理及其结构实现方案;以其可调面积涵道引射器的设计为例,进行了模式转换机构运动仿真及其关键件的有限元分析,从机构运动和强度分析方面确定了该方案的可行性.     

某型三叶螺旋桨的设计及性能试验

根据飞行速度、需用拉力、螺旋桨转速等参数,设计了某型飞机的三叶螺旋桨,获得了弦长和桨叶角沿着径向的分布.制造了三叶复合材料螺旋桨（直径为1.75m）,在螺旋桨试验台上测试了不同转速下螺旋桨的拉力.为了获得螺旋桨的动态性能,制造了螺旋桨的缩比模型（直径为0.96m）,在西北工业大学NF-3风洞的三元试验段测试了螺旋桨的气动性能数据,包括:拉力、扭矩、功率、效率.结果表明:螺旋桨最大效率为85.63%,所设计的三叶复合材料螺旋桨适用于螺旋桨需用功率为70kW左右的发动机（比如Rotax912）,提出的螺旋桨设计方法具有较好的应用价值.