Pc5 Oscillation Analysis by the Satellite and Ground-Based Data

Large amplitude Pc5 event was observed in the space and on ground on August 3, 2001, about three hours after contact of the strong discontinuity in the solar wind with the magnetosphere according to data from ACE and Wind satellites. The Pc5 amplitude was as high as 15 nT in the tail of magnetosphere and about 5 nT at the ground based stations. In the magnetosphere Pc5 waves were observed by Cluster and Polar satellites, which occupied positions in the morning part of the near tail at the close field lines but were parted by distance of 11.5 Re, mainly along the x-axis of the GSM coordinate system. Both compressional and transverse components of the Pc5 wave activity were observed in the space, with the transverse component having the larger amplitude. Time delay between the Cluster and Polar satellites was about 8 minutes, which could be interpreted as a wave propagation from the geomagnetic tail to the Earth with the 150 km/s group velocity. The ground-based Pc5 activity was analysed by using data from the Image magnetometer network. Doubtless demonstrations of a field line resonant structure were found in variations of amplitude and polarization with latitude. Finnish chain of search coil magnetometers observed modulated Pc1 emission simultaneously with the Pc5 wave train. A possibility of non-linear impact of Pc5 wave energy on the plasma and waves in the magnetosphere is discussed.     

A Method of Inversing the Peak Density of Atomic Oxygen Vertical Distribution in the MLT Region From the OI (557.7nm) Night Airglow Intensity

In this paper, using the MSISE-90 model as the reference atmosphere, we discuss the feasibility and method of deducing the peak densities of the undisturbed atomic oxygen profiles in the MLT region (the mesosphere and lower thermosphere region) from OI (557.7 nm) night airglow intersities. The peak densities for different seasons, latitudes and longitudes are deduced from OI (557.7nm) airglow intensities through this expression. We analyze the features of inversion relative errors and discuss the influence of the variations in temperature on inversion errors. The results indicate that all inversion errors are less than 5% except for those at high altitudes in the summer hemisphere. And the impact of the variations in temperature on errors is not significant.      

行星际磁场的螺旋扇形过渡区

从行星际磁场的大尺度螺旋形构型和扇形边界附近太阳风流动与冕旒的可能相关,本文得到一个推论,即在行星际空间可能存在一种较厚的螺旋扇形过渡区。行星际磁场和太阳风的实地观测证实了这种较厚的螺旋扇形过渡区的存在。在所分析的45个螺旋扇形过渡区中,磁场强度都不为零;大部分大于或小于周围平均场强。本文进一步分析了磁增大和磁减小两类过渡区中的物理性质和可能成因。      

Science Missions Using CubeSats

As the role of missions and experiments carried out in outer space becomes more and more essential in our understanding of many earthly problems, such as resource management, environmental problems, and disaster management, as well as space science questions, thanks to their lower cost and faster development process CubeSats can benefit humanity and therefore, young scientists and engineers have been motivated to research and develop new CubeSat missions. Not very long after their inception, CubeSats have evolved to become accepted platforms for scientific and commercial applications. The last couple of years showed that they are a feasible tool for conducting scientific experiments, not only in the Earth orbit but also in the interplanetary space. For many countries, a CubeSat mission could prompt the community and young teams around the world to build the national capacity to launch and operate national space missions. This paper presents an overview of the key scientific and engineering gateways opened up to the younger scientific community by the advent and adaptation of new technology into CubeSat missions. The role of cooperation and the opportunities for capacity-building and education are also explored. Thus, the present article also aims to provide useful recommendations to scientists, early-career researchers, engineers, students, and anyone who intends to explore the potential and opportunities offered by CubeSats and CubeSats-based missions.      

密封件的技术发展趋势

在飞机设计中,尽管密封件是一个"小部件",但它却发挥着非常重要的作用。从未来的发展趋势来看,密封件的发展必须要跟得上飞机或发动机对于温度、压力、转速等环境条件的设计要求,具备在翼寿命更长、密封性能更好等特性。     

航天飞机指控中心Unix工作站中专家系统的实时数据获取

最具代表性的美国技术杰作之一可能是位于德克萨斯州休斯顿的约翰逊航天中心的航天指挥控制中心(MCC)。该中心各指挥室经历了美国技术史上许多重大事件,如首次登月、营救天空实验室以及首次发射航天飞机。60年代初MCC首次启用时,的确是技术杰作。然而该设施自阿波罗任务后只进行过不大的改进。直到最近,它仍然维持着以单主机的结构,     

电离层对GPS相对大地测量的影响

本文分析了对 GPS 相对大地测量有重要影响的电离层误差特性。电离层误差、星历预报误差和对流层延迟误差是影响 GPS 测地精度的三个主要误差源。借助高精度数字式 GPS 接收机(如 T14100GPS 导航接收机),星历估计和预报技术在日益改善。现在正在研究精确的对流层延迟修正技术,例如使用便携式水汽辐射计测量大气中水汽含量对 GPS 信号延迟的影响。为了获得相应的 GPS 测地精度还必须重视电离层误差的修正。本文讨论了三维基线精度,它随电离层条件、电离层修正精度、基线间隔、定向和事后处理方法而变化,给出了使用 T14100GPS 导航接收机和德克萨斯仪器公司 Geomark 事后处理软件包的实际测量结果。     

压力浸渍过程中P-55纤维和铝合金界面反应的控制

 压力浸渍法是制造金属基复合材料方便而廉价的方法。在这种工艺过程中,能独立控制纤维预制件温度T_p、熔融金属温度T_m、浸渍压力P和冷却速度等重要工艺参数。在金属基复合材料中,纤维与基体间的界面反应使纤维强度下降,复合材料性能恶化,从而限制了复合材料的广泛使用。本文主要研究如何控制无涂层的P-55纤维与1100Al和Al-0.34％Ti合金之间的界面反应,讨论压力浸渍法工艺参数对P55/Al和P55/Al-Ti复合材料组织、性能的影响。结果表明:通过控制工艺参数来缩短纤维与熔融金属铝之间的接触时间和在基体中加入钛元素以降低碳在熔融铝中的活性可以制造出高性能的复合材料。     

单元数字化机载雷达的自适应杂波对消

本文描述了用于大型单元数字化阵列雷达（EDAR）的多层自适应波束形成方法。各阵列单元的距离相关增益自适应（RDGA）提供了有效的杂波对消。机载截击（AI）雷达的模拟试验验证了这种方法的效率，并说明了它相对于阵列中随机相位误差和幅度误差的稳定性。