Star Map Recognition Algorithm Based on Improved Log-Polar Transformation

Xuliang Yan; Wang Xu; Gongliu Yang; Lu Wang

doi:10.3788/AOS202141.1010001

[1] Wu Q, Zhang R. Wavelet denoising of near-earth all-day star map based on local outlier factor[J]. Acta Optica Sinica, 40, 0810001(2020).

[2] Jia Y D, Qiang J, Zhang L et al. Spaceborne long-distance tracking method based on adaptive vibration suppression[J]. Acta Optica Sinica, 40, 2212003(2020).

[3] Gai E, Daly K, Harrison J et al. Star-sensor-based satellite attitude/attitude rate estimator[J]. Journal of Guidance, Control, and Dynamics, 8, 560-565(1985).

[4] Yang J, Liang B, Zhang T et al. A novel systematic error compensation algorithm based on least squares support vector regression for star sensor image centroid estimation[J]. Sensors (Basel), 11, 7341-7363(2011).

[5] Zhang L J, Yang H B, Lu H P et al. Cubature Kalman filtering for relative spacecraft attitude and position estimation[J]. Acta Astronautica, 105, 254-264(2014). http://www.zhangqiaokeyan.com/academic-journal-foreign_other_thesis/0204110939309.html

[6] Wang Q, Fu Y T. Restoration of smearing stars in fine image stabilization of high-orbit satellites[J]. Acta Optica Sinica, 40, 1311002(2020).

[7] Cao Y, Li B Q, Li H T et al. High-accuracy star sensor centroid algorithm based on star image resampling[J]. Acta Optica Sinica, 39, 0712003(2019).

[8] Jin H, Zhai Z Y, Du W F et al. Method for experimental analysis of thermostability of star sensors[J]. Chinese Journal of Lasers, 47, 0404002(2020).

[9] Li X L, Yang J H, Zhang L et al. A fast all-sky autonomous star pattern identification algorithm[J]. Journal of Changchun University of Science and Technology (Natural Science Edition), 37, 43-47(2014).

[10] Guo L L, Zhao Q C, Yang Y et al. Method for suppression of impulse noise in spaceborne Fourier transform infrared spectrometer[J]. Acta Optica Sinica, 40, 0830003(2020).

[11] Wang H Y, Wang T F, Zhu H Y et al. Method for determining optimal radius value of defocused image spot of star sensor[J]. Laser & Optoelectronics Progress, 56, 101101(2019).

[12] Zhang K, Hu B X, Xu X P et al. A fast correlation matching algorithm based on log-polar transform[J]. Flight Dynamics, 38, 61-65(2020).

[13] Ran H C[J]. Review of image matching based on logarithmic polar coordinates Modern Computer, 2020, 65-69.

[14] Wei X G, Zhang G J, Jiang J. Star identification algorithm based on log-polar transform[J]. Journal of Aerospace Computing, Information, and Communication, 6, 483-490(2009).

[15] Toloei A, Zahednamazi M, Ghasemi R et al. A comparative analysis of star identification algorithms[J]. Astrophysics and Space Science, 365, 1-9(2020). http://www.researchgate.net/publication/340381582_A_comparative_analysis_of_star_identification_algorithms

[16] Li J, Wei X G, Wang G Y et al. Improved grid algorithm based on star pair pattern and two-dimensional angular distances for full-sky star identification[J]. IEEE Access, 8, 1010-1020(2019). http://ieeexplore.ieee.org/document/8937537/

[17] Liu X Y, Zhou Z F, Zhang Z L et al. Improvement of star identification based on star trace in star images[J]. Measurement, 105, 158-163(2017). http://www.sciencedirect.com/science/article/pii/S026322411730218X