Tempestas ex machina: A review of machine learning methods for wavefront control
J. Fowler, Rico Landman

TL;DR
This paper reviews the application of machine learning techniques to wavefront control in adaptive optics, highlighting recent advances, challenges, and potential improvements for high-contrast imaging systems.
Contribution
It provides a comprehensive overview of machine learning methods used in wavefront control, emphasizing recent innovations and their potential to enhance adaptive optics performance.
Findings
Machine learning methods can address temporal lag and dynamic errors in wavefront control.
Traditional integrator controllers are limited in handling fast-evolving errors.
Recent literature shows promising machine learning approaches for improved wavefront correction.
Abstract
As we look to the next generation of adaptive optics systems, now is the time to develop and explore the technologies that will allow us to image rocky Earth-like planets; wavefront control algorithms are not only a crucial component of these systems, but can benefit our adaptive optics systems without requiring increased detector speed and sensitivity or more effective and efficient deformable mirrors. To date, most observatories run the workhorse of their wavefront control as a classic integral controller, which estimates a correction from wavefront sensor residuals, and attempts to apply that correction as fast as possible in closed-loop. An integrator of this nature fails to address temporal lag errors that evolve over scales faster than the correction time, as well as vibrations or dynamic errors within the system that are not encapsulated in the wavefront sensor residuals; these…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAdaptive optics and wavefront sensing · Optical Systems and Laser Technology · Stellar, planetary, and galactic studies
MethodsSPEED: Separable Pyramidal Pooling EncodEr-Decoder for Real-Time Monocular Depth Estimation on Low-Resource Settings
