Poster + Presentation + Paper
27 August 2022 Machine learning wavefront sensing for the James Webb Space Telescope
Heriniaina F. Rajaoberison, Joseph S. Tang, James R. Fienup
Author Affiliations +
Conference Poster
Abstract
The fine alignment of the James Webb Space Telescope (JWST)’s 18 primary mirror segments relies on image-based wavefront sensing. Previously a convolutional neural network (CNN) produced phase estimates with around 0.37 waves RMS error, which were adequate as starting guesses for phase retrieval to accurately predict global Zernike coefficients. In contrast, our study uses a CNN to sense segment piston errors between the 18 segments. Our trained CNN model could retrieve segment piston phase errors of ±0.5 waves from a single defocused point-spread function to within 0.02 waves RMS, without the need of additional phase retrieval algorithms.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Heriniaina F. Rajaoberison, Joseph S. Tang, and James R. Fienup "Machine learning wavefront sensing for the James Webb Space Telescope", Proc. SPIE 12180, Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave, 121806A (27 August 2022); https://doi.org/10.1117/12.2630621
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KEYWORDS
Point spread functions

James Webb Space Telescope

Data modeling

Wavefront sensors

Wavefronts

Machine learning

Computational imaging

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