细长旋成体大迎角非定常运动数值研究

利用DES方法对处于非对称流态下的细长旋成体进行了俯仰和偏航振荡的数值模拟,观察细长体气动特性尤其是背风面非对称分离涡的变化。计算结果表明在大迎角非对称多涡系情况下,固定频率和振幅的非定常运动可以改变流场结构和气动力,对细长体背风面流态有巨大的影响。俯仰振荡对非对称分离涡有明显的控制作用,抑制流场的非对称性,使分离涡趋于对称;而固定频率的偏航振荡则破坏背风面分离涡的稳定性,激励非对称背涡产生随时间变化的周期性脱落。所进行的非定常运动与细长体流场耦合作用研究在国内外研究尚少。     

襟翼不对称运动和襟翼倾斜的保护逻辑研究

实现高升力系统的故障保护对提高电传飞机安全性具有重要的意义.本文描述了高升力系统后缘襟翼的架构;针对不对称故障和倾斜故障的监控和和保护方式问题,分析了上述两类故障的监控和保护措施及其工作逻辑,在确定工作逻辑的阈值参数时综合考虑了检测和确认故障、襟翼动力驱动装置的制动过程以及系统机械误等因素;建立了故障保护逻辑的Simulink模型,并对不同的失效情况进行了仿真分析,仿真结果表明本文设计的故障保护措施能够很好地监控系统并防止故障蔓延,研究结果对民机高升力系统设计具有一定的借鉴意义.     

On radiation belt dynamics during magnetic storms

Temporal variations of the radiation belt particle during the magnetic storms are investigated using measurements by the low altitude satellite spectrometer. Along with several known effects, such as the outer radiation belt intensity decrease at the main phase, the radial diffusion with the particle acceleration and the recovery of the radiation belt during the recovery phase, some less known features were investigated, such as the dawn–dusk asymmetry of the radiation belt.     

细长旋成体大迎角非对称流动特性的试验研究

简要介绍了细长体大迎角流动非对称性的试验结果,分析了Re数、湍流度和安装条件等因素对大迎角流动非对称性的影响,探讨了大迎角流动非对称性的产生机制。文章最后着重阐述了该研究得出的一些支持细长体大迎角流动非对称性产生机制的空间动力不稳定性观点的理由。     

背风涡隔离对大攻角旋成体表面压力分布的影响

通过在背风母线处沿纵向对称面嵌入隔离板，观测了大攻角旋成体在这种背风涡被隔离状态下的表面压力分布情况。隔离板的作用旨在削弱、隔阻两侧背风涡间的相互联系和诱导，以便考察背风涡诱导作用对物面流动的影响。不同隔离（包括无隔离情况）状态下的实验结果表明，背风涡的隔离对表面压力分布有不同程度的影响，故这一研究和结果可供探讨大攻角流动非对称性成因作参考。     

非对称空战体系对抗研究

对战斗机分代及其空战能力评估进行了研究,提出了空战体系对抗中,交战双方武器装备非对称度的概念和计算方法.基于体系对抗物理描述和数学模型,发展了非对称战役优势参数的概念.通过对典型的对称、非对称和极限非对称战役想定的作战模拟和分析,探讨了战斗机武器装备的数量与质量关系问题,装备质量太差就很难用数量去弥补.计算结果表明考虑非对称度影响的分析更接近当今战争的实际.      

喉部不对称对微喷管性能影响

以FLUENT 6.1软件为工具,利用数值计算求解二维稳态可压缩Navier-Stokes(N-S)方程,模拟了微喷管内超声速流体流动,分析了喷管喉部结构不对称对喷管内部的流场和喷管性能的影响.这种喉部结构不对称是由于喉部上下顶点在x方向偏离一定距离所造成的.数值计算结果表明,喷管喉部在流体流动方向的不对称,将导致喷管内部流体流场不平衡性,使得流量增大,喷管出口的x方向推力增加,y方向产生了多余的推力.      

Dy和Yd类变压器联结组的微机判别

三相变压器的联结组标号必须判别确定。选较复杂的 Dy和 Yd类联结组为例 ,对其进行理论分析 ,获得作筛选法判别基准的理想计算值的规律性。在实测时考虑三相电源电压不对称的影响 ,用实测计算值代替理想计算值作判别基准。经微机的硬件与软件系统联试 ,能对全部联结组标号快捷地判别 ,不仅能判定对与错 ,还能指出错误联成何种标号     

可压缩流中声激励对细长体大迎角流动非对称性的影响研究

在跨声速风洞中研究了声激励对于可压缩流中细长旋成体大迎角流动非对称性的影响效果。结果表明,在可压缩流场中,声激励对于细长体典型迎角下的流动非对称性依然有着一定的影响,但由于高速风洞中流场本身的湍流度较高,声激励效果要比低湍流度不可压缩流中的影响弱。     

Evolutionary features of polar and non-polar coronal holes during solar cycle 24 and the rising phase of cycle 25

This paper presents the results of the analysis of the evolution of coronal holes (CHs) on the Sun during the period May 13, 2010 – March 20, 2022, covering Solar Cycle 24. Our study uses images in the extreme-ultraviolet iron line (Fe XII 193 Å) obtained with the Atmospheric Imager Assembly of the Solar Dynamics Observatory (AIA/SDO). To localize CHs and determine their areas, we used the Heliophysics Event Knowledgebase (HEK). We separate the CHs into polar and non-polar and study the evolutionary features of each group. During this period, an asymmetry between the Northern (N) and Southern (S) Hemispheres (N-S or hemispheric asymmetry) is detected both in the solar activity (SA) indices and in the localization of the maximum areas of the polar and non-polar CHs. It is shown that the hemispheric asymmetry of the areas of polar and non-polar CHs varies significantly over time and that the nature of these changes is clearly related to the SA cycle. We find that for most of the period, the polar CHs were predominated generated in the S- hemisphere while the non-polar CHs were dominant in the N- hemisphere. It is found that the maximum and minimum of the hemispheric imbalance in the areas of non-polar CHs are close in time to the maximum and minimum of the asymmetry of the SA indices (the number and areas of sunspots). The maximum hemispheric imbalance of the polar CH areas is observed at the maximum of Cycle 24, and the minimum imbalance is found at the cycle minimum. These results confirm our assumption that these two types of CHs are of a different nature and that the non-polar CHs, like sunspots, are elements of the general magnetic activity.