EGU25-8293, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-8293
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Wednesday, 30 Apr, 16:15–18:00 (CEST), Display time Wednesday, 30 Apr, 14:00–18:00
 
Hall X4, X4.82
Radiometric Calibration using Artificial Intelligence: Constituting Uniform Observing Systems for Infrared Satellites
Boyang Chen1, Aiqun Wu2, Wen Hui1, Peng Rao3, Xuang Feng4, Fansheng Chen3, Changpei Han3, Qichao Ying5, Yapeng Wu3, Miao Liu6, Damian Moss7, and Zhenxing Qian5
Boyang Chen et al.
  • 1National Satellite Meteorological Center, China (chenby@cma.gov.cn)
  • 2Tongji University
  • 3Shanghai Institute of Technical Physics, Chinese Academy of Science
  • 4Technology and Engineering Center for Space Utilization, Chinese Academy of Science
  • 5Fudan University
  • 6Beijing University of Posts and Telecommunications
  • 7Albion Business College
Radiometric Calibration (RC) is a critical process in aerospace infrared remote sensing that establishes the relationship between the radiation energy of observed objects and the Digital Number (DN) output from sensors, which is fundamental for ensuring high-precision applications of infrared remote sensing data. At present, Source-Based RC (SBRC) is the predominant method, relying on a variety of Radiometric Sources (RS) including in-orbit blackbodies, or natural targets such as lakes, oceans. This approach, while effective, imposes constraints on remote sensing systems such as space & weight allocation for RS and additional observation time for RC. Moreover, the reliance on physical calibration sources can introduce uncertainties due to factors such as imperfect emissivity of in-orbit blackbodies, lack of data consistency due to varied RS types, and variations in environmental conditions. In this paper, we propose a novel RC method named Artificial Intelligence Radiometric Calibration (AIRC), which directly generates RC coefficients for the in-orbit remote sensing satellites using the physical and environmental parameters of the sensor. We first theoretically prove that RC coefficients can be derived as functions of the sensor states. Next, we propose our Neural Networks for infrared Radiometric Calibration (RCNN), to learn this relationship based on historical high-accuracy calibration data, enabling a shift from Reference Traceability (RT) to States Traceability (ST). Then, to verify the feasibility of the proposed scheme, we train and test an Multi-layered Perceptron (MLP) as a simple implementation of RCNN based on our long-term well-curated RC data from our FengYun-4A Avanced Geosynchronous Radiation Imager (FY-4A AGRI), and the experiments show that the proposed method achieves high-accuracy RC comparable with the official RC method applied on FY-4A AGRI that uses an in-orbit blackbody. Our study showcases how to conduct RC using the “reason (the states of sensor) - results (calibration coefficient)” logic, as supplement to the existing “result (observation to RS) - reason (calibration coefficient)” logic, which promotes constituting a uniform observing system for cross-platform infrared satellites.

How to cite: Chen, B., Wu, A., Hui, W., Rao, P., Feng, X., Chen, F., Han, C., Ying, Q., Wu, Y., Liu, M., Moss, D., and Qian, Z.: Radiometric Calibration using Artificial Intelligence: Constituting Uniform Observing Systems for Infrared Satellites, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8293, https://doi.org/10.5194/egusphere-egu25-8293, 2025.