Diagnosing the pattern effect in the atmosphere-ocean coupled system through linear response theory

Fabrizio Falasca, Aurora Basinski-Ferris, Laure Zanna, Ming Zhao
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Abstract

The energy surplus resulting from radiative forcing causes warming of the Earth system. This initial warming drives a myriad of changes including in sea surface temperatures (SSTs), leading to different radiative feedbacks. The relationship between the radiative feedbacks and the pattern of SST changes is referred to as the "pattern effect". The current approach to study the pattern effect relies on diagnosing the response of atmosphere-only models to perturbations in the SST boundary condition. Here, we argue that the fluctuation-dissipation relation (FDR), together with coarse-graining procedures, is a computationally cheap and theoretically grounded alternative to model experiments. We introduce a protocol to study the pattern effect and present its application in a state-of-the-art coupled climate model. By focusing on the coupled dynamics, we unveil the role of the slow ocean component in setting the pattern effect. We present a new "sensitivity map", representing a first, qualitative prediction of the response of the average top-of-the-atmosphere (TOA) radiative flux to perturbations in the SST field. We find negative sensitivity throughout the tropics, in contrast to the current understanding of a positive-negative dipole of sensitivity in the tropical Pacific. Considering only the shortest time scales, the response is dominated by the fast atmospheric variability and we recover results in qualitative agreement with the literature. Therefore, the difference between our results and previous studies, largely comes from including the atmosphere-ocean coupling. The framework offers a conceptually novel perspective on the pattern effect: feedbacks in the coupled system are encoded in a temporally and spatially dependent response operator, rather than time-independent maps as for previous studies.
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通过线性响应理论诊断大气-海洋耦合系统中的模式效应
辐射强迫产生的能量过剩导致地球系统变暖。这种最初的变暖会引起包括海面温度在内的各种变化,从而导致不同的辐射反馈。辐射反馈与 SST 变化模式之间的关系被称为 "模式效应"。目前研究模式效应的方法主要是诊断纯大气模式对 SST 边界条件扰动的响应。在这里,我们认为波动-消散关系(FDR)与粗粒化程序相结合,是一种替代模式实验的计算廉价且有理论基础的方法。我们介绍了一种研究模式效应的方案,并介绍了它在最先进的耦合气候模式中的应用。通过关注耦合动力学,我们揭示了慢海洋成分在模式效应中的作用。我们提出了一个新的 "灵敏度图",首次定性预测了平均大气层顶(TOA)辐射通量对 SST 场扰动的响应。仅考虑最短的时间尺度,反应主要由快速的大气变率引起,我们得出的结果与文献在质量上是一致的。因此,我们的研究结果与以往研究结果之间的差异主要来自大气-海洋耦合。该框架从概念上为模式效应提供了一个新的视角:耦合系统中的反馈被编码为一个与时间和空间相关的响应算子,而不是以往研究中与时间无关的地图。
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