计算沿转子叶高损失分布的半经验模型法

本文对现有的几种计算转子损失的半经验模型进行了系统的对比验算,发现这些损失模型在准确性和适用范围方面均不能满足工程计算的要求。通过对这些模型进行加权平均,并采用了减振凸台损失模型,得到一种新的模型,该模型在除叶尖和叶根外的大部分叶高上,能够比较准确地估算沿转子叶高的损失分布。本文还成功地将此模型用于流线曲率法,得到一种能满意地预测轴流压气机转子损失和流场的计算方法。     

涡喷发动机加速控制系统数学模型及数字仿真

 本文介绍了航空涡轮喷气发动机加速控制系统数学模型建立、数字仿真方法。由于加速过程是一个大偏离动态过程,因而发动机与加速控制器模型均用非线性方程描述,对非线性方程组求解和系统迭代方法本文进行了讨论。算例中分析了在不同飞行条件下发动机的加速规律。     

发动机故障隔离技术的主特征量模型

本文提出了发动机气路分析故障隔离技术的主特征量模型。主特征量模型的基本原理如下:发动机征兆量和发动机特征量之间存在着特殊的函数关系,即 n 个征兆量小偏差方程可以被少于 n 的 t 个故障量偏差所满足。利用这一特性可以对多于征兆量数目的 m 个特征量进行故障隔离。与目前广泛采用的影响系数矩阵法比较,主特征量模型不仅具有更广泛的实用意义,而且数学模型更加严格,并且能提供较多的故障诊断信息。文中给出了主持征量模型的两种求解方法,即最小征兆量偏差残差模法和最小特征量偏差法。文中还给出了主特征量模型的计算例题,并对计算结果进行了分析。     

航空发动机气动热力参数的趋势分析

航空发动机状态的趋势分析,是一种广泛地应用于航空发动机性能监控的分析技术。本文建立了发动机气动热力参数趋势分析的数学模型,着重讨论了有关数据处理中的四个问题:参数的换算;野点的判断和剔除;趋势性的判断和数据的平滑与预测。并将上述模型应用于JT9D发动机的气动热力参数的趋势分析。     

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。