矩形蜗壳内三维紊流场的热线测量

在3个不同流量工况, 对矩形蜗壳内三维紊流流场进行了测量。结果表明, 在矩形蜗壳进口突变截面两侧壁的角区存在有回流区。在回流区中紊动能和雷诺应力明显大于中间截面主流区中的值。随着试验流量的增加, 回流区减小, 紊动能和雷诺应力很快下降。在同一流量工况, 随着半径增加, 紊动能和雷诺应力减小。在蜗壳圆周方面的不同横截面上存在有大旋涡, 气体在蜗壳中按螺旋管线运动。      

TVD格式数值模拟斜腔内旋涡运动

 采用ＴＶＤ有限体积格式,通过求解非定常可压缩Ｎ－Ｓ方程,对恒定出入口压力比驱动下的斜腔内部流动进行了数值模拟。计算后得到清晰的流场涡系结构及其发展过程；显示了空腔流动中的自维持振荡现象；并分析了剪切层不稳定对周期性振荡的作用机制。     

The autocorrelation of m-sequences over nonprime finitefields

Nonbinary m-sequences (maximal length sequences) for spread-spectrum communication systems that have a two-level autocorrelation are presented. The autocorrelation function of an m -sequence over the Galois field of q elements GF(q), where q=p^k, for p a prime and k an integer greater than 1, is developed and shown to be bilevel when the elements of GF(q) are expressed as elements of a vector space over the pth roots of unity     

旋流燃烧效率的试验研究

一、设备及试件 本文采用两种不同结构的旋流加力室模型,其燃烧机理不同。模型Ⅰ(图1a)利用强旋流产生中心回流区来稳定火焰,组织燃烧;模型Ⅱ(图1b)根据离心力效应组织燃烧,值班稳定器产生稳定的外环火焰,热气流与中心旋转气流之间存在密度差,在离心力作用下火焰向中心传播,旋转的混气由中心向外运动,两者在相对运动中点燃新鲜混气。这种由相对运动产生的火焰传播速度是常规紊流火焰速度的4～5倍。试验在常     

高负荷跨音涡轮导向器环形叶栅试验研究

对一个高负荷跨音速涡轮导向器进行了环形叶栅吹风试验 ,对其根、中截面进行了平面叶栅吹风试验。本文对试验的损失特性、出气角特性、速度特性、叶型表面速度分布特性等作了对比分析。认为导向器环形叶栅试验结果与平面叶栅试验结果有可比性 ,其叶中截面相当一致 ,根、尖截面则由于导向器流动的复杂性而与平面叶栅试验结果有较大差异     

舰载直升机系留载荷及全机应力计算方法研究

 舰载直升机的系留问题是舰、机双系统联系的关键。与地面系留的不同在于舰载系留是基于运动着的基础。特别在高海情下,机体承受各个方向的过载,且载荷较大。这样,机体结构及系留索具是否有足够的承载能力,就显得异常重要。 运动着的基础、系留索具单向承载性以及起落架承载与变形的非线性关系构成了舰载系留的特点。本文针对这些特殊问题,进行了合理而有效的处理。分别采用了“矩阵力法”及“矩阵位移法”进行系留索具的载荷和机体结构应力的计算,并与实验进行了对比分析,得到了满意的结果。     

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.     

A design procedure for the phase-controlled parallel-loadedresonant inverter

High-frequency-link power conversion and distribution based on a resonant inverter has been recently proposed. The design of several topologies is reviewed and a simple approximate design procedure is developed for the phase-controlled parallel-loaded resonant inverter. This design procedure seeks to ensure the expected benefits of resonant conversion and is verified by data from a laboratory 2.5 kVA, 20-kHz converter. A simple phasor analysis is introduced as a useful approximation for design purposes. Experimental results show that under transient conditions such as load short-circuit, a reversal of the expected commutation sequence is possible. This should be accounted for in the design of the power circuit, or prevented by the design of the controller     

Frequency estimation techniques for high dynamic trajectories

A comparison is presented of four different estimation techniques applied to the problem of continuously estimating the rapidly varying parameters of a sinusoidal signal, observed in the presence of additive noise. Frequency estimates are emphasized, although phase and/or frequency rate are also estimated by some of the algorithms. These parameters are related to the velocity, position, and acceleration of the maneuvering receiver or transmitter. Estimated performance at low carrier-to-noise ratios and high dynamics is investigated for the purpose of determining the useful operating range of an approximate maximum likelihood estimator, an extended Kalman filter, a cross-product automatic frequency loop and a phase-locked loop. Numerical simulations are used to evaluate performance while tracking a common trajectory exhibiting high dynamics     

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。