Acta Optica Sinica, Volume. 43, Issue 18, 1828003(2023)
Radiometric Response Evaluation of FY-3D/MERSI-II Reflective Solar Bands Based on Deep Convective Cloud
Fig. 1. Flowchart of the MERSI-II radiometric response evaluate method based on DCC
Fig. 2. DCC reflectance PDF curves for different VZA angle intervals. (a) 0.65 μm; (b) 1.64 μm
Fig. 3. Normalized monthly DCC reflectance corrected by BRDF models from 2018 to 2022. (a) 0.65 μm; (b) 1.64 μm
Fig. 4. Geographical distribution of monthly DCC from 2020 to 2022. (a) Every April; (b) every July
Fig. 5. Annual variation curves of DCC monthly reflectance from 2018 to 2022. (a) 1.64 μm; (b) 2.13 μm
Fig. 7. Comparison of deseasonalization and BRDF correction results. (a) 0.65 μm; (b) 0.865 μm; (c) 1.64 μm; (d) 2.13 μm
Fig. 8. Normalized monthly DCC reflectance and linear fitting of FY-3D/MERSI-II in RSB from 2018 to 2022. (a) VIS bands; (b) NIR bands; (c) SWIR bands
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Bei Zhang, Xiuqing Hu, Weiwei Zhou, Ling Wang, Lin Chen, Peng Zhang. Radiometric Response Evaluation of FY-3D/MERSI-II Reflective Solar Bands Based on Deep Convective Cloud[J]. Acta Optica Sinica, 2023, 43(18): 1828003
Category: Remote Sensing and Sensors
Received: Apr. 18, 2023
Accepted: Jul. 18, 2023
Published Online: Sep. 11, 2023
The Author Email: Xiuqing Hu (huxq@cma.cn)