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Research Article

Radiance consistency and deviation characteristics in the regions of overlap between three new-generation GEO meteorological satellites

ORCID Icon, , , &
Pages 197-208 | Received 24 Aug 2022, Accepted 27 Jan 2023, Published online: 08 Feb 2023
 

ABSTRACT

The combination of multi-source Geostationary Earth Orbit (GEO) satellites can realize simultaneous global observation with high frequency, which is significant to fine weather forecast and global climate change research. Here the radiance consistency and deviation characterization in the overlapping regions are analysed for three new generation GEO satellites, including the Advanced Himawari Imager (AHI) onboard the Himawari-8 satellite, the Advanced Baseline Imager (ABI) onboard the Geostationary Operational Environmental Satellite-17 (GOES-17) and the Advanced Geostationary Radiation Imager (AGRI) onboard FengYun satellite-4A (FY-4A). The result shows that the radiance has higher consistency for visible and near-infrared (VNIR) channels with correlation coefficient r > 0.98 than infrared (IR) channels with r > 0.90 in the overlapping regions of different GEO satellites. For FY-4A & Himawari-8, the average percentage deviation (APD) of VNIR channels is 5.54%–9.03%. The brightness temperature (BT) bias of IR channels is 1.16 K-2.50 K. For GOES-17 & Himawari-8, the APD of VNIR channels is 4.48%–6.71%, and the BT bias of IR channels is 0.96 K −2.76 K. Solar-viewing geometries significantly influence the radiance deviation in the over regions. The future work is to design a radiance fusion method and achieve cloud detection in ample space with high frequency by combining multi-source GEO satellites.

Acknowledgments

We thank the National Oceanic and Atmospheric Administration (NOAA), Japan Aerospace Exploration Agency (JAXA), and National Satellite Meteorological Center (NSMC) for providing the GOES-17, Himawari-8, and FY-4A Level 1B data.

Disclosure statement

No potential conflict of interest was reported by the author(s).

Additional information

Funding

The work was supported by the National Natural Science Foundation of China (42276188, 61890964, 41506203, U1906217) and China–Korea joint ocean research project (PI-2019-1-01)

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