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...     

带五分量抑制机构的高精度滚转力矩测量技术

滚转通道是飞行器控制的重要通道,且在试验中滚转单元受天平其它元干扰较大。为了准确测量滚转力矩,特别开发了带五分量抑制机构的高精度滚转测量技术。该技术设计原理是通过带机械深沟球轴承的抑制机构对除滚转力矩外的五个分量进行抑制。该技术一方面具有较高的滚转力矩测量灵敏度,另一方面能够有效抑制除滚转力矩外的其它五个分量,从而得到准确滚转力矩信号。     

颤振抑制中的测量点和压电驱动器的分布

对于一个具有分布式压电驱动器的模型，设计了单输入／单输出（SISO），单输入／多输出（SIMO），多输入／多输出（MIMO）颤振主动抑制控制律，并进行了风洞试验验证。在此基础上，研究了测量点和压电驱动器的分布。     

SuperDARN cross polar cap potential dependence on the solar wind conditions and comparisons with models

In this study SuperDARN Cross Polar Cap Potentials (CPCPs), collected over the year 2000, are investigated with a goal to statistically assess its relationship with various parameters of the solar wind and Interplanetary Magnetic Field (IMF). We show that SuperDARN CPCPs tend to cluster around discrete values, prescribed by the statistical model, unless the amount of points on each convection map is above ∼300. By selecting CPCP data obtained with radar coverage of >300 points, we investigate the CPCP relationship with IMF B_z and B_y, IMF clock angle, solar wind speed and dynamic pressure, Alfven velocity, Alfven–Mach number, and interplanetary electric field. Some reported tendencies, such as dependence upon IMF B_z, were found to be consistent with measurements by other instruments. We demonstrate that SuperDARN CPCPs show consistency with several theories/empirical models (predicting the CPCP) in terms of a linear trend but, on average, the slopes of the dependencies are at least two times smaller. We also determine the coupling function, out of those published in literature, best correlating with SuperDARN CPCPs.