基于背景纹影技术的随机介质折射率场测量

针对光线通过复杂流场时产生的光传输效应问题,提出了基于背景纹影技术的复杂折射率场测量方法,给出了根据粒子图像偏移量求解折射率场分布的计算方法和推导过程,并对该方法的分辨率与灵敏度进行了理论分析。在此基础上,对火焰上方折射率场的分布进行了实验测量,利用粒子图像测量(PIV)技术对实验图像进行处理。结果表明:实验测量得到的空气折射率最大值为100029,最小值为100009,测量有效值小于00001。表明该方法具有较高的测量精度,能够有效实现复杂折射率场的实时精确测量。      

卫星遥测功率谱分析和调制度测量方法研究

残余载波调制是卫星测控中的常用调制体制。文章从理论上给出了该体制下信号的功率谱密度表达式,得到奇次谐波谱线展宽等结论,并通过仿真和实验进行了验证。利用所得结论讨论了遥测调制度测量方法,提出通过功率谱的2阶边带进行测量可以使结果得到改善。     

微阴极真空电弧点火起弧及加速机理研究综述

微阴极真空电弧推力器具有结构简单、重量轻、功耗低、比冲高等优点,因而在航天推进领域有着广阔应用前景.当前推力器设计研制、可靠性和寿命的提高等方面遇到的一些关键问题均与微阴极真空电弧放电过程的基本物理问题密切相关.对微阴极电弧推力器运行中涉及的电子发射、电极间起弧过程、阴极斑点形成及特点、烧蚀和形貌变化、电极间等离子体射...     

AIRCRAFT CONCEPT EVALUATION AND EFFECTIVENESS-BASED DECISION-MAKING

Based on effectiveness analysis, a novel method is presented for combat aircraft top-hierarchy concept evaluation and decision-making. Applying multi-criterion decision-making （MCDM） and analytic hierarchy process, the new method can help to overcome the limitations of existing evaluation systems and decision-make methods. The proposed method includes the following process~ （1） Establish a multi-criterion and multi-hierarchy evaluation attribute system by introducing combat effectiveness~ （2） Assign weight to the attributes and normalize them; （3） Evaluate and decision-make top-hierarchy aircraft concept based on effectiveness to reach a satisfactory design by comprehensively applying four multi-criterion decision-making methodologies, i.e. grey correlation pro- jection method, weighted summation method, weighted quadrature method and ideal solution decision-making method, while considering the attribute hierarchy system and the logical relations among the attributes. Finally, an example is given to indicate the validity and feasibility of the proposed method.     

多孔介质隔热材料中的辐射热传递分析

新型的多孔材料以其重量轻、强度高备受航天工程设计人员的亲睐,尤其是作为隔热材料使用,可以说是航天工程热防护系统的热门材料.多孔介质在辐射热传递方面具有吸收发射和散射的功能,这些功能在其接受外来热流的作用下,于内部达到热能量平衡,求解这一平衡方程就可以求出辐射热流在材料中的分布.由于求解这一方程的困难,许多学者对材料特性...     

XMM-Newton study of soft excess X-ray emission in clusters of galaxies

We discuss the detection of soft excess X-ray emission in a sample of 19 clusters of galaxies observed by XMM-Newton. In 6/19 clusters evidence for a soft X-ray excess is found. Four of these clusters show soft X-ray and O VII line emission from gas with a temperature of 0.2 keV. The centroid of this oxygen line is consistent with the redshift of the cluster. The intensity and spatial extend of the soft excess agrees with previous PSPC measurements. These observations are interpreted as emission from warm-hot intergalactic medium filaments, with density enhancements near the cluster centers, consistent with theoretical predictions. In the other two soft excess clusters a non-thermal origin is consistent with the data.     

左、右手媒质间电磁传输特性的对比分析

文章通过重新表述折射率，对比分析了左、右手媒质不同组合情况下，电磁波在媒质界面上的折射特性。通过引入色散关系的时域有限差分法对无限大左手介质板以及线源置于左手媒质覆层内两种模型进行了模拟，模拟结果与分析相符合。分析表明，负折射现象出现在界面两侧媒质类型（LHM／RHM或RHM／LHM）不同的情况下。对于同种类型媒质的情况，左手媒质并不能引起反常的折射现象。LHM引起的反常现象通过与RHM的对比才能得以有效考察。     

Cosmic ray acceleration by supernova shocks

We analyse the results of recent measurements of nonthermal emission from individual supernova remnants (SNRs) and their correspondence to the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is shown that the theory fits these data in a satisfactory way and provides the strong evidences for the efficient CR production in SNRs accompanied by significant magnetic field amplification. Magnetic field amplification leads to considerable increase of CR maximum energy so that the spectrum of CRs accelerated in SNRs is consistent with the requirements for the formation of Galactic CR spectrum up to the energy ∼10¹⁷ eV.     

基于主成分的编队级网络对抗效能评估指标体系

分析建立编队级网络对抗评估指标体系的原则,用主成分分析法对指标进行处理,求得7个主成分.根据正交原则将20个指标分配到7个主成分中,赋予每个主成分以实际含义,最终建立了编队级网络对抗效能评估指标体系.     

XMM-Newton survey of non-thermal shell candidates: Preliminary results on DA 530

The investigation of the general properties of non-thermal (NT) X-ray shell supernova remnants (SNRs), of which SN 1006 is the prototype, is important to understand how electrons are accelerated in SNR shocks and what is the origin of cosmic rays. Using the XMM-Newton satellite, we are carrying on a survey of putative non-thermal SNR candidates previously unknown or little studied in the X-ray band, in order to investigate the different manifestations of NT emission in SNR shells. The SNRs we have selected are likely to expand in a low density medium, and therefore to have a low thermal X-ray emission, that usually outshines the non-thermal one. We report here preliminary results obtained on the SNR shell DA 530.