TURBO-RL: turbulence mitigation using reinforcement learning for severe optical aberrations

Optical distortion or aberration remains a vital challenge that prohibits high-resolution imaging in various applications such as space domain awareness, terrestrial remote sensing, and astronomy. However, due to the stochastic nature of these optical distortions, reducing their effect without directly measuring wavefronts is challenging. Furthermore, in the case of extreme turbulence, due to the limited size of the lenslet array in the wavefront sensor, the sensor fails to correctly quantify or minimize the image distortions of a guide star from turbulence. While numerous studies have shown effectiveness of guide star-based adaptive optics in mitigating mild turbulence, severe turbulence has remained a persistent challenge. To target this, we present TURBO-RL: TURBulence mitigatiOn using Reinforcement Learning, which uses just a single optical element (e.g., deformable mirror) to estimate and correct the wavefront errors from a guide star. TURBO-RL adopts reinforcement learning with a convolutional neural network to extract and estimate turbulence. Unlike other methods, TURBO-RL is capable of guide star imaging in severe turbulence (<i>D</i>/<i>r</i><sub>0</sub>=100) with only about 590 photons, making it possible to overcome the strong turbulence and possibly replace bulky and expensive wavefront sensors.

Authors

Institutions

Publication Details

Journal
Journal of the Optical Society of America A
Published
2025-12-12
DOI
https://doi.org/10.1364/josaa.568108
Primary Topic
Adaptive optics and wavefront sensing
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

TURBO-RL: turbulence mitigation using reinforcement learning for severe optical aberrations

Hyunsoo Choi, Vaneet Aggarwal, Zubin Jacob, Jiayu Chen
Journal of the Optical Society of America A
Adaptive optics and wavefront sensing
article

TURBO-RL: turbulence mitigation using reinforcement learning for severe optical aberrations

Hyunsoo Choi, Vaneet Aggarwal, Zubin Jacob, Jiayu Chen
article en

Abstract

Optical distortion or aberration remains a vital challenge that prohibits high-resolution imaging in various applications such as space domain awareness, terrestrial remote sensing, and astronomy. However, due to the stochastic nature of these optical distortions, reducing their effect without directly measuring wavefronts is challenging. Furthermore, in the case of extreme turbulence, due to the limited size of the lenslet array in the wavefront sensor, the sensor fails to correctly quantify or minimize the image distortions of a guide star from turbulence. While numerous studies have shown effectiveness of guide star-based adaptive optics in mitigating mild turbulence, severe turbulence has remained a persistent challenge. To target this, we present TURBO-RL: TURBulence mitigatiOn using Reinforcement Learning, which uses just a single optical element (e.g., deformable mirror) to estimate and correct the wavefront errors from a guide star. TURBO-RL adopts reinforcement learning with a convolutional neural network to extract and estimate turbulence. Unlike other methods, TURBO-RL is capable of guide star imaging in severe turbulence (<i>D</i>/<i>r</i><sub>0</sub>=100) with only about 590 photons, making it possible to overcome the strong turbulence and possibly replace bulky and expensive wavefront sensors.

Journal of the Optical Society of America AVol. 43(2)
Purdue University West Lafayette (US), Sungkyunkwan University (KR)
Openalex Percentile: Top 67%
Adaptive optics and wavefront sensing
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.