Proceedings Paper
Research on aberration theory of star track systems| Format | Member Price | Non-Member Price |
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Paper Abstract
CCD star tracker is a key equipment of satellites. It works at a broad range of wavelength, from visible
wavelength to near infrared. Here we just try to analyze the influence of aberrations based on an actual
system (focal length: 120mm, F number: 1.3, field of view: 12deg, wavelength range: 0.45 micron to
0.85 micron). A double Gauss system is used to decrease the chromatic aberration while other
aberrations are also controlled very well. The result shows that we can get some conclusions about the
influence of coma which is the most significant aberration in this system.
Paper Details
Date Published: 28 January 2009
PDF: 8 pages
Proc. SPIE 7156, 2008 International Conference on Optical Instruments and Technology: Optical Systems and Optoelectronic Instruments, 715632 (28 January 2009); doi: 10.1117/12.811799
Published in SPIE Proceedings Vol. 7156:
2008 International Conference on Optical Instruments and Technology: Optical Systems and Optoelectronic Instruments
Yunlong Sheng; Yongtian Wang; Lijiang Zeng, Editor(s)
PDF: 8 pages
Proc. SPIE 7156, 2008 International Conference on Optical Instruments and Technology: Optical Systems and Optoelectronic Instruments, 715632 (28 January 2009); doi: 10.1117/12.811799
Show Author Affiliations
Jun Chang, Beijing Institute of Technology (China)
Yuncai Hao, Beijing Institute of Controller (China)
Yuncai Hao, Beijing Institute of Controller (China)
Jian Liu, Beijing Institute of Technology (China)
Published in SPIE Proceedings Vol. 7156:
2008 International Conference on Optical Instruments and Technology: Optical Systems and Optoelectronic Instruments
Yunlong Sheng; Yongtian Wang; Lijiang Zeng, Editor(s)
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