对偶变换及其在冗余度机器人中的应用

给出了用对偶数矩阵来描述冗余度机器人的雅可毕方程的方法，对偶阵及其变换是这一方法的基础，对偶阵方法可使机器人节点参数的描述变得简洁，尤其在可毕矩阵的直接确定过程中这一方法更显得有效，对偶变换这一方法对机器人运动学、动力学、控制系统之建模提供一种简化的有效方法。     

CAPP系统中工艺路线生成研究

本文研究ＣＡＰＰ中回转体类零件在工序组合之后，确定各工序间的前趋和后继关系，建立拓扑排序的ＡＯＶ网，并由此形成工艺路线的方法。     

铬白口铸铁中硅对组织形态的影响

本文采用高硅进行白口铸铁的合金化。实验发现，随着硅含量的增加，碳化物形貌由网状向断网状、直至分散孤立的条块状变化，碳化物的含量逐渐增加，碳化物的尺寸细化，碳化物硬度、基体硬度也逐渐增大。当硅量〉２．５％，铬量〉５％时，组织中出现了Ｍ７Ｃ３。     

资料转移技术在三维有限元中的应用

本文研究了两类用于三维h自适应网络管理的资料转移方法。文中将牺牲解的精度以节省计算时间的一类资料转移的简单方法（简法）与另一类在资料转移中确保解决的精度的严格方法（严法）进行了比较分析，并通过数值计算例题进行了论证，结果表明：对于简单问题，两类方法都能满足精度，完成资料转移。对于复杂应力状态问题，严法可靠，特别是在网络稀疏时，严法明显优越。     

Multi-scale reconnections in a complex CME

A series of three flares of GOES class M, M and C, and a CME were observed on 20 January 2004 occurring in close succession in NOAA 10540. Types II, III, and N radio bursts were associated. We use the combined observations from TRACE, EIT, Hα images from Kwasan Observatory, MDI magnetograms, GOES, and radio observations from Culgoora and Wind/ WAVES to understand the complex development of this event. We reach three main conclusions. First, we link the first two impulsive flares to tether-cutting reconnections and the launch of the CME. This complex observation shows that impulsive quadrupolar flares can be eruptive. Second, we relate the last of the flares, an LDE, to the relaxation phase following forced reconnections between the erupting flux rope and neighbouring magnetic field lines, when reconnection reverses and restores some of the pre-eruption magnetic connectivities. Finally, we show that reconnection with the magnetic structure of a previous CME launched about 8 h earlier injects electrons into open field lines having a local dip and apex (located at about six solar radii height). This is observed as an N-burst at decametre radio wavelengths. The dipped shape of these field lines is due to large-scale magnetic reconnection between expanding magnetic loops and open field lines of a neighbouring streamer. This particular situation explains why this is the first N-burst ever observed at long radio wavelengths.     

TC16钛合金六角自锁螺母加工技术研究

TC16钛合金六角自锁螺母是飞机结构中一种先进的连接件,具有质量轻、强度高、耐腐蚀、抗振动等特点,大量应用于新型飞机中。本文在TC16钛合金自锁螺母加工技术研究中,解决了热处理加工技术,热处理污染去除技术,缩紧工艺技术,性能试验技术,完成了工艺路线设计,收口尺寸的确定等加工技术关键,全面掌握钛合金六角自锁螺母加工技术。     

不同金属基体上W-C:H 溅射薄膜的摩擦学性能

采用非平衡磁控溅射技术在40Cr、9Cr18、GCr15、TC4及LY12等5种金属基体上沉积了钨掺杂含氢类金刚石(W-C:H)薄膜。采用Raman光谱仪、扫描电子显微镜、纳米硬度计及纳米划痕仪分别测试了薄膜的微结构、厚度、硬度及附着力,采用球-盘摩擦试验机及光学轮廓仪分别在干摩擦和PFPE脂润滑条件下评价了5种金属材料基体上薄膜的摩擦磨损性能。薄膜性能测试结果显示,该厚度为1μm的薄膜具有典型的类金刚石结构,硬度与弹性模量分别为11.56和128.34 GPa,附着力为645 m N;摩擦试验结果显示,在干摩擦条件下几种金属基体表面W-C:H薄膜的摩擦因数和磨损率差别比较显著,而在脂润滑条件下基体材料的影响较小;与干摩擦条件相比,脂润滑条件下薄膜的磨损可减少60%~75%;在干摩擦与脂润滑条件下,9Cr18与40Cr基体上的W-C:H薄膜摩擦体系分别具有最小的磨损率1.71×10-7mm3/(N·m)及4.55×10-8mm3/(N·m)。     

Microwave Diagnostics of Dynamic Processes and Oscillations in Groups of Solar Coronal Magnetic Loops

Low-frequency (LF) modulations of the solar microwave radiation (37 GHz) recorded at the Metsähovi Radio Observatory, are analyzed. Since the intensity of solar microwave radiation, produced by the electron gyrosynchrotron mechanism, is dependent on a value of the background magnetic field [Dulk, G. A.: 1985, Ann. Rev. Astron. Astrophys. 23, 169–224], slow variations of the magnetic field associated with disturbances of the electric current in a radiating source, can modulate the intensity of the microwave radiation. The observed multi-track features of the LF spectra are interpreted as a signature of a complex multi-loop structure of the radiating source. Application of the equivalent electric circuit models of interacting loops allows to explain and reproduce the main dynamical features of the observed LF modulation dynamic spectra.     

Production of QPOs in accreting neutron star systems

Kilohertz QPOs have been detected from more than 20 neutron stars in low-mass X-ray binaries. Several different ideas have been proposed for their generation, involving resonances, magnetic interactions, and sharp transitions in the accretion flow. We show that although details are uncertain at this time, it is clear that the stellar magnetic field has a dynamic influence on the accretion flow. We also discuss the inferences about dense matter and strong gravity that can be drawn from all models, and the qualitative advances expected with a future X-ray timing mission.     

Fast spectroscopy of the 4 November 1978 gamma-ray burst

The Franco-Soviet Signe experiments on Venera 11 and Venera 12 allow a spectral analysis of gamma-ray bursts with a time resolution of 250 ms. Evidence is presented for i) short annihilation flashes of up to 20 photons cm⁻²s⁻¹ and ii) rapid variations of the continuum, from a study of the intense 4 November 1978 event.