Preprints
https://doi.org/10.5194/egusphere-2025-2467
https://doi.org/10.5194/egusphere-2025-2467
13 Jun 2025
 | 13 Jun 2025

Understanding the Mid-Pleistocene transition with a simple physical model

Sergio Pérez-Montero, Jorge Alvarez-Solas, Jan Swierczek-Jereczek, Daniel Moreno-Parada, Alexander Robinson, and Marisa Montoya

Abstract. The climate of the Quaternary period is dominated by glacial-interglacial variability due to changes in the Earth’s orbital parameters that control the incoming solar radiation. However, certain features of this variability remain puzzling. A notable example is the so-called Mid-Pleistocene Transition (MPT, circa 1 million years ago), characterized by the shift of the predominant periodicity in climate variability from 40 kyr during the Early Pleistocene to 100 kyr at the Late Pleistocene. Previous studies have tried to explain its origin by invoking two main hypotheses. The first one is based on the observed decreasing trends in temperature and CO2 throughout various climatic proxies. The second one, the regolith hypothesis, is based on the change in the basal friction regime of the Northern Hemisphere ice sheets via a progressive elimination of sediment layers of sediments above the continents. Here, we use the Physical Adimensional Climate Cryosphere mOdel (PACCO) to reproduce orbital-scale climate variability throughout the entire Pleistocene through a physical albeit simplified approach. We find that the decreasing trends in CO2 and temperature during the Pleistocene can be explained with PACCO as a consequence of an MPT triggered by regolith removal that changes the size of the Northern Hemisphere ice sheets. The pre- and post MPT world respectively yield dominant periodicities around 40 and 100 kyr, the timing of the MPT corresponds to what is observed in proxies and the amplitude of sea-level changes is well matched.

Competing interests: At least one of the (co-)authors is a member of the editorial board of Climate of the Past.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Sergio Pérez-Montero, Jorge Alvarez-Solas, Jan Swierczek-Jereczek, Daniel Moreno-Parada, Alexander Robinson, and Marisa Montoya

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  • RC1: 'Comment on egusphere-2025-2467', Lorraine Lisiecki, 17 Jul 2025
  • RC2: 'Comment on egusphere-2025-2467', Anonymous Referee #2, 04 Aug 2025
Sergio Pérez-Montero, Jorge Alvarez-Solas, Jan Swierczek-Jereczek, Daniel Moreno-Parada, Alexander Robinson, and Marisa Montoya
Sergio Pérez-Montero, Jorge Alvarez-Solas, Jan Swierczek-Jereczek, Daniel Moreno-Parada, Alexander Robinson, and Marisa Montoya

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Short summary
Almost 3 million years ago, the planet began to experience a succession of cold and warm periods every 40,000 years. However, about 1 million years ago, they began to occur every 100,000 years. In this paper we explore how the change in the basal velocity of the ice sheets could have produced this change in behavior. On the other hand, we also see that in our model, decreasing in time the sensitivity of snowfall to temperature is also an effective mechanism with which to reproduce the records.
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