| Literature DB >> 29109454 |
Pradeep Srivastava1, Rajesh Agnihotri2, Deepti Sharma3, Narendra Meena4, Y P Sundriyal3, Anju Saxena2, Ravi Bhushan5, R Sawlani6, Upasana S Banerji5, C Sharma6, P Bisht4,3, N Rana3, R Jayangondaperumal4.
Abstract
We provide the first continuous Indian Summer Monsoon (ISM) climate record for the higher Himalayas (Kedarnath, India) by analyzing a 14C-dated peat sequence covering the last ~8000 years, with ~50 years temporal resolution. The ISM variability inferred using various proxies reveal striking similarity with the Greenland ice core (GISP2) temperature record and rapid denitrification changes recorded in the sediments off Peru. The Kedarnath record provides compelling evidence for a reorganization of the global climate system taking place at ~5.5 ka BP possibly after sea level stabilization and the advent of inter-annual climate variability governed by the modern ENSO phenomenon. The ISM record also captures warm-wet and cold-dry conditions during the Medieval Climate Anomaly and Little Ice Age, respectively.Entities:
Year: 2017 PMID: 29109454 PMCID: PMC5674060 DOI: 10.1038/s41598-017-15143-9
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1(a) Location, altitudinal map and photograph of the Kedarnath peat sequence. (b) Field photograph and litholog (panel ‘b’) were made using the MS-Coral Draw-X6c). Litholog is juxtaposed with sample locations of the studied peat sequence taken for AMS radiocarbon dates. (c) The age-depth model constructed using seven AMS radiocarbon dates using licensed version of sigma plot (v.10). Satellite image frame used in ‘panel a’ is adopted from Google Earth (version freely available for Windows 7).
Figure 2Depth profiles of sedimentary section (A) δ 15N and magnetic susceptibility (χlf), (B) δ 13C, (C) TC and TN weight fractions; (D) Weight fractions of crustal elements Fe, Al; (E–I) depth profiles of pollen assemblages. Higher TC, TN contents, lower δ 15N and χlf represent warmer periods (viz. medieval warm period MWP; shown by green coloured horizontal bands) supporting atmospheric N fixation, while colder periods (viz. Little Ice Age LIA; shown by pink coloured horizontal bands) are dominated by higher χlf, δ 15N, crustal element abundance. Pollen assemblage patterns collectively corroborate aforesaid contention (see text for details).
Figure 3Comparison of Kedarnath’s proxy-based ISM variability with contemporary palaeo-climatic records recovered from diverse geographic locations. (A) δ15N and magnetic susceptibility (χlf) records show compelling resemblance with (B) air-temperature variability recorded at GISP2 ice core at Greenland. (C) Similarity between the two records is more conspicuous since mid-Holocene (~5500 yr BP), where a −200 yr a constant offset was applied to age-depth model of Kedarnath peat sequence. (D) ENSO events per 100 year recorded in a Peruvian-lake showing dominance of ENSO system since mid-Holocene. (E) Covariance between d 15N patterns of Kedarnath peat-sequence and those recorded at Peru-margin (Agnihotri et al., 2006), noticeable arrival of high- frequency oscillations since mid-Holocene. (F) Hematite stained grains (HSG) counts in north Atlantic showing ‘Bond events’ indicating a significant change in the system at ~5.5 ka BP.
Figure 4Panel ‘A’ shows cross-coherency spectrum computed between χlf time-series data of Kedarnath peat-sequence with air-temperature data recorded in GISP2 ice core from Greenland (a −200 yr offset applied to the age-depth model of Kedarnath peat-sequence). Panel ‘B’ be shows cross-coherence between δ 15N records of Kedarnath peat-sequence and that of Peru margin (a +230 yr offset applied to the age-depth model of Peru δ 15N record). Cross-coherency spectral analysis was carried out using SPECTRUM program (Schulz & Stagger, 1997) designed for handling unevenly spaced palaeo-climatic time-series data. Significant coherencies (>80% confidence level) have been shown in respective panels. (See text for detailed interpretation).