Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary Mirror

Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary Mirror

A low frequency wavefront aberration correction method for solar telescopes based on secondary mirror movement is proposed to correct dynamic wavefront aberration during the operation of solar telescope. The correction ability of this method is analyzed and validated by numerical simulation and expe...

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Bibliographic Details
Main Authors: Yawei Xiao, Simin Zhao, Junbo Zhang, Linhai Huang, Naiting Gu
Format: Article
Language:English
Published: IEEE 2024-01-01
Series:IEEE Photonics Journal
Subjects:
Imaging system
aberration correction
secondary mirror
sensitivity matrix method
solar telescope
Online Access:https://ieeexplore.ieee.org/document/10480536/

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