基于机器视觉的高精度螺孔定位方法研究

针对手工安装工件、劳动强度大以及效率低等问题,提出了一种基于机器视觉的螺孔定位检测方法.利用CCD摄像机实时采集局部待定位物图像,并对图像进行处理,提取螺孔坐标,然后通过物理坐标关系得到拍摄范围外的螺孔的坐标,最后经过eye-hand手眼标定转换到机器人坐标系下的坐标.该方法解决了受外界条件限制,对目标测量的过程不能一步完成的问题-实现了较大物件的自动、快速、准确定位功能.     

Outflow Velocities at the Base of a Polar Coronal Hole During the 1998 Total Eclipse

Polar coronal holes represent the most convincing site from which the high-speed solar wind originates. Here we report high-accuracy Doppler shifts measured in the O VI (1037.6 Å) line obtained by SUMER on SOHO inside an interplume region within the south polar coronal hole. We infer limits on the outflow velocity and draw hints about the flow geometry.     

An Update on Ultra-Heavy Elements in Solar Energetic Particles above 10 MeV/Nucleon

Measurements below several MeV/nucleon from Wind/LEMT and ACE/ULEIS show that elements heavier than Zn (Z=30) can be enhanced by factors of ∼100 to 1000, depending on species, in ³He-rich solar energetic particle (SEP) events. Using the Solar Isotope Spectrometer (SIS) on ACE we find that even large SEP (LSEP) shock-accelerated events at energies from ∼10 to >100 MeV/nucleon are often very iron rich and might contain admixtures of flare seed material. Studies of ultra-heavy (UH) SEPs (with Z>30) above 10 MeV/nucleon can be used to test models of acceleration and abundance enhancements in both LSEP and ³He-rich events. We find that the long-term average composition for elements from Z=30 to 40 is similar to standard solar system values, but there is considerable event-to-event variability. Although most of the UH fluence arrives during LSEP events, UH abundances are relatively more enhanced in ³He-rich events, with the (34<Z<40)/O ratio on average more than 50 times higher in ³He-rich events than in LSEP events. At energies >10 MeV/nucleon, the most extreme event in terms of UH composition detected so far took place on 23 July 2004 and had a (34<Z<40)/O enhancement of ∼250–300 times the standard solar value.     

双S形进气道焊接时存在的问题及解决方法

进气道筒体纵向呈双S形曲度,分三块拉伸成形后,采用氩弧焊组合焊接;整个焊接组合件由筒体与角材连接（采用电阻缝焊和氩弧焊）而成。焊接时容易产生气孔、焊接变形和漏气,焊后整体气密检查困难,采用相应措施后,解决了上述问题。     

MHD Waves and Heating in Coronal Holes

Coronal holes have been identified as source regions of the fast solar wind, and MHD wave activity has been detected in coronal holes by remote sensing, and in situ in fast solar wind streams. I review some of the most suggestive wave observations, and discuss the theoretical aspects of MHD wave heating and solar wind acceleration in coronal holes. I review the results of single fluid 2.5D MHD, as well as multi-fluid 2.5D MHD models of waves in coronal holes, the heating, and the acceleration of the solar wind be these waves.     

高压涡轮冷却叶片叶顶结构气动与传热

开展了叶顶结构及间隙变化对高压涡轮冷却叶片气动与传热性能影响的研究,建立了四种不同叶顶结构的涡轮冷却叶片几何与数值分析模型,进行了高精度流热固耦合分析,得到了不同叶顶结构及间隙对涡轮冷却叶片气动与传热性能影响的数值分析结果。结果表明:不带射流孔叶片随着叶顶间隙的增大,总压损失增加;由于近壁面处存在的涡流,凹槽叶顶结构能够减少叶顶燃气泄漏,阻碍叶顶平面高温燃气的流动与热交换;叶顶射流孔冷却效果明显,能够大幅度降低叶顶平面温度。在相同叶顶间隙下,凹槽射流叶片具有最高的气动性能。     

基于加力内锥冷却的红外隐身技术研究

应用数值仿真方法计算多种冷却方式下的加力内锥流场和温度场,利用红外辐射特性计算软件分析加力内锥的红外辐射特性。研究结果表明：采用小孔与缝隙组合冷却的效果比单用小孔冷却或单用缝隙冷却的好,采用孔/缝组合冷却的加力内锥的红外辐射强度降低68.49%。     

压力探针临壁效应的试验与计算

临壁效应会使压力探针的测量结果发生误差。由于探针属非流线形物休，所以其临壁效应的机理与流线形的机翼不同，不能简单套用机翼的结论．对圆柱三孔针的试验结果表明，可以用叠加点涡的方法来描述其临壁效应。点涡强度随离壁距离的减少而增强．     

气体介质中深小孔电火花加工技术研究

 深小孔加工一直是机械制造领域的难题之一。在分析和研究气体介质中电火花加工技术的基础上,就其在深小孔加工中的应用进行了深入的理论与实验研究。分别用管状圆柱电极和削边电极在通用电火花成形加工机床上成功地加工出直径为2 mm、深径比大于20、锥度小于0.5%的深小孔。研究表明,相对于传统的液中电火花加工,气体介质中电火花加工深小孔具有电极损耗率低、加工过程稳定等特点。而且由于无需庞大的工作液系统,该方法适合于大型零部件上深小孔加工。     

Solar physics with the Square Kilometre Array

The Square Kilometre Array (SKA) will be the largest radio telescope ever built, aiming to provide collecting area larger than 1?km². The SKA will have two independent instruments, SKA-LOW comprising of dipoles organized as aperture arrays in Australia and SKA-MID comprising of dishes in South Africa. Currently the phase-1 of SKA, referred to as SKA1, is in its late design stage and construction is expected to start in 2020. Both SKA1-LOW (frequency range of 50–350?MHz) and SKA1-MID Bands 1, 2, and 5 (frequency ranges of 350–1050, 950–1760, and 4600–15,300?MHz, respectively) are important for solar observations. In this paper we present SKA’s unique capabilities in terms of spatial, spectral, and temporal resolution, as well as sensitivity and show that they have the potential to provide major new insights in solar physics topics of capital importance including (i) the structure and evolution of the solar corona, (ii) coronal heating, (iii) solar flare dynamics including particle acceleration and transport, (iv) the dynamics and structure of coronal mass ejections, and (v) the solar aspects of space weather. Observations of the Sun jointly with the new generation of ground-based and space-borne instruments promise unprecedented discoveries.