甲基乙烯基生胶分子量的测定方法研究

本文提出以庚烷作溶剂，用粘度法测定甲基乙烯基生胶的分子量。经试验结果表明：本法与标准法用甲苯作溶剂测得的结果相一致。本法具有溶剂毒性小、溶解性好、准确度高，操作简便等优点。     

一种多元函数的可视化方法

利用数学可视化概念和向量的正交性，本文提出了一种将多维函数在三维欧氏空间可视化的方法，旨在描述多维函数图形。本方法在多维数据图形的显示方面会有广泛的应用价值。     

干好气象观测工作之经验谈

认真负责和及时主动是干好气象观测工作的基本条件。如何提高观测技能，更好地为飞行安全服务，通过多年的工作实践，笔者积累了一些工作经验和观测体会，现呈现给大家，供共同交流和探讨。     

不同形状弹头的导弹目标雷达散射截面的计算

对处于高频区的导弹目标的电磁散射特性进行了研究分析,综合运用各种高频方法,计算了三种典型形状弹头的飞航导弹目标的雷达散射截面,并经过了文献中给出的测量结果的验证。最后,依据仿真结果对如何实现导弹目标隐身的措施进行了讨论。     

敏捷制造使能技术开发研究

探索、分析了适合我国国情的敏捷制造使能技术，提出了８ 项主要研究内容和应部署的使能技术实质性工作。     

GPS scintillation and TEC depletion near the northern crest of equatorial anomaly over South China

This study presents a statistical analysis of GPS L-band scintillation with data observed from July 2008 to March 2012 at the northern crest of equatorial anomaly stations in Guangzhou and Shenzhen of South China. The variations of the scintillation with local time, season, solar activity and duration of scintillation patches were investigated. The relationship between the scintillation and TEC depletion was also reported. Our results revealed that GPS scintillation occurred from 19:30 LT (pre-midnight) to 03:00 LT (post-midnight). During quiet solar activity years, the scintillation was only observed in pre-midnight hours of equinox months and patches durations were mostly less than 60 min. During high solar activity years, more scintillation occurred in the pre-midnight hours of equinox and winter months; and GPS scintillation started to occur in the post-midnight hours of summer and winter. The duration of scintillation patches extended to 180 min in high solar activity years. Solar activity had a larger effect to strong scintillations (S₄ > 0.6) than to weak scintillations (0.6 ? S₄ > 0.2). Strong scintillations were accompanied by TEC depletion especially in equinox months. We also discussed the relationship between TEC depletion and plasma bubble.     

The detection of “magnetic element” – Why we need a one-meter Space Solar Telescope

The nature of a magnetic element, the elemental structure of the solar magnetic field, is one of the most important mysteries in solar physics. In this paper, we will discuss the requirements of magnetic element detection, such as spatial resolution and magnetic sensitivity. By these discussions, we conclude that it is almost impossible to detect magnetic element with currently used ground-based telescopes and techniques. The proposed Space Solar Telescope, a one-meter Chinese space project, can match these requirements.     

基于简化误差修正的卫星姿态确定算法

针对典型的星敏感器/陀螺姿态卫星确定算法运算复杂这一问题,提出了一种基于简化误差修正的星敏感器/陀螺卫星姿态确定算法.通过对陀螺角速度进行简化修正,减少了滤波器的状态变量,降低滤波器的复杂性.仿真结果表明：该算法在保证姿态确定精度的条件下,能够减少运算量,提高算法的实时性.     

环境水质远程监测技术研究

在监测现场采用ADAM5510数据采集器,将PH值、溶解氧、温度和浊度等分析测试仪器的数据通过MODBUS现场总线采集并储存,主监控室通过电话线或卫星实现与各个监测现场ADAM5510数据采集器的通讯,完成各个流域不同监测端面的水质数据的记录、曲线显示、查询、报表和打印,同时,主监控室可对某些现场检测设备远程操作。     

复合材料中、长寿命区S-N曲线方程

提出一种新的基于两个假设条件下,用于复合材料层压板中、长寿命区S-N曲线构造的四参数模型。与其它方法相比,此方法不用考虑疲劳机理,只是根据疲劳试验数据,用纯数学方法来确定S-N曲线方程。算例结果表明:本文提出的方法不仅具有良好的拟合效果,而且具有较强的适用范围,因而具有潜在的工程应用价值。