• Chinese Optics Letters
  • Vol. 17, Issue 6, 061101 (2019)
Min Li1,2,3, Xin Liu2, Ang Zhang1,2,*, and Hao Xian1,2,**
Author Affiliations
  • 1Key Laboratory of Adaptive Optics, Chinese Academy of Sciences, Chengdu 610209, China
  • 2Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China
  • 3University of Chinese Academy of Sciences, Beijing 100049, China
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    DOI: 10.3788/COL201917.061101 Cite this Article Set citation alerts
    Min Li, Xin Liu, Ang Zhang, Hao Xian, "Telescope alignment based on the sharpness function of under-sampled images," Chin. Opt. Lett. 17, 061101 (2019) Copy Citation Text show less

    Abstract

    The precise alignment of a high-performance telescope is a key factor to ensure the imaging quality. However, for telescopes with a wide field of view, the images are sometimes under-sampled. To study the effects of under-sampled images on the precision of telescope alignment, numerical simulations are implemented with the stochastic parallel gradient descent algorithm. The results show that the alignment program can converge stably and quickly. However, with the reduction of the full width at half-maximum of images, the relative residual errors increase from 9.5% to 19.5%, and the wavefront errors raise from 0.0972λ to 0.1074λ, indicating that the accuracy of the alignment decreases.
    vs=1000a2lp/mmvN=vs2=500a2lp/mm,(1)

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    δ2=1.22λDftelescope=1.22λF#,(2)

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    vmax=2δ=11.22λF#.(3)

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    vmaxvs/2δ42a.(4)

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    uk+1=ukγδJkδuk,(5)

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    J=(xx0)2+(yy0)2I(x,y)dxdyI(x,y)dxdy,(6)

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    Min Li, Xin Liu, Ang Zhang, Hao Xian, "Telescope alignment based on the sharpness function of under-sampled images," Chin. Opt. Lett. 17, 061101 (2019)
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