CMIP6 模型中的副极地环流可变性:是否存在双稳态机制?

Swinda K. J. Falkena, Anna S. von der Heydt
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引用次数: 0

摘要

副极地涡旋有可能越过一个临界点,导致拉布拉多海对流崩溃。了解其作用机制以及气候模式中如何体现这些机制非常重要。在这项研究中,我们利用因果推理来验证所提出的副极地涡旋双稳态机制是否在 CMIP6 模式中得到了体现。在许多模式中,海表盐度的增加导致混合层的加深,从而导致中间深度的海水冷却,这与理论是一致的。在许多模式中,海表盐度增加导致混合层加深,从而使中层深度的海水变冷,这与理论是一致的。那些表明有重要联系的模式对其符号并不一致。有一个模式(CESM2)包含了所有的相互作用,既有负反馈回路,也有延迟的正反馈回路。
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Subpolar Gyre Variability in CMIP6 Models: Is there a Mechanism for Bistability?
The subpolar gyre is at risk of crossing a tipping point which would result in the collapse of convection in the Labrador Sea. It is important to understand the mechanisms at play and how they are represented in climate models. In this study we use causal inference to verify whether the proposed mechanism for bistability of the subpolar gyre is represented in CMIP6 models. In many models an increase of sea surface salinity leads to a deepening of the mixed layer resulting in a cooling of the water at intermediate depth, in line with theory. The feedback from the subsurface temperature through density to the strength of the gyre circulation is more ambiguous, with fewer models indicating a significant link. Those that do show a significant link do not agree on its sign. One model (CESM2) contains all interactions, with both a negative and delayed positive feedback loop.
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