Presentation + Paper
20 December 2022 An in-orbit correction method based on CNN for the figure errors and component misalignments of TMA telescope
Author Affiliations +
Abstract
To realize the fast and simple in-orbit aberration correction of TMA telescope, an aberration correction method based on Convolutional Neural Network (CNN) is proposed. CNN is trained to establish the relationship between the defocus point spread function and the misalignments of the secondary mirror. The wavefront aberration caused by the figure errors of the primary mirror and the misalignments of the secondary mirror and the tertiary mirror can be compensated by adjusting the secondary mirror according to the outputs of the well-trained CNN (named as Cor-Net). This method can correct the system aberration quickly and the RMS of the system wavefront aberration is reduced from about 1.5 λ to 0.1 λ by only three correction cycles.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bingdao Li, Xiaofang Zhang, Yun Gu, and Xinqi Hu "An in-orbit correction method based on CNN for the figure errors and component misalignments of TMA telescope", Proc. SPIE 12315, Optical Design and Testing XII, 123150T (20 December 2022); https://doi.org/10.1117/12.2643878
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Point spread functions

Telescopes

Wavefront aberrations

Mirrors

Monochromatic aberrations

Wavefront sensors

Wavefronts

Back to Top