Performance of software-based solar adaptive optics system

被引：7
|
作者：
Miura N. [1 ]
Noto Y. [1 ]
Kato S. [1 ]
Kuwamura S. [1 ]
Baba N. [2 ]
Hanaoka Y. [3 ]
Ueno S. [4 ]
Kitai R. [4 ]
机构：
[1] Department of Computer Sciences, Kitami Institute of Technology, Kitami, Hokkaido 090-8507
[2] Department of Applied Physics, Graduate School of Engineering, Hokkaido University
[3] National Astronomical Observatory, Mitaka, Tokyo 181-8588
[4] Hida Observatory, Graduate School of Science, Kyoto University, Kamitakara, Takayama
来源：
Optical Review | 2007年 / 14卷 / 3期
关键词：
Adaptive optics; Solar observation;
D O I：
10.1007/BF02919417
中图分类号：
学科分类号：
摘要：
This paper reports the performance of our modified adaptive optics system for solar observations. This system operates at a frame rate of about 400 Hz and has the closed-loop cutoff frequency at 105 Hz. The results of the laboratory experiments show that this system compensates for a temporal wavefront-variation of less than 99 Hz and improves the Strehl ratio by a factor of five. © 2007 The Optical Society of Japan.
引用
收藏
页码：159 / 160
页数：1
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