• Laser & Optoelectronics Progress
  • Vol. 58, Issue 20, 2001003 (2021)
Yu Deng1、2、**, Qiang Fu1, Su Zhang1, Changli Li2、*, Juntong Zhan1, and Yingchao Li1
Author Affiliations
  • 1Key Laboratory of Space Optoelectronic Technology in Jilin Province, Changchun, Jilin 130022, China
  • 2Faculty of Science, Changchun University of Science and Technology, Changchun, Jilin 130022, China
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    DOI: 10.3788/LOP202158.2001003 Cite this Article Set citation alerts
    Yu Deng, Qiang Fu, Su Zhang, Changli Li, Juntong Zhan, Yingchao Li. Method of Suppressing Sea Surface Solar Flare Based on Polarization Detection Technology[J]. Laser & Optoelectronics Progress, 2021, 58(20): 2001003 Copy Citation Text show less
    Principle of the polarization measurement system
    Fig. 1. Principle of the polarization measurement system
    Schematic diagram of the BRDF
    Fig. 2. Schematic diagram of the BRDF
    Schematic diagram of the Fresnel reflection
    Fig. 3. Schematic diagram of the Fresnel reflection
    Relationship curve between θi and Cp
    Fig. 4. Relationship curve between θi and Cp
    Experimental setup
    Fig. 5. Experimental setup
    SALSA full polarization camera. (a) Structure diagram; (b) physical map
    Fig. 6. SALSA full polarization camera. (a) Structure diagram; (b) physical map
    Selection of target and glare background ROI. (a) Glare background; (b) target
    Fig. 7. Selection of target and glare background ROI. (a) Glare background; (b) target
    Image of the change in contrast between the target and the glare background in the 550 nm band. (a) Observation zenith angle; (b) solar zenith angle
    Fig. 8. Image of the change in contrast between the target and the glare background in the 550 nm band. (a) Observation zenith angle; (b) solar zenith angle
    Image of the change in contrast between the target and the glare background in the 670 nm band. (a) Observation zenith angle; (b) solar zenith angle
    Fig. 9. Image of the change in contrast between the target and the glare background in the 670 nm band. (a) Observation zenith angle; (b) solar zenith angle
    Change curve of the contrast between the target and the solar flare with the observation zenith angle. (a) 550 nm; (b) 670 nm
    Fig. 10. Change curve of the contrast between the target and the solar flare with the observation zenith angle. (a) 550 nm; (b) 670 nm
    Change curve of the contrast between the target and the flare with the solar zenith angle when the observation zenith angle is 53°. (a) 550 nm; (b) 670nm
    Fig. 11. Change curve of the contrast between the target and the flare with the solar zenith angle when the observation zenith angle is 53°. (a) 550 nm; (b) 670nm
    Yu Deng, Qiang Fu, Su Zhang, Changli Li, Juntong Zhan, Yingchao Li. Method of Suppressing Sea Surface Solar Flare Based on Polarization Detection Technology[J]. Laser & Optoelectronics Progress, 2021, 58(20): 2001003
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