Poster + Paper
29 August 2022 Making adaptive optics available to all: a concept for 1m class telescopes
Author Affiliations +
Conference Poster
Abstract
Adaptive optics is an advanced technique developed for large telescopes. It turns out to be challenging for smaller telescopes (0.5~2m) due to the small isoplanatic angle, small subapertures and high correction speeds needed at visible wavelengths, requiring bright stars for guiding, severely limiting the sky coverage. The motivation to develop compact and robust AO system for small telescopes is two-fold: On the one hand, schools and universities often have access to small telescopes as part of their education programs. Also, researchers in countries with fewer resources could also benefit from well-engineered and reliable adaptive optics on smaller telescopes for research and education purposes. On the other hand, amateur astronomers and enthusiasts want improved image quality for visual observation and astrophotography. Implementing readily accessible adaptive optics in astronomy clubs would also likely have a significant impact on citizen science.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Olivier Lai, Stefan Kuiper, Niek J. Doelman, Mark Chun, Dirk Schmidt, Frantz Martinache, Marcel Carbillet, Mamadou N'Diaye, and Jean Pierre Rivet "Making adaptive optics available to all: a concept for 1m class telescopes", Proc. SPIE 12185, Adaptive Optics Systems VIII, 1218576 (29 August 2022); https://doi.org/10.1117/12.2626074
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Stars

Wavefront sensors

Adaptive optics

Turbulence

Deformable mirrors

Sensors

RELATED CONTENT


Back to Top