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Please use this identifier to cite or link to this item: http://scholars.ntou.edu.tw/handle/123456789/9200
Title: Holocene surface hydroclimate changes in the Indo-Pacific warm pool
Authors: Li, Ziye
Chen, Min-Te 
Lin, Da-Cheng
Wang, Houjie
Shi, Xuefa
Liu, Shengfa
Yokoyama, Yusuke
Yamamoto, Masanobu
Shen, Chuan-Chou
Mii, Horng-Sheng
Troa, Rainer Arief
Zuraida, Rina
Triarso, Eko
Hendrizan, Marfasran
Keywords: SOUTH CHINA SEA;INTERTROPICAL CONVERGENCE ZONE;GLOBIGERINOIDES-RUBER WHITE;TERRESTRIAL ORGANIC-MATTER;PLANKTONIC-FORAMINIFERA;INDIAN-OCEAN;TETRAETHER LIPIDS;HIGH-RESOLUTION;MARITIME CONTINENT;SEDIMENT RECORDS
Issue Date: 20-Jul-2018
Publisher: PERGAMON-ELSEVIER SCIENCE LTD
Journal Volume: 482
Start page/Pages: 1-12
Source: QUATERN INT
Abstract: 
The Indo-Pacific warm pool (IPWP) is an area hosting key tropical climate processes such as the El Nino Southern Oscillation (ENSO) and Indian Ocean Dipole (IOD). The tropical climate processes, via various feedback mechanisms, control the surface ocean climate in the Indian Ocean and its surrounding continents on annual to inter-annual timescales. However, little has been known about how the tropical processes are effective forcing climate mechanism over longer timescales. Here we presented a reconstruction of the spatiotemporal pattern of sea surface temperature (SST) with inferred hydroclimate changes since the early Holocene (similar to 11ka), using proxies of planktonic foraminifer shell Mg/Ca, organic biomarker (TEX86), foraminifer oxygen isotopes, and a terrigenous BIT index measured from a 220 cm long Core BS24 (2.724041 degrees N, 97.010943 degrees E, 1015 m water depth) which was taken offshore of northwest Sumatra in the eastern Indian Ocean. With an age model of 13 AMS C-14 dating by the uses of planktonic foraminiferal shells from the core, the TEX86H temperatures of BS24 show as summer-weighted, and reflect integrated thermal effects from the surface to thermocline water, while the Mg/Ca temperature of BS24 better reflects mean annual SST. Our results, along with a regional synthesis of published SST records from the IPWP, suggest that the IPWP has migrated eastwardly since the mid-Holocene (similar to 5ka). In phase with this eastward migration, the IPWP SSTs have decreased, but the upwelling in the eastern Indian Ocean appears to have been a persistent feature since the mid-Holocene. Our Empirical Orthogonal Function (EOF) analysis on the compiled IPWP SST records indicates two dominant modes of spatio-temporal variability of surface hydrographes in the IPWP that are attributed to a combined effect of orbital and solar forcing, with expressions analogous to the Indian ocean basin-wide mode (IOBM) and the Indian Ocean dipole model (IOD).
URI: http://scholars.ntou.edu.tw/handle/123456789/9200
ISSN: 1040-6182
DOI: 10.1016/j.quaint.2018.04.027
Appears in Collections:地球科學研究所
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