自适应光学反馈干涉测量的实际问题

D. Cheung, A. Somervell, T. H. Barnes, T. Haskell
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引用次数: 0

摘要

作者提出了用反馈干涉法进行像差校正的思想。传统的自适应光学系统通常使用单独的子系统来进行波前传感和校正,这涉及到大量的矩阵操作。在反馈干涉仪中,干涉图样的强度被用来控制波前校正器,从而将两个子系统结合在一起。为了开发一个在真实湍流环境中使用的实用系统,有几个问题需要考虑。在实际应用中,控制算法也存在一些问题。闪烁和频率响应是主要问题。频率响应决定了系统跟踪和纠正像差的速度。大气引起的像差可能具有高达200hz的频率成分。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Practical issues of feedback interferometry for adaptive optics
The idea of feedback interferometry for aberration correction was proposed by the author. Conventional adaptive optics (AO) systems usually use separate subsystems to perform wavefront sensing and correction, which involve large matrix manipulation. In a feedback interferometer, the intensity of the interference pattern is used to control the wavefront corrector, thus combining the two subsystems together. To develop a practical system for use in real turbulent environments, there are several issues that need to be considered. There are concerns in the control algorithm as well when try to use the system in practice. Scintillation and frequency response are the major issues. The frequency response determines how fast the aberration that the system can track and correct. Atmospheric induced aberration might have frequency components as high as 200 Hz.
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