Poster + Paper
27 August 2024 Estimating atmospheric wind speeds from Gemini planet imager AO telemetry
Zhenxi Du, Saavidra Perera, Daniel Levinstein, Quinn Konopacky, Alex Madurowicz, Bruce Macintosh, Lisa Poyneer, Richard Wilson, Ollie Farley
Author Affiliations +
Conference Poster
Abstract
The Earth’s atmosphere is comprised of turbulent layers that result in speckled and blurry images from ground-based visible and infrared observations. Adaptive Optics (AO) systems are employed to measure the perturbed wavefront with a wavefront sensor (WFS) and correct for these distortions with a deformable mirror. Therefore, understanding and characterising the atmosphere is crucial for the design and functionality of AO systems. One parameter for characterizing the atmosphere is the atmospheric coherence time, which is a function of the effective wind velocity of the atmosphere. This parameter dictates how fast the AO system needs to correct for the atmosphere. If not fast enough, phenomena such as the wind butterfly effect can occur, hindering high-contrast coronographic imaging. This effect is a result of fast, strong, high-altitude turbulent layers. This paper presents two methods for estimating the effective wind velocity, using pseudo-open loop WFS slopes. The first method uses a spatial-temporal covariance map and the second uses the power spectral density of the defocus term. We show both simulated results and preliminary results from the Gemini Planet Imager AO telemetry.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Zhenxi Du, Saavidra Perera, Daniel Levinstein, Quinn Konopacky, Alex Madurowicz, Bruce Macintosh, Lisa Poyneer, Richard Wilson, and Ollie Farley "Estimating atmospheric wind speeds from Gemini planet imager AO telemetry", Proc. SPIE 13097, Adaptive Optics Systems IX, 130974E (27 August 2024); https://doi.org/10.1117/12.3020607
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KEYWORDS
Covariance

Wind speed

Adaptive optics

Gemini Planet Imager

Wavefront sensors

Turbulence

Wind measurement

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