A preliminary Chandra X-ray spectroscopy of the supernova remnant N132D

We present the preliminary results of a Chandra X-ray study of N132D, a young shell-like supernova remnant (SNR) in the Large Magellanic Cloud. The equivalent width maps of emissions from O, Ne, Mg, Si, and S are provided. Spatially resolved spectral analysis for the small-scale regions were tentatively performed. X-ray spectra of the interior can be described with a single-thermal model. The faint interior regions have lower density, higher temperature above 1 keV than that of bright interior regions. The X-ray spectra along the shell can be phenomenally fitted with either a double-vpshock model or a vpshock + powerlaw model. If the non-thermal component is true, N132D would be listed as another X-ray synchrotron SNR.     

等效地球半径法应用中的问题

为阐明等效地球半径法应用的范围和应用中应该注意的问题,从等效地球半径法的定义推导了等效地球半径模型与实际地球模型之间量的映射关系.给出并证明了等效过程中等效地球半径模型与实际地球模型下的射线高度、仰角、长度相等,而地心角在转换过程中约为3/4的映射关系.讨论了需要利用地心角映射关系进行计算时的两种情况,同时给出计算结果和误差分析.     

SSRT: First results of millisecond spike observations

We present the results of the first observations of spike-like phenomena with the Siberian Solar Radio Telescope (SSRT) in the one-dimensional mode at the frequency of 5.7 GHz with high spatial and temporal resolutions.     

柔性空间结构的分散模糊变结构控制

提出了一种适用于一类不确定大系统的分散变结构控制方法 ,并将该方法用于柔性空间结构的控制系统设计中。考虑到复杂大系统的系统关联及不确定因素复杂 ,在控制律中引入了模糊控制规则来确定分散控制律中的非线性分量大小 ,使控制系统设计时不需知道系统不确定变化及关联的具体情况 ,简化了控制器的设计。同时 ,模糊控制规则的引入还有效减弱了一般分散变结构控制系统的抖颤问题。所设计的控制系统可以保证柔性空间结构系统在未知参数摄动以及外界干扰情况下的稳定。数字仿真结果表明该方法的有效性。     

空间望远镜的热设计和热光学分析综述

文章对国内外典型空间望远镜的热设计进行综述 ,并详细介绍了空间望远镜热光学分析的概念 ,讨论了热设计和热光学分析的关系 ,提出了将卫星热控制技术与光学波像差理论相结合 ,以光学指标作为热设计的最终评价标准 ,并应用于我国空间太阳望远镜(SST)的热设计和热光学分析之中     

大型飞机研制中的若干数字化智能装配技术

大型飞机的研制是国家提高自主创新能力的战略重点.为了提高大飞机装配质量与生产效率,采用数字化智能装配技术是必然的发展趋势.本文介绍了飞机智能化装配的系统框架与其技术体系架构,阐述了目前大型飞机装配所面临的难题,并指出虚拟现实仿真优化技术、专用智能装配工艺装备的开发,以及飞机总装智能装配生产线技术是智能装配技术的热点与发展方向,并分别进行了介绍,并阐述了国内外应用发展现状,最后指出了国内现有智能装配技术的不足与差距.     

极区F层不规则结构的分形模型

本文利用1986年9—12月期间17个电离层吸收事件的Riometer资料计算了电离层闪烁强度的Fourier谱和Bessel谱。求出了谱遵从的k~(-β)型函数的β值,1.8<β<2.5,平均为2.1;求出了不规则结构的漂移速度平均为129m/s。计算了各个事件的闪烁指数S_4<0.4。求出相位涨落空间谱,且指出其也遵从幂型函数k~(-α)规律。根据上述结果,本文提出极区F层不规则结构为分立的分形,不是分立的“斑块”。利用β值求出分形的分数维D=2.45。给出了不规则结构的近似分形模型。     

Evolution of an electron beam pulse influenced by coulomb collision effects in the solar corona

Electrons accelerated in the corona during solar activity give rise to radio emission events that can be observed over a wide range of frequencies. Among different finer-scale structures in the dynamic spectra observed in the radio range, fast transients with extents of some milliseconds known as solar radio spikes are observed accompaning the background continuum emission. Fundamental to the generation of radio spikes is a propagating electron beam and following its evolution allows us to understand the physical processes occurring in the solar corona. With the use of a numerical Fokker–Planck code we follow a previous numerical study to simulate the propagation of an electron beam pulse injected in a small region at the top of a magnetic field and outwards the solar corona under typical flare conditions. It was found that in large ambient densities of ${10}^{10}$ cm⁻³ at the injection point, Coulomb collision effects have an important effect on the propagation of the electrons, causing that the injected electrons thermalize faster in a time of $0.1$ and $0.4$ s for an electron distribution with a low-energy cut off of 16 and 7 keV respectively and a spectral index of 3. For a tenous ambient medium of density ${10}^9$ cm⁻³ thermalization occurs only for an electron distribution with smaller low-energy cut off (7 keV) with a duration of $\approx$1.5 s, while for a larger low-energy cut off (16 keV) the loss of accelerated electrons is very slow, regardles of the spectral index ($3,7$). The electron loss time by Coulomb collisions, which depends on the low boundary ambient density, might be an important parameter that influences the generation of radio spikes due to the formation of instabilities in the corona.     

0.5—1.5GHz快速射电频谱仪研究中的几个科学问题

本文介绍了０．５－１．５ＧＨｚ频段上的研究课题和技术方案，主要科学目标是：粒子加速过程及加速区位置的研究；小惊讶磁流力管的振荡；射电爆发精细结构和ＨＸＲ事件的相关性研究等。     

分布传递函数方法的梁杆几何非线性分析

本文提出了一种基于动坐标的、适用于梁大变形分析的传递函数方法，在本方法中，一个复杂系统被分为若干一维子系统，各子系统根据梁的有限变形理论进行推导，推导中把轴力看作子系统的参数，引入状态向量后，可以将子系统的控制方程改写为含参状态空间的形式，然后利用传递函数方法求解，系统的合成借鉴了有限元的处理方法，引入了动坐标关系，使方法可以用于对大变形的分析。文后给出了算例表明本文方法有很高的精度和很好的收敛性。