Study of UV Ne II line shapes in the cathode sheath of an abnormal glow discharge

We report results of an experimental and theoretical study of complex UV line shapes of Ne II 369.421 nm, Ne II 370.962 nm, Ne II 371.308 nm, and.Ne II 372.711 nm lines in the cathode sheath (CS) region of an abnormal DC glow discharge in pure neon. Two sets of experimental profiles and electric field distributions, one for discharge with tungsten and the other with titanium cathode, were obtained by means of the optical emission spectroscopy (OES) and theoretically studied by the iterative CS kinetic model. It is shown that our theoretical model enables the determination of the most important CS parameters (e.g. the thickness of the CS region, and the theoretical distributions of electric field and gas temperature) and thereupon based accurate theoretical predictions of the experimentally observed profiles of the studied lines.     

固体火箭发动机点火瞬时内流场轴对称数值分析

应用流体计算软件(FLUENT),通过UDF(用户定义函数)编程,考虑了辐射热量的影响,对固体火箭发动机点火瞬时内流场进行了轴对称数值分析,得出了点火瞬时的压强．时间曲线、各时刻的流场和推进剂燃面上的辐射热量。从具体数值上分析了辐射热量对点火瞬时的影响。研究结果表明,该方法可较好地预示点火瞬时的内流场和压强变化情况。     

复合固体推进剂裂尖复合型变形场和约束场分析

用有限元法分析了不同Ⅰ-Ⅱ复合型裂端的变形场和约束场（裂端形状改变能和应力三维度水平Rσ）分布。结果表明：复合型裂端变形为不对称的相反变形,符合钝化-锐化模型。Ⅰ-Ⅱ复合加载时裂纹尖端出现负约束区域（该区Rσ〈0）,当Ⅱ型分量增加,负约束区域增大,最大约束水平Rσmax降低,且绕裂纹尖端顺时针转动。Rσmax出现距裂纹尖端有一定距离处。Ⅰ-Ⅱ复合载荷下偏离原裂纹方向的裂纹在钝化区内某处危险点开始萌生,并与应力三维度最大位置处产生的空穴或孔洞聚合向前扩展。     

风洞短试验段中基于被动技术的大气边界层模拟

针对西南交通大学XNJD-1风洞第一试验段的特点,采用被动模拟装置,通过多次流场校测、反复试凑,成功地在风洞中模拟了C类地表情况下的高湍流度大气边界层,实测平均风速剖面、湍流度剖面及风谱特性等与目标值较为吻合.此外,还对比讨论了平均风速和离地高度等因素对风场特性影响, 并计算了湍流积分尺度.研究表明边界层调试过程中应重点考查气流在对应结构卓越频段范围内的脉动情况,而仅将湍流度作为参考指标.     

远场应变法测量应力强度因子

本文给出一种将常规电阻应变片贴在距裂纹尖端较远处测量Ⅰ型裂纹应力强度因子K_1的方法。此法实际上是一种实验法与数值法相结合的方法。用实验法测出应变,应变又可以用含待定系数的Williams级数表示,它们组成一组线性代数方程组。解此方程组,可获得待定系数,由待定系数与应力强度因子的已知关系,可求出K_1。 远场应变测量法,避开了裂纹尖端邻域应变梯度很大的区域和可能的塑性区,因而应变测量比较准确。 测出的应变输入数据处理设备及计算机就可以快速实时地知道含裂纹结构在承载情况的K_1,便于进行破坏控制,使设备安全而可靠的工作。     

超燃冲压发动机电弧加热器试验流场调试

利用电弧加热器提供超燃冲压发动机地面模拟试验的纯空气流场,需要在前电极与喷管之间由冷气混合室加入冷气以降低电弧加热气体的焓值;为了较为准确地获得流场的总温参数,采用了总温探针对流场总温900-1600K进行了校测,总温的测量值与计算的焓值、流量匹配法计算的总温进行了对比,结果表明：总温越高,测量值与计算值相差越大,在名义总温1600K时达到了450K,笔者分析了产生的原因。     

基于混合RANS/LES方法的亚声速空腔流动主要影响因素的数值研究

随着计算流体力学（Computational fluid dynamics, CFD）技术的发展,混合雷诺平均N-S方程（Reynolds averaged Navier-Stokes, RANS）/大涡模拟（Large eddy simulation, LES）类方法被越来越多地应用于航空领域的大分离流动及气动噪声的仿真分析中,并取得了很好的效果。本文选取M219空腔流动风洞试验模型,在Ma=0.85的情况下,进行了混合RANS/LES方法的验证,并进行了网格敏感性分析;然后针对影响空腔流动的几个关键因素进行了仿真研究,并给出了主要的研究结果;最后,针对L/D=7的大长深比空腔,研究了增加隔板形成前后两个L/D=3.5的串列空腔的流动特点。     

Longitudinal variations of geomagnetic and ionospheric parameters in the Northern Hemisphere during magnetic storms according to multi-instrument observations

We present a joint analysis of longitude-temporal variations of ionospheric and geomagnetic parameters at middle and high latitudes in the Northern Hemisphere during the two severe magnetic storms in March and June 2015 by using data from the chains of magnetometers, ionosondes and GPS/GLONASS receivers. We identify the fixed longitudinal zones where the variability of the magnetic field is consistently high or low under quiet and disturbed geomagnetic conditions. The revealed longitudinal structure of the geomagnetic field variability in quiet geomagnetic conditions is caused by the discrepancy of the geographic and magnetic poles and by the spatial anomalies of different scales in the main magnetic field of the Earth. Variations of ionospheric parameters are shown to exhibit a pronounced longitudinal inhomogeneity with changing geomagnetic conditions. This inhomogeneity is associated with the longitudinal features of background and disturbed structure of the geomagnetic field. During the recovery phase of a storm, important role in dynamics of the mid-latitude ionosphere may belong to wave-like thermospheric disturbances of molecular gas, propagating westward for several days. Therefore, it is necessary to extend the time interval for studying the ionospheric effects of strong magnetic storms by a few days after the end of the magnetospheric source influence, while the disturbed regions in the thermosphere continues moving westward and causes the electron density decrease along the trajectories of propagation.     

Installation and preliminary data analysis of Penang magnetic data Acquisition system (MAGDAS) in Malaysia

MAGDAS PEN was established on 19th September 2019 as one of the MAGDAS observatory arrays located at Universiti Sains Malaysia (USM) (5.15°, 100.50°). The main objective of the MAGDAS project is to monitor global electromagnetic and the ambient plasma density in the geospace environment. This installation has contributed to a better understanding of the Sun-Earth coupling system. This paper presents the installation process of one of the MAGDAS magnetometers named YU-8 T magnetic sensor and provides a preliminary analysis of geomagnetic HDZ components amplitude-time that was observed at PEN station. A one-month HDZ-geomagnetic field data was processed from 1st November to 30th November 2019. The daily variations with a consistent pattern in delta H geomagnetic field components are observed throughout the day with eastward electric field effects that are observed during solar peak hours. The delta H-component gradually increases around 0700LT and reaches the maximum reading at 1300LT with a range of value ~ 40-70nT. The value slowly decreases that started from 1400LT until the night time. The reading during the night time shows a constant variation with magnitude varies in between ?10nT to + 10nT. The average H-component value of the night time is used as the baseline for the observation system. Overall, the observed trends portray a good sign of solar quiet field and Sq with no solar-terrestrial disturbances.     

线阵CCD交汇测量系统结构布局的优化设计

介绍了由两个线阵ＣＣＤ所组成的交汇测量系统的基本原理,分析了有效视场、坐标测量误差和系统结构参数之间的关系。由仿真研究表明,当给定有效视场的大小及各结构参数的测量误差值时,可寻求系统最优结构布局,使坐标测量误差最小。