Optical design and coating optimization of the Wolter-I X-ray telescope

The optical design of the nested paraboloid and hyperboloid Wolter I X-ray telescope of the eXTP satellite in the 1–8 keV band was systematically studied. The recursive relationship of nested structures is derived, and an analysis is conducted on the influence of initial parameters on performance. Considering the requirements of X-ray astronomical observation in China, we propose the initial structure of the model and design seven groups of Au/C/Ni non-periodic dual-layer coatings between the innermost and outermost layers of the mirror. The effective area, half-power diameter, and stray light were calculated in the simulation. The results show that the effective area can reach 1000cm 2 at 2 keV, the effective area can reach 890cm 2 at 6 keV without hub obscuration, the half-power diameter is 10 arcsec, and the proportion of stray light is 4.2%.

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Publication Details

Journal
Applied Optics
Published
2024-09-10
DOI
https://doi.org/10.1364/ao.533818
Citations
2
Primary Topic
Advanced X-ray Imaging Techniques
Type
article
Field-Weighted Citation Impact
1.22
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article

Optical design and coating optimization of the Wolter-I X-ray telescope

Qingyong Zhou, Lizhi Sheng, Pengfei Qiang, Yongqing Yan et al.
2 citations
Applied Optics
Advanced X-ray Imaging Techniques
1.22
article

Optical design and coating optimization of the Wolter-I X-ray telescope

Qingyong Zhou, Lizhi Sheng, Pengfei Qiang, Yongqing Yan, Yanji Yang, Yujia Geng, Yue Li, renzhou zheng, Bingqing Yang
article en
2 citations

Abstract

The optical design of the nested paraboloid and hyperboloid Wolter I X-ray telescope of the eXTP satellite in the 1–8 keV band was systematically studied. The recursive relationship of nested structures is derived, and an analysis is conducted on the influence of initial parameters on performance. Considering the requirements of X-ray astronomical observation in China, we propose the initial structure of the model and design seven groups of Au/C/Ni non-periodic dual-layer coatings between the innermost and outermost layers of the mirror. The effective area, half-power diameter, and stray light were calculated in the simulation. The results show that the effective area can reach 1000cm 2 at 2 keV, the effective area can reach 890cm 2 at 6 keV without hub obscuration, the half-power diameter is 10 arcsec, and the proportion of stray light is 4.2%.

Applied OpticsVol. 63(28)
Chinese Academy of Sciences (CN), Xi'an Institute of Optics and Precision Mechanics (CN), University of Chinese Academy of Sciences (CN)
Affordable and clean energy
Openalex Percentile: Top 21%
Advanced X-ray Imaging Techniques
1.22
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