波状扰动激发的重力波波包在中层大气中能量传播和转换特性的数值研究

采用谱配置方法对具有高斯分布的波状扰动激发重力波过程中的能量传播和转换特性进行数值研究．模拟结果表明：初始时刻单一的水平风、垂直风、密度或温度的波状扰动都可以激发出两支重力波波包，其中一文向上传播，而另一支则向下传播；在相同的波参数下，4种波状扰动所激发的重力波波包的能量传播路径几乎完全一致，与线性理论给出的射线路径却有些差异．进一步的数值分析则表明：4种波状扰动转化为波动的特征时间基本相等，约为2个波动周期，但是在这个转换过程中，不同扰动的能量转换效率却差别很大．     

三维空间双机格斗的捕捉区和危险区

 本文应用微分对策理论对三维空间双机格斗问题进行研究,给出了以目标机进入方向、界栅和等时线组成的捕捉区与危险区的确定方法,画出二架飞机的捕捉区和危险区,并讨论了这些区域的性质,得出与实际空战相符的结论。     

DQPSK数传接收机

重点介绍用于航天测控系统的 DQPSK数传接收机的主要技术问题及解决途径 ;应用超大规模集成电路芯片进行 QPSK信号调制解调、解调控制、差分编码和差分解码等     

IP网络设备典型故障分析及其对策

针对IP网络设备在使用过程中产生的广播风暴、传输数据丢包、MP-group(Multilink-group,复用链路组)接口链路层运行PPP(Point to Point Protocol,点对点协议)异常等问题,结合华为S9300交换机设备、NE40E路由器设备的工作原理,对策略路由机理、STP(Spanning Tree Protocol生成树协议)、广播数据帧复制过程进行了研究和分析。并通过分析问题产生的机理,发现了目前网络数据配置存在的不足,提出了在核心层交换机上配置流过滤策略等应对措施和快速处理故障的方法,对系统进行了完善与改进,并优化了相关领域的应用,为维护人员在任务中迅速、合理地实施应急处置提供了参考。     

IPX实时通信软件的设计与实现

分析了基于IPX(Internetwork Packet eXchange)协议的实时通信编程原理,讨论了针对某网络所开发的实时通信软件IPXSR的设计思想、特点、实现技术和调用方法.目前该软件已经通过了验收和鉴定,在实际系统中得到应用,效果良好.并能够方便地移植到其他的物理网络系统中,具有较大的实用价值.      

使用复小波包的MIMO-OFDM无线系统

为了在频率选择性信道中提供高速数据业务, 提出了一种新的多入多出-正交频分复用系统MIMO-OFDM(Multi-Input Multi-Output -Orthogonal Frequency Division Multiplexing).该系统使用复小波包变换CWPT(Complex Wavelet Packet Transform)来实现OFDM,而不是使用传统的快速傅立叶变换FFT(Fast Fourier Transform).由于复小波包函数具有很好的特性,通过对有2个用户的MIMO-OFDM系统进行仿真的结果表明,基于CWPT的MIMO-OFDM系统性能要比使用传统的FFT的MIMO-OFDM 系统好,但是复杂度略高.      

一种卫星数管中心计算机软件的工程实现

文章主要针对一种卫星数管中心计算机的软件需求,进行了操作系统和应用软件的设计和实现,并在数管分系统内部联试及与其它分系统接口匹配试验中对设计进行了验证。在软件的设计中,借鉴了空间数据系统咨询委员会的航天器星载接口业务(SOIS)和欧洲航天局的包应用标准(PUS),有助于软件的构件化和产品化。     

The investigation of powerful solar flares characteristics by analysis of excited states of C and various neutrons capture lines

Accelerated energetic particles in solar flares produced nuclear γ-lines in interactions with ambient solar atmosphere. Analysis of intensity of ratios between various γ-lines allows us to make estimations of abundance of elements, parameters of surrounding media and other solar characteristics. In this article we discuss the flux ratio between two lines from excited states of ¹²C (f_15.11/f_4.44) and our results of preliminary calculation of intensity ratio between two neutron capture lines at ³He and ¹H (f_20.58/f_2.223). In particular we consider the opportunity to obtain n(³He)/n(¹H) ratio during solar flares and using high-energy gamma-emission studying, based on the satellite data. Possible interpretation of spectral features observed during the January 20, 2005 solar flare is discussed. Preliminary analysis of energy spectrum in the band of 2–21 MeV gives n(³He)/n(¹H) ∼ 8 × 10⁻⁴ for January 20, 2005 solar flare.     

Resonant motion, ballistic escape, and their applications in astrodynamics

A special set of solutions governing the motion of a particle, subject to the gravitational attractions of the Earth, the Moon, and, eventually, the Sun, is discussed in this paper. These solutions, called resonant orbits, correspond to a special motion where the particle is in resonance with the Moon. For a restricted set of initial conditions the particle performs a resonance transition in the vicinity of the Moon. In this paper, the nature of the resonance transition is investigated under the perspective of the dynamical system theory and the energy approach. In particular, using a new definition of weak stability boundary, we show that the resonance transition mechanism is strictly related to the concept of weak capture. This is shown through a carefully computed set of Poincaré surfaces, at different energy levels, on which both the weak stability boundary and the resonant orbits are represented. It is numerically demonstrated that resonance transitioning orbits pass through the weak stability boundaries. In the second part of the paper the solar perturbation is taken into account, and the motion of the resonant orbits is studied within a four-body dynamics. We show that, for a wide class of initial conditions, the particle escapes from the Earth–Moon system and targets an heliocentric orbit. This is a free ejection called a ballistic escape. Astrodynamical applications are discussed.     

一种多热力循环组合发动机进气道设计方案

针对马赫数0~6的预冷涡轮+冲压组合多热力循环发动机的宽范围工作要求，提出了一种在马赫数2~6范围内流量系数为1.0的宽范围轴对称进气道变几何调节方案，通过中心锥与分流板的协同平移运动，可在满足涡轮与冲压两通道流量分配要求的同时，实现两通道压缩量的匹配调节。对起始半锥角分别为20°和13°的两种变几何进气道方案开展了设计与对比研究。结果表明：起始半锥角对最终方案设计影响最大，起始半锥角为13°的进气道方案较起始半锥角为20°的方案，冲压通道和涡轮通道在来流马赫数为6时临界总压恢复分别提高了16%和14%，最大迎风面积减小了12.4%，但中心锥和分流板平移调节距离分别增加84%和91%。