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

页码：159 / 160

页数：1

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