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.     

AN ELEMENTARY ANALYSIS OF PROBLEMS IN APPLICATION OF SPACE METHOD IN STRATEGIC MANAGEMENT OF ENTERPRISES

企业战略管理在我国还是一门新兴学科，随着改革发展的深入，越来越多的企业已认识到它的重要性，并最终采用它。本文论述了在企业战略管理ＳＰＡＣＥ方法中，如何应用Ｄｅｌｐｈｉ方法确定企业战略要素及评价。而它的确定及评价，真实刻划了企业在目前竞争环境中所处的战略位置，为企业正确选择发展战略奠定了基础。     

月球着陆探测器发动机推力线测量及标定

月球着陆探测器发动机推力线测量及标定是发动机装配与调整的关键环节.通过创建精测镜坐标系,实现发动机在对接面坐标系中的推力线平行量与偏斜的转换,得到热试车后标定推力线的方法.通过发动机热试车后数据分析,推力线测量及标定方法满足技术条件要求.     

Constraints on Coronal Outflow Velocities Derived from UVCS Doppler Dimming Measurements and in-Situ Charge State Data

We constrain coronal outflow velocity solutions, resolved along the line-of-sight, by using Doppler dimming models of H I Lyman alpha and O VI 1032/1037 Å emissivities obtained with data from the Ultraviolet Coronagraph Spectrometer (UVCS) on SOHO. The local emissivities, from heliocentric heights of 1.5 to 3.0 solar radii, were determined from 3-D reconstructions of line-of-sight intensities obtained during the first Whole Sun Month Campaign (10 August to 8 September 1996). The models use electron densities derived from polarized brightness measurements made with the visible light coronagraphs on UVCS and LASCO, supplemented with data from Mark III at NCAR/MLSO. Electron temperature profiles are derived from 'freezing-in' temperatures obtained from an analysis of charge state data from SWICS/Ulysses. The work concentrates on neutral hydrogen outflow velocities which depend on modeling the absolute coronal H I Lyα emissivities. We use an iterative method to determine the neutral hydrogen outflow velocity with consistent values for the electron temperatures derived from a freezing-in model.     

有向图的矩阵表示

本文用定义的方式对有向图中相邻矩阵的概念在含有平行边和自回路两种情形上做了推广，建立了方和有向图之间的一一对应关系。     

STA5型用户板软件的设计

STA5型用户板用于数字程控交换机的用户接口 ,也可做为各类接入网系统的远端二线模拟接口。本文对该用户板软件设计难点、特点 ,以及软件的组成部分做以阐述。     

宽带有线接入技术探讨

本文针对基于双绞线的ADSL技术、HFC网的Cable Modem技术、五类线的以太网技术以及光纤接入技术等方面，详细地解析了宽带有线接入网技术。此外，从网络模型的不同层次出发，探讨了宽带有线接入网技术的发展趋势。     

方形同轴线色散特性的研究

文章研究了一种横截面为方形结构的同轴线，采用有限差分原理^[1]分析方同轴线中TM波的两个最低模式的色散特性及横截面电磁场分布的问题，理论分析了该模式下的色散方程；利用Matlab编程得到方同轴线中TM波的两个最低模式的色散曲线，然后利用CST模拟了该结构的场分布^[2]和色散曲线；将CST仿真结果与理论数值模拟结果进行比较，二者的结果基本一致。     

吸气式脉冲爆震发动机壁温试验

为了探索各频率下管壁温度随时间的变化趋势及爆震管外壁面的温度分布规律,对爆震室内径68mm,长2 000mm,以汽油为燃料、空气为氧化剂的吸气式脉冲爆震发动机进行试验,用热成像仪对稳定工作在10Hz,20Hz,40Hz下的管壁温度进行了监测。结果表明:同一频率下随时间的增加壁面温度增加速度减小;热平衡时壁面温度随频率的增加而增长,10Hz,20Hz,40Hz热平衡时外壁面最高温度分别在726℃,1011.5℃,1159.5℃以上;热平衡前管壁温度的增长速度随频率的增加而增加,管壁温度的增长速度跟频率约成正比;爆震室上沿着压缩波叠加至形成爆震的方向,温度在外壁面上递增分布,在爆震形成区温度最高,从爆震形成区到发动机出口处,温度在外壁面上逐渐降低;各频率下最高温度区位置基本不变,距点火位置1 350mm左右;同一轴向位置上的外壁面温度随频率的增加而增加,温度的增长幅度随频率的增加而减小。     

一起TCAS干扰所致电子设备通风系统故障分析

针对一起电子设备通风系统故障进行了深入分析,在排故过程中发现其原因是导航系统的TCAS计算机干扰所致,这种非相关系统的关联故障在航线维护中较为罕见。