South Asian Summer Monsoon precipitation variability during late Pliocene: Role of Indonesian Throughflow

被引:7
作者
Sarathchandraprasad, T. [1 ]
Tiwari, Manish [1 ]
Behera, Padmasini [1 ]
机构
[1] Minist Earth Sci, Natl Ctr Polar & Ocean Res, Vasco Da Gama 403804, Goa, India
关键词
IODP; Major elements; Monsoon drivers; Seaway changes; Periodicity; Spectral analysis; EASTERN ARABIAN SEA; INDIAN-OCEAN; HEAT-TRANSPORT; CLIMATE-CHANGE; WATER COLUMN; SEDIMENT; CIRCULATION; SURFACE; DENITRIFICATION; INTENSIFICATION;
D O I
10.1016/j.palaeo.2021.110447
中图分类号
P9 [自然地理学];
学科分类号
0705 ; 070501 ;
摘要
Understanding the response of the South Asian Summer Monsoon (SASM) to high atmospheric pCO(2) is required to predict future SASM changes under the current global warming scenario. The mid-Piacenzian Warm Period (mPWP), 3.0 to 3.3 Ma (million years ago) during the late Pliocene, provides us with such an opportunity as it had atmospheric pCO(2) comparable to the present. To reconstruct SASM variability during this period, we studied multiple proxies of terrigenous input (Ti), elasticity (Ti/Ca), chemical weathering (K/Al, Mg/Al), and productivity (Ba/Al, Ca-excess) in sediment collected during IODP Expedition 355 (Site U1456) spanning the mid to late Piacenzian (3.3-2.6 Ma). We find that the SASM intensified (weakened) during interglacials (glacials) of the mPWP and beyond in close correspondence with the global climate. However, we note that the SASM shifted to a higher mean state at 2.95 Ma. It could be because of the tectonically induced reorganization of the Indonesian Throughflow (ITF), which enhanced the cross-equatorial pressure gradient by changing the source of water to the southern equatorial Indian Ocean. This enhanced pressure gradient resulted in the intensification of the SASM during the late Piacenzian. During the northern hemisphere glaciation after 2.95 Ma, the SASM shows a long-term decline over and above the glacial-interglacial variability. The spectral and wavelet transform analysis indicates the control of the earth's orbital parameters, especially eccentricity, over the SASM variations during the late Piacenzian.
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页数:8
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