抗辐照通用扩展SiP芯片设计

研究微小卫星综合电子系统的SiP技术实现方法。首先介绍微小卫星综合电子系统结构的组成和采用SiP技术的必要性，然后对综合电子系统进行功能模块划分，并对其通用扩展模块进行详细的SiP设计，包括抗辐照器件选型、原型验证、SiP原理图、基板管壳一体化设计、建模仿真、制造加工、实装测试验证等，通过SiP技术实现了一种星载综合电子系统中通用扩展SiP芯片产品，经过实际验证测试，在保证模块功能和性能的前提下，整体模块重量从230 g减轻到48 g，体积由180 mm?130 mm?17 mm减小到46 mm?46 mm?8 mm，很好地满足了星载功能模块小型化、轻量化设计需求。     

关于一维非定常气─固二相流特征理论的讨论

本文研究了一维非定常气－团二相流的特征，对于目前常用的、包含一定近似的运动方程组，它有两个虚部很小的复根，研究表明这种很小的虚部出现与方程中引入的近似有关。从十多个算例的结果看，这样的虚部不影响人们在工程计算中用该方程组求解初值问题。针对具有上述特征的气－团二相流方程组，本文发展了一种类特征线方法，它保留了双曲型方程特征线方法的若干优点，但它允许方程的特征根中有微小的虚部。含灰气体激波管流动的计算表明，类特征线法具有精度高、数值耗散和弥散小等优点     

薄膜充气管充气展开特性试验

用展开导轨消除因重力产生的摩擦力,在不同充气速率与初始展开角条件下对薄膜材料充气管的充气展开特性进行了试验研究,获得了展开角,以及展开加速度和内气压的变化规律。试验及分析结果表明:充气管的充气膨胀与展开相互独立,充气膨胀过程近似为等压增容过程,折叠部位的气压变化特性与整体气压变化特性差异明显。     

吸尘器弯管连接头模具的设计

分析了吸尘器弯管连接头的结构特点,着重阐述了应用于本模具中的一种新颖的专用来解决大角度,长距离抽芯的连杆机构的工作原理。对模具设计过程中遇到的困难,如:小嵌件如何固定,很小的侧型芯如何固定于侧滑块上,及三个液压缸按顺序抽芯,圆弧型芯如何插入圆柱型芯2中等都作了详细的叙述与探讨。另外本论文还涉及到了主要成型零部件的加工问题。     

Solar and Heliospheric Modulation of Galactic Cosmic Rays

The significance of external influences on the environment of Earth and its atmosphere has become evident during recent years. Especially, on time scales of several hundred years, the cosmogenic isotope concentration during the Wolf-, Spoerer-, Maunder- and Dalton-Minimum indicates an increased cosmic ray flux. Because these grand minima of solar activity coincide with cold periods, a correlation of the Earth climate with the cosmic ray intensities is plausible. Any quantitative study of the effects of energetic particles on the atmosphere and environment of the Earth must address their transport to Earth and their interactions with the Earth’s atmosphere including their filtering by the terrestrial magnetosphere. The first problem is one of the fundamental problems in modern cosmic ray astrophysics, and corresponding studies began in the 1960s based on Parker’s cosmic ray modulation theory taking into account diffusion, convection, adiabatic deceleration, and (later) the drift of energetic particles in the global heliospheric magnetic field. It is well established that all of these processes determining the modulation of cosmic rays are depending on parameters that are varying with the solar magnetic cycle. Therefore, the galactic cosmic ray intensities close to Earth is the result of a complex modulation of the interstellar galactic spectrum within the heliosphere. The modern view of this cosmic ray modulation is summarized in our contribution.     

Measuring the matter distribution within z = 0.2 cluster lenses with XMM-Newton

We present an analysis of seven clusters observed by XMM-Newton as part of our survey of 17 most X-ray luminous clusters of galaxies at z  0.2 selected for a comprehensive and unbiased study of the mass distribution in massive clusters. Using the public software FTOOLS and XMMSAS we have set up an automated pipeline to reduce the EPIC MOS and pn spectro-imaging data, optimized for extended sources analysis. We also developped a code to perform intensive spectral and imaging analysis particularly focussing on proper background estimate and removal. XMM-Newton deep spectro-imaging of these clusters allowed us to fit a standard β-model to their gas emission profiles as well as a standard MEKAL emission model to their extracted spectra, and test their inferred characteristics against already calibrated relations.     

Late Stages of Stellar Evolution

A large fraction of ISO observing time was used to study the late stages of stellar evolution. Many molecular and solid state features, including crystalline silicates and the rotational lines of water vapour, were detected for the first time in the spectra of (post-)Asymptotic Giant Branch (AGB) stars. Their analysis has greatly improved our knowledge of stellar atmospheres and circumstellar environments. A surprising number of objects, particularly young planetary nebulae with Wolf-Rayet (WR) central stars, were found to exhibit emission features in their ISO spectra that are characteristic of both oxygen-rich and carbon-rich dust species, while far-IR observations of the PDR around NGC 7027 led to the first detections of the rotational line spectra of CH and CH⁺. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

全天球实时恒星模拟器技术

阐述了研制全天球实时恒星模拟器的意义以及国内外发展趋势,介绍第二代恒星模拟器的系统组成、特点、技术指标以及解决的技术问题。     

复合材料层板中就位横向拉伸强度的研究

本文利用弹性力学和断裂力学方法对纤维增强复合材料的横向拉伸强度进行了分析，其中考虑了９０度开裂层厚度和开裂邻层的约束效应的影响，推导出正交各向异性对称铺层中昨合就位横向拉伸强度的数学表达式，得出开裂层的厚度和约束邻层铺设角对就位横向拉伸强度都有影响的结论，理论计算与Ｆｌａｇｇｓ实验结果吻合较好。     

关于危险品运输的紧急救援

危险品运输是技术要求最高的一类特种货物运输。在运输、装卸及贮存保管过程中,稍有不慎便会发生事故,造成人身伤亡和财产毁损。笔者认为:灾害=事故十损失。严格执行危险品运输规章,减少事故发生率,从技术上进行要求。仅是问题的一个方面。而另一方面还应立足于事故发生后的紧急救援,以最大限度地减少损失,两者并重才不致酿成灾害。为此,提出了建立“危险品运输紧急救援中心”的建议。