4.7 Article

Multiple forcing on Late Miocene East Asian Summer Monsoon Precipitation Variability in NE Tibetan Plateau

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CATENA
卷 221, 期 -, 页码 -

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ELSEVIER
DOI: 10.1016/j.catena.2022.106752

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Pollen; Probability density function; Global cooling Tectonic uplift; Eccentricity forcing

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Understanding the evolution of the East Asian Summer Monsoon (EASM) at different time scales is important for revealing the interactions between the hydrosphere, land, oceans, and atmosphere. By studying the late Miocene period, researchers have reconstructed the EASM precipitation and found that it is influenced by global climate and the uplift of the Tibetan Plateau. Additionally, on orbital time scales, the eccentricity periodicity plays a dominant role in the EASM precipitation cycles.
Understanding how the East Asian Summer Monsoon (EASM) evolves at different time scales affords a valuable opportunity to reveal the interactions between the hydrosphere, land, oceans and atmosphere. However, the pre -Quaternary evolutionary history and the driving forces that controlled its variability in response to different boundary conditions remain enigmatic. Here, we focus on the late Miocene (-10.8 to 6.3 Ma) - a period of profound climatic and topographic changes in Asia - and present a quantitative reconstruction of EASM pre-cipitation using the probabilistic CREST (Climate Reconstruction Software) method with a high temporal reso-lution pollen record from the Tianshui Basin in NE Tibetan Plateau (TP). Our new EASM precipitation record shows a slowly decreasing long-term trend during the period of -10.8-7.6 Ma, which was followed by a strengthening period from -7.6 to 6.3 Ma with a large amplitude of precipitation variability. We argue the decrease and increase periods of EASM precipitation were primarily response to late Miocene global cooling and TP uplift after -8 Ma, respectively. These results are supported by existing climate model simulations, wherein both global climate and paleotopography play key roles in regulating the long-term evolution of late Miocene EASM. On orbital time scales, the precipitation time series exhibit a dominant -410 kyr eccentricity periodicity, with lower (higher) values intervals corresponding to eccentricity minima (maximum). The synchronous phase of the precipitation and eccentricity records indicate that the eccentricity exerts a dominant influence on the EASM precipitation cycles via its modulation of the precessional amplitude, and the period expansion and contraction of Antarctic ice sheet (AIS) also probably play an important role during that time. Our quantitative late Miocene EASM precipitation records provide new insight into late Miocene EASM precipitation evolution and its relation with global climate, paleotopography, and cryosphere.

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