风扇出口导向叶片低噪声设计Ⅱ:数值验证

作为风扇出口导向叶片（Outlet Guide Vanes，OGV）低噪声设计系列文章的第2篇，本文对气动/声学一体化设计获得的2个OGV低噪声方案的降噪效果进行了数值验证。为了对低噪声优化方案的降噪效果进行详细评估，首先，采用非线性谐波法对优化前后的风扇/增压级开展了数值仿真，对OGV不同截面和叶片表面脉动压力进行了对比分析，发现低噪声优化设计方案有效降低了转/静干涉引起的脉动压力；然后，通过掠形和倾斜的合理组合，改变了叶片表面的相位分布，沿径向的相位变化增加了OGV对尾迹响应相互抵消的机会，从而有利于噪声的降低；最后，采用Wilson的波分解方法开展了对各方案的模态分析，对降噪效果进行了量化评估。结果显示，优化后的低噪声方案除起飞状态1BPF外，降噪量均超过了5 dB。     

描述弹塑性材料损伤演变行为的3种计算方法的研究与应用

借助于双向组合坐标系,就弹塑性材料的损伤演变速率和寿命提出了3种计算方法.它包括:单参数法、比值法、乘积法,同时本文给出了许多新的计算方程,还提供了一个同各个常用材料参数有着函数关系的综合性材料常数的新概念.这些常用参数有:疲劳强度系数σ'f、疲劳强度指数b'1、疲劳延性系数ε'f、疲劳延性指数c'1、平均应力、平均应变和临界加载时间等等.用汽车的一个零件做了实例计算,并对计算结果进行了一些比较.预计这些计算方法对避免过多的疲劳试验,对节省疲劳试验的时间、人力和资金,对方便工程应用在某种程度上将有着实际意义.     

关于矩阵方程AX+XTC=B的解的存在性的探讨

以矩阵广义逆为工具，给出了矩阵方程Ax X^tC=B解的存在的充要条件。将该方程的求解问题转化为对其等价方程的求解，得出一些相应的很有价值的结论。并在理论上进行了较为严密的证明，同时，对该方程的常见的某些特殊情形做了进一步的推导。     

一种改进的Dolph—Chebyshev方法在阵列天线方向图综合中的应用

通过对传统Chebyshev多项式增加修正因子得到一种修正的Chebyshev多项式，并以此为基础提出了一种新的阵列天线方向图综合方法。与传统Chebyshev综合法相比，该方法可以在保持副瓣电平不变的情况下对主瓣进行任意展宽，待求参数少，综合过程简单，有很强的实用性。     

Properties of the high area-to-mass ratio space debris population at high altitudes

In the framework of its space debris research activities ESA established an optical survey program to study the space debris environment at high altitudes, in particular in the geostationary ring and in the geostationary transfer orbit region. The Astronomical Institute of the University of Bern (AIUB) performs these surveys on behalf of ESA using ESA’s 1-m telescope in Tenerife. Regular observations were started in 1999 and are continued during about 120–140 nights per year. Results from these surveys revealed a substantial amount of space debris at high altitudes in the size range from 0.1 to 1 m. Several space debris populations with different dynamical properties were identified in the geostationary ring. During the searches for debris in the geostationary transfer orbit region a new population of objects in unexpected orbits, where no potential progenitors exist, was found. The orbital periods of these objects are clustered around one revolution per day; the eccentricities, however, are scattered between 0 and 0.6. By following-up some of these objects using the ESA telescope and AIUB’s 1-m telescope in Zimmerwald, Switzerland, it was possible to study the properties of this new population. One spectacular finding from monitoring the orbits over time spans of days to months is the fact that these objects must have extreme area-to-mass ratios, which are by several orders of magnitudes higher than for ‘normal-type’ debris. This in turn supports the hypothesis that the new population actually is debris generated in or near the geostationary ring and which is in orbits with periodically varying eccentricity and inclination due to perturbations by solar radiation pressure. In order to further study the nature of these debris, multi-color and temporal photometry (light curves) were acquired with the Zimmerwald telescope. The light curves show strong variations over short time intervals, including signals typical for specular reflections. Some objects exhibit distinct periodic variations with periods ranging from 10 to several 100 s. All this is indicative for objects with complicated shapes and some highly reflective surfaces.     

Calculation of the effect of opacity in the solar spectral lines of carbon ions

In this paper, using the intensity ratio of carbon ions emission lines, we determined the optical depths at the line center of the CI at about 165.7 nm, CII at about 133.5 nm, CIII at about 117.5 nm and CIV at about 154.9 nm emission lines by escape factor treatment. For CI and CII emission lines, we discuss the intensity ratio of two lines arising from the common upper levels; while for CIII and CIV emission lines, we discuss the intensity ratio of two lines arising from the common lower levels. By introducing the measured abundance of carbon and the results of ionization balance calculations, we make an estimate of the line-of-sight physical thickness of the regions of carbon ions. This discussion will provide some results in the discussion of opacity on the solar ultraviolet (UV) or extreme-ultraviolet (EUV) spectrum.     

浮动块硬盘磁头抛光机的运动学分析

通过对抛光盘摩擦驱动力矩和导轮阻力矩等影响因素的仿真分析计算,研究了各因素与抛光机运动学行为的关系。结果表明,转速比是主要的运动学行为,导轮的滚动摩擦系数和偏心距对抛光机转速比的影响比较大,偏心距需要和其它抛光因素协调选择。     

栅格绕流数值模拟研究

栅格长宽比是影响栅格翼气动特性的重要参数,为研究它对栅格翼气动特性的影响规律,本文通过求解NS方程数值模拟研究单栅格长宽比对栅格气动特性的影响,并且对栅格边框厚度和形状对阻力的影响,在亚、跨、超声速多个马赫数下进行了数值模拟.结果显示,在所选择的长宽比范围内,长宽比对阻力的影响不大,对法向力有明显的影响,选择适当的栅格边框外形和厚度,可以大大减小栅格的阻力.     

一类（F，α，ρ，d）-凸多目标半无限分式规划的最优性充分条件

本文考虑了一类(F,α,ρ,d)-凸下的多目标半无限分式规划问题,得到了这类规划问题的一些最优性充分条件。     

卫星转发器载波互调噪声比的工程计算

阐述了卫星转发器在多载波工作时载波互调噪声比的工程计算方法，并给出了一个实际的计算例子。