Last FY-2 Series Satellite Successfully Launched on A LM-3A

正A LM-3A launch vehicle lifted off from the Xichang Satellite Launch Center at21:07 Beijing time on June 5,launching the FY-2H satellite into orbit.This was the 277th flight mission of the LM family launch vehicle.FY-2H was the last flight unit of the     

双模块下颌式内转进气道/圆锥前体一体化布局研究

为实现三维内转进气道的内收缩流场与圆锥前体的外压缩流场的良好匹配，提出了一种双模块下颌式内转进气道/圆锥前体(Double-modules Chin Inward-turning Inlet and Conical Forebody，DCII/CF)一体化设计方法，获得一种新颖的双发并置、侧向安装的DCII/CF一体化布局。针对该布局形式，开展了DCII/CF一体化构型与传统的单模块内转进气道/圆锥前体(Single-module Inward-turning Inlet and Conical Forebody，SII/CF)一体化构型的数值对比研究。结果表明：DCII/CF一体化布局不仅为内转进气道提供了优秀的前体附面层排移效果，还有效避免了传统SII/CF布局中前体附面层与进气道内部流场之间的相互干扰。在Ma∞=6.0设计状态，DCII/CF一体化布局的进气道总压恢复系数相较传统的SII/CF布局有了显著提高，从0.403提高至0.482；但由于前体附面层的排移，该布局的捕获流量略有降低， SII/CF的流量系数为0.956，该布局则为0.917。而在非设计状态，该布局形式同样具备较好的总压恢复性能，在Ma∞=5.0与Ma∞=4.0的总压恢复系数分别达到了0.586和0.682，明显高于SII/CF的总压恢复系数0.507和0.619。     

电铸镍Wolter I型光学系统制造技术发展综述

摘要： 为满足未来脉冲星导航和空间天文观测任务对X射线望远镜的载荷需求，Wolter I光学系统的研制正逐渐成为新的研究热点，电铸镍方案是当前国内外X射线光学系统镜筒制造的主要技术方案.文章对电铸镍X射线光学系统制造工艺、国内外研制现状、未来应用需求进行了介绍和整理，梳理了电铸镍X射线光学系统研制遇到的关键技术和难点，提出了后续研究发展建议，以促进中国在 X射线脉冲星自主导航、空间探测领域的快速发展.     

面向学生的智能解题专家系统的研究与设计

探讨了网络在专家系统中的应用 ,给出了一个基于网络的面向学生的智能解题专家系统的模型 ,分析了设计的基本过程。从专家系统出发 ,探讨了基于知识的推理系统。最后 ,从以上设计出发 ,总结了基于该模型的系统需进一步研究的工作。     

基于C167CS和MAS3507＋DAC3550解码器的音频播放器设计

多媒体播放器市场的快速发展为低成本的DSP/MCU混合器件的应用提供了发展的良机.本文分析了Infineon(SIEMENS)C167CS的结构,提出了Infineon(SIEMENS)C167CS单片机和MAS3507 DAC3550解码器开发的MP3播放器的方案,采用了自顶向下的设计方法对总体设计方案、硬件各个组成部分(播放器的硬件解码技术、数模转换的控制技术)和软件进行了分析和设计.全部程序用Keil公司的C编译器和链接器编译通过并运行良好,该系统具有实现简单,成本低,运行效率高,功能强大等优点,有很好的发展前途.     

rom 15 sel

with primary goat embryonic fibroblast showed no difference from traditional feederlayer-based culture method used in mouse and human. The putative primary EG colonies were multilayer clumps ofcompact cel     

利用热源温度场迭加法诊断持续点热源的强度及位置

可重复使用运载器的防热瓦故障会使航天器的局部结构产牛热源，并在结构中形成温度场。应用热源温度场迭加法的解函数，解得结构温度历程，然后据此温度的变化率趋势判断出热源位置，在此基础上依据多点测最值构造出辨识参数用于热强度识别，通过对一薄壁结构模型算例的计算仿真，证明了本文所提方法的有效性。论文工作为进一步开展热源诊断技术研究，提供了可资工程实践应用的数值算法体系以及有益的数值计算结论。     

计算机帧时间对半实物仿真的影响

半实物仿真试验中,要求计算机帧时间与计算积分步长相一致,但在实际试验中不容易精确地做到。本文分析了这种不一致给半实物仿真试验带来的影响,给出了解决的办法,文章中还给出了一实例来说明。     

Field formation around negatively biased solar arrays in the LEO-plasma

Heavy emission caused by impacting plasma ions results in a fast discharging effect of the initially large surface potentials on the dielectric solar cells. This eventually counteracts the energization process of the plasma ions to the cover glasses and leaves no significant electric fields. Thus, with an existing thermal plasma, electrons are again able to reach dielectric surfaces. Strong localized electric fields of the order of several 10 kV/cm form near the interconnector-cover glass interface.     

EUV emission from normal galaxies

Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band.