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Radiative entropy balance and vertical stability of a gray atmosphere

机译:灰色大气的辐射熵平衡和垂直稳定性

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Radiative entropy production and entropy flux are subject to ongoing controversial discussion in the scientific literature. The entropy export of planets such as Earth enables and limits all processes of self-organisation in the atmosphere, hydrosphere and biosphere, and is of fundamental importance for climate studies in the context of the so-called greenhouse effect. In this paper, as tutorial examples, formulas for the entropy balance are derived for two simplified gray atmosphere models, each in radiation balance with a black planetary surface of given temperature and with the cold cosmic background. It is shown that the atmospheric entropy production increases strongly with the absorptivity of the atmosphere, while the stationary surface air temperature is always very close to that of the black surface underneath, even though sensible heat flow is intentionally omitted from the models.
机译:辐射熵的产生和熵的通量在科学文献中一直受到有争议的讨论。诸如地球这样的行星的熵输出使大气层,水圈和生物圈中的所有自组织过程得以实现并受到限制,并且在所谓的温室效应的背景下对气候研究至关重要。在本文中,作为教学示例,为两个简化的灰色大气模型导出了熵平衡的公式,每个模型在辐射平衡下均具有给定温度的黑色行星表面,并且具有寒冷的宇宙背景。结果表明,大气熵的产生随大气的吸收率而大大增加,而固定表面的空气温度总是非常接近其下面的黑色表面的温度,即使模型中有意地省略了明显的热流。

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