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上新世气候由升高的痕量气体辐射强迫引起的极地放大效应。

Polar amplification of Pliocene climate by elevated trace gas radiative forcing.

机构信息

School of Geography, Earth & Environmental Sciences, University of Birmingham, Birmingham B15 2TT United Kingdom;

Laboratoire des Sciences du Climat et de l'Environnement, Institut Pierre Simon Laplace, Commissariat à l'énergie atomique et aux énergies alternatives-Centre National de la Recherche Scientifique-Université de Saint-Quentin en Yvelines, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France.

出版信息

Proc Natl Acad Sci U S A. 2020 Sep 22;117(38):23401-23407. doi: 10.1073/pnas.2002320117. Epub 2020 Sep 4.

Abstract

Warm periods in Earth's history offer opportunities to understand the dynamics of the Earth system under conditions that are similar to those expected in the near future. The Middle Pliocene warm period (MPWP), from 3.3 to 3.0 My B.P, is the most recent time when atmospheric CO levels were as high as today. However, climate model simulations of the Pliocene underestimate high-latitude warming that has been reconstructed from fossil pollen samples and other geological archives. One possible reason for this is that enhanced non-CO trace gas radiative forcing during the Pliocene, including from methane (CH), has not been included in modeling. We use a suite of terrestrial biogeochemistry models forced with MPWP climate model simulations from four different climate models to produce a comprehensive reconstruction of the MPWP CH cycle, including uncertainty. We simulate an atmospheric CH mixing ratio of 1,000 to 1,200 ppbv, which in combination with estimates of radiative forcing from NO and O, contributes a non-CO radiative forcing of 0.9 [Formula: see text] (range 0.6 to 1.1), which is 43% (range 36 to 56%) of the CO radiative forcing used in MPWP climate simulations. This additional forcing would cause a global surface temperature increase of 0.6 to 1.0 °C, with amplified changes at high latitudes, improving agreement with geological evidence of Middle Pliocene climate. We conclude that natural trace gas feedbacks are critical for interpreting climate warmth during the Pliocene and potentially many other warm phases of the Cenezoic. These results also imply that using Pliocene CO and temperature reconstructions alone may lead to overestimates of the fast or Charney climate sensitivity.

摘要

地球历史上的温暖时期为我们提供了了解地球系统动力学的机会,这些条件与我们预计在不久的将来会遇到的条件相似。中上新世暖期(Middle Pliocene warm period,MPWP)发生在 3300 万至 300 万年前,是大气 CO2 水平与今天相当的最近时期。然而,上新世气候模式模拟低估了从化石花粉样本和其他地质档案中重建的高纬度变暖。造成这种情况的一个可能原因是,上新世增强的非 CO 痕量气体辐射强迫,包括甲烷(CH),尚未纳入建模。我们使用一系列陆地生物地球化学模型,这些模型受到来自四个不同气候模型的 MPWP 气候模型模拟的驱动,以全面重建 MPWP CH 循环,包括不确定性。我们模拟了大气 CH 混合比为 1000 至 1200ppbv,这与来自 NO 和 O 的辐射强迫估计相结合,对非 CO 辐射强迫的贡献为 0.9 [Formula: see text](范围为 0.6 至 1.1),占 MPWP 气候模拟中 CO 辐射强迫的 43%(范围为 36%至 56%)。这种额外的强迫会导致全球表面温度升高 0.6 至 1.0°C,高纬度地区的变化幅度更大,从而提高了与上新世气候地质证据的一致性。我们得出结论,自然痕量气体反馈对于解释上新世和新生代许多其他温暖阶段的气候变暖至关重要。这些结果还意味着,仅使用上新世 CO 和温度重建可能会导致对快速或 Charney 气候敏感性的高估。

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本文引用的文献

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Constraints on global mean sea level during Pliocene warmth.上新世暖期全球平均海平面的限制因素。
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Trajectories of the Earth System in the Anthropocene.人类世地球系统的轨迹。
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Understanding the glacial methane cycle.了解冰川甲烷循环。
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