Queuing theory application in imaging service analysis for small Earth observation satellites

The performance of Earth observation satellites is usually analyzed by real data or system simulation, which is accurate but not systematic. Modelling satellite service systems with queueing theory and analysing the performance statistics systematically will provide a useful guide in designing satellite systems. Earth observation satellites could be regarded as a two tandem server system with a finite buffer in between, providing two-stage service: image capture and image download service. In this paper, we introduce the queueing models for different service systems: the pure image capture service system, the two-stage service system with Poisson distribution download service, the pure download service system, and the two-stage system with general download service. Formulated solutions are given and some results are shown. From this work we can see queueing theory provides a good way to analyse the performance of small earth observation satellites, which is useful for system mission analysis and optimisation in design stage.     

圆度误差的一种微机图像测量法

将圆度误差测量的影像法与最小二乘圆法相结合，利用多媒体图像处理技术，设计了一种圆度误差的微机自动测量系统，实现了非接触、远距离快速测量，提高了测量精确度，为某些特殊工件的测量提供了一套实用的测量方法。     

一种Ka频段宽带3dB功分桥的实现技术研究

文章简要介绍了波导宽边耦合3dB功分桥的工作原理，重点阐述四耦合窗Ka频段宽带波导宽边耦合3dB功分桥的仿真设计过程、仿真结果以及最终的实物测试结果。最后得到一个性能优良的Ka频段宽带波导宽边耦合3dB功分桥。     

亚跨超CFD软件平台研制

亚跨ＣＦＤ软件平台研制的宗旨是综合国内外计算流体动力学的最新研究成果，用计算机软件技术的新发展，建立一个面向对象的计算流体动力学的研究开发环境，加快计算流体动力学最新成果向工程应用的转换速度。本文介绍初级版本的研究进展和研究成果，主要匝数值网格生成技术，流场解算器，面向对象的界面设计等三部分组成。     

旋翼着陆器在火星探测中的研究进展

旋翼着陆器是下一轮国际火星探测的重要发展方向.论文首先回顾了火星探测软着陆的发展概况,分析了旋翼着陆器的结构组成、火星探测工作原理及特点.其次,阐述了开展旋翼着陆器设计过程中所需的关键技术.     

系级教学档案管理模式研究

系级教学档案有自身的特殊性，并且形式多种多样。通过对系级教学档案的类型分析，坚持科学的系级教学档案整理工作的原则，才能高效完成系级教学档案的管理工作。     

BP网络进行0-9十个数字图像的识别

在BP算法和数字图像处理技术的基础上,本文在MATLAB软件环境下提取Word文档中26种字体的0-9十个数字的图像,使用MATLAB神经网络工具箱及图像处理工具箱进行数字的识别,给出了较详细的处理步骤及相关程序,并比较了各种识别算法的收敛速度和识别率。     

On the Acquisition Time for an Apollo Ranging Code

An Apollo ranging system is considered whose phase reference is obtained by a phase-locked loop for bit synchronization. The bit phase reference is noisy, and the error probability for the ranging code is shown to depend on the input signal energy per bit to noise density ratio. The procedure of computing the acquisition time for the ranging code is then presented and the acquisition time for a lunar ranging code is plotted versus the input signal-to-noise density ratio.