密集型空气雾化流场破碎特征数学模型研究

低速液体射流在高速湍流气体作用下的气液同轴射流雾化流场是瞬态密集型喷雾场,高速湍流中影响和控制雾化的因素很多。针对空气雾化流场液核分布与特征进行分析,开发了模拟液核的随机浸入体模型,结合大涡模拟方法对同轴射流空气雾化喷嘴下游流场进行数值模拟。模拟结果与实验结果对比表明：随机浸入体模型可快速捕捉液核的长度和位置信息。当气液动量比M为3~10000时,能够较准确地预测液核长度,当M>10时,其预测结果远优于唯象模型;该模型能够捕捉回流区、大尺度涡等流场结构。同时,可以准确地预测喷嘴附近的液滴粒径,特别是在气流速度较大（>60m/s）时,液滴平均直径预测误差<10%。     

特种加工技术在某新型微叠层复合材料中的应用

目前航空航天领域采用的微叠层复合材料主要集中在Fe、Ni、Ti和Al的合金或金属间化合物上。这类金属的金属间化合物具有熔点高、密度低、热导率好及抗高温性能好等优点,可被用作航空飞行器或航空发动机的高温结构材料。但是这类金属间化合物具有其本征脆性,导致其室温下的断裂韧性很差,因而应用受到限制。为解决这一问题,采用特种加工技术制备出具备微叠层结构的金属/金属间化合物复合材料是理想的手段之一。     

Observations of Magnetic Reconnection in the Magnetotail Associated With Substorms

Magnetic reconnection is one of the most important, dynamic phenomena in the magnetotail in terms of magnetic field line configuration change and energy release. It is believed to occur in the distant magnetotail mainly during southward interplanetary magnetic field periods and in the near-Earth magnetotail in association with substorms. In the present paper, we discuss several important issues concerning magnetic reconnection in the magnetotail associated with substorms, such as reconnection signatures, location, timing, spatial scale, and behavior, from the macroscopic, observational point of view.      

Computational aerodynamic analysis on perimeter reinforced （PR）-compliant wing

Abstract Implementing the morphing technique on a micro air vehicle （MAV） wing is a very chal- lenging task, due to the MAWs wing size limitation and the complex morphing mechanism. As a result, understanding aerodynamic characteristics and flow configurations, subject to wing structure deformation of a morphing wing MAV has remained obstructed. Thus, this paper presents the investigation of structural deformation, aerodynamics performance and flow formation on a pro- posed twist morphing MAV wing design named perimeter reinforced （PR）-compliant wing. The numerical simulation of two-way fluid structure interaction （FSI） investigation consist of a quasi- static aeroelastic structural analysis coupled with 3D incompressible Reynolds-averaged Navier- Stokes and shear-stress-transport （RANS-SST） solver utilized throughout this study. Verification of numerical method on a rigid rectangular wing achieves a good correlation with available exper- imental results. A comparative aeroelastic study between PR-compliant to PR and rigid wing per- formance is organized to elucidate the morphing wing performances. Structural deformation results show that PR-compliant wing is able to alter the wing＇s geometric twist characteristic, which has directly influenced both the overall aerodynamic performance and flow structure behavior. Despite the superior lift performance result, PR-compliant wing also suffers from massive drag penalty, which has consequently affected the wing efficiency in general. Based on vortices investigation, the results reveal the connection between these aerodynamic performances with vortices formation on PR-comoliant wing.     

边界层对可调节进气道性能的影响

给出了马赫数2-6、单位雷诺数（0．8-6．0）×10^7／m时下吹式风洞中可调节三维进气道的试验研究结果。研究了前缘前掠和后掠方案以及进气道人口前边界层的影响。测量了内流道内的压力分布、质量流量和总压恢复系数;确定了进气道启动与马赫数和流动工况的关系。研究结果表明：边界层对流场结构和模型进气道的性能有着决定性影响,相对简单的进气道调节方案可以增大其稳定运行范围。     

Alfvn Waves in the Solar Wind

Alfvn waves are found to be ubiquitous in the solar wind.Recent progress in observational studies of the waves is reviewed to formulate a microscopic picture for the Alfvenic fluctuations. The main aspects of the observational properties of these waves,including the wave intervals, propagation,evolution,origin and generation,are presented.Then Alfven wave heating and acceleration of the solar wind plasma are briefly introduced.The relation of the waves to rotational and tangential discontinuities,magnetic decreases,and other relatively large-scale structures such as flux tubes/ropes,magnetic clouds and interplanetary coronal mass ejections in the solar wind is particularly investigated.Finally,some remaining open questions are also indicated due to their fundamental importance of understanding of the physical nature of Alfven waves and the role of the waves in heating and accelerating the solar wind.     

DIRECT NUMERICAL SIMULATIONS OF MULTIPHASE FLOWS

INTRODUCTIONMultiphase and multifluid flows are commonin many natural and technologically importantprocesses. Rain,spray combustion,spray paint-ing,and boiling heat transfer are just a few ex-amples.While it is the overall,integral charac-teristics of such flows that are of most interest,the global behavior is determined to a large de-gree by the evolution of the smallestscales in theflow.The combustion of sprays,for example,depends on the size and the number density ofthe drops.Generally…     

PARAMETRIC OPTIMIZATION AND STRUCTURAL DESIGN OF NLS

INTRODUCTIONIn general,nitrogen launching system[1,2 ] iscomprised of nitrogen cylinder,launching mecha-nism,framework and electrical system,withcompressed Nitrogen as launching energy re-sources.A physical and mathematical model isdeveloped for describing the relations betweenthe detached time and the force,volume,pres-sure,flow,displacement,velocity,acceleration ofnitrogen cylinder and launching mechanism.Thekey technique of NL S is to control detached pa-rameters by changing the press…     

液氧/液氢高压膨胀循环发动机初步试验

膨胀循环具有很好的性能和很高的可靠性,这一点已由普拉特·惠特尼公司的“半人马座”上面级推进系统RL10发动机证实,但是这种循环对燃烧室压力增加和推力增加都有限制作用,因为它仅仅利用了燃料在冷却燃烧室和喷管延伸段时吸收的热能,来推进燃料和氧化剂涡轮泵.建议采用具有内部热交换器的先进方案燃烧室,这种热交换器可以收集许多燃烧热量.叙述使用内部热交换器的高压膨胀循环发动机的主要性能,并给出了这种发动机的初步试验结果.热交换器中的平均热通量是Bartz相关计算值的70%.燃烧性能不会因装了内部热交换器而受到严重影响.     

固体推进剂的非线性结构模型

在大多数固体推进剂特性的线性和非线性理论中,一个主要的缺陷在于忽略了内部损伤。对于那些已引出损伤参数的非线性理论,数值常数与推进剂的物理性质无关。而且,这些理论具有如此复杂的性质以至于要完成一个庞大的实验测试程序。已经提出了一个表示固体推进剂性质的简单方法。这个方法以一个基本定律为基础,该定律用一个应力衰减函数修正粘弹表达式。根据单轴试验数据,可用衰减函数表示推进剂的非线性性质。在卸载期损伤的表达式中,这个方法比过去的方法显示出重大的改进。分别定义松弛和再加载为过去最大应力的正态函数。利用这种方法对复杂的过程进行了预测,而且实测应力与预测应力很接近。