Acta Optica Sinica, Volume. 37, Issue 11, 1128003(2017)

A Star Sensor Calibration Method Based on Attitude Correlated Frame

Yu Liu, Dongkai Dai*, Liheng Ma, Sihua Fu, and Xingshu Wang
Author Affiliations
  • College of Optoelectronic Science and Engineering, National University of Defense Technology, Changsha, Hunan 410073, China
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    A star sensor calibration method based on the attitude correlated frame (ACF) is proposed, which can realize the calibration by the astronomical observation outdoors. First, the correlated superposition among the multi-frame star maps is achieved by utilizing the high accuracy angle information provided by the gyro unit which is installed in a strapdown manner with the star sensor. Then, the imaging mapping model between the star and the image point among the multi-frame star maps is established. Finally, the global optimization of the intrinsic parameters for the star sensor is realized by using the least square algorithm. The simulation results show that the proposed method is more precise and robust than the calibration method based on the interstar angles. Moreover, the installation matrix between the star sensor and the gyro unit can be calibrated simultaneously by this method, and thus it is suitable for the parameter calibration of the shipboard, airborne inertial/celestial integrated navigation systems.

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    Yu Liu, Dongkai Dai, Liheng Ma, Sihua Fu, Xingshu Wang. A Star Sensor Calibration Method Based on Attitude Correlated Frame[J]. Acta Optica Sinica, 2017, 37(11): 1128003

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    Paper Information

    Category: Remote Sensing and Sensors

    Received: Jun. 14, 2017

    Accepted: --

    Published Online: Sep. 7, 2018

    The Author Email: Dai Dongkai (daidongkai@nudt.edu.cn)

    DOI:10.3788/AOS201737.1128003

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