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Novel Active Tuned Mass Damper Control Method for Space Telescope
Xu, Z. B.; J. F. Yang; Y. Y. Gu; Q. W. Wu; Z. T. Luo and H. W. Liu
2016
Source PublicationJournal of Guidance Control and Dynamics
Volume39Issue:3
AbstractPolarization aberration (PA) is a serious issue that affects imaging quality for optical systems with high numerical aperture. Numerous studies have focused on the distribution rule of PA on the pupil, but the field remains poorly studied. We previously developed an orthonormal set of polynomials to reveal the pupil and field dependences of PA in rotationally symmetric optical systems. However, factors, such as intrinsic birefringence of cubic crystalline material in deep ultraviolet optics and tolerance, break the rotational symmetry of PA. In this paper, we extend the polynomials from rotationally symmetric to M-fold to describe the PA of M-fold optical systems. Two examples are presented to verify the polynomials. (C)2016 Optical Society of America
Subtype期刊
Indexed BySCI ; EI
Language英语
Document Type期刊论文
Identifierhttp://ir.ciomp.ac.cn/handle/181722/57321
Collection中科院长春光机所知识产出
Recommended Citation
GB/T 7714
Xu, Z. B.,J. F. Yang,Y. Y. Gu,et al. Novel Active Tuned Mass Damper Control Method for Space Telescope[J]. Journal of Guidance Control and Dynamics,2016,39(3).
APA Xu, Z. B.,J. F. Yang,Y. Y. Gu,Q. W. Wu,&Z. T. Luo and H. W. Liu.(2016).Novel Active Tuned Mass Damper Control Method for Space Telescope.Journal of Guidance Control and Dynamics,39(3).
MLA Xu, Z. B.,et al."Novel Active Tuned Mass Damper Control Method for Space Telescope".Journal of Guidance Control and Dynamics 39.3(2016).
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