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.     

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。     

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。     

采用正弯静叶的压气机在不同轴向间隙下时序效应的实验

实验研究了一台采用正弯静叶的低速压气机在不同轴向间隙下的时序效应,详细测量了二级静叶出口的横截面流场.实验结果表明:随着轴向间隙的减小,时序效应未见明显变化,压气机扩压能力增强,输入扭矩随之增加,效率则呈现出先增大后减小的趋势,表明存在最佳周向间隙,同时喘振裕度有所下降.     

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.     

CME dynamics using coronagraph and interplanetary ejecta data

In this work, we present a study of the coronal mass ejection (CME) dynamics using LASCO coronagraph observations combined with in-situ ACE plasma and magnetic field data, covering a continuous period of time from January 1997 to April 2001, complemented by few extreme events observed in 2001 and 2003. We show, for the first time, that the CME expansion speed correlates very well with the travel time to 1 AU of the interplanetary ejecta (or ICMEs) associated with the CMEs, as well as with their preceding shocks. The events analyzed in this work are a subset of the events studied in Schwenn et al. (2005), from which only the CMEs associated with interplanetary ejecta (ICMEs) were selected. Three models to predict CME travel time to Earth, two proposed by Gopalswamy et al. (2001) and one by Schwenn et al. (2005), were used to characterize the dynamical behavior of this set of events. Extreme events occurred in 2001 and 2003 were used to test the prediction capability of the models regarding CMEs with very high LASCO C3 speeds.     

火箭弹射座椅乘员抓握中央拉环耐限力研究

火箭弹射座椅中央拉环是乘员启动应急离机程序的操纵手柄,同时还承载着对乘员手腕的防护功能。中央拉环的外形影响了抓握的姿势,而不同的抓握姿势,也直接决定了人体手臂的气流吹袭载荷。文中先分析了国内外典型弹射座椅中央拉环的外形和使用特点,通过对乘员不同姿势握持中央拉环的耐受力实测,提出了一种有利于乘员做出对抗动作的抓握姿势和外形,并对其进行了仿真分析和试验,为后续弹射座椅的中央拉环改进设计和乘员上肢防护提供参考。     

火星进入舱开伞弹伞载荷动力放大系数研究与试验验证

首先推导了单自由度系统在矩形和半正弦波形脉冲冲击下响应谱动力放大系数与脉冲作用时间的理论解析公式,然后采用有限元显示冲击动力学分析方法,分析了火星探测器进入舱进入过程中开伞弹伞低频大冲击载荷的载荷波形、脉冲作用时间以及结构阻尼对进入舱主结构动力放大系数的影响;最后介绍了开伞载荷悬吊冲坠模拟冲击动载试验和弹伞载荷真实弹伞筒冲击动载试验。分析与试验结果表明:冲击作用时间在1 ms以下时,结构衰减效应明显,冲击作用时间大于5 ms后,动力放大系数同波形下趋于稳定;开伞载荷由于指数型前沿上升时间较长,动力放大系数基本为1;弹伞载荷上升前沿较陡,矩形前沿波放大倍数在1～2倍之间。上述研究可为火星探测器进入舱结构载荷条件的确定提供参考。