微型直升机动力学建模的研究现状

从模型修改、结构分析、神经网络及系统辨识几个方面介绍了微型直升机动力学建模的研究现状,并对几种不同的建模方法进行了比较。然后,指出了系统辨识方法中存在的问题。通过讨论和比较,为微型直升机的不同建模目标提供了可供借鉴的建模方法。     

空调制冷故障考核仿真实训系统的设计与应用

以空调制冷故障考核仿真系统为例，介绍空调制冷仿真实验实训系统在国家级试点专业——供热通风与空调工程技术专业教学中的作用。该系统重点解决了空调制冷故障的考核仿真模拟，阐明了仿真技术对于高职高专学生培养的重要性和可行性。仿真实验实训技术在技能型人才培养中将有很大的发展空间。     

用科学发展观构建高职高专学报创新发展之路

胡锦涛同志倡导的科学发展观，不仅对全面实现建设小康社会、构建社会主义和谐社会的宏伟目标有着极其重要的意义，同时，对高职高专学报的创新和发展，也有着非常重要的意义。高职高专学报目前存在着实力不强、质量不高、特色不明、办刊因难的局面，要改变这种状况，就要贯彻落实科学发展观，明确学报的发展方向、本质和核心，发展的基本内涵和基本要求，使高职高专学报在林立的高校学报队伍中真正拥有一席之地。     

Instability and unsteadiness of aircraft wake vortices

This paper presents a review of theoretical and experimental results on stability and other unsteady properties of aircraft wakes. The basic mechanisms responsible for the propagation and the amplification of perturbation along vortices, namely the Kelvin waves and the cooperative instabilities, are first detailed. These two generic unsteady mechanisms are described by considering asymptotic linear stability analysis of model flows such as vortex filaments or Lamb–Oseen vortices. Extension of the linear analysis to more representative flows, using a biglobal stability approach, is also described. Experimental results obtained using LDV, hot wire and PIV in wind tunnels are presented and they are commented upon the light of theory.     

叉排型扰流柱排内部流场的实验研究

在特别建造的小型扰流柱排风洞上，测量了6个不同雷诺数下叉排型短扰流柱排内部的流场分布，发现不同雷诺数下流场分布非常相似，在奇数和偶数测量截面上，速度分布规律不同，在奇数截面上可以观察到通道涡，在偶数截面的端壁附近存在马蹄涡。     

谈知识经济时代对图书馆人力资源管理的构想

知识经济时代图书馆的地位更加重要，对图书馆员也提出了新的要求，因此，搞好图书馆人力资源管理势在必行。通过分析了图书馆人力资源管理的现状及存在的问题，提出和强调了图书馆在人力资源管理方面要以人为本，引入竞争机制、激励机制的新模式。     

有序递推滤波修正系统误差方法

本文将推广卡尔曼滤波的原理拓展到对测量元素逐个进行滤波的处理。从理论上证明它可以提高状态向量滤波结果的估值精度，而且它可以减少求逆公式的计算量。本文应用该方法导出了轨道测量数据处理的有序递推自校准系统误差的方法及公式。     

喷管流场数值仿真CFD／Nozzle软件包设计

ＣＦＤ／Ｎｏｚｚｌｅ软件包是一套专门的二维轴对称跨音速喷管流场计算机辅助设计分析工具。它采用高度集成化的操作环境，将网格生成、数值计算、图形显示全部过程集于一体。具有西文环境下的全中文用户界面，操作环境同时提供详尽的彩色图文方式下的中文提示。数值方法稳健，兼具源程序开放与编译连接自动化特点。叙述了ＣＦＤ／Ｎｏｚｚｌｅ软件包设计思想和实现方式，并给出了流场计算、参数分析、功能扩充几方面的应用实例。     

Evolution of the Protosolar Nebula and Formation of the Giant Planets

The formation of planetary systems is intimately tied to the question of the evolution of the gas and solid material in the early nebula. Current models of evolution of circumstellar disks are reviewed here with emphasis on the so-called “alpha models” in which angular momentum is transported outward by turbulent viscosity, parameterized by an dimensionless parameter α. A simple 1D model of protoplanetary disks that includes gas and embedded particles is used to introduce key questions on planetesimal formation. This model includes the aerodynamic properties of solid ice and rock grains to calculate their migration and growth. We show that the evolution of the nebula and migration and growth of its solids proceed on timescales that are generally not much longer than the timescale necessary to fully form the star-disk system from the molecular cloud. Contrary to a widely used approach, planet formation therefore can neither be studied in a static nebula nor in a nebula evolving from an arbitrary initial condition. We propose a simple approach to both account for sedimentation from the molecular cloud onto the disk, disk evolution and migration of solids. Giant planets have key roles in the history of the forming Solar System: they formed relatively early, when a significant amount of hydrogen and helium were still present in the nebula, and have a mass that is a sizable fraction of the disk mass at any given time. Their composition is also of interest because when compared to the solar composition, their enrichment in elements other than hydrogen and helium is a witness of sorting processes that occured in the protosolar nebula. We review likely scenarios capable of explaining both the presence of central dense cores in Jupiter, Saturn, Uranus and Neptune and their global composition. This revised version was published online in August 2006 with corrections to the Cover Date.     

皮托管式轴对称进气道跨音速内,外流场的AF—2方法计算

本文构造了轴向大扰动,径向小扰动轴对称速势方程的AF-2分解格式,计算了IC型皮托管式进气道的跨音速内外流场,并对这种分解格式进行了线化的稳定性分析。分析表明:AF-2方法的稳定性优于SLOR方法,其收敛速度至少比SLOR方法快10倍。