整体叶轮侧铣数控加工刀位轨迹生成新方法

为提高整体叶轮的加工质量和效率,提出了分段侧铣的方法,在每一段曲面上,基于斜等距曲面的原理,推导出叶片分段侧铣加工时刀位轨迹的生成和计算;并用计算仿真和刀心轨迹图对刀位进行了验证。结果表明,采用分段侧铣的方法,生成的刀位轨迹刀轴矢量变化均匀,刀轴未发生干涉,且加工效率和加工质量明显得到提高。     

Relative ionizations in the nearest interstellar gas

We compare CLOUDY predictions for the equilibrium ionization in the interstellar cloud surrounding the solar system with pick-up ion data. The incident radiation field includes contributions from hot stars, the emission from the conductive cloud boundary and the diffuse FUV back-ground. To within the observational uncertainties, CLOUDY predictions for the ratios n(He)/n(O), n(N)/n(O), n(Ne)/n(O), and n(He)/n(Ne) are consistent with pick-up ion data, provided that O and N are filtered by 50% in the heliopause region and the outer heliosphere as predicted by others. Thus, the steady-state ionization model and assumed radiation field appear approximately valid. However, the youth and low intervening column density towards the Vela pulsar leave open the possibility that the parent supernova explosion 10,500 years ago, and 200 pc distant, may also have affected LISM ionization, although the mechanism is uncertain. Support for this last possibility is provided by the apparent signature of the Vela explosion in the terrestrial geological record.Abbreviations ISM Interstellar Medium - FUV Far Ultraviolet - EUV Extreme Ultraviolet - SNR SN remnant - SXRB SXR Background - LISM Local Interstellar Matter     

Manifestation of magnetic reconnection in coronal streamer current sheets

We investigate the possibility of observing the effects of magnetic reconnection inside a current sheet forming in a coronal streamer in the extended corona. In particular we study the possibility to observe with the UVCS of SOHO the excitation of the tearing instability in the current sheet.     

数控线切割加工四轴联动轨迹合成研究

 对四轴联动数控线切割加工进行轨迹合成研究。在线切割四轴联动的基础上对轨迹合成的对应标注进行了分类 ,提出了轨迹合成准则 ;给出在各种标注情况下的轨迹合成公式。采用此理论编制的后置处理程序处理上下异型的三维直纹曲面 ,得到四轴联动的 ISO线切割加工程序     

隔振系统限位器的非线性动力学设计

根据经典线性理论设计隔振系统弹性限位器的约束空间往往太小,在小阻尼情况下会诱发非线性共振,使隔振系统变为放大系统。从非线性动力学角度讨论了弹性限位器的设计问题,给出了若干设计原则及参数选择范围     

基于细观结构的三维机织复合材料弹性性能的分析

三维机织复合材料具有复杂的细观结构,通过采用双凸透镜的几何形状来描述被压扁的纤维束横截面,引入细观结构和几何参数,建立了基于织物细观结构预测三维机织复合材料的纤维体积分数和弹性常数的方法。通过参数分析预测了结构和几何参数对三维复合材料弹性性能的影响。开发了一个具有友好界面的三维机织复合材料弹性性能的分析软件,为复合材料结构设计者选定适合的织物增强结构提供了有效的计算工具。理论计算结果与实验值的比较,表明了分析方法的正确性。     

Lamb波传播特性研究

应用三维弹性理论对Lamb波频散曲线进行理论建模.在Lamb波主动监测系统中,应用Gabor小波变换理论分析Lamb波信号的时延及相位角,获得了板中Lamb波的相群速度频散曲线.比较理论曲线与实验数据,证明了三维弹性理论建模方法的有效性.     

弹性模量对铝胶焊搭接接头应力分布的影响

运用利用弹塑性有限元方法,研究了胶粘剂弹性模量对铝合金胶焊搭接接头上工作应力分布的影响.研究结果表明:随着胶粘剂弹性模量的增加,胶焊搭接区焊点中心线上的应力分布趋于均匀,胶层-焊点边缘处的峰值应力降低,但靠近搭接区端部胶层中的各应力峰值增大;距胶层中心线0.15mm的面上与焊点中心相对应点的峰值应力随弹性模量提高而下降.为提高胶焊接头承载能力,建议采用弹性模量适中的胶粘剂.     

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.     

Long-Term Fluences of Solar Energetic Particles from H to Fe

Data from ACE and GOES have been used to measure Solar Energetic Particle (SEP) fluence spectra for H, He, O, and Fe, over the period from October 1997 to December 2005. The measurements were made by four instruments on ACE and the EPS sensor on three GOES satellites and extend in energy from ∼0.1 MeV/nuc to ∼100 MeV/nuc. Fluence spectra for each species were fit by conventional forms and used to investigate how the intensities, composition, and spectral shapes vary from year to year.