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首页> 外文期刊>Journal of geophysical research. Planets >Climate-tectonic coupling: Variations in themean, variations about the mean, and variations in mode
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Climate-tectonic coupling: Variations in themean, variations about the mean, and variations in mode

机译:气候构造耦合:theean的变化,均值的变化以及模式的变化

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摘要

Interactions among tectonics, volcanism, and surface weathering are critical to the long-term climatic state of a terrestrial planet. Volcanism cycles greenhouse gasses into the atmosphere. Tectonics creates weatherable topography, and weathering reactions draw greenhouse gasses out of the atmosphere. Weathering depends on physical processes governed partly by surface temperature, which allows for the potential that climate-tectonic coupling can buffer the surface conditions of a planet in a manner that allows liquid water to exist over extended timescales (a condition that allows a planet to be habitable by life as we know it). We discuss modeling efforts to explore the level to which climate-tectonic coupling can or cannot regulate the surface temperature of a planet over geologic time. Thematically, we focus on how coupled climate-tectonic systems respond to the following: (1) changes in the mean pace of tectonics and associated variations in mantle melting and volcanism, (2) large-amplitude fluctuations about mean properties such as mantle temperature and surface plate velocities, and (3) changes in tectonic mode.We consider models that map the conditions under which plate tectonics can or cannot provide climate buffering as well as models that explore the potential that alternate tectonic modes can provide a level of climate buffering that allows liquid water to be present at a planet's surface over geological timescales. We also discuss the possibility that changes in the long-term climate state of a planet can feedback into the coupled system and initiate changes in tectonic mode.
机译:构造,火山和表面风化之间的相互作用对于陆地行星的长期气候状态至关重要。火山主义循环温室气体进入大气。构造创造了可风的地形,风化反应将温室气体从大气中散发出来。风化取决于部分由表面温度支配的物理过程,这允许气候构造耦合可以以允许液态水在延长的时间尺度上存在的方式缓冲行星的表面条件(这种条件允许行星成为行星我们所知道的生活可以居住)。我们讨论了建模工作,以探索气候构造耦合在地质时间内可以或无法调节行星表面温度的水平。从主题上讲,我们专注于耦合的气候构造系统如何响应以下内容:(1)构造构造的平均速度和地幔熔化和火山的相关变化的变化,(2)关于均值和诸如地幔温度和诸如平均温度的大幅度波动表面板速度和(3)构造模式的变化。我们考虑绘制板块构造在哪些条件下或无法提供气候缓冲的条件以及探索替代构造模式的潜力的模型,可以提供一定程度的气候缓冲,以提供一定程度的气候缓冲允许液态水在地质时间标准上的行星表面存在。我们还讨论了行星长期气候状态的变化可以反馈到耦合系统中并启动构造模式的变化的可能性。

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