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	Design of reflective Fizeau optical synthetic aperture imaging system 会议论文 OAI收割 Beijing, China, 2023-07-25 作者: Zhang, Wenmao; Yang, Jianfeng; Zhao, Yiyi \| 收藏 \| 浏览/下载：4/0 \| 提交时间：2024/02/28 Optical synthetic aperture Fizeau-type Off-axis three-mirror Optical design
	Experimental study on the extension of nodal aberration theory to pupil-offset off-axis three-mirror anastigmatic telescopes 期刊论文 OAI收割 Journal of Astronomical Telescopes Instruments and Systems, 2019, 卷号: 5, 期号: 2, 页码: 12 作者: G.H.Ju; H.C.Ma; Z.Y.Gu; C.X.Yan \| 收藏 \| 浏览/下载：29/0 \| 提交时间：2020/08/24 aberration fields,off-axis three-mirror anastigmatic telescopes,lateral misalignments,nodal aberration theory,5th-order optical aberrations,rotational symmetry,systems
	Optical design of diffractive telescope system based on off-axis three mirror 会议论文 OAI收割 Chengdu, PEOPLES R CHINAChengdu, PEOPLES R CHINA, JUN 26-29, 2018JUN 26-29, 2018 作者: He, Chuanwang; Huang, Peng; Dong, Xiaochun; Fan, Bin \| 收藏 \| 浏览/下载：32/0 \| 提交时间：2019/08/23 Diffractive telescope Off-axis three mirror Schupmann Optical design Image analysis
	A large field of view optical system design for space target detection 会议论文 OAI收割 Shanghai, China, 2018-05-08 作者: Ni, Dongwei; Li, Xuyang \| 收藏 \| 浏览/下载：30/0 \| 提交时间：2018/09/20 Target Detection Off-axis Three-mirror Large Field Of View Zernike Polynomials Xy Polynomials Freeform Surfaces
	Broadband and wide field of view foveated imaging system in space 期刊论文 OAI收割 optical engineering, 2008, 卷号: 47, 期号: 10, 页码: 103202 作者: Zhao, Xiaoxia; Xie, Yongjun; Zhao, Wei 收藏 \| 浏览/下载：13/0 \| 提交时间：2011/09/30 aberration compensation optical systems design three-mirror off-axis optical system microelectromechanical system deformable mirrors
	Optical system design with high resolution and large field of view for the remote sensor (EI CONFERENCE) 会议论文 OAI收割 Chang J.; Weng Z.-C.; Wang Y.-T.; Cheng D.-W.; Jiang H.-L. 收藏 \| 浏览/下载：29/0 \| 提交时间：2013/03/25 In this paper we are presenting a design method and its results for a space optical system with high resolution and wide field of view. This optical system can be used both in infrared and visible configurations. The designing of this system is based on an on-axis three-mirror anastigmatic (TMA) system. Here the on-axis concept allows wide field of view (FOV) enabling a diversity of designs available for the Multi-Object Spectrometer instruments optimized for low scattered and low emissive light. The available FOVs are upto 1 in both spectrum ranges whereas the available aperture range is F/15 - F/10. The final optical system is a three-mirror telescope with two on-axis and one off-axis segment and its resolution is 0.3m or even lower. The distinguished feature of this design is that it maintains diffraction-limited image at wide wavelengths. The technological developments in the field of computer generated shaping of large-sized optical surface details with diffraction-limited imagery have opened new avenues towards the designing techniques. Such techniques permit us to expand these technological opportunities to fabricate the aspherical off-axis mirrors for a complex configuration.
	Method for computer-aided alignment of complex optical system (EI CONFERENCE) 会议论文 OAI收割 2nd International Symposium on Advanced Optical Manufacturing and Testing Technologies: Optical Test and Measurement Technology and Equipment, November 2, 2005 - November 5, 2005, Zian, China 作者: Yu J. 收藏 \| 浏览/下载：27/0 \| 提交时间：2013/03/25 For making complex optical system meet the design requirement such as the space camera used in remote sensing and UVX lithophotography especially for off-axis all-reflecting optical system alignment technology is so necessary. In this paper a method is presented. Based on the ideas of linearity instead of non-linearity and difference quotient instead of differential quotient a mathematical model for computer-aided alignment is proposed. This model included the characteristics of the optical system wavefront difference of its exit pupil and its misalignment of the misaligned optical system. Then comparing self-compiled software with alignment package of CODE V as a result this self-compiled software is much more valid than alignment package of CODE V. For a large aperture long focal length and off-axis three-mirror optical system computer-aided alignment is successful. Finally the wavefront error of the middle field is 0.094 waves RMS and the wavefront error of +0.7 field is 0.106 waves RMS and the wavefront error of -0.7 field is 0.125 waves RMS at =632.8nm are obtained.