• Acta Optica Sinica
  • Vol. 39, Issue 3, 0315006 (2019)
Junfeng Xie1, Hong Zhu1、*, Pin Li2, Fan Mo1, and Xiang Li1、2
Author Affiliations
  • 1 Satellite Surveying and Mapping Application Center, National Administration of Surveying, Mapping and Geoinformation, Beijing 100048, China
  • 2 School of Surveying and Geographical Science, Liaoning Technical University, Fuxin, Liaoning 123000, China
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    DOI: 10.3788/AOS201939.0315006 Cite this Article Set citation alerts
    Junfeng Xie, Hong Zhu, Pin Li, Fan Mo, Xiang Li. Stellar Image Denoising Method for Active Pixel Sensor Based on Dynamic Sequential Noise Template[J]. Acta Optica Sinica, 2019, 39(3): 0315006 Copy Citation Text show less

    Abstract

    A stellar image denoising method for active pixel sensor (APS) based on dynamic sequential noise template is proposed. In this method, a dynamic sequential noise template is constructed based on the short-term static background noise and the random noise threshold, which is used to realize the denoising treatment of APS stellar images. The original APS stellar image of the ZY-3 is used as the test data and the research results show that the proposed method can eliminate strip and edge noises very well. Compared with the traditional denoising method, the proposed method can improve the extraction accuracy of the stellar image centroid by approximately 12.98″. Compared with the global threshold segmentation method, the proposed method can improve the extraction accuracy by about 2.16″. Compared with the static background noise method, the proposed method can improve the extraction accuracy by around 9.64″. These fully indicate that the proposed method can effectively improve the positioning accuracy of APS stellar centroid and can be used in attitude post-processing.
    Junfeng Xie, Hong Zhu, Pin Li, Fan Mo, Xiang Li. Stellar Image Denoising Method for Active Pixel Sensor Based on Dynamic Sequential Noise Template[J]. Acta Optica Sinica, 2019, 39(3): 0315006
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