多功能天文经纬仪图像处理系统
An Image Processing System for a Multi-Function Astronomical Theodolite
查看参考文献22篇
|
文摘
|
多功能天文经纬仪是云南天文台新研制的一种基于通用CCD观测的天体测量望远镜。介绍了多功能天文经纬仪的图像处理系统，从系统的整体框架和主要功能算法两个方面说明了整个图像处理系统的实现流程和工作方法。介绍了星像搜索算法、定心算法和VC++ 程序设计的流程图。给出了图像处理软件的界面，以及恒星像、人造星像和轴准直星像3种星像的定心结果，并对其结果进行了分析。 |
|
其他语种文摘
|
A new Multi-Function Astronomical Theodolite has been built in the Yunnan Observatory. Its main imaging device is a digital CCD camera without cooling. This paper presents an image processing system for the Multi-Function Astronomical Theodolite. The system is used to determine the centers of the stellar profiles in images obtained by the theodolite. The algorithm of the image-processing system includes two main parts, for searching the star and centering the star (object-centering),respectively. An image obtained with this instrument is unusual as it includes only one star. This makes it possible to adopt an efficient searching algorithm for the system. This is to smooth the image with a suitable method, then find the maximum-value pixel as the initial location of the center of the star. After comparing commonly used centering methods in astrometry for the adaptability,accuracy,calculation amount,and programming difficulty,we decide to use the method of two-dimensional modified moments as the object-centering method. The paper shows a block diagram of the image processing system and a program flowchart of the corresponding software written in the VC++. The paper also shows the main design of the program, a screenshot of the user interface of the software, and results of using the object-centering method to a star, an artificial stellar profile, and an aperture profile (which is through the axis collimator on the instrument). The paper finally presents a brief analysis of these results. |
|
来源
|
天文研究与技术
,2014,11(1):65-71 【扩展库】
|
|
关键词
|
多功能天文经纬仪
;
图像处理系统
;
编程
;
算法
;
定心
|
|
地址
|
1.
昆明理工大学信息工程与自动化学院, 云南, 昆明, 650500
2.
中国科学院云南天文台, 中国科学院天体结构与演化重点实验室, 云南, 昆明, 650011
|
|
语种
|
中文 |
|
文献类型
|
研究性论文 |
|
ISSN
|
1672-7673 |
|
学科
|
自动化技术、计算机技术 |
|
基金
|
国家自然科学基金
;
云南省专项基金
;
昆明市科技合作重大项目
|
|
文献收藏号
|
CSCD:5063086
|
参考文献 共
22
共2页
|
|
1.
冒蔚.
CCD天体测量学,2003
|
被引
8
次
|
|
|
|
|
2.
Stone R C. The flagstaff astrometric scanning transit telescope (FASTT) and star positions determined in the extragalactic reference frame.
The Astronomical Journal,1996,111(4):1721-1742
|
被引
5
次
|
|
|
|
|
3.
Viateau B. The Bordeaux and Valinhos CCD meridian circles.
Astronomy and Astrophysics Supplement,1999,134:173-186
|
被引
1
次
|
|
|
|
|
4.
Lopes P A A. Observations of radio stars at the Valinhos CCD meridian circle.
Astronomy and Astrophysics Supplement,1999,136:531-537
|
被引
1
次
|
|
|
|
|
5.
李彬华.
低纬度子午环控制系统及数据预处理系统的研究,2002
|
被引
1
次
|
|
|
|
|
6.
Auer L H. The stellar atmospheres problem.
Journal of Quantitative Spectroscopy and Radiative Transfer,1971,11(6):573-587
|
被引
2
次
|
|
|
|
|
7.
van Altena W F. Digital Image Centering, I..
Image Processing Techniques in Astronomy,1975:411-418
|
被引
3
次
|
|
|
|
|
8.
季凯帆.
CCD在天体测量中的应用及数字星像处理方法,1993
|
被引
1
次
|
|
|
|
|
9.
Stone R C. Positions for the outer planets and many of their satellites. IV. FASTT observations taken in 1999-2000.
The Astronomical Journal,2000,120:2124-2130
|
被引
4
次
|
|
|
|
|
10.
季凯帆. CCD图像的二维修正矩定心方法.
天文学报,1996,37(1):85-90
|
被引
11
次
|
|
|
|
|
11.
Lu C L. Digital image centering with the maximum likelihood method.
Astronomy and Astrophysics,1993,275:349-352
|
被引
2
次
|
|
|
|
|
12.
Sato I. Filtering theory with orthogonal function for two-dimensional astrometry.
Astronomy and Astrophysics Supplement Series,1995,113:185-197
|
被引
1
次
|
|
|
|
|
13.
Stone R C. Positions for the outer planets and many of their satellites. V. FASTT observations taken in 2000-2001.
The Astronomical Journal,2001,122:2723-2733
|
被引
4
次
|
|
|
|
|
14.
Peng Q Y. Image-processing techniques in precisely measuring positions of saturn and its satellites.
Science in China Series G: Physics, Mechanics and Astronomy,2003,46(4):362-370
|
被引
4
次
|
|
|
|
|
15.
李展. CCD图像数字定心算法的比较.
天文学报,2009,50(3):340-348
|
被引
20
次
|
|
|
|
|
16.
Li B H. Automatic processing method for astronomical CCD images.
Proceedings of SPIE,4847,2002:305-312
|
被引
1
次
|
|
|
|
|
17.
Stone R C. A comparison of digital centering algorithms.
The Astronomical Journal,1989,97(4):1227-1237
|
被引
14
次
|
|
|
|
|
18.
Mao W. Constructing an observational model of the neutral atmospheric refraction delay from measured values of the astronomical refraction.
The Astronomical Journal,2007,134(5):2054-2060
|
被引
4
次
|
|
|
|
|
19.
Mao W. A possible means of improving the accuracy of refraction delay correction of neutral atmosphere.
Chinese Astronomy and Astrophysics,2007,31(2):211-220
|
被引
3
次
|
|
|
|
|
20.
铁琼仙. 建立经纬度异常变化三角监测网的仪器和误差的测定.
天文研究与技术——国家天文台台刊,2008,5(4):360-364
|
被引
2
次
|
|
|
|
|
了解气象卫星更多信息，请访问