Determination of Angular Distribution Models for Indian desert scene: Comparison with other desert models

In this paper, the shortwave and longwave anisotropy for clear sky Indian desert scene has been estimated using long-term surface data, radiative transfer calculations and Helmholtz reciprocity for missing values. This study is important in the perspective of the low inclination satellites like Megha–Tropiques (MT) mission, carrying Scanner for Radiation Budget (ScaRaB) payload, which will provide broadband radiative fluxes at the top of the atmosphere (TOA). Due to low inclination angle, the angular models for clear sky land scenes for the MT-ScaRaB orbits will be dominated by desert points.The Angular Distribution Models (ADMs) determined in this study were compared with existing desert models. It is observed that for longwave radiation, the largest disagreement is observed for higher values of viewing zenith angle, especially for the summer season, where the difference in flux can reach up to 13 W/m². For the shortwave radiation, higher values of both solar zenith angle and viewing zenith angle cause largest incongruity in the computed albedo from the different models, suggesting the need of caution in interpretation of the flux computations from these bins. In fact at the higher solar zenith angle bin, the disparity in albedo can go up to 6.4%.     

High energy charged particle experiment – A payload proposal to KuaFu-B mission

High Energy Charged Particle Experiment (HECPE) is to measure the fluxes of MeV electrons and tens of MeV protons. The two satellites of KuaFu-B are in the same polar orbit with apogee 7.0R_E, perigee 1.8R_E. They can sweep large L values and pass through the inner and outer radiation belts. The high energy electrons and protons in the radiation belts are principal sources for failures of satellites and spacecrafts in the Earth orbits. The enhancements of the high energy electrons and protons, so-called energetic particle events, are important phenomena of the Space Weather. The energy ranges monitored by HECPE are 0.3–0.5 MeV, 0.5–1.0 MeV, 1.0–2.0 MeV, and E > 2.0 MeV for electrons, 5–10 MeV, 10–20 MeV, 20–40 MeV, and 40–80 MeV for protons.     

电磁屏蔽材料的研究进展

阐述了研究电磁屏蔽材料的重要性。综述了表层导电型、填充复合型、本征型导电高分子、导电织物、透明导电薄膜等电磁屏蔽材料的性能及特点,简要阐述了电磁屏蔽材料的发展趋势。     

SRAM型FPGA单粒子效应试验研究

针对军品级SRAM型FPGA的单粒子效应特性,文中采用重离子加速设备,对Xilinx公司Virtex-II系列可重复编程FPGA中一百万门的XQ2V1000进行辐射试验。试验中,被测FPGA单粒子翻转采用了静态与动态两种测试方式。并且通过单粒子功能中断的测试,研究了基于重配置的单粒子效应减缓方法。试验发现被测FPGA对单粒子翻转与功能中断都较为敏感,但是在注入粒子LET值达到42MeV·cm 2/mg时仍然对单粒子锁定免疫。本文对翻转敏感度、测试方法与减缓技术进行了讨论,试验结果说明SRAM型FPGA对单粒子效应比较敏感,利用重配置技术的减缓方法能够有效降低敏感度,实现空间应用。
     

飞机铆接构件PRFECT探头的线圈夹角影响

远场涡流检测技术不受集肤效应影响,对金属铆接构件隐藏缺陷检测具有巨大优势。针对飞机金属铆接构件的远场涡流检测,建立了铆接构件隐藏缺陷检测三维模型,分析不同屏蔽阻尼材料及组合方式的屏蔽性能,采用激励线圈与检测线圈均环绕铆钉旋转的检测方法,对比激励线圈-铆钉-检测线圈夹角为90°、135°和180°时缺陷检测灵敏度,研究不同缺陷尺寸检测信号特征。仿真与试验结果表明：当屏蔽阻尼为铝+铜时具有最佳屏蔽性能,且远场区距离激励线圈中心最近;当激励线圈和检测线圈间距为30 mm时,激励线圈-铆钉-检测线圈夹角为180°时检测效果最佳;优化后的探头可检测埋深为6 mm、长×宽×深尺寸为5 mm×0.2 mm×1 mm的铆接构件隐藏缺陷,缺陷信号幅值与其体积当量关系相对应,且随缺陷长度及深度的增加呈上升趋势。     

Enhanced electromagnetic-interference shielding effectiveness and mechanical strength of Co-Ni coated aramid-carbon blended fabric

An efficient method was proposed to prepare high-performance conductive Aramid-Carbon Blend Fabrics (ACBF) with cobalt–nickel (Co-Ni) alloy coatings, which is conducive to industrial production. The grid-like substrate composed of aramid and carbon fibers was innovatively used in flexible Electromagnetic Interference (EMI) shielding materials. The natural network structure is advantageous to the uniform deposition of metal particles to the establishment of conductive pathways subsequently in order to improve conductivity. The induction of a synergistic effect from Electromagnetic (EM) wave-reflection and EM wave-absorption through the whole carbon-Co-Ni-ternary system notably enhanced the EMI Shielding Effectiveness (SE) value to an average of 42.57 dB in the range of 30–6000 MHz. On the other hand, together with the inherent toughness of the alloy coatings, the tensile strength of the aramid fibers used for bulletproof made a significant contribution to the desired mechanical properties. The light weight of the resultant composite made it applicable to aerospace vehicles simultaneously. X-ray Photoelectron Spectroscopy (XPS) was conducted to investigate the variations of elements and groups on the sample surface in pre-treating process. The elemental components and surface morphologies of fabric samples during different stages of the process were investigated by Scanning Electron Microscope (SEM) and Energy Dispersive spectrometer (EDX) measurements. X-Ray Diffraction (XRD) results indicated that the obtained Co-Ni alloy coating had a combined Hexagonal Closed-Packed (HCP) and Faced-Centered Cubic (FCC) crystalline phase. The relatively high corrosion resistance demonstrated in different acid and alkaline conditions was instrumental in more complex environments as well.     

磁场敏感度（EMS）自动测试系统

介绍一种磁场敏感度自动测试系统,该系统可检验电子仪器对磁场的敏感程度。可按国家标准GB6833.2～87和国家军用标准GJB151-86、GJB152-86进行测试,还可根据用户的需要产生更强的磁场。着重介绍该系统主要技术性能指标、工作原理、结构设计、软件设计和误差分析,并且与国外的测试系统进行了比较。     

Measured properties of the cosmic background radiation

After a pioneering period when the observers were mainly interested in checking the general properties of the Cosmic Background Radiation through observations at still higher frequencies, the observational efforts are now devoted to the discovery of features in the mean panorama, in particular :i) Distortions in the frequency spectrum, ii) Spatial anisotropies at various angular scales; iii) Polarization. The observational information is reviewed.     

屏蔽材料对木星轨道卫星内部介质充电效应的影响研究

在木星轨道的空间辐射环境中,占主导地位的粒子是能量大于1 MeV(甚至高于100 MeV)的高能电子,这可能会产生卫星内部介质充电效应.在卫星的防辐射设计中,通常需要一定厚度的材料来屏蔽这些电子,使得进入卫星内部的电子通量达到安全的水平.利用所建立的GEANT4-RIC(radiation induced conduc...