Acta Photonica Sinica, Volume. 39, Issue 6, 1115(2010)

Measuring the Tip-tilt Angles of the Active Mirror in the Stellar Interferometer

LU Yi*, FAN Wei-jun, and KONG Ming
Author Affiliations
  • [in Chinese]
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    Using laser interference technology,computer control technology and data image processing technology,the CCD interferometer measuration system is designed.Then,the mathematical model between the interferogram and the tip-tilt angles is deduced.After preprocessing the interferogram and thinning the fringes,least square method is used to fit the fringes.Based on equal thickness interferometer theory,the tip-tilt angle parameters of the active mirrors are obtained.The X axis′s movement range is 56″.872,and the resolution is 0″.113.The Y axis′s movement range is 49″.835,and the resolution is 0″.112.

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    LU Yi, FAN Wei-jun, KONG Ming. Measuring the Tip-tilt Angles of the Active Mirror in the Stellar Interferometer[J]. Acta Photonica Sinica, 2010, 39(6): 1115

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    Paper Information

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    Received: Nov. 11, 2009

    Accepted: --

    Published Online: Aug. 31, 2010

    The Author Email: Yi LU (luyi9798@cjlu.edu.cn)

    DOI:

    CSTR:32186.14.

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