A transient CGCM simulation of the past 3 million years

Driven primarily by variations in earth’s axis wobble, tilt, and orbit eccentricity, our planet experienced massive glacial/interglacial reorganizations of climate and atmospheric CO 2 concentrations during the Pleistocene (2.58 Ma–11.7 ka). Even after decades of research, the underlying climate res...

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Main Authors: Yun, Kyung-Sook, Timmermann, Axel, Lee, Sun-Seon, Willeit, Matteo, Ganopolski, Andrey, Jadhav, Jyoti
Format: Text
Language:English
Published: 2023
Subjects:
Online Access:https://doi.org/10.5194/cp-2023-34
https://cp.copernicus.org/preprints/cp-2023-34/
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spelling ftcopernicus:oai:publications.copernicus.org:cpd111550 2023-06-11T04:12:52+02:00 A transient CGCM simulation of the past 3 million years Yun, Kyung-Sook Timmermann, Axel Lee, Sun-Seon Willeit, Matteo Ganopolski, Andrey Jadhav, Jyoti 2023-05-22 application/pdf https://doi.org/10.5194/cp-2023-34 https://cp.copernicus.org/preprints/cp-2023-34/ eng eng doi:10.5194/cp-2023-34 https://cp.copernicus.org/preprints/cp-2023-34/ eISSN: 1814-9332 Text 2023 ftcopernicus https://doi.org/10.5194/cp-2023-34 2023-05-29T16:23:53Z Driven primarily by variations in earth’s axis wobble, tilt, and orbit eccentricity, our planet experienced massive glacial/interglacial reorganizations of climate and atmospheric CO 2 concentrations during the Pleistocene (2.58 Ma–11.7 ka). Even after decades of research, the underlying climate response mechanisms to these astronomical forcings have not been fully understood. To further quantify the sensitivity of the earth system to orbital-scale forcings we conducted an unprecedented quasi-continuous coupled general climate model simulation with the Community Earth System Model version 1.2 (CESM1.2, ~ 3.75° horizontal resolution), which covers the climatic history of the past 3 million years ago (3 Ma). In addition to the astronomical insolation changes, CESM1.2 is forced by estimates of CO 2 and ice-sheet topography which were obtained from a simulation previously conducted with the CLIMBER-2 earth system model of intermediate complexity. Our 3 Ma simulation consists of 42 transient interglacial/glacial simulation chunks, which were partly run in parallel to save computing time. The chunks were subsequently merged, accounting for spin-up and overlap effects to yield a quasi-continuous trajectory. The computer model data were compared against a plethora of paleo-proxy data and large-scale climate reconstructions. For the period from the Mid-Pleistocene Transition (MPT, ~1 Ma) to the late Pleistocene we find good agreement between simulated and reconstructed temperatures in terms of phase and amplitude (−5.7 °C temperature difference between Last Glacial Maximum and Holocene). For the earlier part (3 Ma–1 Ma), differences in orbital-scale variability occur between model simulation and the reconstructions, indicating potential biases in the applied CO 2 forcing. Our model-proxy data comparison also extends to the westerlies, which show unexpectedly large variance on precessional timescales, and hydroclimate variables in major monsoon regions. Eccentricity-modulated precessional variability is also responsible ... Text Ice Sheet Copernicus Publications: E-Journals
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Driven primarily by variations in earth’s axis wobble, tilt, and orbit eccentricity, our planet experienced massive glacial/interglacial reorganizations of climate and atmospheric CO 2 concentrations during the Pleistocene (2.58 Ma–11.7 ka). Even after decades of research, the underlying climate response mechanisms to these astronomical forcings have not been fully understood. To further quantify the sensitivity of the earth system to orbital-scale forcings we conducted an unprecedented quasi-continuous coupled general climate model simulation with the Community Earth System Model version 1.2 (CESM1.2, ~ 3.75° horizontal resolution), which covers the climatic history of the past 3 million years ago (3 Ma). In addition to the astronomical insolation changes, CESM1.2 is forced by estimates of CO 2 and ice-sheet topography which were obtained from a simulation previously conducted with the CLIMBER-2 earth system model of intermediate complexity. Our 3 Ma simulation consists of 42 transient interglacial/glacial simulation chunks, which were partly run in parallel to save computing time. The chunks were subsequently merged, accounting for spin-up and overlap effects to yield a quasi-continuous trajectory. The computer model data were compared against a plethora of paleo-proxy data and large-scale climate reconstructions. For the period from the Mid-Pleistocene Transition (MPT, ~1 Ma) to the late Pleistocene we find good agreement between simulated and reconstructed temperatures in terms of phase and amplitude (−5.7 °C temperature difference between Last Glacial Maximum and Holocene). For the earlier part (3 Ma–1 Ma), differences in orbital-scale variability occur between model simulation and the reconstructions, indicating potential biases in the applied CO 2 forcing. Our model-proxy data comparison also extends to the westerlies, which show unexpectedly large variance on precessional timescales, and hydroclimate variables in major monsoon regions. Eccentricity-modulated precessional variability is also responsible ...
format Text
author Yun, Kyung-Sook
Timmermann, Axel
Lee, Sun-Seon
Willeit, Matteo
Ganopolski, Andrey
Jadhav, Jyoti
spellingShingle Yun, Kyung-Sook
Timmermann, Axel
Lee, Sun-Seon
Willeit, Matteo
Ganopolski, Andrey
Jadhav, Jyoti
A transient CGCM simulation of the past 3 million years
author_facet Yun, Kyung-Sook
Timmermann, Axel
Lee, Sun-Seon
Willeit, Matteo
Ganopolski, Andrey
Jadhav, Jyoti
author_sort Yun, Kyung-Sook
title A transient CGCM simulation of the past 3 million years
title_short A transient CGCM simulation of the past 3 million years
title_full A transient CGCM simulation of the past 3 million years
title_fullStr A transient CGCM simulation of the past 3 million years
title_full_unstemmed A transient CGCM simulation of the past 3 million years
title_sort transient cgcm simulation of the past 3 million years
publishDate 2023
url https://doi.org/10.5194/cp-2023-34
https://cp.copernicus.org/preprints/cp-2023-34/
genre Ice Sheet
genre_facet Ice Sheet
op_source eISSN: 1814-9332
op_relation doi:10.5194/cp-2023-34
https://cp.copernicus.org/preprints/cp-2023-34/
op_doi https://doi.org/10.5194/cp-2023-34
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