摘要
Dispersed Rayleigh Interferometry has been verified a potential way to co-phasing segmented mirror in orbit using natural star as beacon. Measurement error caused by background star around beacon is analyzed under specific system parameters, and tolerances of magnitude difference in two orthogonal directions are also presented. To achieve 10nm / 20nm accuracy, minimum magnitude difference of background star and beacon star is about 2.5M / 1.7M. Furthermore, it is proved by calculating more than 6000 positions of background star distributed in an area about twice larger than the Airy disk in diameter.
源语言 | 英语 |
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主期刊名 | 5th International Symposium on Advanced Optical Manufacturing and Testing Technologies |
主期刊副标题 | Large Mirrors and Telescopes |
DOI | |
出版状态 | 已出版 - 2010 |
活动 | 5th International Symposium on Advanced Optical Manufacturing and Testing Technologies: Large Mirrors and Telescopes - Dalian, 中国 期限: 26 4月 2010 → 29 4月 2010 |
出版系列
姓名 | Proceedings of SPIE - The International Society for Optical Engineering |
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卷 | 7654 |
ISSN(印刷版) | 0277-786X |
会议
会议 | 5th International Symposium on Advanced Optical Manufacturing and Testing Technologies: Large Mirrors and Telescopes |
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国家/地区 | 中国 |
市 | Dalian |
时期 | 26/04/10 → 29/04/10 |
指纹
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Wang, S., Zhu, Q., & Huang, T. (2010). Co-phasing of segmented mirrors using Dispersed Rayleigh Interferometry in the presence of background star. 在 5th International Symposium on Advanced Optical Manufacturing and Testing Technologies: Large Mirrors and Telescopes 文章 76540X (Proceedings of SPIE - The International Society for Optical Engineering; 卷 7654). https://doi.org/10.1117/12.867108