冲压发动机突扩燃烧室内标量输运的大涡模拟

为弄清突扩燃烧室内标量输运机理，采用大涡模拟方法数值模拟了几何结构简化的冲压发动机突扩燃烧室内湍流流动中燃料浓度以及温度等标量的扩散和输运过程。研究了大尺度涡结构随时间在空间的演化过程，给出了燃料浓度和温度场的瞬时空间分布。研究表明燃料的扩散特征直接决定于大涡结构，大涡结构也强烈的影响温度的输运过程。该研究结果为冲压发动机突扩燃烧室设计和改进燃烧状况提供了细观依据。     

支线飞机的非常规/常规融合布局研究

为了在支线飞机设计中利用非常规布局的优势提高其性能,同时避免其所带来的问题,提出基于飞翼的非常规/常规融合布局。首先介绍运输类飞机非常规气动布局飞翼的突出优势和面临的问题,然后提出非常规/常规融合布局,最后通过设计方案的逐步迭代改进和优化,得到气动性能优于新一代支线飞机的非常规/常规融合外形布局方案,其中巡航升阻比提高了约7.5%、阻力发散马赫数提高了约2.5%、巡航效率因子提高了约7.5%,同时确保了飞机具有良好的机场适应性。基于飞翼的非常规/常规融合布局方案具有进一步提升性能的潜力,同时避免飞翼的其他一些不利方面,为未来非常规布局运输飞机的研究奠定一定的基础。     

The Cold-Dense Plasma Sheet: A Geotail Perspective

GEOTAIL observations of the low-latitude boundary layer (LLBL) in the tail-flanks show that they are the region where the cold-dense plasma appears with stagnant flow signatures accompanied by bi-directional thermal electrons (< 300 eV). It is concluded from these facts that the tail-LLBL is the site of capturing the cold-dense plasma of the magnetosheath origin on to the closed field lines of the magnetosphere. There are also cases that strongly suggest that the cold-dense plasma entry from the flanks can be significant to fill a substantial part of the magnetotail. In such cases, the cold-dense plasma is not spatially restricted to a layer attached to the magnetopause (that is, the LLBL), but continues to well inside the magnetotail, constituting the cold-dense plasma sheet. Inspired by the fact that these remarkable cases are found for northward interplanetary magnetic field (IMF), a statistical study on the status of the near-Earth plasma sheet is made. The results show that the plasma sheet becomes significantly colder and denser when the northward IMF continues than during southward IMF periods, and that the cold-dense status appears most prominently near the dawn and dusk flanks. These are consistent with the idea that, during northward IMF periods, the supply of cold-dense ions to the near-Earth tail from the flanks dominates over the hot-tenuous ions transported from the distant tail.     

运输类飞机的机身抗烧穿性适航要求解析

运输类飞机可生存坠撞后的火灾是客舱安全范畴内的重要问题之一.提高机身抗烧穿性,即推迟火焰进入客舱的时间,可为乘员应急撤离提供时间保证.介绍了运输类飞机坠撞后的池火火焰特征,包括最高温度、热流密度等特征的范围及其影响因素,重点论述了机身结构烧穿过程,剖析了适航规章中的抗烧穿符合性判据,梳理了抗烧穿性试验方法的发展过程,最后对我国未来运输类飞机机身抗烧穿研究的发展进行了展望.     

固体火箭发动机真实流体输运系数的自动模拟

为缩短固体火箭发动机的研究周期、降低研究成本和揭示工作机理,需要对其工作过程进行三维数值仿真,但数值计算中许多物性参数如输运系数的确定存在困难,为此主要研究了适合于固体火箭发动机内高温高压下的多组分混合物输运系数的计算方法,并通过高级计算机语言管理数据库等方法实现自动计算,可准确快速地计算发动机内流过程中输运系数的变化,为真实模拟发动机的工作过程提供正确的物性参数。     

Challenges to cosmic ray modeling: From beyond the solar wind termination shock

Voyager 1 crossed the solar wind termination shock on December 16, 2004 at a distance of 94 AU from the Sun, to become the first spacecraft to explore the termination shock region and to enter the heliosheath, the final heliospheric frontier. By the end of 2006, Voyager 1 will be at ∼101 AU, with Voyager 2 at ∼81 AU and still approaching the termination shock. Both spacecraft have been observing the modulation of galactic and anomalous cosmic rays since their launch in 1977. The recent observations close to or inside the heliosheath have provided several interesting ‘surprises’ with subsequent theoretical and modeling challenges. Examples are: what does the modulation of galactic cosmic rays amount to in this region?; how do the anomalous cosmic rays get accelerated and modulated?; why are there ‘breaks’ in the power-law slopes of the spectra of accelerated particles? Several numerical models have been applied to most of these topics over the years and comprehensive global predictions have been made the past decade, thought to be based on reasonable assumptions about the termination shock and the heliosheath. Examples of these predictions and assumptions are concisely discussed within the context of the main observed features of cosmic rays in the vicinity of the termination shock, ending with a discussion of some of the issues and challenges to cosmic ray modeling in particular.     

Four Contemporary Issues Concerning Ionospheric Plasma Flow to the Magnetosphere

Space Science Reviews - In this review, we examine four specific questions/issues of contemporary interest within the overall topic of ionospheric plasma outflow into the magnetosphere. These four...     

高纬极区离子速度分布函数多项式解及非相干散射谱计算

为更准确描述高纬极区电离层离子分布函数, 分别采用弛豫碰撞模型和麦克斯韦分子碰撞模型描述玻耳兹曼方程的碰撞项, 通过求解两种模型下的输运方程, 分别得到两种模型基于麦克斯韦分布下离子分布函数的13矩近似和基于双麦克斯韦分布下离子分布函数的16矩近似. 进一步根据Sheffield理论, 利用两种模型下离子分布函数的13矩和16矩近似, 计算了非相干散射谱, 并对结果进行对比分析. 结果表明, 相对于弛豫碰撞模型, 麦克斯韦分子碰撞模型能更好地描述电离层E层中离子与中性成分的相互作用. 相对于离子分布函数的13矩近似, 16矩近似更适合描述由于电场增加导致的离子温度各向异性特征.      

麦克斯韦分子碰撞下的离子分布函数及其非相干散射谱的计算

采用麦克斯韦分子碰撞模型描述玻耳兹曼方程的碰撞项, 基于双麦克斯韦分布函数得到的输运方程包含了粘滞和热流的影响, 通过求解输运方程得到了离子漂移速度, 平行和垂直磁场的离子温度, 应力张量以及平行和垂直能量的热流矢量的表达式. 进而得到了麦克斯韦分子碰撞模型下离子分布函数的16矩近似. 利用非相干散射理论, 计算得到了非相干散射谱. 相对于简单的驰豫碰撞模型, 麦克斯韦分子碰撞模型能更准确地描述非麦克斯韦分布的电离层E 层的碰撞过程.      

CCSDS SCPS网络层与传输层协议分析与仿真验证

空间数据系统咨询委员会(CCSDS)针对空间通信的特点制定了空间通信协议标准SCPS(Space Communications Protocal Specification)。文章从CCSDS标准在中国空间技术的实际应用出发,对CCSDS SCPS协议中网络层协议(NP)和传输层协议(TP)进行研究,分析其特点和适用性,并与TCP/IP协议进行对比,最后设计演示验证系统对所提方案进行验证并得出结论:在空间通信环境下,采用SCPS协议后的性能优于采用TCP/IP协议。