Abstract

A way of calculating the field of solar radiation in Earth’s atmosphere is described that considers the thermodynamic non-equilibrium in the vibrational bands of CO₂ and O₃. The proposed technique allows calculations with high spectral resolution (line by line), along with parameterizations of the optical parameters of the Earth’s upper atmosphere that can be used in calculating the field of solar radiation.

中文翻译：

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地球大气全环流模型辐射块中二氧化碳分子振动带中的局部热力学非平衡

摘要

描述了一种计算地球大气中太阳辐射场的方法，该方法考虑了CO ₂和O ₃振动带中的热力学非平衡。所提出的技术允许以高光谱分辨率（逐行）进行计算，以及可用于计算太阳辐射场的地球高层大气光学参数的参数化。