Laser & Optoelectronics Progress, Volume. 62, Issue 10, 1037004(2025)
Star-Identification Method Based on Voronoi Graph
Fig. 2. Algorithm feature distribution (limit magnitude 9.0). (a) Voronoi polygon edge number characteristics; (b) Voronoi polygon perimeter characteristics; (c) Voronoi polygon area characteristics; (d) adjacent star polygon perimeter characteristics; (e) adjacent star polygon area characteristics
Fig. 4. Experimental results of the algorithm. (a) Matching rate of the algorithm; (b) average running time of algorithm; (c) average number of stars matched by the algorithm; (d) local amplification graph of Fig.4 (c)
Fig. 5. Relationship diagram of limit magnitude, field radius and matching rate. (a) Contour map of limiting magnitude, field radius and matching rate; (b) contour map of field of view radius and limiting magnitude
Fig. 7. Influence of pseudo stars and missing stars on the algorithm. (a) Add N pseudo stars; (b) add M pseudo stars; (c) remove N stars; (d) remove M stars; (e) change M stars
Fig. 8. Comparison between the proposed algorithm and traditional algorithms. (a) Comparison of algorithm performance; (b) comparison of algorithm performance after adding stellar position error
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Xin Guo, Jiabin Wu, lin Li, Chun Jiang, Zhiyong Wu. Star-Identification Method Based on Voronoi Graph[J]. Laser & Optoelectronics Progress, 2025, 62(10): 1037004
Category: Digital Image Processing
Received: Aug. 28, 2024
Accepted: Nov. 26, 2024
Published Online: May. 8, 2025
The Author Email: Zhiyong Wu (wuzy@ciomp.ac.cn)
CSTR:32186.14.LOP241916