EGU25-8158, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-8158
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Friday, 02 May, 10:45–12:30 (CEST), Display time Friday, 02 May, 08:30–12:30
 
Hall X4, X4.32
Arctic Sea Ice Lead Detection From China FY-3D MERSI-II Quality Enhanced Images 
Lu Zhang1, Fengming Hui1, Xiao Cheng1, Gang Li1, Xiaopo Zheng1, Zhaohui Chi2, Hang Yu3, Ling Sun4, and Shengli Wu4
Lu Zhang et al.
  • 1School of Geospatial Engineering and Science and the Key Laboratory of Comprehensive Observation of Polar Environment, Ministry of Education, Sun Yat-sen University, Zhuhai 519082, China, and also with the Southern Marine Science and Engineering Guangdong
  • 2Department of Geography, Texas A&M University, College Station, TX 77843 USA (zchi@tamu.edu)
  • 3Ji Hua Laboratory, Foshan, Guangdong 528200, China (yuhang@jihualab.com)
  • 4Key Laboratory of Radiometric Calibration and Validation for Environmental Satellites, National Satellite Meteorological Center (National Center for Space Weather), China Meteorological Administration, Beijing 100081, China (sunling@cma.gov.cn; wusl@cma.g

The 250-m resolution Chinese Fengyun-3D (FY-3D) Medium Resolution Spectral Imager-II (MERSI-II) thermal infrared (TIR) data can help us understand the rapid variations of Arctic sea ice leads, which are key features within the sea ice. The challenges of utilizing the 250-m FY-3D MERSI-II TIR data are bowtie effect and nonuniform brightness stripe noise.

While previous solutions have addressed these issues separately, this study introduces a more integrated two-step image quality enhancement strategy for MERSI-II TIR images. It considered the interactions between the two issues and overcame the excessive or inadequate destriping in existing models due to the ideal stripe-type assumption. Specifically, for the bowtie effect, a rigorous geometric model suitable for MERSI-II was constructed. For the nonuniform brightness stripe noise, a novel adaptive multiscale frequential (AMSF) algorithm was developed. The proposed strategy was outperforming existing methods in quantitative and qualitative assessments with higher efficiency on both bowtie effect and stripe noise removal. To validate the effectiveness of proposed strategy in sea ice lead detection, the temperature anomaly method was used to extract leads in winter Arctic Baffin Bay from images of varying quality. The results show that the overall accuracy improved from 0.88 to 0.95.

However, the sea ice lead extraction results from the traditional temperature anomaly method on TIR images is affected by the subjective selection of window sizes and is prone to misclassification caused by clouds. To address these issues, a novel deep learning method is applied to quality-enhanced FY-3D MERSI-II TIR images, which adaptively extracts sea ice leads and reduces cloud interference. Several commonly image segmentation networks: PSP Net, U-Net, and Deeplabv3, were compared to identify the most suitable network for extracting sea ice leads from TIR images, with the U-Net architecture providing the best segmentation results.

Nevertheless, the segmentation results of U-Net network still exist some misclassification caused by clouds. Therefore, the network was further optimized by introducing frequency domain filtering modules, which eliminate the interference of low-frequency clouds and enhance the model's focus on the high-frequency regions like linear features of sea ice leads, thereby improving the extraction accuracy of sea ice leads from thermal infrared images. Results show that the novel network effectively reduces misclassification caused by clouds, thereby providing more accurate and reliable sea ice lead data. 

How to cite: Zhang, L., Hui, F., Cheng, X., Li, G., Zheng, X., Chi, Z., Yu, H., Sun, L., and Wu, S.: Arctic Sea Ice Lead Detection From China FY-3D MERSI-II Quality Enhanced Images , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8158, https://doi.org/10.5194/egusphere-egu25-8158, 2025.