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南京天文光学技术研究... [2]
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会议论文 [5]
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2018 [2]
2011 [3]
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Orbital and formation optimization for space gravitational waves observatory mission
会议论文
Bremen, Germany, October 1, 2018 - October 5, 2018
作者:
Wang, Youliang
;
Zheng, Jianhua
;
Li, Mingtao
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浏览/下载:20/0
  |  
提交时间:2019/07/10
Origin of Jupiter’s cloud-level zonal winds remains a puzzle even after Juno
会议论文
国内, 2018
作者:
Dali Kong, Keke Zhang, Gerald Schubert, and John D. Anderson
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  |  
浏览/下载:18/0
  |  
提交时间:2019/01/11
A dual-channel imaging polarimetry system
会议论文
Beijing, China, 2011-11-6
Xue Wang
;
Deqing Ren
;
Jiangpei Dou
;
Yongtian Zhu
;
Xi Zhang
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  |  
浏览/下载:34/0
  |  
提交时间:2014/01/07
extra-solar planets
imaging polarimetry
data reduction
distortion correction
Testing of a high-contrast imaging coronagraph based on an active liquid crystal array
会议论文
Beijing, China, 2011-11-6
Xi Zhang
;
Deqing Ren
;
Yongtian Zhu
;
Jiangpei Dou
;
Xue Wang
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  |  
浏览/下载:23/0
  |  
提交时间:2014/01/08
Exoplanets detection
high-contrast imaging
liquid crystal array
amplitude correction
non-uniformity compensation
Astronomical image restoration through atmosphere turbulence by lucky imaging (EI CONFERENCE)
会议论文
3rd International Conference on Digital Image Processing, ICDIP 2011, April 15, 2011 - April 17, 2011, Chengdu, China
Zhang S.
;
Wu Y.
;
Zhao J.
;
Wang J.
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浏览/下载:18/0
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提交时间:2013/03/25
In this paper
we develop a lucky imaging system to restore astronomical images through atmosphere turbulence. Our system takes very short exposures
on the order of the atmospheric coherence time. The rapidly changing turbulence leads to a very variable point spread function (PSF)
and the variability of the PSF leads to some frames having better quality than the rest. Only the best frames are selected
aligned and co-added to give a final image with much improved angular resolution. Our system mainly consists of five parts: preprocessing
frame selection
image registration
image reconstruction
and image enhancement. Our lucky imaging system has been successfully applied to restore the astronomical images taken by a 1.23m telescope. We have got clear images of moon surface and Jupiter
and our system can be demonstrated to greatly improve the imaging resolution through atmospheric turbulence. 2011 Copyright Society of Photo-Optical Instrumentation Engineers (SPIE).
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