脉冲式燃烧风洞起动特性数值研究

利用计算流体力学软件Fluent,采用隐式双时间步方法模拟非定常过程,控制方程的离散采用二阶迎风格式,湍流模型选择剪切应力输运(SST)k-ω模型,并求解组分扩散方程,对脉冲式燃烧风洞的起动过程进行了数值模拟,分析了喷管起动时流场结构的变化情况和自由射流区超声速流场的建立过程.计算结果为改进风洞起动特性提供了一定的参考依据.      

风切变对飞机平飞特性的影响分析

利用对风切变的描述,建立微下冲气流工程化模型。随后根据建立起的风切变运动方程,对飞机穿越微下冲气流风场进行仿真,分析了风切变对飞机飞行性能的影响。     

二元混压超音速进气道数值模拟与试验研究

通过多方案二元混压超音速进气道的设计分析,优选出5种方案进行了数值仿真,确定了用于试验研究的进气道方案。在此基础上,进行了1∶3缩比模型风洞吹风试验,获得了多种工况下进气道的工作特性,分析了马赫数、攻角和侧滑角等参数对进气道性能的影响。结果表明,设计分析方法可行,可用于弹用超音速进气道的设计和验证。     

大气潮汐风场诱导中纬突发E层的观测证据及理论模拟分析

统计分析了中纬突发E层的测高仪数据,给出了潮汐风场诱导Es层的观测证据,证实了大气潮汐风场和突发E层的强烈相关性.另外,依据风剪切理论,从连续性方程出发,并结合运动方程,运用特征线方法求解,模拟了Es层在潮汐风场作用下的形成.模拟结果证实了风剪切理论的合理性及潮汐风场导致突发E层形成的可能性.      

螺旋桨动力模拟试验直接影响校准与扣除

螺旋桨动力试验的目的在于获得螺旋桨滑流影响(间接影响).由于滑流影响量与直接影响量直接相关,因此在试验前应对直接影响量进行校准,在试验过程中应扣除直接影响.结合某带动力试验任务,对CARDC的4m×3m风洞带动力试验技术进行了改进,完善了单体试验(即校准试验)方法及全机试验时螺旋桨直接影响扣除方法,使试验结果更趋合理.     

Study of hot flow anomalies using Cluster multi-spacecraft measurements

Hot flow anomalies (HFAs) were first discovered in the early 1980s at the bow shock of the Earth. In the 1990s these features were studied, observed and simulated very intensively and many new missions (Cluster, THEMIS, Cassini and Venus Express) focused the attention to this phenomenon again. Many basic features and the HFA formation mechanism were clarified observationally and using hybrid simulation techniques. We described previous observational, theoretical and simulation results in the research field of HFAs. We introduced HFA observations performed at the Earth, Mars, Venus and Saturn in this paper. We share different observation results of space mission to give an overview to the reader.     

国外火星飞机及火星风洞研究

在简述火星与地球大气飞行环境差异的基础上,分析研究了火星飞机主要布局特征和动力推进问题;阐述了国外开展火星飞机研究发展的地面模拟设备--火星风洞的情况,意在跟踪国外新技术走向,为国内航空航天未来发展提供参考.     

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.     

复杂群塔风荷载试验研究

介绍了一复杂群塔结构节段刚性测压试验概况和主要试验结果,讨论了结构典型部位风压分布的基本特征和结构风压分布的基本规律.试验结果表明,由于该结构由多个单体高耸塔结构组成,相互干扰严重,风压的分布相当复杂.根据风压试验结果得到了风力沿各塔高度的分布,并讨论了分布规律,进一步得出基底剪力系数和基底弯矩系数,分析了最危险风向,给出了用于结构设计的荷载建议.     

A Review of Density Holes Upstream of Earth's Bow Shock

Larmor size transient structures with density depletions as large as 99% of ambient solar wind density levels occur commonly upstream of Earth＇s collisionless bow shock. These ＂density holes＂ have a me...