Cascade adaptive optics: contrast performance analysis of a two-stage controller by numerical simulations

TL;DR

This paper analyzes a two-stage adaptive optics system through numerical simulations, demonstrating significant contrast improvements and turbulence decorrelation benefits for exoplanet imaging.

Contribution

It introduces a dynamical model for cascade AO systems with two control stages and evaluates their control properties and performance improvements.

Findings

Second stage improves imaging contrast by one order of magnitude.

Second stage reduces decorrelation time of atmospheric turbulence.

Analysis shows how disturbance transfer affects control stability and mitigation strategies.

Abstract

The contrast performance of current eXtreme Adaptive Optics (XAO) systems can be improved by adding a second AO correction stage featuring its own wavefront sensor, deformable mirror, and real-time controller. We develop a dynamical model for such a cascade AO (CAO) system with two stages each controlled by a standard integrator, and study its control properties. We study how such a configuration can improve an existing system without modifying the first stage. We analyze the CAO architecture in general and show how part of the disturbance is transferred from low to high temporal frequencies with a nefarious effect of the second stage integrator overshoot, and suggest possible ways to mitigate this. We also carry out numerical simulations of the particular case of a first stage AO using a Shack-Hartmann wavefront sensor and a second stage AO with a smaller deformable mirror running at a higher framerate to reduce temporal error. In this case, we demonstrate that the second stage improves imaging contrast by one order of magnitude and shortens the decorrelation time of atmospheric turbulence speckles by even a greater factor. The results show that CAO presents a promising and relatively simple way to upgrade some existing XAO systems and achieve improved imaging contrasts fostering a large number of science cases including the direct imaging of Exoplanets.