Image based automatic wind velocity profiler for adaptive optics

Sebastian J Diaz, Cristian Tejos, Andres Guesalaga
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Abstract

Adaptive optics (AO) systems correct optical phase aberrations of the incoming light generated by the atmosphere. To do so simultaneous estimators of the atmospheric turbulence parameters are required. For the family of wide-field AO systems (WFAO), this information must be stratified in altitude. Among these vectorized estimations, wind profiling in altitude is needed for the reduction of temporal errors in AO loops or for the estimation of turbulence coherence time. This paper proposes a turbulence wind profiler called image processing based peak tracking algorithm (IPTA). IPTA is an image-processing based approach that automatically and reliably estimates wind velocity for several turbulent layers along the line of sight. The estimation of each wind layer is achieved by tracking peaks produced in cross-correlation maps from pairs of wavefront sensors (WFSs) slopes using the technique known as SLODAR (slope detection and ranging). Results for simulated and on-sky WFS datasets demonstrate that IPTA outperforms one of the state of the art wind profiler methods (the profiler covariance parametrization of wind velocity (CAW)) in terms of accuracy and speed. Results also show that, in terms of execution time, our method scales better when the number of WFS lenslets is increased. Being an open source and reliable tool, we believe IPTA can be a useful wind profiler for the adaptive optics community.
基于图像的自适应光学自动风速剖面仪
自适应光学(AO)系统可以纠正大气层产生的入射光的光学相位差。为此,需要同时估算大气湍流参数。对于宽视场光学系统(WFAO)家族来说,这些信息必须在高度上分层。在这些矢量化估算中,为了减少光学观测环路中的时间误差或估算湍流相干时间,需要在高度上进行风剖面估算。本文提出了一种称为基于图像处理的峰值跟踪算法(IPTA)的湍流风剖面仪。IPTA 是一种基于图像处理的方法,可自动、可靠地估算沿视线方向多个湍流层的风速。每个风层的估算都是通过跟踪一对波前传感器(WFS)斜坡的交叉相关图中产生的峰值来实现的,采用的技术称为 SLODAR(斜坡探测和测距)。模拟和天空 WFS 数据集的结果表明,就精度和速度而言,IPTA 优于最先进的风廓线方法之一(风速廓线协方差参数化 (CAW))。结果还显示,就执行时间而言,当 WFS 微透镜数量增加时,我们的方法扩展性更好。作为一个开源和可靠的工具,我们相信 IPTA 可以成为自适应光学领域一个有用的风廓线工具。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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