始新世中晚期温室气候,采用CESM 1.0.5模型

M. Baatsen, A. S. von der Heydt, M. Huber, M. Kliphuis, P. Bijl, A. Sluijs, H. Dijkstra
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引用次数: 25

摘要

摘要虽然许多模拟研究都考虑了始新世早期,但对始新世中期和晚期气候的详细模拟目前很少。为了更好地了解始新世-渐新世过渡时期(~34 Ma)的南极冰川作用和中始新世晚期的变暖,对始新世中晚期气候进行充分的重建是至关重要的。高分辨率(类似cmip5)耦合气候模拟的结果在这里使用社区地球系统模式(CESM)版本1表示。采用新的38 Ma详细地理重建,考虑了两个始新世中晚期的情况,它们具有相同的一般边界条件,但辐射强迫不同。在CO2(即1120 ppm)和CH4 (~2700 ppb)的4倍工业化前浓度(PIC)下,平衡海表温度与中始新世晚期(42-38 Ma)相对应;~巴尔顿阶)代理。2× PIC强迫下的模拟气候总体较冷,与晚始新世(38 ~ 34 Ma)相似;~ Priabonian)。陆地温度代用物虽然地理覆盖较少,但也表明本文的结果是现实的。重建的38 Ma气候与工业化前相比,赤道到极点的温度梯度减小,经向热分布更加对称。地理、植被和冰的集体效应解释了工业化前和始新世38 Ma边界条件之间全球平均5-7°C的差异,其中云和水蒸气反馈的重要贡献。这些模拟结果有效地表明,在不需要温室气体浓度远高于替代估算值(即~ 500-1200 ppm CO2)的情况下,可以重建一个真实的始新世中晚期气候。平衡气候敏感性降低(0.62°C/W m2;与现今气候(0.79°C/W m2;每二氧化碳加倍3.1°C)。尽管在这两个38Ma的情况下,海冰和积雪都非常有限,但该模式仍然显示出对大气温室气体浓度进一步增加的响应因子~2的极性放大。与工业化前相比,模拟始新世气候中的高纬度地区主要是由于辐射平衡的改变、全球地理变化和极地冰盖的消失而保持温暖的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The middle-to-late Eocene greenhouse climate, modelled using the CESM 1.0.5
Abstract. While the early Eocene has been considered in many modelling studies, detailed simulations of the middle and late Eocene climate are currently scarce. To get a better understanding of both Antarctic glaciation at the Eocene-Oligocene transition (~34 Ma) and late middle Eocene warmth, it is vital to have an adequate reconstruction of the middle-to-late Eocene climate. Results of higher (CMIP5-like) resolution coupled climate simulations are represented here using the Community Earth System Model (CESM) version 1. Two middle-to-late Eocene cases are considered with the same general boundary conditions but a different radiative forcing, using a new detailed 38 Ma geography reconstruction. Under 4× pre-industrial concentrations (PIC) of both CO2 (i.e. 1120 ppm) and CH4 (~2700 ppb), equilibrium sea surface temperatures correspond well to the available late middle Eocene (42–38 Ma; ~Bartonian) proxies. Being generally cooler, the simulated climate under 2× PIC forcing is a good analog for that of the late Eocene (38–34 Ma; ~Priabonian). Terrestrial temperature proxies, although their geographical coverage is sparse, also indicate that the results presented here are realistic. The reconstructed 38 Ma climate has a reduced equator-to-pole temperature gradient and a more symmetric meridional heat distribution compared to the pre-industrial reference. The collective effects of geography, vegetation and ice accounts for a global mean 5–7 °C difference between pre-industrial and 38 Ma Eocene boundary conditions, with important contributions from cloud and water vapour feedbacks. These simulations effectively show that a realistic middle-to-late Eocene climate can be reconstructed without the need for greenhouse gas concentrations much higher than proxy estimates (i.e. ~500–1200 ppm CO2). Equilibrium climate sensitivity is reduced (0.62 °C/W m2; 3.2 °C warming between 38 Ma 2× PIC and 4× PIC) compared to that of the present-day climate (0.79 °C/W m2; 3.1 °C per CO2 doubling). Despite very limited sea ice and snow cover in both 38Ma cases, the model still shows a factor ~2 polar amplification in response to a further increase of atmospheric greenhouse gas concentrations. High latitudes in the modelled Eocene climate are mainly kept warm by an altered radiative balance in combination with global changes in geography and the absence of polar ice sheets compared to the pre-industrial reference.
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