What caused Earth's temperature variations during the last 800,000 years? Data-based evidence on radiative forcing and constraints on climate sensitivity

International audience The temperature on Earth varied largely in the Pleistocene from cold glacials to interglacials of different warmths. To contribute to an understanding of the underlying causes of these changes we compile various environmental records (and model-based interpretations of some of...

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Published in:Quaternary Science Reviews
Main Authors: Köhler, Peter, Bintanja, Richard, Fischer, Hubertus, Joos, Fortunat, Knutti, Reto, Lohmann, Gerrit, Masson-Delmotte, Valérie
Other Authors: Alfred Wegener Institute for Polar and Marine Research (AWI), Royal Netherlands Meteorological Institute (KNMI), Climate and Environmental Physics Bern (CEP), Physikalisches Institut Bern, Universität Bern / University of Bern (UNIBE)-Universität Bern / University of Bern (UNIBE), Institute for Atmospheric and Climate Science Zürich (IAC), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich), Glaces et Continents, Climats et Isotopes Stables (GLACCIOS), Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2010
Subjects:
Online Access:https://hal.science/hal-03101772
https://hal.science/hal-03101772/document
https://hal.science/hal-03101772/file/Khl2008d.pdf
https://doi.org/10.1016/J.QUASCIREV.2009.09.026
id ftinsu:oai:HAL:hal-03101772v1
record_format openpolar
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language English
topic radiative forcing
temperature
Pleistocene
greenhouse gases
albedo
climate sensitivity
[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology
spellingShingle radiative forcing
temperature
Pleistocene
greenhouse gases
albedo
climate sensitivity
[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology
Köhler, Peter
Bintanja, Richard
Fischer, Hubertus
Joos, Fortunat
Knutti, Reto
Lohmann, Gerrit
Masson-Delmotte, Valérie
What caused Earth's temperature variations during the last 800,000 years? Data-based evidence on radiative forcing and constraints on climate sensitivity
topic_facet radiative forcing
temperature
Pleistocene
greenhouse gases
albedo
climate sensitivity
[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology
description International audience The temperature on Earth varied largely in the Pleistocene from cold glacials to interglacials of different warmths. To contribute to an understanding of the underlying causes of these changes we compile various environmental records (and model-based interpretations of some of them) in order to calculate the direct effect of various processes on Earth's radiative budget and, thus, on global annual mean surface temperature over the last 800,000 years. The importance of orbital variations, of the greenhouse gases CO2, CH4 and N2O, of the albedo of land ice sheets, annual mean snow cover, sea ice area and vegetation, and of the radiative perturbation of mineral dust in the atmosphere are investigated. Altogether we can explain with these processes a global cooling of 3.9 ± 0.8 K in the equilibrium temperature for the Last Glacial Maximum (LGM) directly from the radiative budget using only the Planck feedback that parameterises the direct effect on the radiative balance, but neglecting other feedbacks such as water vapour, cloud cover, and lapse rate. The unaccounted feedbacks and related uncertainties would, if taken at present day feedback strengths, decrease the global temperature at the LGM by −8.0 ± 1.6 K. Increased Antarctic temperatures during the Marine Isotope Stages 5.5, 7.5, 9.3 and 11.3 are in our conceptual approach difficult to explain. If compared with other studies, such as PMIP2, this gives supporting evidence that the feedbacks themselves are not constant, but depend in their strength on the mean climate state. The best estimate and uncertainty for our reconstructed radiative forcing and LGM cooling support a present day equilibrium climate sensitivity (excluding the ice sheet and vegetation components) between 1.4 and 5.2 K, with a most likely value near 2.4 K, somewhat smaller than other methods but consistent with the consensus range of 2–4.5 K derived from other lines of evidence. Climate sensitivities above 6 K are difficult to reconcile with Last Glacial Maximum ...
author2 Alfred Wegener Institute for Polar and Marine Research (AWI)
Royal Netherlands Meteorological Institute (KNMI)
Climate and Environmental Physics Bern (CEP)
Physikalisches Institut Bern
Universität Bern / University of Bern (UNIBE)-Universität Bern / University of Bern (UNIBE)
Institute for Atmospheric and Climate Science Zürich (IAC)
Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich)
Glaces et Continents, Climats et Isotopes Stables (GLACCIOS)
Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)
format Article in Journal/Newspaper
author Köhler, Peter
Bintanja, Richard
Fischer, Hubertus
Joos, Fortunat
Knutti, Reto
Lohmann, Gerrit
Masson-Delmotte, Valérie
author_facet Köhler, Peter
Bintanja, Richard
Fischer, Hubertus
Joos, Fortunat
Knutti, Reto
Lohmann, Gerrit
Masson-Delmotte, Valérie
author_sort Köhler, Peter
title What caused Earth's temperature variations during the last 800,000 years? Data-based evidence on radiative forcing and constraints on climate sensitivity
title_short What caused Earth's temperature variations during the last 800,000 years? Data-based evidence on radiative forcing and constraints on climate sensitivity
title_full What caused Earth's temperature variations during the last 800,000 years? Data-based evidence on radiative forcing and constraints on climate sensitivity
title_fullStr What caused Earth's temperature variations during the last 800,000 years? Data-based evidence on radiative forcing and constraints on climate sensitivity
title_full_unstemmed What caused Earth's temperature variations during the last 800,000 years? Data-based evidence on radiative forcing and constraints on climate sensitivity
title_sort what caused earth's temperature variations during the last 800,000 years? data-based evidence on radiative forcing and constraints on climate sensitivity
publisher HAL CCSD
publishDate 2010
url https://hal.science/hal-03101772
https://hal.science/hal-03101772/document
https://hal.science/hal-03101772/file/Khl2008d.pdf
https://doi.org/10.1016/J.QUASCIREV.2009.09.026
genre Antarc*
Antarctic
Ice Sheet
Sea ice
genre_facet Antarc*
Antarctic
Ice Sheet
Sea ice
op_source ISSN: 0277-3791
EISSN: 1873-457X
Quaternary Science Reviews
https://hal.science/hal-03101772
Quaternary Science Reviews, 2010, 29 (1-2), pp.129-145. ⟨10.1016/J.QUASCIREV.2009.09.026⟩
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hal-03101772
https://hal.science/hal-03101772
https://hal.science/hal-03101772/document
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doi:10.1016/J.QUASCIREV.2009.09.026
op_rights info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.1016/J.QUASCIREV.2009.09.026
container_title Quaternary Science Reviews
container_volume 29
container_issue 1-2
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spelling ftinsu:oai:HAL:hal-03101772v1 2024-04-28T08:00:04+00:00 What caused Earth's temperature variations during the last 800,000 years? Data-based evidence on radiative forcing and constraints on climate sensitivity Köhler, Peter Bintanja, Richard Fischer, Hubertus Joos, Fortunat Knutti, Reto Lohmann, Gerrit Masson-Delmotte, Valérie Alfred Wegener Institute for Polar and Marine Research (AWI) Royal Netherlands Meteorological Institute (KNMI) Climate and Environmental Physics Bern (CEP) Physikalisches Institut Bern Universität Bern / University of Bern (UNIBE)-Universität Bern / University of Bern (UNIBE) Institute for Atmospheric and Climate Science Zürich (IAC) Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich) Glaces et Continents, Climats et Isotopes Stables (GLACCIOS) Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA) 2010 https://hal.science/hal-03101772 https://hal.science/hal-03101772/document https://hal.science/hal-03101772/file/Khl2008d.pdf https://doi.org/10.1016/J.QUASCIREV.2009.09.026 en eng HAL CCSD Elsevier info:eu-repo/semantics/altIdentifier/doi/10.1016/J.QUASCIREV.2009.09.026 hal-03101772 https://hal.science/hal-03101772 https://hal.science/hal-03101772/document https://hal.science/hal-03101772/file/Khl2008d.pdf doi:10.1016/J.QUASCIREV.2009.09.026 info:eu-repo/semantics/OpenAccess ISSN: 0277-3791 EISSN: 1873-457X Quaternary Science Reviews https://hal.science/hal-03101772 Quaternary Science Reviews, 2010, 29 (1-2), pp.129-145. ⟨10.1016/J.QUASCIREV.2009.09.026⟩ radiative forcing temperature Pleistocene greenhouse gases albedo climate sensitivity [SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology info:eu-repo/semantics/article Journal articles 2010 ftinsu https://doi.org/10.1016/J.QUASCIREV.2009.09.026 2024-04-05T00:37:03Z International audience The temperature on Earth varied largely in the Pleistocene from cold glacials to interglacials of different warmths. To contribute to an understanding of the underlying causes of these changes we compile various environmental records (and model-based interpretations of some of them) in order to calculate the direct effect of various processes on Earth's radiative budget and, thus, on global annual mean surface temperature over the last 800,000 years. The importance of orbital variations, of the greenhouse gases CO2, CH4 and N2O, of the albedo of land ice sheets, annual mean snow cover, sea ice area and vegetation, and of the radiative perturbation of mineral dust in the atmosphere are investigated. Altogether we can explain with these processes a global cooling of 3.9 ± 0.8 K in the equilibrium temperature for the Last Glacial Maximum (LGM) directly from the radiative budget using only the Planck feedback that parameterises the direct effect on the radiative balance, but neglecting other feedbacks such as water vapour, cloud cover, and lapse rate. The unaccounted feedbacks and related uncertainties would, if taken at present day feedback strengths, decrease the global temperature at the LGM by −8.0 ± 1.6 K. Increased Antarctic temperatures during the Marine Isotope Stages 5.5, 7.5, 9.3 and 11.3 are in our conceptual approach difficult to explain. If compared with other studies, such as PMIP2, this gives supporting evidence that the feedbacks themselves are not constant, but depend in their strength on the mean climate state. The best estimate and uncertainty for our reconstructed radiative forcing and LGM cooling support a present day equilibrium climate sensitivity (excluding the ice sheet and vegetation components) between 1.4 and 5.2 K, with a most likely value near 2.4 K, somewhat smaller than other methods but consistent with the consensus range of 2–4.5 K derived from other lines of evidence. Climate sensitivities above 6 K are difficult to reconcile with Last Glacial Maximum ... Article in Journal/Newspaper Antarc* Antarctic Ice Sheet Sea ice Institut national des sciences de l'Univers: HAL-INSU Quaternary Science Reviews 29 1-2 129 145