Improvements in an anisotropic ocean surface emissivity model based on WindSat polarimetric brightness observations

Dean F. Smith, A. Gasiewski
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Abstract

The goal of this research has been to develop a standardized fast full-Stokes ocean surface emissivity model with Jacobian for a wind-driven ocean surface applicable at arbitrary microwave frequencies, polarizations, and incidence angles. The model is based on the Ohio State University (OSU) two-scale code for surface emission developed by Johnson (2006, IEEE TGRS, 44, 560) as presented in our 2013 URSI talk. A total of five physical tuning parameters were identified, including the spectral strength and the hydrodynamic modulation factor. The short wave part of the spectrum is also allowed to have an arbitrary ratio relative to the long wave part. The foam fraction is multiplied by a variable correction factor, and also modulated to allow an anisotropic foam fraction with more foam on the leeward side of a wave.
基于WindSat偏振亮度观测的各向异性海洋表面发射率模型的改进
本研究的目标是建立一个标准化的快速全斯托克斯海洋表面发射率模型,该模型具有雅可比矩阵,适用于任意微波频率、极化和入射角。该模型基于俄亥俄州立大学(OSU)表面排放的双尺度代码,该代码由Johnson(2006年,IEEE TGRS, 44,560)开发,并在2013年URSI演讲中提出。共确定了5个物理调谐参数,包括光谱强度和流体动力调制因子。还允许频谱的短波部分相对于长波部分具有任意的比率。泡沫分数乘以一个可变的校正系数,并进行调制,使泡沫分数在波浪的背风侧具有更多的泡沫。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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