Fabrication and Investigation on Double-Hollow Shell CoFe Oxide@TiO2 Nanocube with Superior Electromagnetic Properties

Electromagnetic wave absorbing materials are urgently required in the fields of medicine, communication, and military. However, the thickness, weight, narrow effective bandwidth, and weak absorbing ability of the materials restrict their further application. In this work, a double-layer hollow nanocube with a dielectric titanium dioxide (TiO2) shell and a magnetic CoFe oxide inner shell is prepared. Prussian blue (PB) is prepared by the hydrothermal method, and used as the template to prepare PB@CoFe PB analogue (PBA). After selective etching and further calcination, hollow CoFe oxide particles are obtained. The obtained particles are then coated with SiO2 and TiO2, respectively, and the intermediate layer is dislodged to obtain the final CoFe oxide@TiO2 with the hollow double shell structure. The obtained double-layer hollow structure can effectively capture the incident electromagnetic waves, and increase the propagation path. Moreover, the obvious enhancement of interface polarization and the improvement of impedance matching enhance the wave absorbing ability of the material. The analysis results show that, the structure is stable and the dispersion is good. The maximum reflection loss (RL) at 10 GHz is as high as -46.1 dB with the sample thickness of 1.6 mm. The light-weight and high-efficiency CoFe oxide@TiO2 absorber is promised to be used in commercial and military aerospace fields.     

星载主动遥感气溶胶-云参数技术需求与进展

面对越来越迫切的气象和气候预测及大气环境监测需求,利用主动星载仪器在全球范围内探测云和气溶胶参数成为快速发展的研究领域。相比被动遥感仪器,主动仪器可以获取云和气溶胶参数的垂直分布信息,这将在天气气候模式的改进方面发挥重要作用。通过云和气溶胶遥感需求分析,从雷达数据应用角度,首先介绍了数值模式对云和气溶胶的科学参数需求和定量需求,进一步分析了云和气溶胶联合观测的需求,以及星载微波激光雷达的探测特点;然后对国内外正在规划的星载云和气溶胶微波激光雷达探测任务进行了综述,包括仪器指标和数据产品设计;最后展望这一领域的应用前景。     

E-弹-大规模电性毁伤武器

高功率电磁脉冲和高功率微波产生技术已经逐渐成熟,常规E-弹的发展允许其在非核条件下使用,E-弹在战略和战术信息战上的应用,其在技术上已成熟。文中讨论了E-弹的相关的技术原理和投射技术,并提出了E-炸弹和战斗部应用的领域和依据。     

某型机燃烧室外套爆破故障剖析和安全使用寿命评估

针对某型机燃烧室外套发生的空中爆破故障 ,进行应力分析、断裂机理分析、爆破时剩余材样的板厚分析计算及不同焊接试片疲劳对比试验等 ,确定了故障发生的原因为原设计的纵向搭接焊缝不合理 ,不适于在交变载荷作用下使用。参照英军标Defstan 0 0 -971上轮盘的寿命评估方法 ,按疲劳寿命对数正态分布规律和搭接焊试片疲劳试验结果选定了外套的寿命散度系数 ,并把使用多年的外套都看成试验件 ,评估出了现役外套的安全使用寿命和失效概率     

单层均匀吸波材料电磁参数的匹配研究

用Steffensen加速法求出了单层均匀吸波材料对入射电磁波无限吸收时电磁参数所需满足的必要条件及其边界曲线 ,同时 ,通过数值模拟得到了吸波材料无限吸收时电磁参数边界曲线的数值模拟等式和有限吸收时宽带吸波材料电磁参数的匹配规律和频散特性     

射频识别技术在仓储物流系统中的应用

射频识别技术在仓储物流系统中的应用,能记录从生产、配送到仓储管理的全过程,能进行成批的读写操作.文中通过介绍射频识别技术,及其相关硬件设备电子标签和读写器的组成和工作原理,分析出射频识别技术在仓储物流系统中应用的方法和工作流程,并给出应用这一技术的仓储物流管理系统的组装、工作流程图和实验模型图.同时简要介绍了选用美国德州仪器生产的最新一代射频系列＂Tag-it＂的优势.     

Transient Effects and Disturbed Conditions

In the present phase of the solar cycle no big transients leading to strong modulation had been observed after 1991. Apart from a few minor disturbances cosmic rays were still recovering to a new intensity maximum. It was suggested, therefore, that existing literature from previous cycles should be critically reviewed. The scene was set by the introductory papers on— phenomenology of cosmic ray modulation in successive solar cycles throughout the heliosphere— the present state of models for long term modulation and their shortcomings— the relation between cosmic ray variations and the magnitude of the interplanetary magnetic field (the CR-B-relation)— charge dependent effects.In the discussions, the study of propagating diffusive disturbances and the CR-B-relation played a central role. The difference was stressed between isolated transient disturbances in the inner solar system (Forbush decreases), and the long lasting, step-like decreases caused by merged interaction regions in the outer heliosphere. The recovery rates following the step-like decreases vary with the phase in the 22-year solar cycle. In some cases this requires a modification of existing drift models. In the outer heliosphere, the CR-B-relation leads to the result 1/ between the diffusion coefficient and the field magnitude . This simple result is a challenge for theoreticians to derive the perpendicular diffusion coefficient fromfirst principles. The three articles in this report essentially follow the list of open points and arguments just presented.The article "Observations and Simple Models" is organised around the model of a propagating diffusive barrier, its application to Forbush effects in the inner heliosphere and to decreases caused by merged interaction regions in the outer heliosphere. Acomparison of observed Forbush decreases with model predictions requires a careful separation of the two steps related to the turbulent region behind the shock front and the closed magnetic field regions of the ejecta (the interplanetary counterparts of coronal mass ejections). It is shown that models for propagating disturbances can be used to derive values of the diffusion coefficients phenomenologically, not only during the disturbance, but also in the ambient medium.The "Modeling of Merged Interaction Regions" summarizes the dynamic and time-dependent process of cosmic ray modulation in the heliosphere. Numerical models with only a time-dependent neutral sheet prove to be successful when moderate to low solar activity occurs but fail to describe large and discrete steps in modulated cosmic rays when solar activity is high. To explain this feature of heliospheric modulation, the concept of global merged interaction regions is required. The com-bination of gradient, curvature and neutral sheet drifts with these global merged interaction regions has so far been the most successful approach in explaining the 11-year and 22-year cycles in the long-term modulation of cosmic rays.The "Remarks on the Diffusion Tensor in the Heliosphere" describe available theories of perpen-dicular diffusion and drift, and discuss their relevance to cosmic rays in the heliosphere. In addition, the information about diffusion coefficients and spatial gradients obtained from the analysis of steady state anisotropies at neutron monitor energies is summarized. These topics are intimately related to the other two articles. They are also part of the general discussion about the "Diffusion Tensor throughout the Heliosphere" which played an important role in all working groups.     

The Solar Wind - Inner Heliosphere

The solar wind in the inner heliosphere, inside ~ 5 AU, has been almost fully characterized by the addition of the high heliographic latitude Ulysses mission to the many low latitude inner heliosphere missions that preceded it. The two major omissions are the high latitude solar wind at solar maximum, which will be measured during the second Ulysses polar passages, and the solar wind near the Sun, which could be analyzed by a Solar Probe mission. Here, existing knowledge of the global solar wind in the inner heliosphere is summarized in the context of the new results from Ulysses.     

Fractionation of SI, NE, and MG Isotopes in the Solar Wind as Measured by Soho/Celias/MTOF

Using the high-resolution mass spectrometer CELIAS/MTOF on board SOHO we have measured the solar wind isotope abundance ratios of Si, Ne, and Mg and their variations in different solar wind regimes with bulk velocities ranging from 330 km/s to 650 km/s. Data indicate a small systematic depletion of the heavier isotopes in the slow solar wind on the order of (1.4±1.3)% per amu (2σ-error) compared to their abundances in the fast solar wind from coronal holes. These variations in the solar wind isotopic composition represent a pure mass-dependent effect because the different isotopes of an element pass the inner corona with the same charge state distribution. The influence of particle mass on the acceleration of minor solar wind ions is discussed in the context of theoretical models and recent optical observations with other SOHO instruments. This revised version was published online in June 2006 with corrections to the Cover Date.     

无线电引信延迟时间的确定

简要介绍了无线电引信延迟时间的作用,提出了几种确定延迟时间的方法,通过对无线电引信延迟时间的计算,得出确定最佳延迟时间的方法。