Disturbing Variability in Microwave Emission from a Non-Gaussian Distributed and Correlated Multiscale Rough Surface

• Published in: Remote sensing (Basel, Switzerland) Switzerland), 2023-07, Vol.15 (13), p.3297
• Main Authors: Yang, Ying, Chen, Kun-Shan
• Format: Article
• Language: English
• Subjects: Analysis; Brightness temperature; Correlation; Density; Distribution (Probability theory); Earth surface; Emissions; Emissions (Pollution); Emissivity; Environmental aspects; Geophysical prediction; height probability density; Look angles (tracking); Methods; Microwave emission; non-Gaussian; Polarization; power spectrum density; Probability distribution; Remote sensing; rough surface; Roughness; Variability
• ISSN: 2072-4292; 2072-4292
• DOI: 10.3390/rs15133297

In passive microwave remote sensing of the Earth’s surface, it is essential to relate the emission to geophysical parameters. The emissivity ranges between 0 and 1. Hence, a slight emissivity variation leads to a significant change in brightness temperature. Many sources of error contribute to such tiny variations in emission. This paper quantifies microwave emission variability from a rough surface through model simulation due to the non-Gaussianity in height probability density (HPD) and power spectrum density (PSD). We considered Gaussian and exponential distributions for surface height and correlation functions, representing two extremes of asperity and skewness. Additionally, the surface under consideration contains multiscale roughness. The impact of the HPD and multiscale roughness on the polarization index of the emissivity is evaluated as a function of frequency and roughness. In general, assuming that Gaussian-distributed height leads to an underestimation of the emissivity, with V polarization being less sensitive to the non-Gaussian HPD and PSD effects than H polarization, the emissions are enhanced at high roughness with small look angles but are reduced for smooth surfaces at large look angles under non-Gaussian PSD. In a specific scenario, the dynamic range of the difference between exponential and Gaussian HPD is 0~10%, and the difference in emissivity caused by non-Gaussian PSD ranges from −2% to 16%. These results should be helpful in interpreting the radiometric measurements that exhibit fluctuations and differences with model predictions.