Inter-hemispheric asymmetry in the sea-ice response to volcanic forcing simulated by MPI-ESM (COSMOS-Mill)
The decadal evolution of Arctic and Antarctic sea ice following strong volcanic eruptions is investigated in four climate simulation ensembles performed with the COSMOS-Mill version of the Max Planck Institute Earth System Model. The ensembles differ in the magnitude of the imposed volcanic perturba...
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doaj-8a0576ac9d2a40f4a3aa54efc3979fcc2020-11-25T00:32:16ZengCopernicus PublicationsEarth System Dynamics2190-49792190-49872014-06-015122324210.5194/esd-5-223-2014Inter-hemispheric asymmetry in the sea-ice response to volcanic forcing simulated by MPI-ESM (COSMOS-Mill)D. Zanchettin0O. Bothe1C. Timmreck2J. Bader3A. Beitsch4H.-F. Graf5D. Notz6J. H. Jungclaus7Max Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, GermanyLeibniz Institute of Atmospheric Physics at the University of Rostock, Kühlungsborn, GermanyMax Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, GermanyMax Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, GermanyMax Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, GermanyUniversity of Cambridge, Centre for Atmospheric Science, Downing Place, Cambridge CB2 3EN, UKMax Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, GermanyMax Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, GermanyThe decadal evolution of Arctic and Antarctic sea ice following strong volcanic eruptions is investigated in four climate simulation ensembles performed with the COSMOS-Mill version of the Max Planck Institute Earth System Model. The ensembles differ in the magnitude of the imposed volcanic perturbations, with sizes representative of historical tropical eruptions (1991 Pinatubo and 1815 Tambora) and of tropical and extra-tropical "supervolcano" eruptions. A post-eruption Arctic sea-ice expansion is robustly detected in all ensembles, while Antarctic sea ice responds only to supervolcano eruptions, undergoing an initial short-lived expansion and a subsequent prolonged contraction phase. Strong volcanic forcing therefore emerges as a potential source of inter-hemispheric interannual-to-decadal climate variability, although the inter-hemispheric signature is weak in the case of eruptions comparable to historical eruptions. The post-eruption inter-hemispheric decadal asymmetry in sea ice is interpreted as a consequence mainly of the different exposure of Arctic and Antarctic regional climates to induced meridional heat transport changes and of dominating local feedbacks that set in within the Antarctic region. Supervolcano experiments help to clarify differences in simulated hemispheric internal dynamics related to imposed negative net radiative imbalances, including the relative importance of the thermal and dynamical components of the sea-ice response. Supervolcano experiments could therefore serve the assessment of climate models' behavior under strong external forcing conditions and, consequently, favor advancements in our understanding of simulated sea-ice dynamics.http://www.earth-syst-dynam.net/5/223/2014/esd-5-223-2014.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
D. Zanchettin O. Bothe C. Timmreck J. Bader A. Beitsch H.-F. Graf D. Notz J. H. Jungclaus |
spellingShingle |
D. Zanchettin O. Bothe C. Timmreck J. Bader A. Beitsch H.-F. Graf D. Notz J. H. Jungclaus Inter-hemispheric asymmetry in the sea-ice response to volcanic forcing simulated by MPI-ESM (COSMOS-Mill) Earth System Dynamics |
author_facet |
D. Zanchettin O. Bothe C. Timmreck J. Bader A. Beitsch H.-F. Graf D. Notz J. H. Jungclaus |
author_sort |
D. Zanchettin |
title |
Inter-hemispheric asymmetry in the sea-ice response to volcanic forcing simulated by MPI-ESM (COSMOS-Mill) |
title_short |
Inter-hemispheric asymmetry in the sea-ice response to volcanic forcing simulated by MPI-ESM (COSMOS-Mill) |
title_full |
Inter-hemispheric asymmetry in the sea-ice response to volcanic forcing simulated by MPI-ESM (COSMOS-Mill) |
title_fullStr |
Inter-hemispheric asymmetry in the sea-ice response to volcanic forcing simulated by MPI-ESM (COSMOS-Mill) |
title_full_unstemmed |
Inter-hemispheric asymmetry in the sea-ice response to volcanic forcing simulated by MPI-ESM (COSMOS-Mill) |
title_sort |
inter-hemispheric asymmetry in the sea-ice response to volcanic forcing simulated by mpi-esm (cosmos-mill) |
publisher |
Copernicus Publications |
series |
Earth System Dynamics |
issn |
2190-4979 2190-4987 |
publishDate |
2014-06-01 |
description |
The decadal evolution of Arctic and Antarctic sea ice following strong
volcanic eruptions is investigated in four climate simulation ensembles
performed with the COSMOS-Mill version of the Max Planck Institute Earth System Model. The ensembles differ in the magnitude of the imposed volcanic
perturbations, with sizes representative of historical tropical eruptions
(1991 Pinatubo and 1815 Tambora) and of tropical and extra-tropical
"supervolcano" eruptions. A post-eruption Arctic sea-ice expansion is
robustly detected in all ensembles, while Antarctic sea ice responds only to
supervolcano eruptions, undergoing an initial short-lived expansion and
a subsequent prolonged contraction phase. Strong volcanic forcing therefore
emerges as a potential source of inter-hemispheric interannual-to-decadal
climate variability, although the inter-hemispheric signature is weak in the
case of eruptions comparable to historical eruptions. The post-eruption inter-hemispheric
decadal asymmetry in sea ice is interpreted as a consequence mainly of the different exposure of Arctic and Antarctic regional climates to induced
meridional heat transport changes and of dominating local feedbacks that set
in within the Antarctic region. Supervolcano experiments help to clarify
differences in simulated hemispheric internal dynamics related to imposed
negative net radiative imbalances, including the relative importance of the
thermal and dynamical components of the sea-ice response. Supervolcano experiments could therefore serve the assessment of climate models' behavior
under strong external forcing conditions and, consequently, favor
advancements in our understanding of simulated sea-ice dynamics. |
url |
http://www.earth-syst-dynam.net/5/223/2014/esd-5-223-2014.pdf |
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