Research on navigation of satellite constellation based on an asynchronous observation model using X-ray pulsar

Pulsar navigation is a promising navigation method for high-altitude orbit space tasks or deep space exploration. At present, an important reason for restricting the development of pulsar navigation is that navigation accuracy is not high due to the slow update of the measurements. In order to improve the accuracy of pulsar navigation, an asynchronous observation model which can improve the update rate of the measurements is proposed on the basis of satellite constellation which has a broad space for development because of its visibility and reliability. The simulation results show that the asynchronous observation model improves the positioning accuracy by 31.48% and velocity accuracy by 24.75% than that of the synchronous observation model. With the new Doppler effects compensation method in the asynchronous observation model proposed in this paper, the positioning accuracy is improved by 32.27%, and the velocity accuracy is improved by 34.07% than that of the traditional method. The simulation results show that without considering the clock error will result in a filtering divergence.     

Earthshine and Asteroseismology Telescope (East) Network

Several automated optical telescopes have been setup at appropriate longitudes around the globe to study earthshine variations and asteroseismology. The first telescope has been setup at Teide Observatory, Tenerife, Spain in October 2004. The intensity of earthshine relates to the average of Earth’s albedo, and in turn relates to the global temperature of the Earth. A global network is necessary because each site can measure the earthshine reflected from only a part of the Earth. The network will also be used for asteroseismology study. It can measure photometric variations of pulsating stars. The long-term and continuous measurements allow the accurate determination of mode frequencies of stellar pulsations, which provides information on the properties of stellar interior.     

三角面元灰度图象三维重建算法研究

三角面元SFS算法是结合三角面元模型和线性反射图来阐述SFS问题的,该算法的基本思想是用三角面元素来近似光滑表面,并用一系列基于节点的线性方程组合来表达该表面。本文在此算法的基础上,求解时通过加权平均迭代,提高了恢复的准确性和迭代的收敛速度。     

硼酸盐玻璃中稀土离子的发光研究

应用荧光光谱、红外振动光谱等研究了在可见光区发光的Ｐｒ（３＋），Ｓｍ（３＋），Ｅｕ（３＋），Ｔｂ（３＋），Ｄｙ（３＋），Ｅｒ（３＋）和Ｔｍ（３＋）等镧系稀土离子在硼酸盐玻璃中的发光行为，系统地分析了稀土离子在硼酸盐玻璃基质中的激发谱和发光谱特性。     

国外航天侦察相机和测绘相机发展概况

航天侦察和测绘是战略武装必不可少的组成部分,航天侦察和测绘相机是对地观测卫星的有效载荷。 该文将简要介绍国外航天侦察和测绘相机发展概况、水平和发展趋势。     

太空中相继升起近80颗中国的人造地球卫星——庆贺中国航天事业创建50周年

回顾了中国自主发展人造地球卫星的历程,以此庆贺中国航天事业创建50周年。     

我国农村义务教育财政专项投资若干问题探析

2006年开始的农村义务教育经费保障机制改革已经在全国全面铺开,自此,我国农村义务教育财政性经费第一次真正地被纳入公共财政的框架。而在这次改革中,财政专项投资发挥了非同寻常的作用,成为财政投入的主体形式。从义务教育财政专项投资的概念、现状和特点出发,解析农村义务教育经费保障机制改革条件下财政专项投资的资金安排、运营、支付和监管等若干问题,并对专项投资的功效和创新做出理论性的初探。     

子母弹分离过程的数值模拟方法

以分区拼接网格数值模拟方法为基础，通过气动方程和弹道方程联立求解数值模拟了子弹从母弹中分离并穿越母弹激波的过程，研究了子母弹干扰流场的气动特性，分析研究了子弹各初始分离状态（如初始抛撒速度、初始姿态角、初始姿态角速度等）对分离过程的影响。     

旋翼塔信号传输系统干扰的排除方法

旋翼塔信号传输系统是旋翼塔测试系统的重要组成部分,信号传输质量是决定测试系统测试数据真实性的最重要因素。由于旋翼试验塔采用长线传输,所以必须排除信号传输系统的干扰,必须对信号传输系统进行调试,以确保试验数据的可靠和准确。     

基于电子数据存储技术的微机化遥测处理系统

通过对某一高码速率光纤遥测系统中数据格式、码速率、数据容量、数据存储宽度、数据存储速率等特点的研究，提出了一种基于大容量电子数据存储器的微机化遥测处理系统，对存储的大容量数据阵列中的帧码识别、分路控制方法进行了讨论，并对受干扰数据处理时帧同步码检测的检测门限和同步对策参数进行了分析，最后给出了整个微机化的大容量遥测数据处理系统的软硬件设计方法，通过在６．５ＭｂｐｓＰＣＭ系统下的运行实验表明，整个方