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Attenuation Tracking of FY-3B/MERSI Based on Ocean Sun Glint |
HU Xiu-qing1, 2, 3, HE Xing-wei1, 2, 3*, HE Yu-qing4, JIANG Meng-die4, CHEN Wei5 |
1. National Satellite Meteorological Center (National Center for Space Weather), China Meteorological Administration, Beijing 100081, China
2. Innovation Center for FengYun Meteorological Satellite (FYSIC), Beijing 100081, China
3. Key Laboratory of Radiometric Calibration and Validation for Environmental Satellites, Beijing 100081, China
4. School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China
5. School of Geosciences and Surveying Engineering, China University of Mining & Technology, Beijing 100083, China
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Abstract This study focuses on the on-orbit attenuation tracking problem of FY-3B/MERSI. Ocean surface sun glints are adopted as stable targets to track the attenuation from 2011 to 2018. Based on cloud-free and effective sun glint area data, the 865 nm band is regarded as the benchmark band; the ratios between other bands' reflectance and the benchmark band's reflectance are calculated to analyze the attenuations of these bands during the 8 years. There are obvious degradations for all FY-3B/MERSI bands, especially for shortwave bands. The annual degradation rate of 412 nm is 7.12%, while the corresponding value is 0.28% for the 765 nm band. The degradation is much bigger for the 1 030 nm band, at around 3.88%. Furthermore, the reflectance ratios between different bands and benchmark bands show obvious oscillation, consistent with the north-south periodic change of latitude at the center of the sun glint. Ocean surface sun glints are an effective target for the inter-band radiometric calibrations, and could help track the long-term attenuation of on-orbit sensors.
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Received: 2023-05-15
Accepted: 2025-05-14
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Corresponding Authors:
HE Xing-wei
E-mail: hexingwei@cma.gov.cn
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