Northern Hemisphere Stratosphere-Troposphere Circulation Change in CMIP6 Models: 2. Mechanisms and Sources of the Spread

IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Journal of Geophysical Research: Atmospheres Pub Date : 2024-07-05 DOI:10.1029/2024JD040823
Alexey Yu. Karpechko, Zheng Wu, Isla R. Simpson, Marlene Kretschmer, Hilla Afargan-Gerstman, Amy H. Butler, Daniela I.V. Domeisen, Hella Garny, Zachary Lawrence, Elisa Manzini, Michael Sigmond
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Abstract

We analyze the sources for spread in the response of the Northern Hemisphere wintertime stratospheric polar vortex (SPV) to global warming in Climate Model Intercomparison Project Phase 5 (CMIP5) and Phase 6 (CMIP6) model projections. About half of the intermodel spread in SPV projections by CMIP6 models, but less than a third in CMIP5 models, can be attributed to the intermodel spread in stationary planetary wave driving. In CMIP6, SPV weakening is mostly driven by increased upward wave flux from the troposphere, while SPV strengthening is associated with increased equatorward wave propagation away from the polar stratosphere. We test hypothesized factors contributing to changes in the upward and equatorward planetary wave fluxes and show that an across-model regression using projected global warming rates, strengthening of the subtropical jet and basic state lower stratospheric wind biases as predictors can explain nearly the same fraction in the CMIP6 SPV spread as the planetary wave driving (r = 0.67). The dependence of the SPV spread on the model biases in the basic state winds offers a possible emergent constraint; however, a large uncertainty prevents a substantial reduction of the projected SPV spread. The lack of this dependence in CMIP5 further calls for better understanding of underlying causes. Our results improve understanding of projected SPV uncertainty; however, further narrowing of the uncertainty remains challenging.

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CMIP6 模型中的北半球平流层-对流层环流变化: 2. 扩散的机制和来源
我们分析了气候模式相互比较项目第 5 阶段(CMIP5)和第 6 阶段(CMIP6)模式预测中北半球冬季平流层极地涡旋(SPV)对全球变暖响应的差异来源。CMIP6 模型对 SPV 预测的模型间差异约有一半可归因于静止行星波驱动的模型间差异,而 CMIP5 模型的差异不到三分之一。在 CMIP6 中,SPV 的减弱主要是由对流层上升波通量的增加驱动的,而 SPV 的增强则与极地平流层赤道波传播的增加有关。我们检验了导致向上和赤道行星波通量变化的假设因素,结果表明,以预测的全球变暖率、副热带喷流的加强和基本状态下平流层风偏作为预测因子的跨模式回归,可以解释 CMIP6 SPV 传播中与行星波驱动几乎相同的部分(r = 0.67)。SPV 分布对基本态风的模式偏差的依赖性提供了一个可能的新兴约束条件;然而,巨大的不确定性阻碍了 SPV 分布预测值的大幅降低。CMIP5 中缺乏这种依赖性,因此需要更好地了解其根本原因。我们的研究结果加深了人们对 SPV 预测不确定性的理解;然而,进一步缩小不确定性仍具有挑战性。
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来源期刊
Journal of Geophysical Research: Atmospheres
Journal of Geophysical Research: Atmospheres Earth and Planetary Sciences-Geophysics
CiteScore
7.30
自引率
11.40%
发文量
684
期刊介绍: JGR: Atmospheres publishes articles that advance and improve understanding of atmospheric properties and processes, including the interaction of the atmosphere with other components of the Earth system.
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