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The temperature and humidity profiles within the planetary boundary layer (PBL) are crucial for Earth’s climate research. The Atmospheric Sounder Spectrometer by Infrared Spectral Technology (ASSIST) measures downward thermal radiation in the atmosphere with high temporal and spectral resolution continuously during day and night. The physics-based retrieval method, utilizing iterative optimization, can obtain solutions that align with the true atmospheric state. However, the retrieval is typically an ill-posed problem and is affected by noise, necessitating the introduction of regularization. To achieve high-precision detection, a systematic evaluation was conducted on the retrieval performance of temperature and humidity profiles using ASSIST by regularization methods based on the Gauss–Newton framework, which include Fixed regularization factor (FR), L-Curve (LC), Generalized Cross-Validation (GCV), Maximum Likelihood Estimation (MLE), and Iterative Regularized Gauss–Newton (IRGN) methods, and the Levenberg–Marquardt (LM) method based on a damping least squares strategy. A five-day validation experiment was conducted under clear-sky conditions at the Anqing radiosonde station in China. The results indicate that for temperature profile retrieval, the IRGN method demonstrates superior performance, particularly below 1.5
Details
Infrared radiation;
Accuracy;
Humidity;
Bias;
Boundary layers;
Radiosondes;
Optimization;
Atmosphere;
Temperature profiles;
Weather forecasting;
Infrared spectrometers;
Radiation measurement;
Machine learning;
Regularization;
Physics;
Fourier transforms;
Thermal radiation;
Ill posed problems;
Spectral resolution;
Damping;
Retrieval;
Lower atmosphere;
Regularization methods;
Maximum likelihood estimation;
Planetary boundary layer
; Xiong, Wei 1 ; Ye Hanhan 2 ; Shi Hailiang 2
; Wang, Xianhua 2 ; Li, Chao 3
; Wu, Shichao 2
; Chen, Cheng 2 1 School of Environmental Science and Optoelectronic Technology, University of Science and Technology of China, Hefei 230026, China; [email protected], Anhui Institute of Optics and Fine Mechanics, Hefei Institutes of Physical Science, Chinese Academy of Sciences, Hefei 230031, China; [email protected] (H.Y.); [email protected] (H.S.); [email protected] (X.W.); [email protected] (S.W.); [email protected] (C.C.), Anhui Province Key Laboratory of Optical Quantitative Remote Sensing, Hefei Institutes of Physical Science, Chinese Academy of Sciences, Hefei 230031, China
2 Anhui Institute of Optics and Fine Mechanics, Hefei Institutes of Physical Science, Chinese Academy of Sciences, Hefei 230031, China; [email protected] (H.Y.); [email protected] (H.S.); [email protected] (X.W.); [email protected] (S.W.); [email protected] (C.C.), Anhui Province Key Laboratory of Optical Quantitative Remote Sensing, Hefei Institutes of Physical Science, Chinese Academy of Sciences, Hefei 230031, China
3 CMA-USTC Laboratory of Fengyun Remote Sensing, Deep Space Exploration Laboratory, School of Earth and Space Science, University of Science and Technology of China, Hefei 230026, China; [email protected]