内外函混合加力燃烧室扩压器内液雾湍流两相流场和浓度场数值模拟

 本文用κ-ε湍流模型和液雾轨道模型,对二维内外函混合加力燃烧室扩压器内有蒸发的液雾两相流动和混合进行了数值预报。其中对气相速度场和温度场的计算结果与实验符合令人满意,液雾两相流的计算结果在趋势上也是合理的,表明本文的模拟方法可用于加力燃烧室性能估算及优化设计。     

燃烧诊断用多功能药条燃烧器系统

本文指出了将固体推进剂药条燃烧器用于实验室燃烧诊断的重要性和必要性,介绍并评述了三十余年来药条燃烧器的发展历程,提出了一种具有多种功能的充压视窗药条燃烧器的设计方案和性能指标,对这种燃烧器的初步实验结果进行了分析讨论,并预示了它的应用前景.     

COS-B views on the diffuse galactic gamma-ray emission and some point sources

The correlation between diffuse galactic gamma rays and gas tracers is studied using the final COS-B database and H i and CO surveys covering the entire galactic plane. A good quantitative fit to the gamma rays is obtained, with a small galacto-centric gradient in the gamma-ray emissivity per hydrogen atom. The average ratio of H₂ column density to integrated CO temperature is determined, the best estimate being (2.3 ± 0.3) × 10² molecules cm^–2 (K km s^–1)^–1. Strictly taken, this value is an upper limit. The corresponding mass of molecular hydrogen in the inner galaxy, derived using both 1st and 4th quadrants, is 1.0 × 10⁹ M .The softer gamma-ray spectrum towards the inner galaxy found in previous work can be attributed to a steeper emissivity gradient at low energies and/or to a softer gamma-ray spectrum of the emission distributed like molecular gas. A steeper emissivity gradient at low energies could be related to cosmic-ray spectral variations in the Galaxy, to different distributions of cosmic-ray electrons and nuclei, or to a contribution from discrete sources. A softer spectrum for the emission associated with molecular clouds may be physically related to the clouds themselves (i.e., cosmic-ray spectral variations) or to an associated discrete source distribution.New results on the temporal and spectral characteristics of the high-energy (50 MeV to 5 GeV) gammaray emission from the Vela pulsar are presented. The whole pulsed flux is found to exhibit long-term variability. Five discrete emission regions within the pulsar lightcurve have been identified, with the spectral characteristics and long-term behaviour being different. These characteristics differ significantly from those reported earlier for the Crab pulsar. However, geometrical pulsar models have been proposed (e.g., Morini, 1983; Smith, 1986) which could explain many of these features.     

前台阶流场的传热实验研究

本文尝试用瞬态实验方法, 在卢德威格风洞实验台上, 对小台阶高度 (H=4.0mm)的前台阶二维流场进行传热实验研究, 测定了当雷诺数为 11800至32200时的流场内热流通量和努谢尔特数的变化规律以及努谢尔特数随雷诺数变化的准则关系式。实验结果是令人满意的。      

压气机旋转失速特征参数的一种声学测量方法

轴流压气机旋转失速试验的重要内容之一,是通过各种测试手段来研究失速团数目、失速团旋转角速度等旋转失速特征参数与压气机气动、几何参数之间的关系,以期对于旋转失速发作机理的理解日臻深化。与现有的方法不同,本文探索一条通过声学测量与分析达到上述目的途径。现将初步试验以及相应的分析阐述如下。      

失重环境下圆柱形容器内稳态旋转液体的液面形状

1.引言 在航天高技术中,由于星体充液量的增大以及飞行器姿态指向精度的严格要求,从而液体晃动问题受到了国内外科技界的广泛重视。飞行器在外层空间正常飞行时,液体处于失重状态,此时,不能忽视表而张力的作用,静止自由液面呈特殊曲面,其形状直接影响着液体的动力学特性由于卫星在入轨后处于稳定的自旋状态,这时液面由液体表面     

超声速机翼－尾翼组合体的非定常气动力边界元法

本文以Ｇｒｅｅｎ函数为基础的边界元，应用时间历程法，计算机翼－尾翼组合体的非定常气动性能。这为飞行器的设计及其非定常气动特性分析提供了一种有效和完善的计算方法。本文介绍的方法，特别适用于研究、分析各类飞行器非定常动态响应过程的数值计算，例如飞机对突风动态响应等。本文提供的三维机翼的超声速启动过程非定常气动力数值结果，与Ｌｏｍａｘ理论解作了比较，可以看到吻合得很好，说明本文所使用的方法是可行的。对于机翼－尾翼组合体的数值结果，则进一步提供了尾翼受到机翼的洗流影响过程。     

圆管内不可压粘流的分布式并行算法

用并行算法求解了圆柱通道内不可压层流流动。采用有重叠的条形区域分裂法时计算域进行分区，分别求解动量方程和压力校正方程，对压力校正方程采用块修正法来加速线代数方程的收敛速度。计算结果表明有较好的并行加速比和并行效率。