中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Mirror seeing of the Antarctic survey telescope

文献类型:期刊论文

作者YUAN Xiangyan; PEI Chong; LI Zhengyang; ZHANG Kaiyuan
刊名Advances in Polar Science
出版日期2014-09
卷号25期号:3页码:133-137
关键词mirror seeing Anta rctic survey telescopes Dome A turbulence
英文摘要Site test ing results indicate thal Antarctic Dome A is an excellent ground-based astronomical sile sui table for observations ranging from visible to infrared wavelengths. However, the harsh environment in Antarctica, especially the very low temperature and atmospheric pressure, always produces frost on the telescopes' mirrors, which are exposed to the air. Since the Dome A site is still unattended, the Antarctic telescope tubes are always designed to be filled with dry nitrogen, and the outer surfaces of the oplical system are heated by an indium-tin oxide thin film. These precautions can prevent optical surfaces from frosting over, but they degrade the image quality by introducing additional rnirror seeing. Based on testing observations of the second Antarctic Survey Telescope (AST3-2) in the Mohe site in China, rnirror seeing resulting from the heated aspheric plate has been rneasured using micro-thennal sensors. Results comparing the real-time atmospheric seeing monitored by Ihe Differenlial Image Motion Monitor and real-time exarninations of image quality agree well.
学科主题南极望远镜 ; 天文技术与方法
公开日期2015-03-13
源URL[http://ir.niaot.ac.cn/handle/114a32/802]  
专题期刊论文
推荐引用方式
GB/T 7714
YUAN Xiangyan,PEI Chong,LI Zhengyang,et al. Mirror seeing of the Antarctic survey telescope[J]. Advances in Polar Science,2014,25(3):133-137.
APA YUAN Xiangyan,PEI Chong,LI Zhengyang,&ZHANG Kaiyuan.(2014).Mirror seeing of the Antarctic survey telescope.Advances in Polar Science,25(3),133-137.
MLA YUAN Xiangyan,et al."Mirror seeing of the Antarctic survey telescope".Advances in Polar Science 25.3(2014):133-137.

入库方式: OAI收割

来源:南京天文光学技术研究所

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