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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Hlavní autoři:	Yawei Xiao, Simin Zhao, Junbo Zhang, Linhai Huang, Naiting Gu
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IEEE 2024-01-01
Edice:	IEEE Photonics Journal
Témata:	Imaging system aberration correction secondary mirror sensitivity matrix method solar telescope
On-line přístup:	https://ieeexplore.ieee.org/document/10480536/
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