Adaptive Optics system of the Evanescent Wave Coronagraph (EvWaCo): optimised phase plate and DM characterisation
Anthony Berdeu (NARIT), Sitthichat Sukpholtham (NARIT), Puttiwat, Kongkaew (NARIT), Adithep Kawinkij (NARIT), Matthew Ridsdill-Smith (NARIT),, Michel Tallon (CRAL), \'Eric Thi\'ebaut (CRAL), Maud Langlois (CRAL), Mary, Angelie Alagao (NARIT)

TL;DR
This paper details the development of a bench to characterize the Extreme Adaptive Optics system of the EvWaCo coronagraph, focusing on precise turbulence simulation, deformable mirror characterization, and influence function analysis.
Contribution
It introduces a method to design phase screens with controlled Kolmogorov statistics and provides a comprehensive characterization of the ALPAO deformable mirror for adaptive optics applications.
Findings
Controlled Kolmogorov turbulence simulation achieved
Deformable mirror influence functions characterized in detail
Linearity and offsets of actuators analyzed
Abstract
The Evanescent Wave Coronagraph (EvWaCo) is an achromatic coronagraph mask with adjustable size over the spectral domain [600nm, 900nm] that will be installed at the Thai National Observatory. We present in this work the development of a bench to characterise its Extreme Adaptive Optics system (XAO) comprising a DM192 ALPAO deformable mirror (DM) and a 15x15 Shack-Hartmann wavefront sensor (SH-WFS). In this bench, the turbulence is simulated using a rotating phase plate in a pupil plane. In general, such components are designed using a randomly generated phase screen. Such single realisation does not necessarily provide the wanted structure function. We present a solution to design the printed pattern to ensure that the beam sees a strict and controlled Kolmogorov statistics with the correct 2D structure function. This is essential to control the experimental conditions in order to…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Optical Wireless Communication Technologies · Stellar, planetary, and galactic studies
