Stronger El Niño could accelerate Antarctic ice melts

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Australian researchers suggest the projected increases to the strength of El Niños, periods of warmer water in Pacific Ocean, in the future could lead to a warming of the Antarctic shelf ocean water, which would likely accelerate the melting of stationary ice shelves and sheets. The team's models showed this change would lead to reduced warming near the surface of the shelves, but accelerate the warming of deeper waters. The one positive they found was that this increase would likely slow the floating sea ice reduction.

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From: CSIRO

Stronger El Niño could cause irreversible melting of Antarctica

New research led by scientists at CSIRO, Australia’s national science agency, has shown that future increases in the strength of El Niño may accelerate the irreversible melting of ice shelves and ice sheets in Antarctica.

The results, published in Nature Climate Change, used climate models to show how an increase in the variability of El Niño Southern Oscillation (ENSO) leads to reduced warming near the surface, but accelerated warming of deeper ocean waters.

ENSO is a key driver of climate variability, as both its warm phase, El Niño, and its colder phase, La Niña, influence weather conditions around the world, including in Australia.

Wenju Cai, lead author of this study and global expert on the relationship between climate change and ENSO, said the research was a critical step in further understanding how Antarctica will be affected by climate change.

“Climate change is expected to increase the magnitude of ENSO, making both El Niño and La Niña stronger,” Dr Cai said.

“This new research shows that stronger El Niño may speed up warming of deep waters in the Antarctic shelf, making ice shelves and ice sheets melt faster.

“Our modelling also revealed that warming around the edges of floating sea ice is slowed during this process, slowing down the melting of sea ice near the surface.

“Models with increased ENSO variability show a reduced upwelling of deeper, warmer waters, leading to slower warming of the ocean surface,” he said.

The associated winds around Antarctica are the mechanism driving this result.

When ENSO variability increases, it slows the intensifying westerly winds along the shelf. As a result, the upwelling of warm water around Antarctica is not able to increase as much.

The research team examined 31 climate models that participated in Phase 6 of the Coupled Model Intercomparison Project (CMIP6) under historical forcings and a high-emissions scenario.

Co-author Ariaan Purich from Securing Antarctica’s Environmental Future at Monash University said the effects of increasing ENSO variability go beyond extreme weather risks, and affect changes in Antarctic sea ice and ice shelves and sheets.

“This could have broad implications for the global climate system, so continuing to understand how ENSO will respond to climate change is a critical area of climate research,” Dr Purich said.

“There is still a lot more we need to understand about processes influencing shelf temperatures, and the finding is an important piece of the puzzle," she said.

Journal/
conference:
Nature Climate Change
Research:Paper
Organisation/s: CSIRO, Monash University, The University of New South Wales
Funder: This work was supported by the National Key Research and Development Program of China 2018YFA0605700, the Science and Technology Innovation Project of Laoshan Laboratory (LSKJ202203302, LSKJ202202402), the Strategic Priority Research Program of the Chinese Academy of Sciences (grant XDB40030000) and the Centre for Southern Hemisphere Oceans Research, a joint research centre between QNLM and CSIRO. F.J. was supported by the National Key Research and Development Program of China 2020YFA0608801, National Natural Science Foundation of China (NSFC) projects (41876008, 41730534) and Youth Innovation Promotion Association of the Chinese Academy of Sciences (2021205). S.L. was supported by the National Natural Science Foundation of China (NSFC) project 42006173 and the National Key Research and Development Program of China 2019YFC1509102. A.P. was supported by the Australian Research Council Special Research Initiative for Securing Antarctica’s Environmental Future (SR200100005). G.W., B.N. and A.S. were supported by the EarthSystems and Climate Change Hub of the Australian Government’s National Environmental Science Program. T.G. was supported by the NSFC project (2206209) and the China National Postdoctoral Program for Innovative Talents (BX20220279). PMEL contribution no. 5447. G.A.M. was supported by the Regional and Global Model Analysis (RGMA) component of the Earth and Environmental System Modeling Program of the US Department of Energy’s Office of Biological and Environmental Research (BER) via National Science Foundation IA 1844590 and under Award Number DE-SC0022070, and also by the National Center for Atmospheric Research, which is a major facility sponsored by the National Science Foundation (NSF) under Cooperative Agreement No. 1852977. Open access funding provided by CSIRO Library Services. We thank the World Climate Research Programme’s Working Group on Coupled Modelling, which led the design of CMIP6 and coordinated the work, and also individual climate modelling groups (listed in Supplementary Table 1) for their effort in model simulations and projections.
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