一种天文用CCD相机的电路设计

简述了一种面向天文应用的CCD相机系统的设计要求,详细介绍了该相机系统电路的基本结构及设计原则,包括CCD及其周边电路、模拟前端、时钟驱动电路、电源电路以及用VHDL编写的植入FPGA的CCD时序发生器电路等一些技术细节.对系统中一些关键电路模块进行了仿真和实测,并对仿真和测试结果进行比较分析,最后给出该CCD相机的图像采集结果.     

DLT方法在遥感相机几何定标中的应用

为建立适用于遥感相机定标的实验室,需要有几何标定的算法和软件对摄影图像进行计算.使用近景摄影测量中基于3维控制场的定标方法,对单CCD四波段遥感相机进行了几何定标,研究并自主编程实现了直接线性变换DLT(Direct Linear Transformation)算法,与基于空间后方交会算法的定标结果进行了精度对比.结论...     

LD2000 System with 3S and Multi—sensor

This paper introduces a car-borne road information collecting and updating system (LD2000) developed by Wuhan Technical University of Surveying and Mapping.This system is capable of collecting road network information and creating digital road network effectively by means of GPS,GIS and multi-sensor integration.The design and development of LD 2000 system are also presented in this paper.     

应用CDOM光学特性估算水体COD——以辽宁省盘锦市双台子河和辽东湾为例

有色可溶性有机物(chromophoric dissolved organic matter,CDOM)是水体中一类重要的光吸收物质,在水色遥感中,其光学特性主要以440 nm处的吸收系数和光谱斜率来表征,利用这些光学特性进行水环境要素遥感反演具有较广泛的应用前景.化学需氧量(chemical oxygen deman...     

利用CCD成像技术进行渤海海冰观测探讨

利用CCD成像技术进行走航海冰观测是国际南极科学委员会海冰过程与气候项目制定的南极海冰观测方法的一部分.本文介绍了利用CCD成像技术进行海冰观测及其图像信息提取的基本原理,分析了该项技术在南北极海冰走航观测应用实践中的成功经验及问题所在,讨论了南北极与渤海冰情和调查作业环境的差异,探讨了利用CCD成像技术进行渤海海冰观测的应用前景.     

天文视频图像采集系统的研究

介绍了采用数字图像处理技术实现软件积分研制成的天文视频图像采集、处理系统。利用该系统 ,我们对 1 997年 3月 9日黑龙江漠河日全食的观测资料进行了处理 ,结果证明 ,该系统完全达到预期研制的目标。     

基于普通数码相机的影像匹配技术

论述了将全数字摄影测量应用于计算煤场煤堆体积的基本理论和方法。重点论述了普通数码相机影像匹配方法和数学模型，系统的物理模型在实验室内得以验证和实现。     

The Ultimate CCD for Laser Guide Star Wavefront Sensing on Extremely Large Telescopes

All of the extremely large telescopes (ELTs) will utilize sodium laser guide star (LGS) adaptive optics (AO) systems. Most of these telescopes plan to use the Shack-Hartmann approach for wavefront sensing. In these AO systems, the laser spots in subapertures at the edge of the pupil will suffer from spot elongation due to the 10 km extent of the sodium layer and the large separation from the projection laser. This spot elongation will severely degrade the performance of standard geometry wavefront sensing systems. In this paper, we present a CCD with custom pixel morphology that aligns the pixels of each subaperture with the radial extension of the LGS spot. This CCD design will give better performance than a standard geometry CCDs for continuous wave lasers. In addition, this CCD design is optimal for a pulsed sodium laser. The pixel geometry enables each subaperture to follow a laser pulse traversing the sodium layer, providing optimal sampling of a limited number of detected photons. In addition to novel pixel layout, this CCD will also incorporate experimental JFET sense amplifiers and use CMOS design approaches to simplify the routing of biases, clocks and video output. This CCD will attain photon-noise limited performance at high frame rates, and is being incorporated in the plans for the Thirty Meter Telescope (TMT).     

A four lens camera design

A camera design with only four lens elements gives good imaging performance at a working focal ratio of f/4.4.     

Digital astro-geodetic camera system for the measurement of the deflections of the vertical: tests and results

This study introduces the new results of a novel low-cost digital zenith camera system operated in Turkey that uses astronomical and geodetic instrumentation. Currently, it is possible to determine deflections of the vertical (DoV) components by using a vast amount of information gathered from geo-referenced star images, tilt measurements, and Global Navigation Satellite System technology. This new design of an astro-geodetic camera system is used for calculating DoV components with 12 independent solutions on a test station in Istanbul, and additional observations were performed to investigate the external accuracy of the system on a test network. A specific leveling method is developed to align system toward the zenithal direction. The final results of the observations on a test station located in Istanbul indicate that the accuracy of the system is about ±0.19 arc-seconds in latitude and ±0.28 arc-seconds in longitude determination. The system has been further tested on a network with 4 control points that have averagely 20?km baselines. At the test network, the root mean square of the average value of the vertical deflections is calculated as ±0.36 arc-seconds. Furthermore, DoV components are compared with the values that are calculated using global geopotential models.