Angular velocity determination of spinning solar sails using only a sun sensor

The direction of the sun is the easiest and most reliable observation vector for a solar sail running in deep space exploration. This paper presents a new method using only raw measurements of the sun direction vector to estimate angular velocity for a spinning solar sail. In cases with a con-stant spin angular velocity, the estimation equation is formed based on the kinematic model for the apparent motion of the sun direction vector;the least-squares solution is then easily calculated. A performance criterion is defined and used to analyze estimation accuracy. In cases with a variable spin angular velocity, the estimation equation is developed based on the kinematic model for the apparent motion of the sun direction vector and the attitude dynamics equation. Simulation results show that the proposed method can quickly yield high-precision angular velocity estimates that are insensitive to certain measurement noises and modeling errors.     

多霍尔器件提高飞轮转速测量精度的研究

对飞轮使用的霍尔器件与转速测量精度之间的关系进行分析,提出了一种基于增加霍尔器件提高飞轮转速测量精度的方法,并根据该方法确定了多霍尔器件安装布局的设计原则和公式。     

超小型高可靠高稳定晶体振荡器

介绍体积仅为３０ｍｍ×３０ｍｍ×４０ｍｍ，重量仅为５０ｇ，适用于宇航系统的新型高稳定、高可靠频率源的研制情况。给出各项技术指标的测试结果。     

The SAX mission

SAX denotes the X-Ray Astronomy Satellite selected by the Italian National Space Plan for inclusion in the Science Programme. The purpose of SAX is to perform spectroscopic, spectral and time variability studies of celestial X-Ray sources in the energy band from 1 to 200 KeV. It is intended to continue and expand upon previous observations of such sources. The instrumentation consists of four X-Ray imaging concentrators sensitive from 1 to 10 KeV (one of them extending down to 0.1 KeV), one Gas Scintillation Proportional Counter sensitive from 3 to 120 KeV, a Sodium Iodide Scintillator Crystal in Phoswich configuration operating from 15 KeV to 200 KeV; these detectors are coaligned to a common pointing axis. Three Wide Field Cameras (2–30 KeV) with axis at 90° to that of the narrow field instruments complete the payload.The Satellite launch is foreseen for 1988, in a low altitude (500 Km), low inclination (12°) orbit.The SAX scientific programme is carried out by a Consortium of Italian Institutes, in cooperation with Institutes from Holland; a partecipation of the Space Science Department of ESA is also foreseen.     

基于SPIHT算法的遥感图像高速实现方案

基于小波变换的SPIHT图像压缩方案是目前公认性能较好的一种实用高性能图像压缩编码算法，但原始SPIHT算法链表式编码限制了其在高速处理中的应用。本文提出了一种改进的SPIHT压缩编码算法，在确保恢复图像质量与原始算法基本上相当的基础上，改进算法可以采用并行流水结构实现，有利于高速处理中的应用，为该算法在遥感图像中的应用提供了理论依据和工程基础。     

大迎角限制器设计与飞机敏捷性

在介绍高机动性飞机大迎角限制器和飞机敏捷性要求的基础上，以典型战半机为例，计算了飞机的敏捷性尺度，根据计算结果进一步分析大迎角限制器对飞机敏捷性的影响，并以空战周期时间为例，说明迎角限制器参数的选择应兼顾飞机的敏捷性与飞行安全两方面。     

均值,方差模型在证券投资组合中的运用

本文阐述了在证券投资组合中应用均值、方差模型的基本原理，给出有效果曲线形态，最后给出了在同等风险下取得最大收益的证券组合形成的求法。     

高Ra数自然对流问题的张力样条数值模拟

本文将基于压力泊松方程技术的原参数Ｎ－Ｓ方程的张力样条数值解法推广应用于自然对流问题的数值模拟，提出了自然对流问题一个新的数值模拟方法，对一方内高Ｒａ数自然对流问题的数值模拟表明，结果是令人满意的。     

富氮高能物质BTATz的热分解动力学和分解机理

为获得富氮高能物质3,6-双(1氢-1,2,3,4-四唑-5-氨基)-1,2,4,5-四嗪(BTATz)的热分解动力学参数、热分解机理函数、气相和凝聚相变化,为建立燃烧过程数学模型提供关键性热化学、热力学和化学动力学参数,通过热重(TG)、差示扫描量热(DSC)和气体(固体)原位反应池/快速扫描傅里叶变换红外光谱(RSFTIR)联用技术,研究了BTATz的热分解。实验结果显示BTATz的热分解过程对压强不敏感。基于Ozawa,Kissinger和Coats-Redfern方法,计算获得了BTATz的热分解动力学参数和方程。Kissinger法求得的活化能Ea和指前因子lgA分别为317.41 kJ.mol-1和28.07s-1。热分解反应机理服从n=1.5的Avrami-Erofeev方程,其热分解反应的动力学方程为dαdt=1.5×1028.07exp(-3.8178×104/T)(1-α)[-1n(1-α)]1/3。分析提出了BTATz的热分解机理,BTATz的热分解是从四嗪和四唑环的开环断裂开始的,分解产物又发生二次反应,465℃热分解凝聚相产物为NH4N3,聚胺和嘧嘞胺。     

析秦门三状元之谬传

秦桧是中国历史上臭名昭著的大奸臣．史书中关于他的记载很多．其中“秦门三状元”的说法更是广为流传。如宋人李心传的《建炎以来朝野杂记》、陈鹄的《耆老续闻》、渚人顾炎武的《日知录》及今人梁羽生的《笔花六记》等书均载秦桧、秦熺 (桧之子)、秦埙(桧之孙)皆为状元．其实这一说法有违史实。事实是秦桧为二甲赐进士出身．秦熺、秦埙均为一甲进士及第．