Interglacial climate response to CO2 and astronomical forcing

The climate of the nine interglacials of the past 800,000 years has been simulated with both snapshot and transient experiments using the model LOVECLIM in response to changes in insolation and CO2 concentration. These simulations allow to investigate the relative contributions of insolation and CO2...

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Main Authors: Yin, Qiuzhen, Berger, A., The International Symposium on Aeolian Deposits in Earth History
Other Authors: UCL - SST/ELI/ELIC - Earth & Climate
Format: Conference Object
Language:Ndonga
Published: 2015
Subjects:
Online Access:http://hdl.handle.net/2078.1/168514
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spelling ftunivlouvain:oai:dial.uclouvain.be:boreal:168514 2024-05-19T07:48:20+00:00 Interglacial climate response to CO2 and astronomical forcing Yin, Qiuzhen Berger, A. The International Symposium on Aeolian Deposits in Earth History UCL - SST/ELI/ELIC - Earth & Climate 2015 http://hdl.handle.net/2078.1/168514 ng ndo boreal:168514 http://hdl.handle.net/2078.1/168514 info:eu-repo/semantics/conferenceObject 2015 ftunivlouvain 2024-04-24T01:26:47Z The climate of the nine interglacials of the past 800,000 years has been simulated with both snapshot and transient experiments using the model LOVECLIM in response to changes in insolation and CO2 concentration. These simulations allow to investigate the relative contributions of insolation and CO2 to the intensity and duration of each interglacial as well as the differences between the interglacials at global and regional scales. The transient simulations which cover a full range of precession, obliquity and eccentricity allow to investigate the response of different climate variables and different latitudes to astronomical parameters. The results show that the relative contribution of insolation and CO2 on the warmth intensity varies from one interglacial to another. They also show that CO2 plays a dominant role on the variations of the global annual mean temperature and the southern high latitude temperature and sea ice, whereas, insolation plays a dominant role on the variations of monsoon precipitation, vegetation and of the northern high latitude temperature and sea ice. The model results show that obliquity and precession have different weight on temperature and precipitation of different latitudes. The response of the climate system is shown to depend strongly upon the phase between obliquity and precession. Based on these simulations, an OPE (obliquity-precession-eccentricity) index is developed to estimate the climate sensitivity to astronomical forcing. The model results suggest that caution should be taken when astronomically tuning the chronology of a proxy record or tuning it to a proxy from other regions. Finally, the past interglacials are compared to the Holocene and the near future natural climate, which allows looking for the best interglacial analogue for the whole Holocene and its natural future. Conference Object Sea ice DIAL@UCLouvain (Université catholique de Louvain)
institution Open Polar
collection DIAL@UCLouvain (Université catholique de Louvain)
op_collection_id ftunivlouvain
language Ndonga
description The climate of the nine interglacials of the past 800,000 years has been simulated with both snapshot and transient experiments using the model LOVECLIM in response to changes in insolation and CO2 concentration. These simulations allow to investigate the relative contributions of insolation and CO2 to the intensity and duration of each interglacial as well as the differences between the interglacials at global and regional scales. The transient simulations which cover a full range of precession, obliquity and eccentricity allow to investigate the response of different climate variables and different latitudes to astronomical parameters. The results show that the relative contribution of insolation and CO2 on the warmth intensity varies from one interglacial to another. They also show that CO2 plays a dominant role on the variations of the global annual mean temperature and the southern high latitude temperature and sea ice, whereas, insolation plays a dominant role on the variations of monsoon precipitation, vegetation and of the northern high latitude temperature and sea ice. The model results show that obliquity and precession have different weight on temperature and precipitation of different latitudes. The response of the climate system is shown to depend strongly upon the phase between obliquity and precession. Based on these simulations, an OPE (obliquity-precession-eccentricity) index is developed to estimate the climate sensitivity to astronomical forcing. The model results suggest that caution should be taken when astronomically tuning the chronology of a proxy record or tuning it to a proxy from other regions. Finally, the past interglacials are compared to the Holocene and the near future natural climate, which allows looking for the best interglacial analogue for the whole Holocene and its natural future.
author2 UCL - SST/ELI/ELIC - Earth & Climate
format Conference Object
author Yin, Qiuzhen
Berger, A.
The International Symposium on Aeolian Deposits in Earth History
spellingShingle Yin, Qiuzhen
Berger, A.
The International Symposium on Aeolian Deposits in Earth History
Interglacial climate response to CO2 and astronomical forcing
author_facet Yin, Qiuzhen
Berger, A.
The International Symposium on Aeolian Deposits in Earth History
author_sort Yin, Qiuzhen
title Interglacial climate response to CO2 and astronomical forcing
title_short Interglacial climate response to CO2 and astronomical forcing
title_full Interglacial climate response to CO2 and astronomical forcing
title_fullStr Interglacial climate response to CO2 and astronomical forcing
title_full_unstemmed Interglacial climate response to CO2 and astronomical forcing
title_sort interglacial climate response to co2 and astronomical forcing
publishDate 2015
url http://hdl.handle.net/2078.1/168514
genre Sea ice
genre_facet Sea ice
op_relation boreal:168514
http://hdl.handle.net/2078.1/168514
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