室温贮存对树脂粘度和加压点的影响

讨论了５４０５改性双马来酰亚胺树脂基体在室温下，贮存时间对粘度以及对固化过程中加压点的影响，给出了相应的计算方法。     

Phased array of large reflectors for deep-space communication

In this paper the problem of uplink array calibration for deep-space communication is considered. A phased array of many modest-size reflectors antennas is used to drastically improve the uplink effective isotropic radiated power of a ground station. A radar calibration procedure for the array phase distribution is presented using a number of in-orbit targets. Design of optimal orbit and the number of calibration targets is investigated for providing frequent calibration opportunities needed for compensating array elements phase center movements as the array tracks a spacecraft. Array far-field focusing based on the near-filed in-orbit (low Earth orbit (LEO)) calibration targets is also presented and array gain degradation analysis based on the position error of the array elements and in-orbit targets has been carried out. It is shown that errors in the in-orbit targets positions significantly degrade the far-field array gain while the errors in array elements positions are not very important. Analysis of phase errors caused by thermal noise, system instability, and atmospheric effects show insignificant array gain degradation by these factors     

The Pre-CME Sun

The coronal mass ejection (CME) phenomenon occurs in closed magnetic field regions on the Sun such as active regions, filament regions, transequatorial interconnection regions, and complexes involving a combination of these. This chapter describes the current knowledge on these closed field structures and how they lead to CMEs. After describing the specific magnetic structures observed in the CME source region, we compare the substructures of CMEs to what is observed before eruption. Evolution of the closed magnetic structures in response to various photospheric motions over different time scales (convection, differential rotation, meridional circulation) somehow leads to the eruption. We describe this pre-eruption evolution and attempt to link them to the observed features of CMEs. Small-scale energetic signatures in the form of electron acceleration (signified by nonthermal radio bursts at metric wavelengths) and plasma heating (observed as compact soft X-ray brightening) may be indicative of impending CMEs. We survey these pre-eruptive energy releases using observations taken before and during the eruption of several CMEs. Finally, we discuss how the observations can be converted into useful inputs to numerical models that can describe the CME initiation.     

基于Riccati方程的离散容错控制系统设计

基于离散系统的Ｒｉｃｃａｔｉ方程，提出一种对传感器失效具有完整性的离散控制系统的设计方法，给出了完整性设计方法的设计步骤，并用设计实例验证了该方法的有效性．该方法还可推广用于执行器失效的情况．     

无穷观问题的研究(Ⅲ)——‘每一''与‘所有''

本组系列论文（I）－（Ⅴ）从数学和认识论的角度系统地研究了无穷观问题的历史发展和现状，确立了无穷观背景世界的三分法原则，指出了两种穷观相互排斥的局限性，形成了统一两种无穷于同一框架中的基本观点，并建立了一个统一实无限与潜无限于同一框架中的公理集合论系统APAS。     

华东地区围护结构节能研究

根据南京市的典型年逐时气象参数，对于该市的某一座高层建筑物，应用自编的逐时动态负荷模拟程序，输入围护结构（窗户、墙体和屋顶）相关的物理参数及其与周围环境的关系（地点及朝向等），计算围护结构冬季采暖期散热量及夏季制冷得热量。结果表明，采用双层塑窗代替单层塑窗，使用节能墙体代替传统墙体能够使得冬季围护结构传散热量减少51％，夏季围护结构总得热量减少46％。因此，这一结果为华东地区建筑节能技术提供了理论依据。     

金属载体上线天线阻抗与辐射特性的矩量法研究

用线网格模拟金属载体表面，应用矩量法求出天线及载体网格上的电流分布，据此研究在该金属载体影响下的天线特性，在计算阻抗矩阵元素时，利用了非对称正弦偶极子辐射场的精确表达式，并采用了直接复数积分，简化了计算公式，本文给出了几种金属载体上线天线的阻抗与辐射特性的计算结果，它们与有关文献上的数据或实验结果一致，最后计算了一种舰船简单模型上两根线天线的远区辐射场及它们的自阻抗与互阻抗。     

铝合金薄板焊接热裂敏感性探索

探讨了用钨极氩弧焊焊接铝合金ＬＹ１２ＣＺ及ＬＹ１２Ｍ薄板时其热裂纹的变化规律，并分析了焊接工艺参数及填充材料对热裂纹的影响。试验结果表明，选择合适的工艺参数和填充材料可以明显提高该类合金的抗裂性能。     

三维CT图象自动分割法

计算机断层扫描图象（ＣＴ）和核磁共振图象（ＭＲＩ）是诊断疾病和制定治疗方案与手术方案的主要依据之一，而分割ＣＴ和ＭＲＩ图象是定量分析其平面与三维信息的关键之一。本文先采用三维自适应滤波，在保留图象细节的前提下滤除高斯分布噪声和脉冲噪声，然后根据ＣＴ或ＭＲＩ各断层多阈值二值化图象采用区域自动增长算法实现了三维ＣＴ图象和ＭＲＩ图象的自动分割。最后给出了腹部ＣＴ图象的分割结果，该方法分割精度高，速度快，具有广泛的临床应用价值     

大迎角三角翼旋涡运动及其破碎特性的数值研究

从流体力学的基本方程出发，利用Ｈａｌｌ的涡核准柱假设，导出反映涡核运动的Ｎ－Ｓ方程。采用差分方法计算旋涡流场，进而分析三角翼上前缘分离涡的运动特点及其破碎机下。从计算结果可以看出，旋涡的轴向速度向下游逐渐下降，且涡心处于降较快，外缘下降较慢，反映了粘性作用自涡心外缘逐渐下降的特点；涡核外缘的径向速度开始为负，说明开始阶段有流体流入涡核，随着旋涡向下游运动，径向速度有所增加，到一定位置后增加迅速，说