北京地区重力波活动及其波谱的季节分布特性研究

利用激光雷达对北京地区上空Na层进行持续观测,通过连续三年累积的夜间观测数据对北京地区重力波活动及其波谱进行研究.根据重力波的线性理论计算,得到北京地区上空的大气密度扰动规律、空间功率谱和时间频率谱.通过选择重力波波长在1~8 km,具有特定波长以及特定周期为60,45,25 min的重力波活动辅助研究重力波的季节变化规律,结果表明北京地区重力波大气密度扰动具有夏季大、冬季小的活动规律.结合波源与背景风场的季节性变化规律,分析得出北京上空重力波活动季节性变化的主要原因为青藏高原地形和对流因素与我国北方地区季节性背景风场共同作用的结果.     

补燃循环发动机强迫起动研究

某泵压式液体火箭发动机是我国首台采用强迫起动方式的补燃循环发动机.结合发动机特点建立了强迫起动模型,进行了系统级冷调试验,根据试验及仿真结果确定了发动机起动参数及起动程序.针对试车暴露的问题,采取一系列措施解决了起动超调、起动爆燃、推力室点火冲击大及喷注器起动变形等问题.研究结果在发动机试车中得到验证.     

A superposed epoch study of the effects of solar wind stream interface events on the upper mesospheric and lower thermospheric temperature

The response of mesosphere and lower thermosphere (MLT) temperature to energetic particle precipitation over the Earth’s polar regions is not uniform due to complex phenomena within the MLT environment. Nevertheless, the modification of MLT temperatures may require an event-based study to be better observed. This work examines the influence of precipitation, triggered by solar wind stream interfaces (SI) event from 2002 to 2007, on polar MLT temperature. We first test the relationship between the ionospheric absorption measured by the SANAE IV (South African National Antarctic Expedition IV) riometer and the layer of energetic particle precipitation from POES (Polar Orbiting Environmental Satellites). The combined particle measurements from POES 15, 16, 17 and 18 were obtained close in time to the pass of the SABER (Sounding of the Atmosphere using Broadband Emission Radiometry) temperature retrieval. Here, a superposed epoch technique is described and implemented to obtain average temperature profiles during SI-triggered particle precipitation. The superposed epoch average shows no significant temperature decrease below 100 km prior to the onset of SI-triggered precipitation, whereas a clear superposed average temperature decrease is observed at 95 km after the SI impact. A case study of SI event also yields similar observations. Results indicate that cooling effects due to the production of mesospheric odd hydrogen might be major contributors to temperature decrease under compressed solar wind stream.     

Dynamics of the convection in the inner magnetosphere by observations of the diffuse aurora,SAR arc and ionospheric drift

The first results of the comparison of subauroral luminosity dynamics in 557,7 and 630,0 nm emission with simultaneous measurements of the ionospheric drift in the F2 region with a digisonde DPS-4 at the Yakutsk meridian (CGMC: 55–60N, 200°E) at Kp = 2–6 are presented. It is shown from the analysis of individual events that during the magnetospheric convection intensification after the turn of the IMF B_z – component to the south the equatorward extension of diffuse aurora takes place. At the same time the westward ionospheric drift velocity increases both in the diffuse aurora region and much equatorward of it due to the occurrence of the northward polarization electric field. We suppose that the generation of polarization field can be associated with the development of the region 2 FAC during the intensification of magnetospheric convection. The comparison of ground-based observations with measurements of the plasma drift aboard the DMSP-F15 satellite has been carried out.     

Dynamic particle accumulation structure (PAS) in half-zone liquid bridge – Reconstruction of particle motion by 3-D PTV

Three-dimensional (3-D) velocity field reconstruction of oscillatory thermocapillary convections in a half-zone liquid bridge with a radius of O (1 mm) was carried out by applying 3-D particle tracking velocimetry (PTV). Simultaneous observation of the particles suspended in the bridge by two CCD cameras was carried out by placing a small cubic beam splitter above a transparent top rod. The reconstruction of the 3-D trajectories and the velocity fields of the particles in the several types of oscillatory-flow regimes were conducted successfully for sufficiently long period without losing particle tracking. With this application the present authors conducted a series of experiments focusing upon the collapse and re-formation process of the PAS by mechanically disturbing fully developed PAS.     

垂直平板层流自然对流的群论分析

本文对由热、质最扩散和化学反应引起的垂直平板定常层流自然对流问题用Ｍｏｒｇａｎ变换群理论进行了分析，得到了壁面温度和浓度分布均按变化时的相似性方程组，并用Ｒｕｎｇｅ－Ｋｕｔｔａ方法和Ｎａｃｈｔｓｈｅｉｎ－Ｓｗｉｇｅｒｔ迭代法，在Ｐｒ＝０．７２和不同的施密特数Ｓ＿ｃ、反应阶ｎ和参数Ｐ、Ｑ下进行了数值求解。给出了相应的速度分布、温度分布和浓度分布曲线。     

层间叉排微针肋液体冷却3D-IC流动及换热特性

用数值模拟的方法,研究了散热面积为1cm2带有层间微散热结构双面均热发热3D-IC内部流体层流流动与换热,对体积流量在36~290mL/min范围内,通道高度为200μm,通道间距为200μm的带有矩形微通道和叉排微针肋液体冷却3D-IC(three-dimensional integration circuit)的流动与换热进行了分析.结果表明:带有层间叉排微针肋液体冷却3D-IC具有良好的换热效果,在热流密度为1.25MW/m2,体积流量为290mL/min时,其发热面平均温度、最大温度只有318.31,323.16K,分别最大减小了12.31,20.14K,此时的功率为250W、体积热源为8.3kW/cm3.      

Analysis of blade vibration response induced by rotating stall in axial compressor

An experimental and numerical study was conducted to investigate the forced response of blade vibration induced by rotating stall in a low speed axial compressor. Measurements have been made of the transient stalling process in a low speed axial compressor stage. The CFD study was performed using solution of 3-dimensional Navier-Stokes equations, coupled with structure finite element models for the blades to identify modal shapes and structural deformations simultaneously. Interactions between fluid and structure were managed in a coupled manner, based on the interface information exchange until convergence in each time step. Based on the rotating stall measurement data obtained from a low speed axial compressor, the blade aeroelastic response induced by the rotating stall flow field was analyzed to study the vibration characteristics and the correlation between the phenomena. With this approach,good agreement between the numerical results and the experimental data was observed. The flow phenomena were well captured, and the results indicate that the rotating field stall plays a significant role in the blade vibration and stress affected by the flow excitation.      

横流对冲击射流换热特性的影响

用实验和数值计算的方法研究了横流对单孔短距冲击换热特性的影响规律.结果表明:①在实验研究范围内,冲击靶面平均努塞尔数Nu_av,is随横流的增大而增大;②冲击靶面前区努塞尔数Nu_fia随横流的增大而减小,这是因为壁面附近x负向流动的气流流速绝对值变小,换热削弱;③靶面冲击点附近及冲击靶面后区努塞尔数Nu_bia随横流的增大而增大,原因是在冲击点上游出现的马蹄涡的旋涡方向和冲击射流自身形成的卷吸涡拉伸涡对方向相同,这两种涡的叠加使该区域冲击靶面的换热得到增强.