Influence of atmospheric turbulence on detecting performance of all-day star sensor
Pan, Yue1,2; Wang, Hu1; Shen, Yang1,2; Xue, Yaoke1; Liu, Jie1
2016
会议名称7th international symposium on precision mechanical measurements, ispmm 2015
会议日期2015-08
会议地点xia'men, china
关键词Star sensor All-day Atmospheric turbulence Long-exposure Signal to noise ratio
卷号9903
英文摘要all-day star sensor makes it possible to observe stars in all-day time in the atmosphere. but the detecting performance is influenced by atmospheric turbulence. according to the characteristic of turbulence in long-exposure model, the modulation transfer function, point spread function and encircled power of the imaging system have been analyzed. combined with typical star sensor optical system, the signal to noise ratio and the detectable stellar magnitude limit affected by turbulence have been calculated. the result shows the ratio of aperture diameter to atmospheric coherence length is main basis for the evaluation of the impact of turbulence. in condition of medium turbulence in day time, signal to noise ratio of the star sensor with diameter 120mm will drop about 4db at most in typical work environment, and the detectable stellar limit will drop 1 magnitude. © 2016 spie.
收录类别EI ; ISTP
产权排序1
会议录seventh international symposium on precision mechanical measurements
会议录出版者spie
学科主题电子、电信技术 ; 光学 ; 天文学、地球科学 ; 机械、仪表
语种英语
ISSN号0277786x
ISBN号9781510601673
内容类型会议论文
源URL[http://ir.opt.ac.cn/handle/181661/27861]  
专题西安光学精密机械研究所_空间光学应用研究室
作者单位1.Xi'An Institute of Optics and Precision Mechanics of CAS, Xi'an, China
2.University of Chinese Academy of Sciences, Beijing, China
推荐引用方式
GB/T 7714
Pan, Yue,Wang, Hu,Shen, Yang,et al. Influence of atmospheric turbulence on detecting performance of all-day star sensor[C]. 见:7th international symposium on precision mechanical measurements, ispmm 2015. xia'men, china. 2015-08.
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