DocumentCode
233684
Title
Star extraction method for star sensor at a high angular rate
Author
Zong Hua ; Wang Bo ; Zhou Zhi Qiang ; Li Sun ; Lu Kun Feng ; Wang Hai Luo
Author_Institution
Sch. of Autom., Beijing Inst. of Technol., Beijing, China
fYear
2014
fDate
28-30 July 2014
Firstpage
613
Lastpage
617
Abstract
When a star sensor slews at a high angular rate, the stars in the sensed image are smeared out over many pixels, which results in a decreasing signal-to-noise ratio (SNR). Therefore, the faint stars are not capable of being detected, and the centroidal precision of the bright stars decrease when using traditional image threshold segmentation algorithm and centroid method. In this paper, we propose a method to obtain accurate star location for star sensor at a high angular rate. We first utilize Laplacian to segment the star image, and then each pixel is marked after it is compared with the neighbouring one. Finally, the centroids of stars are calculated by using target pixels, and the centroiding errors are compensated. The experiment results illustrate that the proposed technique can extract more stars than other traditional methods under the condition of high angular rate, and also can improve the locating precision of star effectively.
Keywords
aerospace instrumentation; angular measurement; image segmentation; image sensors; stars; SNR; bright star; centroidal precision method; image sensor; image threshold segmentation algorithm; signal-to-noise ratio; star extraction method; star image segmentation; star sensor; Accuracy; Adaptive optics; Aircraft; Image segmentation; Imaging; Laplace equations; Signal to noise ratio; Laplacian; Star sensor; star extraction;
fLanguage
English
Publisher
ieee
Conference_Titel
Control Conference (CCC), 2014 33rd Chinese
Conference_Location
Nanjing
Type
conf
DOI
10.1109/ChiCC.2014.6896695
Filename
6896695
Link To Document