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在类似地球的行星上,失控的温室气体过程增加了阳光值
Jérémy Leconte1, Francois Forget1, Benjamin Charnay1
1Laboratoire de Météorologie Dynamique, Institut Pierre Simon Laplace, 4 Place Jussieu, BP 99, 75252 Paris, France.
Nature
|December 17, 2013
概括
地球 地球 地球 地球 地球 地球
科学领域:
- 行星科学 行星科学
- 气候建模气候模型
- 大气物理学 大气物理学
背景情况:
- 增加太阳亮度可能会导致 runaway 温室效应.
- 一维模型在预测关键阳光值方面存在局限性.
- 云和动态反对于地球气候稳定至关重要.
研究的目的:
- 通过使用3D全球气候模型来确定一个失控的温室状态的阳光照射值.
- 研究云和大气动力学在行星可居住性中的作用.
- 重新评估早期金星上液态水的潜力.
主要方法:
- 利用了一个三维的全球气候模型.
- 模拟地球类行星对日照增加的气候反应.
- 分析了平流层水蒸气和辐射效应.
主要成果:
- 失控的温室气体值约为375W m-2,高于此前估计的.
- 云反被发现是破坏稳定的.
- 哈德利循环的稳定效应将失控的极限转移到更高的阳光照射值.
结论:
- 3D模型提供了更准确的评估失控的温室气体极限.
- 星球上的可居住性可能会扩展到比以前认为的更高的阳光照射水平.
- 这些发现影响了对金星过去气候和系外行星可居住性的理解.
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