中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页 机构 成果 学者
  
  1. CAS IR Grid
  2. 国家天文台
  3. 中国科学院国家天文台
Multistar turbulence monitor: a new technique to measure optical turbulence profiles

文献类型：期刊论文

作者Hickson, Paul1,2; Ma, Bin2,3; Shang, Zhaohui2; Xue, Suijian2
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2019-05-01
卷号485期号:2页码:2532-2545
关键词atmospheric effects instrumentation: adaptive optics site testing
ISSN号0035-8711
DOI10.1093/mnras/stz568
英文摘要The strength and vertical distribution of atmospheric turbulence is a key factor determining the performance of optical and infrared telescopes, with and without adaptive optics. Yet, this remains challenging to measure. We describe a new technique using a sequence of short-exposure images of a star field, obtained with a small telescope. Differential motion between all pairs of star images is used to compute the structure functions of longitudinal and transverse wavefront tilt for a range of angular separations. These are compared with theoretical predictions of simple turbulence models by means of a Markov Chain Monte Carlo optimization. The method is able to estimate the turbulence profile in the lower atmosphere, the total and free-atmosphere seeing, and the outer scale. We present results of Monte Carlo simulations used to verify the technique, and show some examples using data from the second AST3 telescope at Dome A in Antarctica.
WOS关键词ADAPTIVE OPTICS ; SURFACE-LAYER ; DOME-C ; SITE ; SCINTILLATION
资助项目Natural Sciences and Engineering Research Council of Canada ; Chinese Academy of Sciences (CAS President's International Fellowship Initiative)[2017VMA0013] ; National Natural Science Foundation of China[11733007] ; National Natural Science Foundation of China[11673037]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000474886200076
出版者OXFORD UNIV PRESS
资助机构Natural Sciences and Engineering Research Council of Canada ; Natural Sciences and Engineering Research Council of Canada ; Chinese Academy of Sciences (CAS President's International Fellowship Initiative) ; Chinese Academy of Sciences (CAS President's International Fellowship Initiative) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Natural Sciences and Engineering Research Council of Canada ; Natural Sciences and Engineering Research Council of Canada ; Chinese Academy of Sciences (CAS President's International Fellowship Initiative) ; Chinese Academy of Sciences (CAS President's International Fellowship Initiative) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Natural Sciences and Engineering Research Council of Canada ; Natural Sciences and Engineering Research Council of Canada ; Chinese Academy of Sciences (CAS President's International Fellowship Initiative) ; Chinese Academy of Sciences (CAS President's International Fellowship Initiative) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Natural Sciences and Engineering Research Council of Canada ; Natural Sciences and Engineering Research Council of Canada ; Chinese Academy of Sciences (CAS President's International Fellowship Initiative) ; Chinese Academy of Sciences (CAS President's International Fellowship Initiative) ; National Natural Science Foundation of China ; National Natural Science Foundation of China
源URL[http://ir.bao.ac.cn/handle/114a11/26906]  
专题中国科学院国家天文台
通讯作者Hickson, Paul
作者单位1.Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z1, Canada
2.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100101, Peoples R China
3.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
推荐引用方式
GB/T 7714		 Hickson, Paul,Ma, Bin,Shang, Zhaohui,et al. Multistar turbulence monitor: a new technique to measure optical turbulence profiles[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,485(2):2532-2545.
APA Hickson, Paul,Ma, Bin,Shang, Zhaohui,&Xue, Suijian.(2019).Multistar turbulence monitor: a new technique to measure optical turbulence profiles.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,485(2),2532-2545.
MLA Hickson, Paul,et al."Multistar turbulence monitor: a new technique to measure optical turbulence profiles".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 485.2(2019):2532-2545.

入库方式： OAI收割

来源：国家天文台

浏览0
下载0
收藏0
其他版本

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。