Evaluation of the performance of large telescope based on normalized point source sensitivity

Qichang, 安其昌 An; Jing-xu, 张景旭 Zhang; Fei, 杨飞 Yang; Hong-chao, 赵宏超 Zhao

doi:10.3788/irla201645.1218001

Cited by 2 publications

(2 citation statements)

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“…Here, MTF e , MTF a , and MTF p are the optical modulation functions of telescope error, atmosphere, and ideal value, respectively (An et al, 2016).…”

Section: Pssn and Perturbation Calculationmentioning

confidence: 99%

Jitter error evaluation in large-aperture optical telescopes based on normalized point source sensitivity

Yuan-Guo,

Fei,

Jia-Kang

et al. 2023

Front. Astron. Space Sci.

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To comprehensively analyze the jitter error in large-aperture optical telescopes, this paper introduces normalized point source sensitivity (PSSn) to evaluate the telescope system. First, the concept and basic properties of PSSn were introduced, and then the jitter error under expected random loads and the contribution percentage of each mode to the total jitter were analyzed through a model. The PSSn of the system under the influence of different error sources was studied, and its variation trend was estimated. A comparison of evaluation methods, such as the Strehl ratio, and the proposed method reflects the characteristics of more accurate data and a more concise calculation. The jitter error evaluation method proposed in this article, combined with PSSn, provides practical and beneficial guidance for the design and detection of large-aperture optical telescope systems.

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“…Here, MTF e , MTF a , and MTF p are the optical modulation functions of telescope error, atmosphere, and ideal value, respectively (An et al, 2016).…”

Section: Pssn and Perturbation Calculationmentioning

confidence: 99%

Jitter error evaluation in large-aperture optical telescopes based on normalized point source sensitivity

Yuan-Guo,

Fei,

Jia-Kang

et al. 2023

Front. Astron. Space Sci.

View full text Add to dashboard Cite

show abstract

“…Alternative methods for rectifying wavefront errors either take place at a telescope's entrance pupil or collaborate to mitigate phase deviations introduced by other components within the optical chain. This collaborative approach is referred to as Active Optics (AO) [2,3].…”

Section: Introductionmentioning

confidence: 99%

Morphing behavior of a piezoelectric deformable mirror under complex environment for space active optics

Gong,

Yu,

Wang

2023

AOPC 2023: Novel Technologies and Instruments for Astronomical Imaging and Spectroscopy

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Evaluation of the performance of large telescope based on normalized point source sensitivity

Cited by 2 publications

References 0 publications

Jitter error evaluation in large-aperture optical telescopes based on normalized point source sensitivity

Jitter error evaluation in large-aperture optical telescopes based on normalized point source sensitivity

Morphing behavior of a piezoelectric deformable mirror under complex environment for space active optics

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