Articles | Volume 21, issue 11
https://doi.org/10.5194/cp-21-2243-2025
https://doi.org/10.5194/cp-21-2243-2025
Research article
 | 
17 Nov 2025
Research article |  | 17 Nov 2025

Climate and stratospheric ozone during the mid-Holocene and Last Interglacial simulated by MRI-ESM2.0

Yasuto Watanabe, Makoto Deushi, and Kohei Yoshida

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Cited articles

Bartlein, P. J. and Shafer, S. L.: Paleo calendar-effect adjustments in time-slice and transient climate-model simulations (PaleoCalAdjust v1.0): impact and strategies for data analysis, Geosci. Model Dev., 12, 3889–3913, https://doi.org/10.5194/gmd-12-3889-2019, 2019. 
Bereiter, B., Eggleston, S., Schmitt, J., Nehrbass-Ahles, C., Stocker, T. F., Fischer, H., Kipfstuhl, S. and Chappellaz, J.: Revision of the EPICA Dome C CO2 record from 800 to 600 kyr before present, Geophys. Res. Lett., 42, 542–549, https://doi.org/10.1002/2014gl061957, 2015. 
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Bitz, C. M. and Polvani, L. M.: Antarctic climate response to stratospheric ozone depletion in a fine resolution ocean climate model, Geophysical Research Letters, 39, https://doi.org/10.1029/2012GL053393, 2012. 
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Short summary
This study uses an Earth System Model, MRI-ESM2.0, to demonstrate that the atmospheric ozone distribution during warm interglacial periods is modified by the changes in the Earth's orbital parameters. We further show that the change in atmospheric ozone works to cool the surface at the high-latitude regions of the northern hemisphere in the past warm interglacial periods (6 and 127 thousand years ago), while its impact is small around Antarctica.
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