中高级教练机机务模拟训练系统研究

从教8型飞机模拟器的研制出发,讨论了其软硬件平台的构建方式.分析了模拟训练科目规划.阐述了开发理念及技术实现手段,探索了现代机务模拟训练系统的设计方向.     

On the Origin of the Strong Intermittent Nature of Interplanetary Magnetic Field

We briefly discuss the strong intermittent nature of the interplanetary magnetic field, observing that similarity between its statistical properties and the passive scalar ones exists, and may arise from different dynamical mechanisms.     

Clusters of Galaxies: Beyond the Thermal View

We present the work of an international team at the International Space Science Institute (ISSI) in Bern that worked together to review the current observational and theoretical status of the non-virialised X-ray emission components in clusters of galaxies. The subject is important for the study of large-scale hierarchical structure formation and to shed light on the “missing baryon” problem. The topics of the team work include thermal emission and absorption from the warm-hot intergalactic medium, non-thermal X-ray emission in clusters of galaxies, physical processes and chemical enrichment of this medium and clusters of galaxies, and the relationship between all these processes. One of the main goals of the team is to write and discuss a series of review papers on this subject. These reviews are intended as introductory text and reference for scientists wishing to work actively in this field. The team consists of sixteen experts in observations, theory and numerical simulations.     

击穿耐压装置容量指标

根据影响介质击穿的主要因素，着重阐述了交流击穿耐压装置的容量指标问题。如被试样件两极间的等效电容值，最大击穿电流值等。     

Shocks: Commonalities in Solar-Terrestrial Chains

Shocks are found throughout the heliosphere, wherever supersonic (or super-magnetosonic) flows encounter obstacles or other, slowly moving, media. Although some of the physical parameters are in different regimes, all shocks heat and decelerate the media incident upon them. Most shocks must propagate in a collisionless plasma, thereby adding importance to the particle interactions with the electromagnetic fields, and enabling some particles to be accelerated to high energies. This paper explores the commonalities, and differences, in shocks throughout the heliosphere, and concentrates on the role of shock microstructure in effecting the shock transition and in governing the resulting energy partition amongst the constituent species. Shocks play a significant role in the solar-terrestrial chain.     

自由空间两点目标法测量旋波媒质的电磁参数

推广自由空间两点目标法测量旋波媒质的电磁参数，通过测量由一导体球和一待测旋波媒质球组成的两点目标的后向散射场和线偏差，从而获得旋波媒质的电磁参数。该方法克服了自由空间难以准确测量相位和难以定位的缺点。数值检验表明，该方法用于旋波媒质电磁参数测量是有效的     

X射线脉冲星导航在行星际轨道上的应用

X射线脉冲星导航技术被认为是新一代导航技术,非常适合于行星际探测.深入分析了利用搜索空间方法求解飞行器真实位置和估计位置相位差的脉冲整周期模糊数,解决了相位导航方法存在的周期模糊数问题.利用轨道动力学模型估计飞行器的位置,并以真实位置和估计位置上的脉冲相位之差作为反馈进行偏差校正.仿真表明,X射线脉冲星导航方法在行星际轨道上是可行和高效的.     

基于MIMO技术的无线局域网跨层协议设计

多输入多输出(MIMO,Multiple Input Multiple Output)技术可以通过实现空分复用有效地提高无线系统的性能.提出了一个对于站点(station)和无线接入点(AP,Access Point)都装配有多天线的无线局域网的介质访问控制层(MAC,Medium Access Control)协议.此协议利用跨层优化设计的方法解决了将MIMO技术用于WLAN(Wireless Local Area Network)中存在的一些问题.例如,如何在传统的802.11协议中加入训练用的导频序列,以及如何实现数据的并行传输等等.随后,提出一个三维离散马尔可夫模型来分析此协议性能,并与理论值进行比较.最后的仿真结果说明此协议能有效的提高系统吞吐量.     

中碳回火钢疲劳小裂纹扩展微观特性的探讨

对超强钢(M4340)和中强钢(SCM435)[1]疲劳小裂纹扩展特性的分析表明,当微观结构以马氏体板条束为主,则微观结构小裂纹长度与原奥氏体晶粒或马氏体板条束尺寸都有很好的相关性,所以,减小这两种微观结构单元尺寸的冶金和热处理都可使微观结构小裂纹长度降低,从而改善材料的疲劳小裂纹扩展的抗力。     

Multi-component synchrotron self-compton emission from NGC 1275

COS-B gamma-ray data (70–5000 MeV) in the latitude range 10°< |b| <90° are compared with the expected emission from cosmic-ray interactions with interstellar gas. An additional component is found to be necessary to explain the latitude dependence of the emission. Two possible origins for this component are discussed: a gamma-ray halo around the Galaxy and a local emission region.