Dynamical evolution of ENSO in a warming background: A review of recent trends & future projections
Dynamical evolution of ENSO in a warming background: A review of recent trends & future projections
The wide-spread implications of El Niño-Southern Oscillation (ENSO) on global and regional climate necessitates a better understanding of how the underlying interannual dynamics have changed over recent years. Year-to-year changes in ENSO impact terrestrial and marine habitats, water availability, food security and social stability (Santoso et al., 2017). With abundant evidence of a warming climate, it is imperative to understand how a large-scale climatic oscillation such as ENSO is evolving and influencing changes in large-scale atmospheric circulation patterns (Alizadeh et al., 2022; Cai et al., 2021). Furthermore, quantifying the influence of the ocean on changes in this climatic pattern is an interesting and important question to answer. Evaluating the ability of models to appropriately represent the underlying physics and dynamical changes impacting the spatiotemporal extent and the intensity of ENSO is crucial to understanding ocean-climate teleconnections and changes in climatic extremes. In this study, we review and evaluate the representation of ENSO in several high-resolution CMIP6 and HighResMIP models and forced ocean-only simulations focusing on the ability of current state-of-the-art models to represent central equatorial pacific warming and cooling. This evaluation involves looking at the development and propagation of warm temperature anomalies on surface and sub-surface levels in the equatorial Pacific and understanding the differences in simulating surface heat budget and exchange with the overlying atmosphere and the deeper ocean. Surface and sub-surface (up to 200m depth) temperature anomalies in the Niño 3.4 region were calculated from modelled data and were then compared with anomalies from observational and reanalysis temperature datasets (like EN4, ORAS5). We find good agreement in the timing and vertical structure of surface/sub-surface temperature anomalies in the forced model simulations, particularly during strong ENSO years. Moreover, the genesis of sub-surface anomalies and their further propagation to the surface was well simulated in the forced simulations. The vertical coherence of temperature anomalies was relatively more pronounced in forced ocean-only simulations than in coupled high-resolution model runs. Furthermore, we comment on the shortcomings and suggest potential improvements that can be made in the models that could improve the model's ability to capture ENSO strength and variability.
Golla, Sreevathsa
dc183162-2ad5-4e22-91b5-9cc5240c56dc
Hirschi, Joel
c8a45006-a6e3-4319-b5f5-648e8ef98906
Mecking, Jennifer
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Blaker, Adam
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Kelly, Stephen
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1 April 2024
Golla, Sreevathsa
dc183162-2ad5-4e22-91b5-9cc5240c56dc
Hirschi, Joel
c8a45006-a6e3-4319-b5f5-648e8ef98906
Mecking, Jennifer
9b090069-5061-4340-b736-9690894ce203
Blaker, Adam
94efe8b2-c744-4e90-87d7-db19ffa41200
Kelly, Stephen
5e453908-a436-4e72-87c0-8ddf1a18e53b
Golla, Sreevathsa, Hirschi, Joel, Mecking, Jennifer, Blaker, Adam and Kelly, Stephen
(2024)
Dynamical evolution of ENSO in a warming background: A review of recent trends & future projections.
EGU General Assembly 2024, , Vienna, Austria.
14 - 19 Apr 2025.
1 pp
.
(doi:10.5194/egusphere-egu24-626).
Record type:
Conference or Workshop Item
(Other)
Abstract
The wide-spread implications of El Niño-Southern Oscillation (ENSO) on global and regional climate necessitates a better understanding of how the underlying interannual dynamics have changed over recent years. Year-to-year changes in ENSO impact terrestrial and marine habitats, water availability, food security and social stability (Santoso et al., 2017). With abundant evidence of a warming climate, it is imperative to understand how a large-scale climatic oscillation such as ENSO is evolving and influencing changes in large-scale atmospheric circulation patterns (Alizadeh et al., 2022; Cai et al., 2021). Furthermore, quantifying the influence of the ocean on changes in this climatic pattern is an interesting and important question to answer. Evaluating the ability of models to appropriately represent the underlying physics and dynamical changes impacting the spatiotemporal extent and the intensity of ENSO is crucial to understanding ocean-climate teleconnections and changes in climatic extremes. In this study, we review and evaluate the representation of ENSO in several high-resolution CMIP6 and HighResMIP models and forced ocean-only simulations focusing on the ability of current state-of-the-art models to represent central equatorial pacific warming and cooling. This evaluation involves looking at the development and propagation of warm temperature anomalies on surface and sub-surface levels in the equatorial Pacific and understanding the differences in simulating surface heat budget and exchange with the overlying atmosphere and the deeper ocean. Surface and sub-surface (up to 200m depth) temperature anomalies in the Niño 3.4 region were calculated from modelled data and were then compared with anomalies from observational and reanalysis temperature datasets (like EN4, ORAS5). We find good agreement in the timing and vertical structure of surface/sub-surface temperature anomalies in the forced model simulations, particularly during strong ENSO years. Moreover, the genesis of sub-surface anomalies and their further propagation to the surface was well simulated in the forced simulations. The vertical coherence of temperature anomalies was relatively more pronounced in forced ocean-only simulations than in coupled high-resolution model runs. Furthermore, we comment on the shortcomings and suggest potential improvements that can be made in the models that could improve the model's ability to capture ENSO strength and variability.
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Published date: 1 April 2024
Venue - Dates:
EGU General Assembly 2024, , Vienna, Austria, 2025-04-14 - 2025-04-19
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Local EPrints ID: 503564
URI: http://eprints.soton.ac.uk/id/eprint/503564
PURE UUID: c10af68f-1e80-4c0a-98b8-c93d8d288fc7
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Date deposited: 05 Aug 2025 16:45
Last modified: 06 Aug 2025 02:10
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Contributors
Author:
Sreevathsa Golla
Author:
Joel Hirschi
Author:
Jennifer Mecking
Author:
Adam Blaker
Author:
Stephen Kelly
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