NAOC Open IR
对强源近周暗弱天体成象的一种方法
叶彬浔1; 初一2
1999
Source Publication科学通报
ISSN0023-074X
Volume044Issue:016Pages:1710
Abstract为了解决对明亮天体近周的暗弱目标进行光学成象的困难,提出并实验了一种方法。有别于传统星晚仪或新出现的抗晕CCD技术,在使暗弱目标获得中够的露光量后仍能不失真地保存明亮对象的图象信息。描述了原理与计算机仿真结果,实验装置结构及在文望远镜上进行天文实验观测的实验效果。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/46497
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.南京大学
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
叶彬浔,初一. 对强源近周暗弱天体成象的一种方法[J]. 科学通报,1999,044(016):1710.
APA 叶彬浔,&初一.(1999).对强源近周暗弱天体成象的一种方法.科学通报,044(016),1710.
MLA 叶彬浔,et al."对强源近周暗弱天体成象的一种方法".科学通报 044.016(1999):1710.
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