End-to-end simulations of photonic phase correctors for adaptive optics systems

被引:1
|
作者
Patel, Dhwanil [1 ]
Diab, Momen [1 ]
Cheriton, Ross [2 ]
Taylor, Jacob [1 ,3 ]
Rojas, Libertad [1 ]
Vachon, Martin [2 ]
Xu, Dan-Xia [2 ]
Schmid, Jens H. [2 ]
Cheben, Pavel [2 ]
Janz, Siegfried [2 ]
Sivanandam, Suresh [1 ,3 ]
机构
[1] Univ Toronto, Dunlap Inst Astron & Astrophys, Toronto, ON, Canada
[2] Natl Res Council Canada, Quantum & Nanotechnol Res Ctr, Ottawa, ON, Canada
[3] Univ Toronto, David A Dunlap Dept Astron & Astrophys, Toronto, ON, Canada
来源
OPTICS EXPRESS | 2024年 / 32卷 / 16期
关键词
MODE FIBERS; WAVE-GUIDES; GRATINGS; LANTERNS; COUPLERS;
D O I
10.1364/OE.530879
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Optical beams and starlight distorted by atmospheric turbulence can be corrected with adaptive optics systems to enable efficient coupling into single-mode fibers. Deformable mirrors, used to flatten the wavefront in astronomical telescopes, are costly, sensitive, and complex mechanical components that require careful calibration to enable high-quality imaging in astronomy, microscopy, and vision science. They are also impractical to deploy in large numbers for non-imaging applications like free-space optical communication. Here, we propose a photonic integrated circuit capable of spatially sampling the wavefront collected by the telescope and co-phasing the subapertures to maximize the flux delivered to an output single-mode fiber as the integrated photonic implementation of a deformable mirror. We present the results of end-to-end simulations to quantify the performance of the proposed photonic solution under varying atmospheric conditions toward realizing an adaptive optics system without a deformable mirror for free-space optical receivers.
引用
收藏
页码:27459 / 27472
页数:14
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