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.     

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。     

对AVR403型电压调节器的分析

当同步发电机输出电流大小与功率因数改变时,其电枢反应与内阻抗压降将改变,则发电机输出电压也将改变。为使发电机输出电压保持额定值,通常都有自动电压调节器与发电机配套工作。本文较详细地分析了MD-80飞机使用的AVR403型电压调节器各部分电路的工作原理,以及整机调压的工作过程,并阐述了该调压器的特点。     

差值法与比值法的误差修正效果比较研究及应用

差值法与比值法对不同测量系统的误差修正效果不一样。本文将两种方法的比较用一个比值来描述,并用推得的公式进行量化表示。在进一步的应用研究中,理论分析与实验数据相互印证,同时得到许多有益的结论,有助于全面掌握测量系统的误差来源,从而灵活选择各种修正方法以获得更加准确的测量结果。     

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.     

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.     

收敛-扩张喷管中运用次流推力矢量控制技术的计算研究

采用二阶1TVD格式的有限体积法耦合RNGκ-ε湍流模型和非平衡壁面函数求解二维守恒型雷诺平均N-S方程,数值模拟了运用次流椎力矢量控制技术的二维收敛-扩张喷管中的流动现象。计算结果表明,随着喷管压比的增加,次流喷射所产生的激波向扩张段下游移动,且喷管矢量角不断减小到一固定值;次流压比的增加将导致激波向扩张段上游移动,且喷管矢量角不断增加;次流压比对激波和矢量角的影响比喷管压比更强。     

二冲程发动机分缸不均匀性分析

针对两缸二冲程航空发动机缸间不均匀性问题,运用试验、仿真相结合的方法分析引起缸间不均匀性原因,建立发动机GT-Power一维仿真模型,通过缸压信号对发动机不同工况分缸不均匀性进行仿真分析,并进行发动机台架试验,对比分析不同工况发动机两缸缸压和空燃比。结果表明:引起缸间不均匀性的原因是缸间进气和喷油的差异,小负荷主要影响因素为喷油差异,部分负荷主要影响因素为缸间进气差异,且随节气门开度的增大差异减小,为发动机均匀性控制的软硬件实现提供理论依据。