Orbital- and millennial-scale Asian winter monsoon variability across the Pliocene–Pleistocene glacial intensification

  • Hong Ao*
  • , Diederik Liebrand
  • , Mark J. Dekkers
  • , Andrew P. Roberts
  • , Tara N. Jonell
  • , Zhangdong Jin
  • , Yougui Song
  • , Qingsong Liu
  • , Qiang Sun
  • , Xinxia Li
  • , Chunju Huang
  • , Xiaoke Qiang
  • , Peng Zhang
  • *Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review

Abstract

Intensification of northern hemisphere glaciation (iNHG), ~2.7 million years ago (Ma), led to establishment of the Pleistocene to present-day bipolar icehouse state. Here we document evolution of orbital- and millennial-scale Asian winter monsoon (AWM) variability across the iNHG using a palaeomagnetically dated centennial-resolution grain size record between 3.6 and 1.9 Ma from a previously undescribed loess-palaeosol/red clay section on the central Chinese Loess Plateau. We find that the late Pliocene–early Pleistocene AWM was characterized by combined 41-kyr and ~100-kyr cycles, in response to ice volume and atmospheric CO2 forcing. Northern hemisphere ice sheet expansion, which was accompanied by an atmospheric CO2 concentration decline, substantially increased glacial AWM intensity and its orbitally oscillating amplitudes across the iNHG. Superposed on orbital variability, we find that millennial AWM intensity fluctuations persisted during both the warmer (higher-CO2) late Pliocene and colder (lower-CO2) early Pleistocene, in response to both external astronomical forcing and internal climate dynamics.

Original languageEnglish
Article number3364
Number of pages10
JournalNature Communications
Volume15
Issue number1
DOIs
Publication statusPublished - 19 Apr 2024

Bibliographical note

Publisher Copyright:
© The Author(s) 2024.

Funding

We thank professor Zhisheng An and Dr. A.C. Da Silva for helpful discussions. This study was supported financially by the Chinese Academy of Sciences Strategic Priority Research Program (XDB 40000000 to H.A.), the Second Tibetan Plateau Scientific Expedition and Research Program (2019QZKK0707 to H.A.), the Chinese Academy of Sciences Key Research Program of Frontier Sciences (QYZDB-SSW-DQC021 to H.A.), the National Natural Science Foundation of China (42074076 to H.A.), the Fund of Shandong Province (LSKJ202203300 to H.A. and\u00A0P.Z.), the Shaanxi Province Youth Talent Support Program (to H.A.), and the Australian Research Council (DP200100765 to A.P.R.). We thank professor Zhisheng An and Dr. A.C. Da Silva for helpful discussions. This study was supported financially by the Chinese Academy of Sciences Strategic Priority Research Program (XDB 40000000 to H.A.), the Second Tibetan Plateau Scientific Expedition and Research Program (2019QZKK0707 to H.A.), the Chinese Academy of Sciences Key Research Program of Frontier Sciences (QYZDB-SSW-DQC021 to H.A.), the National Natural Science Foundation of China (42074076 to H.A.), the Fund of Shandong Province (LSKJ202203300 to H.A. and P.Z.), the Shaanxi Province Youth Talent Support Program (to H.A.), and the Australian Research Council (DP200100765 to A.P.R.).

FundersFunder number
Shaanxi Province
Chinese Academy of SciencesXDB 40000000, 2019QZKK0707
Key Research Program of Frontier Science, Chinese Academy of SciencesQYZDB-SSW-DQC021
Fund of Shandong ProvinceLSKJ202203300
Australian Research CouncilDP200100765
National Natural Science Foundation of China42074076

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