湍流附面层壁面摩擦应力的测量方法

 本文讨论了不可压和可压湍流附面层壁面摩擦应力的测量方法,对Presto管、Stanton管、底层隔板、表面热膜和计算Preston管法进行了校准和测量比较。     

改进跨音速位势方法的讨论

 简要地回顾并讨论了传统位势方法之不足。对改进传统位势方法的两种必要的修正(熵修正和涡修正)的量级在小扰动条件下作了分析和估值。结果表明涡修正是更高阶小量,因而作为第一步修正可采用非等熵位势流来近似。采用熵修正激波算子来计及非等熵的激波突跃条件,并考虑了由熵修正带来的尾迹条件的变化。算例表明非等熵位势方法能得到预期的改进位势方法的效果。     

粘弹性结构振动特性分析的摄动求解技术

 本文根据粘弹性结构的特点,对其振动特性进行简化分析,构造了这类结构振动特性分析的摄动求解方法,给出了低阶摄动求解公式。还讨论了零阶摄动有重特征值时的求解。     

单管和蒸发管燃烧室排气污染性能模拟

为了更深入地探讨单管燃烧室和蒸发型双腔燃烧室的排气污染性能,作者在实验研究的基础上,进一步对二者进行了理论分析和模拟。以通用反应器分析和模拟程序GRASP为基础,针对具体燃烧室,考虑雾化、蒸发、混合、气流的分股和回流流动以及化学反应热力学诸方面,对原程序做了相应的改进和增补,以用来模拟实际燃烧过程(甚至局部存在富油)的11种排气成分和出口温度。计算和实验结果相一致。     

三轴相交度的一种测量方法

介绍了三个回转轴相交度的一种测量方法，并进行了测量不确定度分析。     

非刚性基准浮动工件宽度的在线测量

介绍１种用标准长度作基准，以自扫描光电二极管列阵作光电传换器，微型计算机进行数据处理，对基准浮动的非刚性工件宽度进行在线测量的测量装置。     

Medium PRF set selection using evolutionary algorithms

This paper presents a new and novel method of selecting multiple pulse repetition frequency (PRF) sets for use in medium PRF pulsed-Doppler radars. Evolutionary algorithms are used to minimise the blind areas in the range/Doppler space. The evolutionary algorithm allows optimal solutions to be generated quickly, far faster than with exhaustive searches, and is fully automatic, unlike existing techniques. The evolved solutions compare very favorably against the results of both an exhaustive search and existing published PRF set selection methods. This evolutionary approach to generation of PRF sets is a major advance in medium PRF radar design.     

非参量量化秩检测器的性能研究

 许多作者讨论过非参量秩检测器在雷达信号处理中的应用。秩检测器首先把接收波形样本转换为秩。如果检验单元和参考单元的噪声样本独立和分布,则无信号时检验单元的秩具有离散均匀分布,与输入噪声的分布无关。所以秩检测器可能提供分布自由的恒虚警率性能。量化秩检测器（QRD）只对二进量化秩进行积累,所以它实现起来很经济。本文分析QRD的检测性能。证明QRD有一最佳秩量化门限（ORQT）。确定高斯和韦伯噪声中的ORQT。另外,把QRD同高斯噪声中的局部最佳秩检测器和最佳参量检测器进行比较。     

A gentle process for the formation of Algols

This work is concerned with binary systems that we call ‘moderately close’. These are systems in which the primary (by which we mean the initially more massive star) fills its Roche lobe when it is on the giant branch with a deep convective envelope but before helium ignition (late case B). We find that if the mass ratio q(= M ₁/M ₂) < q _crit = 0.7 when the primary fills its Roche lobe positive feedback will lead to a rapid hydrodynamic phase of mass transfer which will probably lead to common envelope evolution and thence to either coalescence or possibly to a close binary in a planetary nebula. Although most Algols have probably filled their Roche lobes before evolving off the main-sequence we find that some could not have and are therefore ‘moderately close’. Since rapid overflow is unlikely to lead to an Algol-like system there must be some way of avoiding it. The most likely possibility is that the primary can lose sufficient mass to reduce q below q _crit before overflow begins. Ordinary mass loss rates are insufficient but evidence that enhanced mass loss does take place is provided by RS CVn systems that have inverted mass ratios but have not yet begun mass transfer. We postulate that the cause of enhanced mass loss lies in the heating of the corona by by magnetic fields maintained by an α — ω dynamo which is enhanced by tidal effects associated with corotation. In order to model the the effects of enhanced mass loss we ignore the details and adopt an empirical approach calibrating a simple formula with the RS CVn system Z Her. Using further empirical relations (deduced from detailed stellar models) that describe the evolution of red giants we have investigated the effect on a large number of systems of various initial mass ratios and periods. These are notable in that some systems can now enter a much gentler Algol-like overflow phase and others are prevented from transferring mass altogether. We have also investigated the effects of enhanced angular momentum loss induced by corotation of the wind in the strong magnetic fields and consider this in relation to observed period changes. We find that a typical ‘moderately close’ Algol-like system evolves through an RS CVn like system and then possibly a symbiotic state before becoming an Algol and then goes on through a red giant-white dwarf state which may become symbiotic before ending up as a double white dwarf system in either a close or wide orbit depending on how much mass is lost before the secondary fills its Roche lobe.     

微细孔电加工技术

概述微细孔放电加工技术和电化学加工技术的特点和研究进展。