Forecasting Wavefront Corrections in an Adaptive Optics System
Rehan Hafeez, Finn Archinuk, S\'ebastien Fabbro, Hossen Teimoorinia,, Jean-Pierre V\'eran

TL;DR
This paper demonstrates that linear auto-regressive models can significantly forecast wavefront corrections in adaptive optics, reducing errors and improving image quality, with minimal computational cost, while more complex models offer no additional benefit.
Contribution
It introduces a simple, effective linear forecasting method for wavefront correction in adaptive optics and evaluates machine learning models, finding linear models suffice for current conditions.
Findings
Linear auto-regressive models reduce wavefront error by up to 5 times for Tip-Tilt.
Forecasting filters can be updated quickly with minimal telemetry data.
More complex machine learning models do not outperform linear models in this context.
Abstract
We use telemetry data from the Gemini North ALTAIR adaptive optics system to investigate how well the commands for wavefront correction (both Tip/Tilt and high-order turbulence) can be forecasted in order to reduce lag error (due to wavefront sensor averaging and computational delays) and improve delivered image quality. We show that a high level of reduction ( 5 for Tip-Tilt and 2 for high-order modes) in RMS wavefront error can be achieved by using a "forecasting filter" based on a linear auto-regressive model with only a few coefficients ( 30 for Tip-Tilt and 5 for high-order modes) to complement the existing integral servo-controller. Updating this filter to adapt to evolving observing conditions is computationally inexpensive and requires less than 10 seconds worth of telemetry data. We also use several machine learning models (Long-Short Term Memory and…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
