PP53A-2310
Pleistocene Indian Monsoon rainfall variability dominated by obliquity

Friday, 18 December 2015
Poster Hall (Moscone South)
Daniel Gebregiorgis1, Ed C Hathorne1, Liviu Giosan2, Timothy S Collett3, Dirk Nuernberg1 and Martin Frank1, (1)GEOMAR Helmholtz Centre for Ocean Research Kiel, Kiel, Germany, (2)Woods Hole Oceanographic Inst, Woods Hole, MA, United States, (3)USGS Colorado Water Science Center Denver, Denver, CO, United States
Abstract:
The past variability of the Indian Monsoon is mostly known from records of wind strength over the Arabian Sea while Quaternary proxy records of Indian monsoon precipitation are still lacking. Here we utilize scanning x-ray fluorescence (XRF) data from a sediment core obtained by the IODP vessel JOIDES Resolution in the Andaman Sea (Site 17) to investigate changes in sediment supply from the peak monsoon precipitation regions to the core site. We use Ti/Ca and K/Rb ratios to trace changes in terrigenous flux and weathering regime, respectively, while Zr/Rb ratios suggest grain size variations. The age model of Site 17 is based on correlation of benthic C. wuellerstorfi/C. mundulus δ18O data to the LR04 global benthic δ18O stack at a resolution of ~3 kyr (Lisiecki and Raymo, 2005) for the last 2 Myrs. In its youngest part the age model is supported by five 14C ages on planktic foraminifera and the youngest Toba ash layer (Ali et al., 2015) resulting in a nearly constant sedimentation rate of ~6.5 cm/kyr. Frequency analysis of the 4 mm resolution Ti/Ca, K/Rb, and Zr/Rb time series using the REDFIT program (Schulz and Mudelsee, 2002), reveals the three main Milankovitch orbital cycles above the 90% confidence level. Depth domain spectral analysis reveals the presence of significant cyclicity at wavelengths of 28.5 and 2.8 m corresponding to the ~400 kyr and ~41 kyr cycles, respectively, during the last 2 Myr. These records suggest that Indian monsoon variability has varied in the obliquity and eccentricity bands, the latter in particular after the mid Pleistocene transition (MPT), while strong precession forcing is lacking in this super-high resolution record. Northern summer insolation and Southern Hemisphere latent heat export are out of phase during precessional cycles, but in phase in the obliquity band, which indicates that Indian monsoon precipitation has likely been more sensitive to both NH pull and SH push mechanisms (Clemens and Prell, 2003).

References

Ali, S., et al., 2015. Geochem., Geophy., Geosys., 16, 505-521.

Clemens, S.C. and Prell, W.L., 2003. Marine Geology, 201(1): 35-51.

Lisiecki, L. E. and M. E. Raymo ,2005. Paleoceanography, 20, PA1003.

Schulz, M., and Mudelsee, M., 2002. Computers & Geosciences, v. 28, p. 421-426.