• 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
    Schematic of multi-frame continuous stellar image. (a) First frame; (b) second frame; (c) kth frame
    Fig. 1. Schematic of multi-frame continuous stellar image. (a) First frame; (b) second frame; (c) kth frame
    Flow chart of stellar image sequence denoising
    Fig. 2. Flow chart of stellar image sequence denoising
    Schematic of acquisition of static background noise
    Fig. 3. Schematic of acquisition of static background noise
    Original stellar images. (a) First frame; (b) 55th frame; (c) 124th frame
    Fig. 4. Original stellar images. (a) First frame; (b) 55th frame; (c) 124th frame
    Background noise. (a) Template; (b) three-dimensional view
    Fig. 5. Background noise. (a) Template; (b) three-dimensional view
    Comparison of stellar images before and after denoising. (a) Before denoising; (b) after denoising
    Fig. 6. Comparison of stellar images before and after denoising. (a) Before denoising; (b) after denoising
    Partial enlargement images. (a) Before denoising; (b) after denoising
    Fig. 7. Partial enlargement images. (a) Before denoising; (b) after denoising
    Comparison of results of many denoising methods. (a) Gaussian filtering; (b) global threshold method; (c) static background template; (d) proposed method
    Fig. 8. Comparison of results of many denoising methods. (a) Gaussian filtering; (b) global threshold method; (c) static background template; (d) proposed method
    Test results of first frame stellar image. (a) Extracted centroid coordinates; (b) star angular distance error
    Fig. 9. Test results of first frame stellar image. (a) Extracted centroid coordinates; (b) star angular distance error
    Star angular distance error. (a) Gaussian filtering; (b) global threshold segmentation; (c) static noise template; (d) dynamic background noise template
    Fig. 10. Star angular distance error. (a) Gaussian filtering; (b) global threshold segmentation; (c) static noise template; (d) dynamic background noise template
    IndexParameter
    Focal length /mm43.3
    Projection central coordinate(512,512)
    APS array size1024×1024
    Field angle /[(°)×(°)]20×20
    Lens hood /(°)38
    Pixel size /(μm×μm)15×15
    Exposure time /ms125,200,250,500
    Output frequency /Hz2,1.66
    Pointing accuracy5″(3σ)
    Update frequency /Hz4
    Table 1. Parameters of ZY-3 01/02 star stacker component 1 (APS)
    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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