Simulating the climate response to atmospheric oxygen variability in the Phanerozoic: a focus on the Holocene, Cretaceous and Permian

The amount of dioxygen (O.sub.2) in the atmosphere may have varied from as little as 5 % to as much as 35 % during the Phanerozoic eon (54 Ma-present). These changes in the amount of O.sub.2 are large enough to have led to changes in atmospheric mass, which may alter the radiative budget of the atmo...

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Veröffentlicht in:Climate of the past 2019-08, Vol.15 (4), p.1463-1483
Hauptverfasser: Wade, David C, Abraham, Nathan Luke, Farnsworth, Alexander, Valdes, Paul J, Bragg, Fran, Archibald, Alexander T
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Sprache:eng
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Zusammenfassung:The amount of dioxygen (O.sub.2) in the atmosphere may have varied from as little as 5 % to as much as 35 % during the Phanerozoic eon (54 Ma-present). These changes in the amount of O.sub.2 are large enough to have led to changes in atmospheric mass, which may alter the radiative budget of the atmosphere, leading to this mechanism being invoked to explain discrepancies between climate model simulations and proxy reconstructions of past climates. Here, we present the first fully 3-D numerical model simulations to investigate the climate impacts of changes in O.sub.2 under different climate states using the coupled atmosphere-ocean Hadley Centre Global Environmental Model version 3 (HadGEM3-AO) and Hadley Centre Coupled Model version 3 (HadCM3-BL) models. We show that simulations with an increase in O.sub.2 content result in increased global-mean surface air temperature under conditions of a pre-industrial Holocene climate state, in agreement with idealised 1-D and 2-D modelling studies. We demonstrate the mechanism behind the warming is complex and involves a trade-off between a number of factors. Increasing atmospheric O.sub.2 leads to a reduction in incident shortwave radiation at the Earth's surface due to Rayleigh scattering, a cooling effect. However, there is a competing warming effect due to an increase in the pressure broadening of greenhouse gas absorption lines and dynamical feedbacks, which alter the meridional heat transport of the ocean, warming polar regions and cooling tropical regions.
ISSN:1814-9332
1814-9324
1814-9332
DOI:10.5194/cp-15-1463-2019