火烧炉内气相燃烧过程的三维数值模拟

本文对某工业火烧炉内的三维湍流气相燃烧场特性进行了数值模拟,湍流模型采用可实现k-ε双方程模型,湍流燃烧采用有限速率/涡耗散模型,辐射换热采用P1模型,数值方法采用SIMPLE算法,实现了炉内火烧试验的数值再现,特别考察了入口压力、燃料/空气比、多烧嘴不同组合工况等因素对炉内温度场和流场的影响,并对该火烧炉的运行提出了一些合理化建议,为其实际运行提供了有益的参考。     

液体圆柱射流破碎过程的实验

采用高速摄像仪对圆柱射流的表面剥离现象和射流破碎长度进行了实验,在低速射流下,分析了Rayleigh模式下主液滴和卫星液滴形成过程及运动规律.随着射流速度的增大,射流表面开始出现了表面剥离小液滴.并发现存在一个临界雷诺数,当超过临界雷诺数时,射流表面出现表面剥离现象.通过对射流中表面剥离现象的实验和分析,给出了两种射流破碎长度随雷诺数变化规律和破碎长度拟合关系式.      

The infra-red background generated by pregalactic stars and their remnants

We examine whether the IR background reported by Matsumoto (1983) could have been generated by stars or black holes in the pregalactic era, z=10100.     

Primordial black holes and Holeums as progenitors of Galactic diffuse gamma-ray background

Diffuse Galactic gamma-ray flux resulting from the evaporation of primordial black holes has been the subject of intensive research work during the last few decades. Theoretical work addressing this issue started in the 1970s whereas data started pouring in only in the 1990s. We discuss in this paper a model of the potential contribution to the Galactic gamma-ray flux of primordial black holes in binary systems and extend the argument to include stable gravitational bound states called Holeums. The model has a predictive power and can be tested by looking for gamma-ray excess in the vicinity of violent events occurring in the Galaxy such as supernova explosions.     

Comparison of Polar and Equatorial Coronal Holes Observed by UVCS/SOHO: Geometry and Physical Properties

We analyzed UVCS/SOHO data and compared the H I Lyα (121.6 nm) and O VI (103.2 nm, 103.7 nm) emission in the polar and equatorial coronal holes. We found that the emission lines have similar characteristics in these two types of coronal holes. Both types show evidence for superradially diverging boundaries. The latitudinal distribution of the O VI line ratio may indicate that the equatorial coronal hole has O⁺⁵ outflow velocities lower than in the polar coronal holes. This revised version was published online in June 2006 with corrections to the Cover Date.     

UVCS/SOHO Observations of H I Lyman Alpha Line Profiles in Coronal Holes at Heliocentric Heights Above 3.0 R⊙

The Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) has been used to measure spectral line profiles for H I Lyα in the south polar coronal hole at projected heliocentric heights from 3.5 to 6.0 R_⊙ during 1998 January 5–11. Observations from 1.5 to 2.5 R_⊙ were made for comparison. The H I Lyα profile is the only one observable with UVCS above 3.5 R_⊙ in coronal holes. Within this region the outflowing coronal plasma becomes nearly collisionless and the ionization balance is believed to become frozen. In this paper, the 1/e half widths of the coronal velocity distributions are provided for the observed heights. The velocity distributions include all motions contributing to the velocities along the line of sight (LOS). The observations have been corrected for instrumental effects and interplanetary H I Lyα. The half widths were found to increase with projected heliographic height from 1.5 to 2.5 R_⊙ and decrease with height from 3.5 to 5 R_⊙. This revised version was published online in June 2006 with corrections to the Cover Date.     

飞机突防波次规划中若干关键技术研究

现代空袭是以波次为单位实施攻击的,提出波次规划的概念.波次规划研究的主要内容包括不同波次空袭时编队内多机协同航路规划、多机航路碰撞检测及避碰技术、安全评估技术等,同时指出马尔可夫链在解决编队出动强度、编队数量等的应用前景.最后指出了多目标、多战区、多发射区的波次规划技术是未来研究的重点.     

计算机辅助计量孔组位置度

 <正> 一、前言 孔组位置度的计量,在没有专用量具的情况下,以通用量具计量的方法已有过不少讨论。而以计算机辅助计量的探讨,还是个新课题。本文利用计算机辅助数据处理,研究了6孔孔组位置度的计量方法。以孔位坐标、孔间距离及相邻两孔间的弧所对的中心角来建立判别式,作为计算机程序的数学模式,将各孔位坐标的计量数据键入计算机,即可得到结果。本文举例进行了验证。     

层板双孔过盈配合问题

 复合材料结构广泛采用机械连接。由于孔轴配合中存在间隙,影响多孔连接的内力分配和接头强度。螺栓连接的过盈配合和铆钉连接都能消除间隙,但这样就造成孔轴相互挤压,因而引起应力,并可能造成局部损伤。本文探讨层板双孔过盈配合引起的应力,及讨论过盈配合应用的可能性。     

带孔复合材料层板动态拉伸破坏的应变率效应

采用三维Hashin准则作为纤维束损伤判据,根据材料不同损伤模式制定相应的材料性能退化方案,并考虑应变率效应对材料的强度性能进行修正,建立含孔复合材料层合板的渐进损伤分析模型,模拟材料在不同应变率下的损伤破坏过程。通过动态拉伸试验,获得材料在不同应变率下的载荷-位移关系及孔边不同位置的时间-应变关系,讨论了应变率对材料拉伸性能的影响及试件孔边的应力集中情况。有限元分析结果与试验数据相一致,证明了本文所提出分析模型的正确性和有效性。