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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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Principais autores: Yawei Xiao, Simin Zhao, Junbo Zhang, Linhai Huang, Naiting Gu
Formato: Artigo
Idioma:Inglês
Publicado em: IEEE 2024-01-01
coleção:IEEE Photonics Journal
Assuntos:
Imaging system
aberration correction
secondary mirror
sensitivity matrix method
solar telescope
Acesso em linha:https://ieeexplore.ieee.org/document/10480536/
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