[PERSON]  
1 Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China; saiosh1,[EMAIL_ADDRESS] (L.S. ); [EMAIL_ADDRESS] (XL. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.Y. ); [EMAIL_ADDRESS] (XL.) [PERSON]  
1 Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China; saiosh1,[EMAIL_ADDRESS] (XL.S. ); [EMAIL_ADDRESS] (XL. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.Y. ); [EMAIL_ADDRESS] (XL.) [PERSON]  
1 Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China; saiosh1,[EMAIL_ADDRESS] (L.S. ); [EMAIL_ADDRESS] (XL. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.Y. ); [EMAIL_ADDRESS] (XL.) [PERSON]  
1 Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China; saiosh1,[EMAIL_ADDRESS] (L.S. ); [EMAIL_ADDRESS] (XL. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.Y. ); [EMAIL_ADDRESS] (XL.) [PERSON]  
1 Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China; saiosh1,[EMAIL_ADDRESS] (XL.S. ); [EMAIL_ADDRESS] (XL. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.Y. ); [EMAIL_ADDRESS] (XL.) [PERSON]  
1 Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China; saiosh1,[EMAIL_ADDRESS] (L.S. ); [EMAIL_ADDRESS] (XL. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.Y. ); [EMAIL_ADDRESS] (XL.) [PERSON]  
1 Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China; saiosh1,[EMAIL_ADDRESS] (L.S. ); [EMAIL_ADDRESS] (XL. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.C. ); [EMAIL_ADDRESS] (X.Y. ); [EMAIL_ADDRESS] (XL.) [PERSON]  
1 Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China; saiosh1,[EMAIL_ADDRESS] (XL.S. ); [EMAIL_ADDRESS] (XL. ); [EMAIL_ADDRESS] (X.C. indoor mirror conditions, applicable at any incident zenith angle. However, overcoming the effects of sea surface fluctuations remains a challenge in practical applications. Addressing these fluctuations, [PERSON] et al. [16], in 2016, utilized the Fresnel and Cox-Munk models to establish a mid-wave infrared polarization imaging system, achieving glare suppression by adjusting the angles of dual polarizers in front of the detector. In 2017, [PERSON] and colleagues [11] analyzed the polarization characteristics of sea surface glare and maritime targets, designing a visible light polarization detection system based on a dual linear polarizer. Although utilizing fixed polarization angles can effectively suppress sea surface glare, this method lacks adaptability to the varying characteristics of the glare. Consequently, researchers have proposed combined image processing approaches to enhance the adaptability of sea surface glare suppression methods. In 2019, [PERSON] et al. [12] introduced a solar glare suppression method based on the fusion of polarimetric radiance maps. In 2021, [PERSON] and colleagues [7] implemented effective suppression of sea surface glare through the temporal fusion of image sequences generated with real-time polarization information. [PERSON] and her team [14] proposed a method combining polarization filtering with polynomial fitting to suppress solar glare. In 2022, [PERSON] et al. [15] combined both single and dual polarizer modes with digital image filtering algorithms to suppress the background of solar glare. While the integration of fixed polarizers and image processing has improved the adaptability of sea surface glare suppression, its capacity to adapt remains limited. Given the time-varying nature of sea surface glare polarization states, influenced by lighting conditions and water fluctuations, this approach still struggles with precise suppression.