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Preface for article collection “Evolution and variability of Asian Monsoon and its linkage with Cenozoic global cooling”

Although the Asian monsoon (AM) is a regional phenomenon, it exerts a significant impact on global climate. Because uplift of the Himalaya and Tibetan Plateau (HTP) has been considered to play a significant role on the establishment of the AM, numerous attempts have been made to prove the linkage between HTP uplift and AM evolution. On the other hand, comparison of global climate and AM evolution during Cenozoic suggests that AM evolution is significantly affected by global climate. So, it is necessary to evaluate both factors to properly understand the evolution and variability of the AM.

Since the beginning of this century, constraints on the timing and mode of HTP uplift and related onset and spatiotemporal evolution of the AM from terrestrial localities increased drastically. However, information from marine sediments was largely limited to the late Quaternary because no attempt at deep-sea drilling of longer sections in Asia had been made since the end of the last century.

From 2013 to 2016, Integrated Ocean Drilling Program/International Ocean Discovery Program (IODP) conducted a series of expeditions that were focused on AM evolution and its interaction with the wider climate system in the NW Pacific and Indian Ocean regions. In this volume of SPEPS, we introduce some of the new results concerning the evolution and variability of the AM during the Neogene obtained from IODP Expeditions 346, 355, and 359 (Tada et al. 2015; Pandey et al. 2016; Betzler et al. 2017).

AM evolution on tectonic time scales is the major topic of this SPEPS. Betzler et al. (2018) examined the relationship between evolution of the South Asian monsoon, global climatic changes, and sea-level changes during the Neogene based on the results of drilling of the carbonate platform of the Maldives in the Indian Ocean by IODP Expedition 359. They found an abrupt change in sedimentation pattern from platform sedimentation to a current-controlled sedimentation at 12.9-13 Ma, which they interpret to reflect the abrupt onset of strong monsoon winds. This finding changed our understanding concerning the timing of intensification of monsoon winds that had previously been considered to be ~ 8.5 Ma based on increasing abundance of upwelling sensitive planktonic foraminifer Globigerina bulloides in the Arabian Sea (Kroon et al. 1991).

Clift (2017) discussed interactions between AM changes and tectonics in the Western Himalaya based on a comprehensive review of sedimentary records studied in the Himalayan foreland basin and Indus submarine fan, including the result of IODP Expedition 355 from the viewpoint of evolving provenance and weathering. He demonstrated that exhumation of the Greater Himalaya was earlier in the west than in the central Himalaya and peaked in rate in the Middle Miocene, probably due to intensification of the AM. He further demonstrated that exhumation in the Western Himalaya decreased after this time, especially during the Late Miocene because of weakening of summer rains possibly due to Late Miocene cooling and southward migration of the ITCZ.

A continuous Neogene sedimentary record of the AM was also obtained from the Japan Sea by IODP Expedition 346. Kurokawa et al. (2019) demonstrated that gamma-ray attenuation (GRA) density of the hemipelagic sediments of the Japan Sea reflects biogenic silica content that changed in association with glacio-eustatic sea-level changes. They established a high-resolution age model covering the last ~ 12 Myr by tuning a 100-kyr-filtered GRA density profile to short eccentricity cycles for the sediments obtained from IODP Sites U1425 and U1430 in the central and southwestern parts of the Japan Sea. Based on this age model, a hiatus was identified at Site U1430 (water depth = 1072 m) from ~ 7 to ~ 5 Ma corresponding to late Miocene global cooling (Herbert et al. 2016) that may imply intensification of intermediate water production in the Japan Sea during this period.

Matsuzaki et al. (2018) reconstructed shallow-to-deep-water hydrography of the Japan Sea during the Mio-Pliocene based on radiolarian assemblages at Sites U1425 and U1430, and demonstrated that local tectonism and glacio-eustatic sea-level changes influenced the hydrography of the Japan Sea through controlling the position and sill depths of the seaways that connected the basin to the North Pacific. They also demonstrated that late Miocene global cooling and early Pliocene warming significantly affected the hydrography of the sea.

Elemental carbon (EC) in the sediments is considered to reflect biomass burning in the source area that is controlled by the vegetation volume, areal cover, and frequency of lightning. Lu et al. (2018) measured EC in fine (< 2 μm) and coarse (> 2 μm) fractions and pollen assemblage of the sediments at IODP Site U1423 in the northeastern Japan Sea covering the last 4.2 Myr. They interpreted EC in the coarse fraction to have come from the Japanese islands whereas that in the fine fraction came from more distant sources. They compared coarse EC with the pollen assemblage and found coarse EC tends to be higher when the climate was wetter. Coarse EC tends to be higher and shows significant fluctuations after 1.8 Ma suggesting more wet and variable climatic conditions after 1.8 Ma.

Orbital to millennial-scale variability of the AM is the other major theme of this SPEPS volume. Kunkelova et al. (2018) analyzed the last 2 Myr in cores from IODP Site U1467 in the Maldives using an XRF core-scanner, and examined aridity cyclical periods on orbital time-scales in the low latitudes of the Indian-Asian continent using Fe/K ratios. They found 100-kyr-like aridity cycles of around 130 kyr frequency in the interval from 1.25 to 2 Ma, which is not present in the LR04 benthic δ18O record (Lisiecki and Raymo 2005). They interpreted this as implying increased tilt sensitivity to regional eccentricity insolation changes prior to the Mid Pleistocene Transition (MPT).

The Quaternary sediments of the Japan Sea are characterized by centimeter- to decimeter-scale alternations of dark organic carbon-rich layers and light organic carbon-poor layers that were considered to be the result of millennial-scale changes in salinity and nutrient content of the influx from the East China Sea (ECS), which in turn reflected changes in summer precipitation in South China (Tada et al. 1999). IODP Expedition 346 was planned and seven sites in the Japan Sea and two sites in the northern ECS were drilled to test this hypothesis (Tada et al. 2015). Irino et al. (2018) reexamined core photographs and physical properties; data taken onboard from the seven sites in the Japan Sea in order to revise spliced sequences and associated data sets of physical properties measured onboard. They constructed almost perfectly continuous spliced columnar sections and revised the associated data sets of physical properties that are prerequisite for high-resolution paleoclimatic studies of the AM. The revised spliced columnar sections and associated data sets have been used by Tada et al. (2018), Sagawa et al. (2018), Lu et al. (2018), Matsuzaki et al. (2018), and Kurokawa et al. (2019) in this SPEPS.

Tada et al. (2018) constructed a high-resolution age model based on tuning the GRA profile to the LR04 benthic δ18O profile during the last 3 Myr at IODP Site U1424 in the eastern part of the Japan Sea where the best paleomagnetic datum and marker tephras are available, thus providing tight age constraints. Subsequently, Tada et al. (2018) correlated individual dark layers between the six deeper sites (U1422, 1423, 1424, 1425, 1426, and 1430) that allowed projection of a high-resolution age model at Site U1424 to the other sites. The result suggests the synchronous deposition of dark layers started at 1.45 Ma. Since then, the Japan Sea has responded as a single system to paleoceanographic perturbations.

IODP Site U1427 (water depth = 330 m) is located on the southern margin of the Japan Sea where the Quaternary sediments do not show alternation of dark and light layers. Consequently, the high-resolution correlation with dark and light layers of other deeper sites is complex. Sagawa et al. (2018) correlated Site U1427 with Site U1426, ~ 100 km to the north in the Japan Sea, and Site U1429, ~ 500 km to the southwest in the northern ECS using 18 tephra layers. Based on these tephra correlations, they linked the benthic δ18O record at Site U1427 with that at Site U1429 to develop a LR04-tuned age model covering the last 0.4 Myr. They also demonstrated that the subtle color variations at Site U1427 can be correlated to color variations at Site U1426 over orbital time scales, and imported an age model of Tada et al. (2018) from Site U1426 to Site U1427 for the stratigraphic interval covering the last 1.1 Myr. The two age models are conformable and orbital-scale correlation was established between Site U1429 in the ESC and all seven Japan Sea sites for the stratigraphic intervals covering the last 0.4 Myr. This allowed us to examine the linkage between summer precipitation in southern China and dark and light layers deposition in the Japan Sea through the northeastern ECS.

Summer sea surface salinity (SSS) in the northeastern part of the ECS reflects summer monsoon precipitation in southern China (Kubota et al. 2010, 2015). Kubota et al. (2019) reconstructed temporal changes in summer SSS in the northeastern part of the ECS close to IODP Site U1429 during MIS 3 based on δ18O and Mg/Ca ratio of planktonic foraminifera Globigerinoides ruber, and demonstrated millennial-scale changes associated with Dansgaard-Oeschger (D-O) cycles, with lower SSS events corresponding to D-O interstadials. Lower SSS events also correspond to dark layers in the Japan Sea sediments, consistent with the conclusions of Tada et al. (1999).

Papers in this collection demonstrate the results of the first round of research from IODP Expeditions 346, 355, and 359, which serve as the basis for the next stage of work. More research is in progress based on the results presented in this collection. Results from other IODP Expeditions related to Asian monsoon, such as Expedition 353, are also gradually emerging. Integration of the results from all the Asian monsoon related IODP expeditions will be desirable in the next round of analysis and interpretation.

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RT wrote the draft of this manuscript, and PDC and CB rewrote and confirmed the contents. All authors read and approved the final manuscript.

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Correspondence to Ryuji Tada.

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Tada, R., Betzler, C. & Clift, P.D. Preface for article collection “Evolution and variability of Asian Monsoon and its linkage with Cenozoic global cooling”. Prog Earth Planet Sci 7, 55 (2020). https://doi.org/10.1186/s40645-020-00361-z

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Keywords

  • Asian monsoon
  • Global cooling
  • IODP
  • Himalaya and Tibetan Plateau
  • Indian Ocean
  • Japan Sea