虚拟现实技术在CAD中的应用

随着计算机技术的不断发展,信息技术不断融合到传统制造业中,虚拟设计/虚拟制造概念的出现受到学术界和企业界的广泛重视,成为研究的热点.阐述了将三维鼠标、立体眼镜原理及数据手套与CAD/CAM技术相结合在具有开放源代码的CAD系统上,将CAD数据模型转换为虚拟场景,保存为VRML格式,实现场景编辑的可视化,可从任意角度观察产品的设计效果.     

铝基复合材料的脉冲氩弧焊研究

研究了Al_2O_3P/6061Al铝基复合材料在脉冲氩弧焊条件下的可焊性。焊缝金属及热影响区的显微组织观察与分析表明,接头组织致密,无气孔、夹杂和裂纹等缺陷,接头的抗拉强度可达母材强度的80％左右。焊接接头的X射线衍射相结构分析和断口扫描电镜分析的结果表明,接头中含有Al,Al_2O_3,MgAl_2O_4等相,接头拉伸试样断口呈韧性断裂机制。文中还针对这种复合材料在氩弧焊接中存在的问题、以及如何提高接头质量应采取的措施进行了理论探讨。     

镗削声发射信号与镗刀磨损量关系的研究

 对镗削过程中声发射信号与刀具磨损之间的关系进行了实验研究和理论分析,得到了声发射信号的特征量与刀具磨损量之间的关系。本文提出用声发射信号随时间变化的记录长度内最大峰值电压V_(pmax)对时间f的累积均值(?)及累积均方差σ_t为在过程(In-Process)实时辨识镗刀磨损的特征量,以便实现刀具磨损的预报控制。     

通用模糊控制器研究

讨论了通用模拟控制器的设计,用单片机构成硬件电路,用软件实现模糊控制算法,来实现对被控对象的模糊控制。这种模糊控制的特点是资源开销小,灵活性高,通用性强,可广泛应用于家用电器的自动控制系统中。     

Tailored analyses of 24 Galactic WN stars

The fundamental properties of 24 Galactic WN stars are determined from analyses of their optical, UV and IR spectra using sophisticated model atmosphere codes (Hillier, 1987, 1990). Terminal velocities, stellar luminosities, temperatures, mass loss rates and abundances of hydrogen, helium, carbon, nitrogen and oxygen are determined. Stellar parameters are derived using diagnostic lines and interstellar reddenings found from fitting theoretical continua to observed energy distributions.Our results confirm that the parameters of WN stars span a large range in temperature (T_*=30–90,000 K), luminosity (log L_*/L=4.8–5.9), mass loss (M=0.9–12×10^–5 M yr^–1) and terminal velocity (v =630–3300 km s^–1). Hydrogen abundances are determined, and found to be low in WNEw and WNEs stars (<15% by mass) and considerable in most WNL stars (1–50%). Metal abundances are also determined with the nitrogen content found to lie in the range N/He=1–5×10^–3 (by number) for all subtypes, and C/N 0.02 in broad agreement with the predictions of Maeder (1991). Enhanced O/N and O/C is found for HD 104994 (WN3p) suggesting a peculiar evolutionary history. Our results suggest that single WNL+abs stars may represent an evolutionary stage immediately after the Of phase. Since some WNE stars exist with non-negligible hydrogen contents (e.g. WR136) evolution may proceed directly from WNL+abs to WNE in some cases, circumventing the luminous blue variable (LBV) or red supergiant (RSG) stage.     

飞机翼面结构布局综合设计方法研究

为了探讨飞机翼面结构主要纵横骨架的最佳布局问题,并提供符合工程实际的、用于概念设计阶段的飞机结构设计方法,本文采用分级优化与集成的策略,该策略分为3个层次。第一个层次为拓扑优化,并由此确定纵向骨架的个数与位置的最优布局;第二个层次为尺寸优化,它用来确定翼面的中间参数;第三个层次为稳定性准则优化,它确定横向骨架的个数与位置的最优布局。在分级优化的3个层次中,拓扑优化是独立的,尺寸优化与稳定性准则优化是相互耦合的。以国外某飞机机翼为例,结果表明本文提出分级优化的思路与所采用的集成方法是可行的,并且具有很好的数值效果。作者认为：它对从事飞机结构设计的人员有一定的指导性和参考价值,值得在飞机设计部门推广应用。最后,总结给出5点结论供参考。     

大曲率弯道内湍流数值计算与测量

本文用k-ε两方程模型和激光多普勒测速仪研究了大曲率、小高宽比弯道内的湍流流动。实测发现湍流存在强烈的各向异性,最大时均速度u_(max)在25°截面后随θ角增大向外壁移动。计算发现用k-ε模型得到的时均速度u的结果与实验比较,在45°截面前,二者符合得很好,此后,存在较大误差。     

Binary and millisecond radio pulsars

Recent pulsar surveys, especially those using the multibeam receiver on the Parkes radio telescope, have more than doubled the number of known pulsars, bringing the current total to about 1720. Of these, 171 have millisecond periods, 126 are members of binary systems and 99 are associated with globular clusters. Binary pulsars may be divided into several distinct groups depending on their observed properties such as pulsar period and age, binary period, eccentricity and companion mass. These groups all have different evolutionary histories. Correlations between the various properties are discussed using the increased samples now available. The Parkes Pulsar Timing Array is a project which has the goal of using timing observations of millisecond pulsars to make a direct detection of gravitational waves. The parameters and present status of the project are briefly discussed.     

Hard X-ray emission from the recurrent transient A0535+26 during its 1980 high-intensity outburst

The transient X-ray pulsar A0535+26 was observed on October 4, 1980 during a high level intensity outburst with a balloon borne hard X-ray detector. High statistical quality source spectra were determined up to 100 keV. Both blackbody and Wien laws fit well the data. Pulse phase spectroscopy shows variation of temperature index between 7.5 and 8.5 keV in the off source spectra and between 7.4 and 10.5 keV in the off pulse spectra. The time averaged luminosity above 30 keV is 8×10³⁶ erg/s.     

Solar Elemental Composition Based on Studies of Solar Energetic Particles

Solar abundances can be derived from the composition of the solar wind and solar energetic particles (SEPs) as well as obtained through spectroscopic means. Past comparisons have suggested that all three samples agree well, when rigidity-related fractionation effects on the SEPs were accounted for. It has been known that such effects vary from one event to the next and should be addressed on an event-by-event basis. This paper examines event variability more closely, particularly in terms of energy-dependent SEP abundances. This is now possible using detailed SEP measurements spanning several decades in energy from the Ultra Low Energy Isotope Spectrometer (ULEIS) and the Solar Isotope Spectrometer (SIS) on the ACE spacecraft. We present examples of the variability of the elemental composition with energy and suggest they can be understood in terms of diffusion from the acceleration region near the interplanetary shock. By means of a spectral scaling procedure, we obtain energy-independent abundance ratios for 14 large SEP events and compare them to reported solar wind and coronal abundances as well as to previous surveys of SEP events.