关于多项式系数二阶线性微分方程的可积性问题

主要探讨了实域上当ｇ（ｘ），ｈ（ｘ）是多基式，二阶变系数线性微分方程ｙ″＋ｇ（ｘ）ｙ‘＋ｈ（ｘ）ｙ＝０的可积性问题，沿袭了文」１「中算子矩阵理论的思想，得到了该方程要积的充分必要条件，且给出可积时的通解公式，并举例指出了文中「５，６」中收集的许多可积的二阶线性微分方程，其中相应的多项式系数的部分均是本文的特例。     

天线雷达散射截面的分析与实验

本文利用天线散射的基本原理，以波导激励振子抛物面天线为例，计算并分析了天线的结构项散射雷达截面ＲＣＳｓ和模式项散射雷达截面ＲＣＳｅ，给出了此天线雷达截面的预估值。实验结果表明，理论预估值与实测值吻合较好，并且证明天线的模项ＲＣＳｅ大于结构项ＲＣＳｓ，天线总的雷达截面主要受天线模式散射的影响，减小模式项ＲＣＳｅ将有效地降低天线的雷达截面。本文结果为探索以克服天线模式散射为主的天线ＲＣＳ减缩技术提供了理论依据     

步进电机在真空低温下的驱动特性分析

文章对步进电机的特点、应用情况及误差补偿处理进行了分析,并提出了在真空低温环境下,除了按常规计算外还必须进行超常力矩试验。     

表面裂纹理论的回顾与评述(下)

本文简要地介绍了近几十年国内外表面断裂力学理论的发展状况及所取得的一些成果，重点介绍了应力强度因子求法和裂纹扩展速率的描述。同时对应用于圆柱体上的表面裂纹应力强度因子求法及裂纹扩展速率的描述等方面成果进行了评述。     

某型压差活门的动态特性分析

压差活门是航空发动机数控系统燃油计量装置中重要的液压部件,其稳定性和动态性能直接影响控制系统的整体性能。根据压差活门非线性微分方程,采用小偏差线性化方法,推导出了压差活门的动态数学模型,得到了压差活门的方框图以及传递函数。选取某压差活门参数建立了Simulink仿真模型,分别在频域和时域分析了其动态性能。结果表明:在频域上,比较了有无节流器时的回路增益函数伯德图,认为敏感油路上的节流器可以改善稳定性且提高控制精度,通过设计节流器的尺寸可以调节穿越频域,从而改善系统的动态性能;在时域上,分析了不同节流器尺寸下阶跃响应的动态性能,其试验结果与实际工程经验一致。     

民机高速风洞试验的阻力雷诺数效应修正

在飞机设计阶段,获得准确的气动特性数据对设计者是十分重要的,采用缩比模型的风洞试验是主要途径之一。但是风洞条件限制了试验的Re数,从而影响了对跨音速巡航阻力的评估,因此需要对风洞试验结果的阻力进行Re数效应修正。分析了风洞试验结果阻力的误差构成,提出了Re数效应修正的风洞试验数据基础;进一步就跨音速巡航阻力的构成进行分析,论述了对最小阻力和升致阻力分项修正的方法,并对修正结果进行了验证,得到了一种可靠的工程方法。     

耳朵识别身份系统

打击恐怖主义首先要预防恐怖分子,生物识别技术有助于将恐怖分子从人群中识别出来.耳朵是长期保持稳定的一个生物特征,并且耳朵的独特性十分明显.介绍了耳朵识别系统的系统功能和设计思路,采用VC 6.0和SQL SERVER 2000数据库,实现耳朵图像数据采集、图像预处理、图像存储等基本功能.     

The Role of Magnetic Reconnection in CME Acceleration

Observations carried out from the coronagraphs on board space missions (LASCO/SOHO, Solar Maximum and Skylab) and ground-based facilities (HAO/Mauna Loa Observatory) show that coronal mass ejections (CMEs) can be classified into two classes based on their kinematics evolution. These two classes of CMEs are so-called fast and slow CMEs. The fast CME starts with a high initial speed that remains more or less constant; it is also called the constant-speed CME. On the other hand, the slow CME starts with a low initial speed, but shows a gradual acceleration; it is also called the accelerated and slow CME. Low and Zhang [Astrophys. J. 564, L53–L56, 2002] suggested that these two classes of CMEs could be a result of a difference in the initial topology of the magnetic fields associated with the underlying quiescent prominences. A normal prominence magnetic field topology will lead to a fast CME, while an inverse quiescent prominence results in a slow CME, because of the nature of the magnetic reconnection processes. In a recent study given by Wu et al. [Solar Phys. 225, 157–175, 2004], it was shown that an inverse quiescent prominence magnetic topology also could produce a fast CME. In this study, we perform a numerical MHD simulation for CMEs occurring in both normal and inverse quiescent prominence magnetic topology. This study demonstrates three major physical processes responsible for destabilization of these two types of prominence magnetic field topologies that can launch CMEs. These three initiation processes are identical to those used by Wu et al. [Solar Phys. 225, 157–175, 2004]. The simulations show that both fast and slow CMEs can be initiated from these two different types of magnetic topologies. However, the normal quiescent prominence magnetic topology does show the possibility for launching a reconnection island (or secondary O-line) that might be thought of as a “CME’’.     

A Class of TVD Type Combined Numerical Scheme for MHD Equations With a Survey About Numerical Methods in Solar Wind Simulations

It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic field (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere. This role comes as no surprise to numerical modelers that participate in the numerical modelling of atmospheric environments as well as the meteorological conditions at Earth. Space scientists have paid great attention to operational numerical space weather prediction models. To this purpose practical progress has been made in the past years. Here first is reviewed the progress of the numerical methods in solar wind modelling. Then, based on our discussion, a new numerical scheme of total variation diminishing (TVD) type for magnetohydrodynamic equations in spherical coordinates is proposed by taking into account convergence, stability and resolution. This new MHD model is established by solving the fluid equations of MHD system with a modified Lax-Friedrichs scheme and the magnetic induction equations with MacCormack II scheme for the purpose of developing a combined scheme of quick convergence as well as of TVD property. To verify the validation of the scheme, the propagation of one-dimensional MHD fast and slow shock problem is discussed with the numerical results conforming to the existing results obtained by the piece-wise parabolic method (PPM). Finally, some conclusions are made. This revised version was published online in August 2006 with corrections to the Cover Date.     

影响招生计划制定因素的个案分析

通过沈阳航空工业学院2005年招生计划制定的个案，对影响招生计划制定的多重因素作了全面分析和深入研究，旨在说明招生计划的制定不是简单的数量增减，而是一门需要进行综合分析的科学，揭示出影响制定招生计划的外部因素即经济发展环境，以及学校发展定位、就业质量、生源质量等内部因素。