Simulating large atmospheric phase screens using a woofer-tweeter algorithm

被引:5
作者
Buscher, David F. [1 ]
机构
[1] Cavendish Lab, JJ Thomson Ave, Cambridge CB3 0HE, England
来源
OPTICS EXPRESS | 2016年 / 24卷 / 20期
基金
英国科学技术设施理事会;
关键词
TURBULENT PHASE;
D O I
10.1364/OE.24.023566
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We describe an algorithm for simulating atmospheric wavefront perturbations over ranges of spatial and temporal scales spanning more than 4 orders of magnitude. An open-source implementation of the algorithm written in Python can simulate the evolution of the perturbations more than an order-of-magnitude faster than real time. Testing of the implementation using metrics appropriate to adaptive optics systems and long-baseline interferometers show accuracies at the few percent level or better. (C) 2016 Optical Society of America
引用
收藏
页码:23566 / 23571
页数:6
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