Indian Ocean variability changes in the Paleoclimate Modelling Intercomparison Project
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Department of Geosciences, University of ArizonaIssue Date
2023-03-27
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Copernicus PublicationsCitation
Brierley, C., Thirumalai, K., Grindrod, E., and Barnsley, J.: Indian Ocean variability changes in the Paleoclimate Modelling Intercomparison Project, Clim. Past, 19, 681–701, https://doi.org/10.5194/cp-19-681-2023, 2023.Journal
Climate of the PastRights
© Author(s) 2023. This work is distributed under the Creative Commons Attribution 4.0 License.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Indian Ocean exhibits multiple modes of interannual climate variability, whose future behaviour is uncertain. Recent analysis of glacial climates has uncovered an additional El Niño-like equatorial mode in the Indian Ocean, which could also emerge in future warm states. Here we explore changes in the tropical Indian Ocean simulated by the Paleoclimate Model Intercomparison Project (PMIP4). These simulations are performed by an ensemble of models contributing to the Coupled Model Intercomparison Project 6 and over four coordinated experiments: Three past periods-the mid-Holocene (6000 years ago), the Last Glacial Maximum (21ĝ€¯000 years ago), the last interglacial (127ĝ€¯000 years ago)-and an idealized forcing scenario to examine the impact of greenhouse forcing. The two interglacial experiments are used to characterize the role of orbital variations in the seasonal cycle, whilst the other pair focus on responses to large changes in global temperature. The Indian Ocean Basin Mode (IOBM) is damped in both the mid-Holocene and last interglacial, with the amount related to the damping of the El Niño-Southern Oscillation in the Pacific. No coherent changes in the strength of the IOBM are seen with global temperature changes; neither are changes in the Indian Ocean Dipole (IOD) nor the Niño-like mode. Under orbital forcing, the IOD robustly weakens during the mid-Holocene experiment, with only minor reductions in amplitude during the last interglacial. Orbital changes do impact the SST pattern of the Indian Ocean Dipole, with the cold pole reaching up to the Equator and extending along it. Induced changes in the regional seasonality are hypothesized to be an important control on changes in the Indian Ocean variability. © 2023 Copernicus GmbH. All rights reserved.Note
Open access journalISSN
1814-9324Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.5194/cp-19-681-2023
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Except where otherwise noted, this item's license is described as © Author(s) 2023. This work is distributed under the Creative Commons Attribution 4.0 License.