超声速空腔流激振荡与声学特性研究

基于高速风洞试验研究了超声速时空腔流激振荡与声学特性.试验马赫数为1.5,基于每米的雷诺数为2.26×107,来流边界层厚度为0.024 m,试验空腔长深比分别为15,12和6.结果表明:空腔内形成的剪切层与腔后壁相撞诱发腔内较强烈噪声,噪声从腔后缘向腔前缘传播时受到腔内流动的干扰,故同频率下腔后缘处的声压均高于腔前中部区域的声压.闭式和过渡式空腔长深比较大,剪切层与腔底面相撞在腔内形成的压缩波或激波,干扰了从腔内声波反馈回路、限制了流激振荡的形成,故腔内未出现明显的声压峰值激振频率;开式空腔长深比较小,剪切层直接跨过空腔中部与腔后壁相撞,产生的噪声向腔前缘传播,腔内形成流激振荡,并出现多个声压峰值激振频率.      

On the relation of the Forbush decreases detected by ASEC monitors during the 23rd solar activity cycle with ICME parameters

To improve the physical understanding of the Forbush decreases (FD) and to explore the Space Weather drivers, we need to measure as much geospace parameter as possible, including the changing fluxes of secondary cosmic rays. At the Aragats Space Environmental Center (ASEC) are routinely measured the neutral and charged fluxes of secondary cosmic rays. Each of species has different most probable energy of primary “parent” proton/nuclei. Therefore, the energy range of the Galactic Cosmic Rays (GCR) affected by Interplanetary Coronal Mass Ejection (ICME) can be effectively estimated using data of the ASEC monitors. We presented relations of the magnitude of FD observed in different secondary particle fluxes to the most probable energy of the primary protons. We investigate the correlations between the magnitude of FD with the size, speed, density and magnetic field of the ICME. We demonstrate that the attenuation of the GCR flux incident on the Earth’s atmosphere due to passing of the ICME is dependent on the speed and size of the ICME and the magnetic field strength.     

超声速横向气流中燃料雾化的数值模拟

对超声速横向气流中燃料雾化过程采用欧拉-拉格朗日方法进行了数值模拟,气相场用欧拉法计算,液相场采用拉格朗日粒子跟踪方法计算,通过方程源项考虑液相对气相的影响.在液相的拉格朗日计算中采用改进的混合雾化模型来研究雾化过程.针对超声速横向气流中雾化的特点,结合雾化机理和实验测量结果,对原有的混合雾化模型进行了改进,并将改进后的计算结果与TAB(Taylor Analogy Breakup)模型和Reitz波模型的计算结果进行了对比.结果表明:改进的混合雾化模型的计算结果与实验测量值符合较好,更适合用于超声速横向气流中燃料雾化的数值模拟.     

一种基于结构化贴体网格的DSMC方法研究

基于DSMC方法,发展了一种结构化的贴体网格的分子运动轨迹跟踪和定位的方法———网格面法向量判断法。在此基础上建立了一套DSMC数值模拟程序,对球双锥和Apollo飞船在过渡区域流动进行了数值模拟,并分析了其过渡区域超音速、高超音速的气动力、气动热等问题。通过将本文的计算结果与参考文献的计算结果和实验结果进行了比较,验证了所发展的方法的可靠性。     

某型号火箭发动机高空模拟试验中扩压器的 数值计算与试验比较

文章利用FLUENT软件对某型号液氢/液氧火箭发动机在高空模拟引射试验中扩压器进行数值计算,并与试验测量数据进行比较。用Visual C#.NET软件编制了二次喉道扩压器引射过程计算程序,将该程序的计算结果与FLUENT软件的数值计算结果进行了比较。利用FLUENT软件对二次喉道扩压器在不同入口长度、不同收缩比和长径比情况下的流场情况进行了计算,分析了对发动机启动的影响;并把数值计算结果同吹风试验的数据进行了比较,结果表明数值计算具有较高的置信度。     

采用多级主火箭的RBCC发动机性能分析(英文)

采用三维两相数值模拟技术研究火箭基组合推进(RBCC)发动机的燃烧。提出了一种新的主火箭布置方式,该方式采用多级主火箭,一级嵌入到支板之中,另一级置于燃烧室中部上壁面。研究表明,相对于常规的主火箭布局,多级主火箭布局能明显提升发动机性能。置于支板的一级火箭以恰当比工作,起到引射和改善进气道工作特性的作用;二级火箭以富燃状态工作,起到火焰稳定和促进燃烧的作用。多级火箭喷射方案是DAB和SMC模式的综合,可作为火箭引射模态改善二次燃烧一种新的方式。     

超声速有翼飞行器的无粘分区数值模拟

本文采用ＭａｃＣｏｒｍａｃｋ两步显式格式，用空间推进法求解Ｅｕｌｅｒ方程来对有翼飞行器的超声速绕流流场进行数值模拟，应用特征边条件处理场面边界及装配激波的计算，在翼缘及表面斜率不连续处，采用局部解析处理，提高了算法的可靠性，复杂外形的计算采用分区处理技术，网格由代数形式生成，在大攻角的计算中，通过对横流速度型的修正改善了背风面压力分布特性，解决了推进中断问题，同时模拟出背风面涡。     

弹射动力动态性能参数波形与频谱分析的初步研究

 研究飞行员弹射救生系统弹射动力的传递作用,采用线性机械振动系统进行模拟试验,利用数字信号的波形与频谱分析方法进行数据处理。试验结果表明:符合弹射动力与人体模型的特点。计算公式和方法是合理可行的。     

Short term topological changes of coronal holes associated with prominence eruptions and subsequent CMEs

We study the short-term topological changes of equatorial and polar coronal hole (CH) boundaries, such as a variation of their area and disintegration, associated to reconnection with nearby (within 15° distance) quiescent prominence magnetic fields leading to eruptions and subsequent Coronal Mass Ejections (CMEs). The examples presented here correspond to the recent solar minimum years 2008 and 2009. We consider a temporal window of one day between the CH topological changes and the start and end times of prominence eruptions and onset of CMEs. To establish this association we took into account observational conditions related to the instability of prominence/filaments, the occurrence of a CME, as well as the subsequent evolution after the CME. We found an association between short-term local topological changes in CH boundaries and the formation/disappearance of bright points near them, as well as, between short-term topological changes within the whole CH and eruptions of nearby quiescent prominences followed by the appearance of one or more CMEs.